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Properties of Central Regions of the Dark Matter Halos in the Model with a Bump in the Power Spectrum of Density Perturbations 密度扰动功率谱凸起模型中暗物质晕中心区的性质
Pub Date : 2024-09-04 DOI: arxiv-2409.02739
Yu. N. EroshenkoInstitute for Nuclear Research, Russian Academy of Sciences, Moscow, Russia, V. N. LukashAstro Space Center, P. N. Lebedev Physical Institute, Russian Academy of Sciences, Moscow, Russia, E. V. MikheevaAstro Space Center, P. N. Lebedev Physical Institute, Russian Academy of Sciences, Moscow, Russia, S. V. PilipenkoAstro Space Center, P. N. Lebedev Physical Institute, Russian Academy of Sciences, Moscow, Russia, M. V. TkachevAstro Space Center, P. N. Lebedev Physical Institute, Russian Academy of Sciences, Moscow, Russia
A surprisingly large number of galaxies with masses of$sim10^9-10^{10}M_odot$ at redshifts of $zgeq9$ are discovered with theJames Webb Space Telescope. A possible explanation for the increase in the massfunction can be the presence of a local maximum (bump) in the power spectrum ofdensity perturbations on the corresponding scale. In this paper, it is shownthat simultaneously with the growth of the mass function, galaxies from thebump region must have a higher density (compactness) compared to cosmologicalmodels without a bump. These more compact galaxies have been partially includedin larger galaxies and have been subjected to tidal gravitational disruption.They have been less destructed than ``ordinary'' galaxies of the same mass, andsome of them could survive to $z = 0$ and persist on the periphery of somegalaxies. The formation and evolution of compact halos in a cube with a volumeof $(47 ,text{Mpc})^3$ with $(1024)^3$ dark matter particles in the redshiftrange from 120 to 0 have been numerically simulated and observationalimplications of the presence of such galaxies in the current Universe have beendiscussed.
詹姆斯-韦伯太空望远镜(James Webb Space Telescope)发现了数量惊人的质量为$z/geq9$的星系,它们的红移质量为$sim10^9-10^{10}M_odot$。质量函数增大的一个可能解释是在相应尺度的密度扰动功率谱中出现了局部最大值(凸起)。本文表明,在质量函数增长的同时,与没有凹凸的宇宙学模型相比,来自凹凸区域的星系必然具有更高的密度(紧凑性)。与相同质量的 "普通 "星系相比,它们受到的破坏较小,其中一些星系可以存活到 $z = 0$,并持续存在于一些星系的外围。在一个体积为$(47 ,text{Mpc})^3$的立方体中,有$(1024)^3$的暗物质粒子,它们的红移范围从120到0,对紧凑星系的形成和演化进行了数值模拟,并讨论了当前宇宙中存在这类星系的观测启示。
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引用次数: 0
Cosmological constraints on anisotropic Thurston geometries 各向异性瑟斯顿几何的宇宙学约束
Pub Date : 2024-09-04 DOI: arxiv-2409.03008
Ananda Smith, Craig J. Copi, Glenn D. Starkman
Much of modern cosmology relies on the Cosmological Principle, the assumptionthat the Universe is isotropic and homogeneous on sufficiently large scales,but it remains worthwhile to examine cosmological models that violate thisprinciple slightly. We examine a class of such spacetimes that maintainhomogeneity but break isotropy through their underlying local spatialgeometries. These spacetimes are endowed with one of five anisotropic modelgeometries of Thurston's geometrization theorem, and their evolution is sourcedwith perfect fluid dust and cosmological constant. We show that the backgroundevolution of these spacetimes induces fluctuations in the observed cosmicmicrowave background (CMB) temperature with amplitudes coupled to the curvatureparameter $Omega_K$. In order for these fluctuations to be compatible with theobserved CMB angular power spectrum, we find $|Omega_K| lesssim 10^{-5}$ isrequired in all five geometries, with two geometries requiring $|Omega_K|lesssim 10^{-10}$. This strongly limits the cosmological consequences of thesemodels.
现代宇宙学的大部分内容都依赖于宇宙学原理,即假设宇宙在足够大的尺度上是各向同性和均质的,但仍然值得研究稍微违反这一原理的宇宙学模型。我们研究了一类这样的时空,它们保持了均质性,但通过其底层局部空间几何打破了各向同性。这些时空被赋予瑟斯顿几何定理的五个各向异性模型几何之一,它们的演化来源于完美的流体尘埃和宇宙学常数。我们证明,这些时空的背景演变会引起观测到的宇宙微波背景(CMB)温度的波动,其振幅与曲率参数$Omega_K$相耦合。为了使这些波动与观测到的CMB角功率谱相匹配,我们发现在所有五个几何中都需要$|Omega_K| lesssim 10^{-5}$,其中两个几何需要$|Omega_K| lesssim 10^{-10}$。这极大地限制了这些模型的宇宙学后果。
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引用次数: 0
How DREAMS are made: Emulating Satellite Galaxy and Subhalo Populations with Diffusion Models and Point Clouds 梦想是怎样炼成的?用扩散模型和点云模拟卫星星系和子星系种群
Pub Date : 2024-09-04 DOI: arxiv-2409.02980
Tri Nguyen, Francisco Villaescusa-Navarro, Siddharth Mishra-Sharma, Carolina Cuesta-Lazaro, Paul Torrey, Arya Farahi, Alex M. Garcia, Jonah C. Rose, Stephanie O'Neil, Mark Vogelsberger, Xuejian Shen, Cian Roche, Daniel Anglés-Alcázar, Nitya Kallivayalil, Julian B. Muñoz, Francis-Yan Cyr-Racine, Sandip Roy, Lina Necib, Kassidy E. Kollmann
The connection between galaxies and their host dark matter (DM) halos iscritical to our understanding of cosmology, galaxy formation, and DM physics.To maximize the return of upcoming cosmological surveys, we need an accurateway to model this complex relationship. Many techniques have been developed tomodel this connection, from Halo Occupation Distribution (HOD) to empirical andsemi-analytic models to hydrodynamic. Hydrodynamic simulations can incorporatemore detailed astrophysical processes but are computationally expensive; HODs,on the other hand, are computationally cheap but have limited accuracy. In thiswork, we present NeHOD, a generative framework based on variational diffusionmodel and Transformer, for painting galaxies/subhalos on top of DM with anaccuracy of hydrodynamic simulations but at a computational cost similar toHOD. By modeling galaxies/subhalos as point clouds, instead of binning orvoxelization, we can resolve small spatial scales down to the resolution of thesimulations. For each halo, NeHOD predicts the positions, velocities, masses,and concentrations of its central and satellite galaxies. We train NeHOD on theTNG-Warm DM suite of the DREAMS project, which consists of 1024 high-resolutionzoom-in hydrodynamic simulations of Milky Way-mass halos with varying warm DMmass and astrophysical parameters. We show that our model captures the complexrelationships between subhalo properties as a function of the simulationparameters, including the mass functions, stellar-halo mass relations,concentration-mass relations, and spatial clustering. Our method can be usedfor a large variety of downstream applications, from galaxy clustering tostrong lensing studies.
星系与其宿主暗物质(DM)光环之间的联系对于我们理解宇宙学、星系形成和暗物质物理学至关重要。为了最大限度地提高即将到来的宇宙学探测的回报,我们需要对这种复杂的关系进行精确的建模。已经开发了许多技术来模拟这种关系,从晕占位分布(HOD)到经验模型和半解析模型,再到流体力学模型。流体动力学模拟可以包含更详细的天体物理过程,但计算成本昂贵;另一方面,HOD 计算成本低廉,但精度有限。在这项工作中,我们提出了一个基于变异扩散模型和变换器的生成框架 NeHOD,用于在 DM 的基础上绘制星系/副星系,其精度与流体力学模拟相当,但计算成本与 HOD 相似。通过将星系/副光环建模为点云,而不是二进制或体素化,我们可以将小的空间尺度解析到模拟的分辨率。对于每个光环,NeHOD 都能预测其中心星系和卫星星系的位置、速度、质量和浓度。我们在DREAMS项目的TNG-暖DM套件上对NeHOD进行了训练,该套件由1024个高分辨率放大流体力学模拟组成,模拟了具有不同暖DM质量和天体物理参数的银河质量光环。我们的研究表明,我们的模型捕捉到了亚晕属性之间复杂的关系,这些关系是模拟参数的函数,包括质量函数、恒星-亚晕质量关系、浓度-质量关系和空间聚类。我们的方法可用于大量下游应用,从星系聚类到强透镜研究。
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引用次数: 0
Euclid preparation: Determining the weak lensing mass accuracy and precision for galaxy clusters 欧几里得准备确定星系团的弱透镜质量精度和准确度
Pub Date : 2024-09-04 DOI: arxiv-2409.02783
Euclid Collaboration, L. IngogliaDipartimento di Fisica e Astronomia "Augusto Righi" - Alma Mater Studiorum Università di Bologna, via Piero Gobetti 93/2, 40129 Bologna, Italy, M. SerenoINAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Via Piero Gobetti 93/3, 40129 Bologna, ItalyINFN-Sezione di Bologna, Viale Berti Pichat 6/2, 40127 Bologna, Italy, S. FarrensUniversité Paris-Saclay, Université Paris Cité, CEA, CNRS, AIM, 91191, Gif-sur-Yvette, France, C. GiocoliINAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Via Piero Gobetti 93/3, 40129 Bologna, ItalyIstituto Nazionale di Fisica Nucleare, Sezione di Bologna, Via Irnerio 46, 40126 Bologna, Italy, L. BaumontUniversité Paris-Saclay, Université Paris Cité, CEA, CNRS, AIM, 91191, Gif-sur-Yvette, France, G. F. LesciDipartimento di Fisica e Astronomia "Augusto Righi" - Alma Mater Studiorum Università di Bologna, via Piero Gobetti 93/2, 40129 Bologna, ItalyINAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Via Piero Gobetti 93/3, 40129 Bologna, Italy, L. MoscardiniDipartimento di Fisica e Astronomia "Augusto Righi" - Alma Mater Studiorum Università di Bologna, via Piero Gobetti 93/2, 40129 Bologna, ItalyINAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Via Piero Gobetti 93/3, 40129 Bologna, ItalyINFN-Sezione di Bologna, Viale Berti Pichat 6/2, 40127 Bologna, Italy, C. MurrayUniversité Paris Cité, CNRS, Astroparticule et Cosmologie, 75013 Paris, France, M. VannierUniversité Côte d'Azur, Observatoire de la Côte d'Azur, CNRS, Laboratoire Lagrange, Bd de l'Observatoire, CS 34229, 06304 Nice cedex 4, France, A. BivianoINAF-Osservatorio Astronomico di Trieste, Via G. B. Tiepolo 11, 34143 Trieste, ItalyIFPU, Institute for Fundamental Physics of the Universe, via Beirut 2, 34151 Trieste, Italy, C. CarboneINAF-IASF Milano, Via Alfonso Corti 12, 20133 Milano, Italy, G. CovoneDepartment of Physics "E. Pancini", University Federico II, Via Cinthia 6, 80126, Napoli, ItalyINAF-Osservatorio Astronomico di Capodimonte, Via Moiariello 16, 80131 Napoli, ItalyINFN section of Naples, Via Cinthia 6, 80126, Napoli, Italy, G. DespaliDipartimento di Fisica e Astronomia "Augusto Righi" - Alma Mater Studiorum Università di Bologna, via Piero Gobetti 93/2, 40129 Bologna, ItalyINAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Via Piero Gobetti 93/3, 40129 Bologna, ItalyINFN-Sezione di Bologna, Viale Berti Pichat 6/2, 40127 Bologna, Italy, M. MaturiInstitut für Theoretische Physik, University of Heidelberg, Philosophenweg 16, 69120 Heidelberg, GermanyZentrum für Astronomie, Universität Heidelberg, Philosophenweg 12, 69120 Heidelberg, Germany, S. MaurogordatoUniversité Côte d'Azur, Observatoire de la Côte d'Azur, CNRS, Laboratoire Lagrange, Bd de l'Observatoire, CS 34229, 06304 Nice cedex 4, France, M. MeneghettiINAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Via Piero Gobetti 93/3, 40129 Bologna, ItalyINFN-Sezione di Bologna, Viale Berti Pichat 6/2, 40127 Bologna, Italy, M. RadovichINAF-Osservatorio Astronomico di Padova, Via dell'Osservatorio 5, 35122 Padova, Italy, B. AltieriESAC/ESA, Camino Bajo del Castillo, s/n., Urb. Villafranca del Castillo, 28692 Villanueva de la Cañada, Madrid, Spain, A. AmaraSchool of Mathematics and Physics, University of Surrey, Guildford, Surrey, GU2 7XH, UK, S. AndreonINAF-Osservatorio Astronomico di Brera, Via Brera 28, 20122 Milano, Italy, N. AuricchioINAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Via Piero Gobetti 93/3, 40129 Bologna, Italy, C. BaccigalupiIFPU, Institute for Fundamental Physics of the Universe, via Beirut 2, 34151 Trieste, ItalyINAF-Osservatorio Astronomico di Trieste, Via G. B. Tiepolo 11, 34143 Trieste, ItalyINFN, Sezione di Trieste, Via Valerio 2, 34127 Trieste TS, ItalySISSA, International School for Advanced Studies, Via Bonomea 265, 34136 Trieste TS, Italy, M. BaldiDipartimento di Fisica e Astronomia, Università di Bologna, Via Gobetti 93/2, 40129 Bologna, ItalyINAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Via Piero Gobetti 93/3, 40129 Bologna, ItalyINFN-Sezione di Bologna, Viale Berti Pichat 6/2, 40127 Bologna, Italy, S. BardelliINAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Via Piero Gobetti 93/3, 40129 Bologna, Italy, F. BellagambaDipartimento di Fisica e Astronomia, Università di Bologna, Via Gobetti 93/2, 40129 Bologna, ItalyINAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Via Piero Gobetti 93/3, 40129 Bologna, Italy, R. BenderMax Planck Institute for Extraterrestrial Physics, Giessenbachstr. 1, 85748 Garching, GermanyUniversitäts-Sternwarte München, Fakultät für Physik, Ludwig-Maximilians-Universität München, Scheinerstrasse 1, 81679 München, Germany, F. BernardeauInstitut de Physique Théorique, CEA, CNRS, Université Paris-Saclay 91191 Gif-sur-Yvette Cedex, FranceInstitut d'Astrophysique de Paris, UMR 7095, CNRS, and Sorbonne Université, 98 bis boulevard Arago, 75014 Paris, France, D. BoninoINAF-Osservatorio Astrofisico di Torino, Via Osservatorio 20, 10025 Pino Torinese, E. BranchiniDipartimento di Fisica, Università di Genova, Via Dodecaneso 33, 16146, Genova, ItalyINFN-Sezione di Genova, Via Dodecaneso 33, 16146, Genova, ItalyINAF-Osservatorio Astronomico di Brera, Via Brera 28, 20122 Milano, Italy, M. BresciaDepartment of Physics "E. Pancini", University Federico II, Via Cinthia 6, 80126, Napoli, ItalyINAF-Osservatorio Astronomico di Capodimonte, Via Moiariello 16, 80131 Napoli, ItalyINFN section of Naples, Via Cinthia 6, 80126, Napoli, Italy, J. BrinchmannInstituto de Astrofísica e Ciências do Espaço, Universidade do Porto, CAUP, Rua das Estrelas, PT4150-762 Porto, PortugalFaculdade de Ciências da Universidade do Porto, Rua do Campo de Alegre, 4150-007 Porto, Portugal, S. CameraDipartimento di Fisica, Università degli Studi di Torino, Via P. Giuria 1, 10125 Torino, ItalyINFN-Sezione di Torino, Via P. Giuria 1, 10125 Torino, ItalyINAF-Osservatorio Astrofisico di Torino, Via Osservatorio 20, 10025 Pino Torinese, V. CapobiancoINAF-Osservatorio Astrofisico di Torino, Via Osservatorio 20, 10025 Pino Torinese, J. CarreteroCentro de Investigaciones Energéticas, Medioambientales y TecnológicasPort d'Informació Científica, Campus UAB, C. Albareda s/n, 08193 Bellaterra, S. CasasInstitute for Theoretical Particle Physics and Cosmology, M. CastellanoINAF-Osservatorio Astronomico di Roma, Via Frascati 33, 00078 Monteporzio Catone, Italy, G. CastignaniINAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Via Piero Gobetti 93/3, 40129 Bologna, Italy, S. CavuotiINAF-Osservatorio Astronomico di Capodimonte, Via Moiariello 16, 80131 Napoli, ItalyINFN section of Naples, Via Cinthia 6, 80126, Napoli, Italy, A. CimattiDipartimento di Fisica e Astronomia "Augusto Righi" - Alma Mater Studiorum Università di Bologna, Viale Berti Pichat 6/2, 40127 Bologna, Italy, C. Colodro-CondeInstituto de Astrofísica de Canarias, Calle Vía Láctea s/n, 38204, San Cristóbal de La Laguna, Tenerife, Spain, G. CongedoInstitute for Astronomy, University of Edinburgh, Royal Observatory, Blackford Hill, Edinburgh EH9 3HJ, UK, C. J. ConseliceJodrell Bank Centre for Astrophysics, Department of Physics and Astronomy, University of Manchester, Oxford Road, Manchester M13 9PL, UK, L. ConversiEuropean Space Agency/ESRIN, Largo Galileo Galilei 1, 00044 Frascati, Roma, ItalyESAC/ESA, Camino Bajo del Castillo, s/n., Urb. Villafranca del Castillo, 28692 Villanueva de la Cañada, Madrid, Spain, Y. CopinUniversité Claude Bernard Lyon 1, CNRS/IN2P3, IP2I Lyon, UMR 5822, Villeurbanne, F-69100, France, F. CourbinInstitute of Physics, Laboratory of Astrophysics, Ecole Polytechnique Fédérale de LausanneInstitut de Ciències del CosmosInstitució Catalana de Recerca i Estudis Avançats, H. M. CourtoisUCB Lyon 1, CNRS/IN2P3, IUF, IP2I Lyon, 4 rue Enrico Fermi, 69622 Villeurbanne, France, M. CropperMullard Space Science Laboratory, University College London, Holmbury St Mary, Dorking, Surrey RH5 6NT, UK, A. Da SilvaDepartamento de Física, Faculdade de Ciências, Universidade de Lisboa, Edifício C8, Campo Grande, PT1749-016 Lisboa, PortugalInstituto de Astrofísica e Ciências do Espaço, Faculdade de Ciências, Universidade de Lisboa, Campo Grande, 1749-016 Lisboa, Portugal, H. DegaudenziDepartment of Astronomy, University of Geneva, ch. d'Ecogia 16, 1290 Versoix, Switzerland, G. De LuciaINAF-Osservatorio Astronomico di Trieste, Via G. B. Tiepolo 11, 34143 Trieste, Italy, J. DinisDepartamento de Física, Faculdade de Ciências, Universidade de Lisboa, Edifício C8, Campo Grande, PT1749-016 Lisboa, PortugalInstituto de Astrofísica e Ciências do Espaço, Faculdade de Ciências, Universidade de Lisboa, Campo Grande, 1749-016 Lisboa, Portugal, F. DubathDepartment of Astronomy, University of Geneva, ch. d'Ecogia 16, 1290 Versoix, Switzerland, C. A. J. DuncanJodrell Bank Centre for Astrophysics, Department of Physics and Astronomy, University of Manchester, Oxford Road, Manchester M13 9PL, UK, X. DupacESAC/ESA, Camino Bajo del Castillo, s/n., Urb. Villafranca del Castillo, 28692 Villanueva de la Cañada, Madrid, Spain, S. DusiniINFN-Padova, Via Marzolo 8, 35131 Padova, Italy, A. EaletUniversité Claude Bernard Lyon 1, CNRS/IN2P3, IP2I Lyon, UMR 5822, Villeurbanne, F-69100, France, M. FarinaINAF-Istituto di Astrofisica e Planetologia Spaziali, via del Fosso del Cavaliere, 100, 00100 Roma, Italy, F. FaustiniSpace Science Data Center, Italian Space Agency, via del Politecnico snc, 00133 Roma, ItalyINAF-Osservatorio Astronomico di Roma, Via Frascati 33, 00078 Monteporzio Catone, Italy, S. FerriolUniversité Claude Bernard Lyon 1, CNRS/IN2P3, IP2I Lyon, UMR 5822, Villeurbanne, F-69100, France, P. FosalbaInstitut d'Estudis Espacials de CatalunyaInstitute of Space Sciences, M. FrailisINAF-Osservatorio Astronomico di Trieste, Via G. B. Tiepolo 11, 34143 Trieste, Italy, E. FranceschiINAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Via Piero Gobetti 93/3, 40129 Bologna, Italy, M. FumanaINAF-IASF Milano, Via Alfonso Corti 12, 20133 Milano, Italy, S. GaleottaINAF-Osservatorio Astronomico di Trieste, Via G. B. Tiepolo 11, 34143 Trieste, Italy, W. GillardAix-Marseille Université, CNRS/IN2P3, CPPM, Marseille, France, B. GillisInstitute for Astronomy, University of Edinburgh, Royal Observatory, Blackford Hill, Edinburgh EH9 3HJ, UK, P. Gómez-AlvarezFRACTAL S.L.N.E., calle Tulipán 2, Portal 13 1A, 28231, Las Rozas de Madrid, SpainESAC/ESA, Camino Bajo del Castillo, s/n., Urb. Villafranca del Castillo, 28692 Villanueva de la Cañada, Madrid, Spain, A. GrazianINAF-Osservatorio Astronomico di Padova, Via dell'Osservatorio 5, 35122 Padova, Italy, F. GruppMax Planck Institute for Extraterrestrial Physics, Giessenbachstr. 1, 85748 Garching, GermanyUniversitäts-Sternwarte München, Fakultät für Physik, Ludwig-Maximilians-Universität München, Scheinerstrasse 1, 81679 München, Germany, L. GuzzoDipartimento di Fisica "Aldo Pontremoli", Università degli Studi di Milano, Via Celoria 16, 20133 Milano, ItalyINAF-Osservatorio Astronomico di Brera, Via Brera 28, 20122 Milano, Italy, S. V. H. HauganInstitute of Theoretical Astrophysics, University of Oslo, P.O. Box 1029 Blindern, 0315 Oslo, Norway, W. HolmesJet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, CA, 91109, USA, F. HormuthFelix Hormuth Engineering, Goethestr. 17, 69181 Leimen, Germany, A. HornstrupTechnical University of Denmark, Elektrovej 327, 2800 Kgs. Lyngby, DenmarkCosmic Dawn Center, P. HudelotInstitut d'Astrophysique de Paris, UMR 7095, CNRS, and Sorbonne Université, 98 bis boulevard Arago, 75014 Paris, France, S. IlićUniversité Paris-Saclay, CNRS/IN2P3, IJCLab, 91405 Orsay, FranceInstitut de Recherche en Astrophysique et Planétologie, K. JahnkeMax-Planck-Institut für Astronomie, Königstuhl 17, 69117 Heidelberg, Germany, M. JhabvalaNASA Goddard Space Flight Center, Greenbelt, MD 20771, USA, B. JoachimiDepartment of Physics and Astronomy, University College London, Gower Street, London WC1E 6BT, UK, E. KeihänenDepartment of Physics and Helsinki Institute of Physics, Gustaf Hällströmin katu 2, 00014 University of Helsinki, Finland, S. KermicheAix-Marseille Université, CNRS/IN2P3, CPPM, Marseille, France, A. KiesslingJet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, CA, 91109, USA, M. KilbingerUniversité Paris-Saclay, Université Paris Cité, CEA, CNRS, AIM, 91191, Gif-sur-Yvette, France, B. KubikUniversité Claude Bernard Lyon 1, CNRS/IN2P3, IP2I Lyon, UMR 5822, Villeurbanne, F-69100, France, M. KümmelUniversitäts-Sternwarte München, Fakultät für Physik, Ludwig-Maximilians-Universität München, Scheinerstrasse 1, 81679 München, Germany, M. KunzUniversité de Genève, Département de Physique Théorique and Centre for Astroparticle Physics, 24 quai Ernest-Ansermet, CH-1211 Genève 4, Switzerland, H. Kurki-SuonioDepartment of Physics, P.O. Box 64, 00014 University of Helsinki, FinlandHelsinki Institute of Physics, Gustaf Hällströmin katu 2, University of Helsinki, Helsinki, Finland, S. LigoriINAF-Osservatorio Astrofisico di Torino, Via Osservatorio 20, 10025 Pino Torinese, P. B. LiljeInstitute of Theoretical Astrophysics, University of Oslo, P.O. Box 1029 Blindern, 0315 Oslo, Norway, V. LindholmDepartment of Physics, P.O. Box 64, 00014 University of Helsinki, FinlandHelsinki Institute of Physics, Gustaf Hällströmin katu 2, University of Helsinki, Helsinki, Finland, I. LloroNOVA optical infrared instrumentation group at ASTRON, Oude Hoogeveensedijk 4, 7991PD, Dwingeloo, The Netherlands, G. MainettiCentre de Calcul de l'IN2P3/CNRS, 21 avenue Pierre de Coubertin 69627 Villeurbanne Cedex, France, E. MaioranoINAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Via Piero Gobetti 93/3, 40129 Bologna, Italy, O. MansuttiINAF-Osservatorio Astronomico di Trieste, Via G. B. Tiepolo 11, 34143 Trieste, Italy, S. MarcinUniversity of Applied Sciences and Arts of Northwestern Switzerland, School of Engineering, 5210 Windisch, Switzerland, O. MarggrafUniversität Bonn, Argelander-Institut für Astronomie, Auf dem Hügel 71, 53121 Bonn, Germany, K. MarkovicJet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, CA, 91109, USA, M. MartinelliINAF-Osservatorio Astronomico di Roma, Via Frascati 33, 00078 Monteporzio Catone, ItalyINFN-Sezione di Roma, Piazzale Aldo Moro, 2 - c/o Dipartimento di Fisica, Edificio G. Marconi, 00185 Roma, Italy, N. MartinetAix-Marseille Université, CNRS, CNES, LAM, Marseille, France, F. MarulliDipartimento di Fisica e Astronomia "Augusto Righi" - Alma Mater Studiorum Università di Bologna, via Piero Gobetti 93/2, 40129 Bologna, ItalyINAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Via Piero Gobetti 93/3, 40129 Bologna, ItalyINFN-Sezione di Bologna, Viale Berti Pichat 6/2, 40127 Bologna, Italy, R. MasseyDepartment of Physics, Institute for Computational Cosmology, Durham University, South Road, DH1 3LE, UK, E. MedinaceliINAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Via Piero Gobetti 93/3, 40129 Bologna, Italy, S. MeiUniversité Paris Cité, CNRS, Astroparticule et Cosmologie, 75013 Paris, France, M. MelchiorUniversity of Applied Sciences and Arts of Northwestern Switzerland, School of Engineering, 5210 Windisch, Switzerland, Y. MellierInstitut d'Astrophysique de Paris, 98bis Boulevard Arago, 75014, Paris, FranceInstitut d'Astrophysique de Paris, UMR 7095, CNRS, and Sorbonne Université, 98 bis boulevard Arago, 75014 Paris, France, E. MerlinINAF-Osservatorio Astronomico di Roma, Via Frascati 33, 00078 Monteporzio Catone, Italy, G. MeylanInstitute of Physics, Laboratory of Astrophysics, Ecole Polytechnique Fédérale de Lausanne, M. MorescoDipartimento di Fisica e Astronomia "Augusto Righi" - Alma Mater Studiorum Università di Bologna, via Piero Gobetti 93/2, 40129 Bologna, ItalyINAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Via Piero Gobetti 93/3, 40129 Bologna, Italy, E. MunariINAF-Osservatorio Astronomico di Trieste, Via G. B. Tiepolo 11, 34143 Trieste, ItalyIFPU, Institute for Fundamental Physics of the Universe, via Beirut 2, 34151 Trieste, Italy, S. -M. NiemiEuropean Space Agency/ESTEC, Keplerlaan 1, 2201 AZ Noordwijk, The Netherlands, C. PadillaInstitut de Física d'Altes Energies, K. PaechMax Planck Institute for Extraterrestrial Physics, Giessenbachstr. 1, 85748 Garching, Germany, S. PaltaniDepartment of Astronomy, University of Geneva, ch. d'Ecogia 16, 1290 Versoix, Switzerland, F. PasianINAF-Osservatorio Astronomico di Trieste, Via G. B. Tiepolo 11, 34143 Trieste, Italy, K. PedersenDARK, Niels Bohr Institute, University of Copenhagen, Jagtvej 155, 2200 Copenhagen, Denmark, W. J. PercivalWaterloo Centre for Astrophysics, University of Waterloo, Waterloo, Ontario N2L 3G1, CanadaDepartment of Physics and Astronomy, University of Waterloo, Waterloo, Ontario N2L 3G1, CanadaPerimeter Institute for Theoretical Physics, Waterloo, Ontario N2L 2Y5, Canada, V. PettorinoEuropean Space Agency/ESTEC, Keplerlaan 1, 2201 AZ Noordwijk, The Netherlands, S. PiresUniversité Paris-Saclay, Université Paris Cité, CEA, CNRS, AIM, 91191, Gif-sur-Yvette, France, G. PolentaSpace Science Data Center, Italian Space Agency, via del Politecnico snc, 00133 Roma, Italy, M. PoncetCentre National d'Etudes Spatiales -- Centre spatial de Toulouse, 18 avenue Edouard Belin, 31401 Toulouse Cedex 9, France, L. A. PopaInstitute of Space Science, Str. Atomistilor, nr. 409 Măgurele, Ilfov, 077125, Romania, L. PozzettiINAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Via Piero Gobetti 93/3, 40129 Bologna, Italy, F. RaisonMax Planck Institute for Extraterrestrial Physics, Giessenbachstr. 1, 85748 Garching, Germany, A. RenziDipartimento di Fisica e Astronomia "G. Galilei", Università di Padova, Via Marzolo 8, 35131 Padova, ItalyINFN-Padova, Via Marzolo 8, 35131 Padova, Italy, J. RhodesJet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, CA, 91109, USA, G. RiccioINAF-Osservatorio Astronomico di Capodimonte, Via Moiariello 16, 80131 Napoli, Italy, E. RomelliINAF-Osservatorio Astronomico di Trieste, Via G. B. Tiepolo 11, 34143 Trieste, Italy, M. RoncarelliINAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Via Piero Gobetti 93/3, 40129 Bologna, Italy, E. RossettiDipartimento di Fisica e Astronomia, Università di Bologna, Via Gobetti 93/2, 40129 Bologna, Italy, R. SagliaUniversitäts-Sternwarte München, Fakultät für Physik, Ludwig-Maximilians-Universität München, Scheinerstrasse 1, 81679 München, GermanyMax Planck Institute for Extraterrestrial Physics, Giessenbachstr. 1, 85748 Garching, Germany, Z. SakrInstitut für Theoretische Physik, University of Heidelberg, Philosophenweg 16, 69120 Heidelberg, GermanyInstitut de Recherche en Astrophysique et PlanétologieUniversité St Joseph, Faculty of Sciences, Beirut, Lebanon, J. -C. SalvignolEuropean Space Agency/ESTEC, Keplerlaan 1, 2201 AZ Noordwijk, The Netherlands, A. G. SánchezMax Planck Institute for Extraterrestrial Physics, Giessenbachstr. 1, 85748 Garching, Germany, D. SaponeDepartamento de Física, FCFM, Universidad de Chile, Blanco Encalada 2008, Santiago, Chile, B. SartorisUniversitäts-Sternwarte München, Fakultät für Physik, Ludwig-Maximilians-Universität München, Scheinerstrasse 1, 81679 München, GermanyINAF-Osservatorio Astronomico di Trieste, Via G. B. Tiepolo 11, 34143 Trieste, Italy, M. SchirmerMax-Planck-Institut für Astronomie, Königstuhl 17, 69117 Heidelberg, Germany, P. SchneiderUniversität Bonn, Argelander-Institut für Astronomie, Auf dem Hügel 71, 53121 Bonn, Germany, A. SecrounAix-Marseille Université, CNRS/IN2P3, CPPM, Marseille, France, G. SeidelMax-Planck-Institut für Astronomie, Königstuhl 17, 69117 Heidelberg, Germany, S. SerranoInstitut d'Estudis Espacials de CatalunyaSatlantis, University Science Park, Sede Bld 48940, Leioa-Bilbao, SpainInstitute of Space Sciences, C. SirignanoDipartimento di Fisica e Astronomia "G. Galilei", Università di Padova, Via Marzolo 8, 35131 Padova, ItalyINFN-Padova, Via Marzolo 8, 35131 Padova, Italy, G. SirriINFN-Sezione di Bologna, Viale Berti Pichat 6/2, 40127 Bologna, Italy, L. StancoINFN-Padova, Via Marzolo 8, 35131 Padova, Italy, J. SteinwagnerMax Planck Institute for Extraterrestrial Physics, Giessenbachstr. 1, 85748 Garching, Germany, P. Tallada-CrespíCentro de Investigaciones Energéticas, Medioambientales y TecnológicasPort d'Informació Científica, Campus UAB, C. Albareda s/n, 08193 Bellaterra, D. TavagnaccoINAF-Osservatorio Astronomico di Trieste, Via G. B. Tiepolo 11, 34143 Trieste, Italy, A. N. TaylorInstitute for Astronomy, University of Edinburgh, Royal Observatory, Blackford Hill, Edinburgh EH9 3HJ, UK, I. TerenoDepartamento de Física, Faculdade de Ciências, Universidade de Lisboa, Edifício C8, Campo Grande, PT1749-016 Lisboa, PortugalInstituto de Astrofísica e Ciências do Espaço, Faculdade de Ciências, Universidade de Lisboa, Tapada da Ajuda, 1349-018 Lisboa, Portugal, R. Toledo-MoreoUniversidad Politécnica de Cartagena, Departamento de Electrónica y Tecnología de Computadoras, Plaza del Hospital 1, 30202 Cartagena, Spain, F. TorradeflotPort d'Informació Científica, Campus UAB, C. Albareda s/n, 08193 BellaterraCentro de Investigaciones Energéticas, Medioambientales y Tecnológicas, I. TutusausInstitut de Recherche en Astrophysique et Planétologie, L. ValenzianoINAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Via Piero Gobetti 93/3, 40129 Bologna, ItalyINFN-Bologna, Via Irnerio 46, 40126 Bologna, Italy, T. VassalloUniversitäts-Sternwarte München, Fakultät für Physik, Ludwig-Maximilians-Universität München, Scheinerstrasse 1, 81679 München, GermanyINAF-Osservatorio Astronomico di Trieste, Via G. B. Tiepolo 11, 34143 Trieste, Italy, G. Verdoes KleijnKapteyn Astronomical Institute, University of Groningen, PO Box 800, 9700 AV Groningen, The Netherlands, A. VeropalumboINAF-Osservatorio Astronomico di Brera, Via Brera 28, 20122 Milano, ItalyINFN-Sezione di Genova, Via Dodecaneso 33, 16146, Genova, ItalyDipartimento di Fisica, Università degli studi di Genova, and INFN-Sezione di Genova, via Dodecaneso 33, 16146, Genova, Italy, Y. WangInfrared Processing and Analysis Center, California Institute of Technology, Pasadena, CA 91125, USA, J. WellerUniversitäts-Sternwarte München, Fakultät für Physik, Ludwig-Maximilians-Universität München, Scheinerstrasse 1, 81679 München, GermanyMax Planck Institute for Extraterrestrial Physics, Giessenbachstr. 1, 85748 Garching, Germany, G. ZamoraniINAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Via Piero Gobetti 93/3, 40129 Bologna, Italy, E. ZuccaINAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Via Piero Gobetti 93/3, 40129 Bologna, Italy, M. BolzonellaINAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Via Piero Gobetti 93/3, 40129 Bologna, Italy, E. BozzoDepartment of Astronomy, University of Geneva, ch. d'Ecogia 16, 1290 Versoix, Switzerland, C. BuriganaINAF, Istituto di Radioastronomia, Via Piero Gobetti 101, 40129 Bologna, ItalyINFN-Bologna, Via Irnerio 46, 40126 Bologna, Italy, M. CalabreseAstronomical Observatory of the Autonomous Region of the Aosta ValleyINAF-IASF Milano, Via Alfonso Corti 12, 20133 Milano, Italy, D. Di FerdinandoINFN-Sezione di Bologna, Viale Berti Pichat 6/2, 40127 Bologna, Italy, J. A. Escartin VigoMax Planck Institute for Extraterrestrial Physics, Giessenbachstr. 1, 85748 Garching, Germany, R. 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VielIFPU, Institute for Fundamental Physics of the Universe, via Beirut 2, 34151 Trieste, ItalyINAF-Osservatorio Astronomico di Trieste, Via G. B. Tiepolo 11, 34143 Trieste, ItalySISSA, International School for Advanced Studies, Via Bonomea 265, 34136 Trieste TS, ItalyINFN, Sezione di Trieste, Via Valerio 2, 34127 Trieste TS, ItalyICSC - Centro Nazionale di Ricerca in High Performance Computing, Big Data e Quantum Computing, Via Magnanelli 2, Bologna, Italy, M. WiesmannInstitute of Theoretical Astrophysics, University of Oslo, P.O. Box 1029 Blindern, 0315 Oslo, Norway, Y. AkramiInstituto de Física Teórica UAM-CSIC, Campus de Cantoblanco, 28049 Madrid, SpainCERCA/ISO, Department of Physics, Case Western Reserve University, 10900 Euclid Avenue, Cleveland, OH 44106, USA, V. AllevatoINAF-Osservatorio Astronomico di Capodimonte, Via Moiariello 16, 80131 Napoli, Italy, S. AnselmiINFN-Padova, Via Marzolo 8, 35131 Padova, ItalyDipartimento di Fisica e Astronomia "G. 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BorganiDipartimento di Fisica - Sezione di Astronomia, Università di Trieste, Via Tiepolo 11, 34131 Trieste, ItalyIFPU, Institute for Fundamental Physics of the Universe, via Beirut 2, 34151 Trieste, ItalyINAF-Osservatorio Astronomico di Trieste, Via G. B. Tiepolo 11, 34143 Trieste, ItalyINFN, Sezione di Trieste, Via Valerio 2, 34127 Trieste TS, Italy, S. BrutonMinnesota Institute for Astrophysics, University of Minnesota, 116 Church St SE, Minneapolis, MN 55455, USA, R. CabanacInstitut de Recherche en Astrophysique et Planétologie, A. CalabroINAF-Osservatorio Astronomico di Roma, Via Frascati 33, 00078 Monteporzio Catone, Italy, G. Cañas-HerreraEuropean Space Agency/ESTEC, Keplerlaan 1, 2201 AZ Noordwijk, The NetherlandsInstitute Lorentz, Leiden University, Niels Bohrweg 2, 2333 CA Leiden, The Netherlands, A. CappiINAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Via Piero Gobetti 93/3, 40129 Bologna, ItalyUniversité Côte d'Azur, Observatoire de la Côte d'Azur, CNRS, Laboratoire Lagrange, Bd de l'Observatoire, CS 34229, 06304 Nice cedex 4, France, F. CaroINAF-Osservatorio Astronomico di Roma, Via Frascati 33, 00078 Monteporzio Catone, Italy, C. S. CarvalhoInstituto de Astrofísica e Ciências do Espaço, Faculdade de Ciências, Universidade de Lisboa, Tapada da Ajuda, 1349-018 Lisboa, Portugal, T. CastroINAF-Osservatorio Astronomico di Trieste, Via G. B. Tiepolo 11, 34143 Trieste, ItalyINFN, Sezione di Trieste, Via Valerio 2, 34127 Trieste TS, ItalyIFPU, Institute for Fundamental Physics of the Universe, via Beirut 2, 34151 Trieste, ItalyICSC - Centro Nazionale di Ricerca in High Performance Computing, Big Data e Quantum Computing, Via Magnanelli 2, Bologna, Italy, K. C. ChambersInstitute for Astronomy, University of Hawaii, 2680 Woodlawn Drive, Honolulu, HI 96822, USA, S. ContariniMax Planck Institute for Extraterrestrial Physics, Giessenbachstr. 1, 85748 Garching, Germany, A. R. CoorayDepartment of Physics & Astronomy, University of California Irvine, Irvine CA 92697, USA, M. CostanziDipartimento di Fisica - Sezione di Astronomia, Università di Trieste, Via Tiepolo 11, 34131 Trieste, ItalyINAF-Osservatorio Astronomico di Trieste, Via G. B. Tiepolo 11, 34143 Trieste, ItalyIFPU, Institute for Fundamental Physics of the Universe, via Beirut 2, 34151 Trieste, Italy, O. CucciatiINAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Via Piero Gobetti 93/3, 40129 Bologna, Italy, G. DesprezDepartment of Astronomy & Physics and Institute for Computational Astrophysics, Saint Mary's University, 923 Robie Street, Halifax, Nova Scotia, B3H 3C3, Canada, A. Díaz-SánchezDepartamento Física Aplicada, Universidad Politécnica de Cartagena, Campus Muralla del Mar, 30202 Cartagena, Murcia, Spain, J. J. DiazInstituto de Astrofísica de Canarias, S. Di DomizioDipartimento di Fisica, Università di Genova, Via Dodecaneso 33, 16146, Genova, ItalyINFN-Sezione di Genova, Via Dodecaneso 33, 16146, Genova, Italy, H. DoleUniversité Paris-Saclay, CNRS, Institut d'astrophysique spatiale, 91405, Orsay, France, S. EscoffierAix-Marseille Université, CNRS/IN2P3, CPPM, Marseille, France, M. EzziatiAix-Marseille Université, CNRS, CNES, LAM, Marseille, France, A. G. FerrariDipartimento di Fisica e Astronomia "Augusto Righi" - Alma Mater Studiorum Università di Bologna, Viale Berti Pichat 6/2, 40127 Bologna, ItalyINFN-Sezione di Bologna, Viale Berti Pichat 6/2, 40127 Bologna, Italy, P. G. FerreiraDepartment of Physics, Oxford University, Keble Road, Oxford OX1 3RH, UK, I. FerreroInstitute of Theoretical Astrophysics, University of Oslo, P.O. Box 1029 Blindern, 0315 Oslo, Norway, A. FinoguenovDepartment of Physics, P.O. Box 64, 00014 University of Helsinki, Finland, A. FontanaINAF-Osservatorio Astronomico di Roma, Via Frascati 33, 00078 Monteporzio Catone, Italy, F. FornariINFN-Bologna, Via Irnerio 46, 40126 Bologna, Italy, L. GabarraDepartment of Physics, Oxford University, Keble Road, Oxford OX1 3RH, UK, K. GangaUniversité Paris Cité, CNRS, Astroparticule et Cosmologie, 75013 Paris, France, J. García-BellidoInstituto de Física Teórica UAM-CSIC, Campus de Cantoblanco, 28049 Madrid, Spain, T. GasparettoINAF-Osservatorio Astronomico di Trieste, Via G. B. Tiepolo 11, 34143 Trieste, Italy, V. GautardCEA Saclay, DFR/IRFU, Service d'Astrophysique, Bat. 709, 91191 Gif-sur-Yvette, France, E. GaztanagaInstitute of Space SciencesInstitut d'Estudis Espacials de CatalunyaInstitute of Cosmology and Gravitation, University of Portsmouth, Portsmouth PO1 3FX, UK, F. GiacominiINFN-Sezione di Bologna, Viale Berti Pichat 6/2, 40127 Bologna, Italy, F. GianottiINAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Via Piero Gobetti 93/3, 40129 Bologna, Italy, G. GozaliaslDepartment of Computer Science, Aalto University, PO Box 15400, Espoo, FI-00 076, FinlandDepartment of Physics, P.O. Box 64, 00014 University of Helsinki, Finland, C. M. GutierrezInstituto de Astrofísica de Canarias, c/ Via Lactea s/n, La Laguna E-38200, Spain. Departamento de Astrofí sica de la Universidad de La Laguna, Avda. Francisco Sanchez, La Laguna, E-38200, Spain, A. HallInstitute for Astronomy, University of Edinburgh, Royal Observatory, Blackford Hill, Edinburgh EH9 3HJ, UK, H. HildebrandtRuhr University Bochum, Faculty of Physics and Astronomy, Astronomical Institute, J. HjorthDARK, Niels Bohr Institute, University of Copenhagen, Jagtvej 155, 2200 Copenhagen, Denmark, A. Jimenez MuñozUniv. Grenoble Alpes, CNRS, Grenoble INP, LPSC-IN2P3, 53, Avenue des Martyrs, 38000, Grenoble, France, J. J. E. KajavaDepartment of Physics and Astronomy, Vesilinnantie 5, 20014 University of Turku, FinlandSerco for European Space Agency, V. KansalARC Centre of Excellence for Dark Matter Particle Physics, Melbourne, AustraliaCentre for Astrophysics & Supercomputing, Swinburne University of Technology, Hawthorn, Victoria 3122, Australia, D. KaragiannisSchool of Physics and Astronomy, Queen Mary University of London, Mile End Road, London E1 4NS, UKDepartment of Physics and Astronomy, University of the Western Cape, Bellville, Cape Town, 7535, South Africa, C. C. KirkpatrickDepartment of Physics and Helsinki Institute of Physics, Gustaf Hällströmin katu 2, 00014 University of Helsinki, Finland, A. M. C. Le BrunLaboratoire Univers et Théorie, Observatoire de Paris, Université PSL, Université Paris Cité, CNRS, 92190 Meudon, France, J. Le GraetAix-Marseille Université, CNRS/IN2P3, CPPM, Marseille, France, L. LegrandICTP South American Institute for Fundamental Research, Instituto de Física Teórica, Universidade Estadual Paulista, São Paulo, Brazil, J. LesgourguesInstitute for Theoretical Particle Physics and Cosmology, T. I. LiaudatIRFU, CEA, Université Paris-Saclay 91191 Gif-sur-Yvette Cedex, France, A. LoureiroOskar Klein Centre for Cosmoparticle Physics, Department of Physics, Stockholm University, Stockholm, SE-106 91, SwedenAstrophysics Group, Blackett Laboratory, Imperial College London, London SW7 2AZ, UK, J. Macias-PerezUniv. Grenoble Alpes, CNRS, Grenoble INP, LPSC-IN2P3, 53, Avenue des Martyrs, 38000, Grenoble, France, G. MaggioINAF-Osservatorio Astronomico di Trieste, Via G. B. Tiepolo 11, 34143 Trieste, Italy, M. MagliocchettiINAF-Istituto di Astrofisica e Planetologia Spaziali, via del Fosso del Cavaliere, 100, 00100 Roma, Italy, F. MannucciINAF-Osservatorio Astrofisico di Arcetri, Largo E. Fermi 5, 50125, Firenze, Italy, R. MaoliDipartimento di Fisica, Sapienza Università di Roma, Piazzale Aldo Moro 2, 00185 Roma, ItalyINAF-Osservatorio Astronomico di Roma, Via Frascati 33, 00078 Monteporzio Catone, Italy, J. Martín-FleitasAurora Technology for European Space Agency, C. J. A. P. MartinsCentro de Astrofísica da Universidade do Porto, Rua das Estrelas, 4150-762 Porto, PortugalInstituto de Astrofísica e Ciências do Espaço, Universidade do Porto, CAUP, Rua das Estrelas, PT4150-762 Porto, Portugal, L. MaurinUniversité Paris-Saclay, CNRS, Institut d'astrophysique spatiale, 91405, Orsay, France, R. B. MetcalfDipartimento di Fisica e Astronomia "Augusto Righi" - Alma Mater Studiorum Università di Bologna, via Piero Gobetti 93/2, 40129 Bologna, ItalyINAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Via Piero Gobetti 93/3, 40129 Bologna, Italy, M. MiluzioESAC/ESA, Camino Bajo del Castillo, s/n., Urb. Villafranca del Castillo, 28692 Villanueva de la Cañada, Madrid, SpainHE Space for European Space Agency, P. MonacoDipartimento di Fisica - Sezione di Astronomia, Università di Trieste, Via Tiepolo 11, 34131 Trieste, ItalyINAF-Osservatorio Astronomico di Trieste, Via G. B. Tiepolo 11, 34143 Trieste, ItalyINFN, Sezione di Trieste, Via Valerio 2, 34127 Trieste TS, ItalyIFPU, Institute for Fundamental Physics of the Universe, via Beirut 2, 34151 Trieste, Italy, A. MontoroInstitute of Space SciencesInstitut d'Estudis Espacials de Catalunya, A. MoraAurora Technology for European Space Agency, C. MorettiSISSA, International School for Advanced Studies, Via Bonomea 265, 34136 Trieste TS, ItalyICSC - Centro Nazionale di Ricerca in High Performance Computing, Big Data e Quantum Computing, Via Magnanelli 2, Bologna, ItalyINAF-Osservatorio Astronomico di Trieste, Via G. B. Tiepolo 11, 34143 Trieste, ItalyIFPU, Institute for Fundamental Physics of the Universe, via Beirut 2, 34151 Trieste, ItalyINFN, Sezione di Trieste, Via Valerio 2, 34127 Trieste TS, Italy, G. MorganteINAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Via Piero Gobetti 93/3, 40129 Bologna, Italy, S. NadathurInstitute of Cosmology and Gravitation, University of Portsmouth, Portsmouth PO1 3FX, UK, Nicholas A. WaltonInstitute of Astronomy, University of Cambridge, Madingley Road, Cambridge CB3 0HA, UK, L. PaganoDipartimento di Fisica e Scienze della Terra, Università degli Studi di Ferrara, Via Giuseppe Saragat 1, 44122 Ferrara, ItalyIstituto Nazionale di Fisica Nucleare, Sezione di Ferrara, Via Giuseppe Saragat 1, 44122 Ferrara, Italy, L. PatriziiINFN-Sezione di Bologna, Viale Berti Pichat 6/2, 40127 Bologna, Italy, V. PopaInstitute of Space Science, Str. Atomistilor, nr. 409 Măgurele, Ilfov, 077125, Romania, D. PotterDepartment of Astrophysics, University of Zurich, Winterthurerstrasse 190, 8057 Zurich, Switzerland, I. RissoINAF-Osservatorio Astronomico di Brera, Via Brera 28, 20122 Milano, Italy, and INFN-Sezione di Genova, Via Dodecaneso 33, 16146, Genova, Italy, P. -F. RocciUniversité Paris-Saclay, CNRS, Institut d'astrophysique spatiale, 91405, Orsay, France, M. SahlénTheoretical astrophysics, Department of Physics and Astronomy, Uppsala University, Box 515, 751 20 Uppsala, Sweden, E. SarpaSISSA, International School for Advanced Studies, Via Bonomea 265, 34136 Trieste TS, ItalyICSC - Centro Nazionale di Ricerca in High Performance Computing, Big Data e Quantum Computing, Via Magnanelli 2, Bologna, ItalyINFN, Sezione di Trieste, Via Valerio 2, 34127 Trieste TS, Italy, A. SchneiderDepartment of Astrophysics, University of Zurich, Winterthurerstrasse 190, 8057 Zurich, Switzerland, M. SchultheisUniversité Côte d'Azur, Observatoire de la Côte d'Azur, CNRS, Laboratoire Lagrange, Bd de l'Observatoire, CS 34229, 06304 Nice cedex 4, France, P. SimonUniversität Bonn, Argelander-Institut für Astronomie, Auf dem Hügel 71, 53121 Bonn, Germany, A. Spurio ManciniDepartment of Physics, Royal Holloway, University of London, TW20 0EX, UKMullard Space Science Laboratory, University College London, Holmbury St Mary, Dorking, Surrey RH5 6NT, UK, J. StadelDepartment of Astrophysics, University of Zurich, Winterthurerstrasse 190, 8057 Zurich, Switzerland, S. A. StanfordDepartment of Physics and Astronomy, University of California, Davis, CA 95616, USA, K. TanidisDepartment of Physics, Oxford University, Keble Road, Oxford OX1 3RH, UK, C. TaoAix-Marseille Université, CNRS/IN2P3, CPPM, Marseille, France, G. TesteraINFN-Sezione di Genova, Via Dodecaneso 33, 16146, Genova, Italy, R. TeyssierDepartment of Astrophysical Sciences, Peyton Hall, Princeton University, Princeton, NJ 08544, USA, S. ToftCosmic Dawn CenterNiels Bohr Institute, University of Copenhagen, Jagtvej 128, 2200 Copenhagen, Denmark, S. TosiDipartimento di Fisica, Università di Genova, Via Dodecaneso 33, 16146, Genova, ItalyINFN-Sezione di Genova, Via Dodecaneso 33, 16146, Genova, Italy, A. TrojaDipartimento di Fisica e Astronomia "G. Galilei", Università di Padova, Via Marzolo 8, 35131 Padova, ItalyINFN-Padova, Via Marzolo 8, 35131 Padova, Italy, M. TucciDepartment of Astronomy, University of Geneva, ch. d'Ecogia 16, 1290 Versoix, Switzerland, C. ValieriINFN-Sezione di Bologna, Viale Berti Pichat 6/2, 40127 Bologna, Italy, J. ValiviitaDepartment of Physics, P.O. Box 64, 00014 University of Helsinki, FinlandHelsinki Institute of Physics, Gustaf Hällströmin katu 2, University of Helsinki, Helsinki, Finland, D. VerganiINAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Via Piero Gobetti 93/3, 40129 Bologna, Italy, G. VerzaCenter for Cosmology and Particle Physics, Department of Physics, New York University, New York, NY 10003, USACenter for Computational Astrophysics, Flatiron Institute, 162 5th Avenue, 10010, New York, NY, USA, P. VielzeufAix-Marseille Université, CNRS/IN2P3, CPPM, Marseille, France
We investigate the level of accuracy and precision of cluster weak-lensing(WL) masses measured with the Euclid data processing pipeline. We use theDEMNUni-Cov $N$-body simulations to assess how well the WL mass probes the truehalo mass, and, then, how well WL masses can be recovered in the presence ofmeasurement uncertainties. We consider different halo mass density models,priors, and mass point estimates. WL mass differs from true mass due to, e.g.,the intrinsic ellipticity of sources, correlated or uncorrelated matter andlarge-scale structure, halo triaxiality and orientation, and merging orirregular morphology. In an ideal scenario without observational or measurementerrors, the maximum likelihood estimator is the most accurate, with WL massesbiased low by $langle b_M rangle = -14.6 pm 1.7 , %$ on average over thefull range $M_text{200c} > 5 times 10^{13} , M_odot$ and $z < 1$. Due tothe stabilising effect of the prior, the biweight, mean, and median estimatesare more precise. The scatter decreases with increasing mass and informativepriors significantly reduce the scatter. Halo mass density profiles with atruncation provide better fits to the lensing signal, while the accuracy andprecision are not significantly affected. We further investigate the impact ofadditional sources of systematic uncertainty on the WL mass, namely the impactof photometric redshift uncertainties and source selection, the expectedperformance of Euclid cluster detection algorithms, and the presence of masks.Taken in isolation, we find that the largest effect is induced bynon-conservative source selection. This effect can be mostly removed with arobust selection. As a final Euclid-like test, we combine systematic effectsin a realistic observational setting and find results similar to the idealcase, $langle b_M rangle = - 15.5 pm 2.4 , %$, under a robust selection.
我们研究了用(Euclid)数据处理管道测量的星团弱透镜(WL)质量的准确度和精确度。我们使用DEMNUni-Cov $N$体模拟来评估WL质量对真实光环质量的探测程度,以及在存在测量不确定性的情况下WL质量的恢复程度。我们考虑了不同的光环质量密度模型、先验和质量点估计。WL质量不同于真实质量的原因包括:源的内在椭圆度、相关或不相关的物质和大尺度结构、光环的三轴性和方向以及合并或不规则形态。在没有观测或测量误差的理想情况下,最大似然估计是最准确的,WL质量在整个范围内平均偏低$M_text{200c}=-14.6pm 1.7%$。> 5 times 10^{13}M_odot$ 和 $z < 1$.由于先验的稳定作用,双权重、平均值和中位数估计值更加精确。散度随着质量的增加而减小,信息先验显著减小了散度。带截断的光环质量密度曲线能更好地拟合透镜信号,而准确度和精确度并没有受到明显影响。我们进一步研究了系统不确定性的其他来源对WL质量的影响,即测光红移不确定性和源选择的影响、Euclid星团探测算法的预期性能以及掩码的存在。这种影响在很大程度上可以通过稳健的选择来消除。作为最后一个类似于欧几里德的测试,我们在一个现实的观测环境中结合了系统效应,发现在一个稳健的选择下,结果与理想情况类似,$langle b_M rangle = - 15.5 pm 2.4 , %$.
{"title":"Euclid preparation: Determining the weak lensing mass accuracy and precision for galaxy clusters","authors":"Euclid Collaboration, L. IngogliaDipartimento di Fisica e Astronomia \"Augusto Righi\" - Alma Mater Studiorum Università di Bologna, via Piero Gobetti 93/2, 40129 Bologna, Italy, M. SerenoINAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Via Piero Gobetti 93/3, 40129 Bologna, ItalyINFN-Sezione di Bologna, Viale Berti Pichat 6/2, 40127 Bologna, Italy, S. FarrensUniversité Paris-Saclay, Université Paris Cité, CEA, CNRS, AIM, 91191, Gif-sur-Yvette, France, C. GiocoliINAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Via Piero Gobetti 93/3, 40129 Bologna, ItalyIstituto Nazionale di Fisica Nucleare, Sezione di Bologna, Via Irnerio 46, 40126 Bologna, Italy, L. BaumontUniversité Paris-Saclay, Université Paris Cité, CEA, CNRS, AIM, 91191, Gif-sur-Yvette, France, G. F. LesciDipartimento di Fisica e Astronomia \"Augusto Righi\" - Alma Mater Studiorum Università di Bologna, via Piero Gobetti 93/2, 40129 Bologna, ItalyINAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Via Piero Gobetti 93/3, 40129 Bologna, Italy, L. MoscardiniDipartimento di Fisica e Astronomia \"Augusto Righi\" - Alma Mater Studiorum Università di Bologna, via Piero Gobetti 93/2, 40129 Bologna, ItalyINAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Via Piero Gobetti 93/3, 40129 Bologna, ItalyINFN-Sezione di Bologna, Viale Berti Pichat 6/2, 40127 Bologna, Italy, C. MurrayUniversité Paris Cité, CNRS, Astroparticule et Cosmologie, 75013 Paris, France, M. VannierUniversité Côte d'Azur, Observatoire de la Côte d'Azur, CNRS, Laboratoire Lagrange, Bd de l'Observatoire, CS 34229, 06304 Nice cedex 4, France, A. BivianoINAF-Osservatorio Astronomico di Trieste, Via G. B. Tiepolo 11, 34143 Trieste, ItalyIFPU, Institute for Fundamental Physics of the Universe, via Beirut 2, 34151 Trieste, Italy, C. CarboneINAF-IASF Milano, Via Alfonso Corti 12, 20133 Milano, Italy, G. CovoneDepartment of Physics \"E. Pancini\", University Federico II, Via Cinthia 6, 80126, Napoli, ItalyINAF-Osservatorio Astronomico di Capodimonte, Via Moiariello 16, 80131 Napoli, ItalyINFN section of Naples, Via Cinthia 6, 80126, Napoli, Italy, G. DespaliDipartimento di Fisica e Astronomia \"Augusto Righi\" - Alma Mater Studiorum Università di Bologna, via Piero Gobetti 93/2, 40129 Bologna, ItalyINAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Via Piero Gobetti 93/3, 40129 Bologna, ItalyINFN-Sezione di Bologna, Viale Berti Pichat 6/2, 40127 Bologna, Italy, M. MaturiInstitut für Theoretische Physik, University of Heidelberg, Philosophenweg 16, 69120 Heidelberg, GermanyZentrum für Astronomie, Universität Heidelberg, Philosophenweg 12, 69120 Heidelberg, Germany, S. MaurogordatoUniversité Côte d'Azur, Observatoire de la Côte d'Azur, CNRS, Laboratoire Lagrange, Bd de l'Observatoire, CS 34229, 06304 Nice cedex 4, France, M. MeneghettiINAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Via Piero Gobetti 93/3, 40129 Bologna, ItalyINFN-Sezione di Bologna, Viale Berti Pichat 6/2, 40127 Bologna, Italy, M. RadovichINAF-Osservatorio Astronomico di Padova, Via dell'Osservatorio 5, 35122 Padova, Italy, B. AltieriESAC/ESA, Camino Bajo del Castillo, s/n., Urb. Villafranca del Castillo, 28692 Villanueva de la Cañada, Madrid, Spain, A. AmaraSchool of Mathematics and Physics, University of Surrey, Guildford, Surrey, GU2 7XH, UK, S. AndreonINAF-Osservatorio Astronomico di Brera, Via Brera 28, 20122 Milano, Italy, N. AuricchioINAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Via Piero Gobetti 93/3, 40129 Bologna, Italy, C. BaccigalupiIFPU, Institute for Fundamental Physics of the Universe, via Beirut 2, 34151 Trieste, ItalyINAF-Osservatorio Astronomico di Trieste, Via G. B. Tiepolo 11, 34143 Trieste, ItalyINFN, Sezione di Trieste, Via Valerio 2, 34127 Trieste TS, ItalySISSA, International School for Advanced Studies, Via Bonomea 265, 34136 Trieste TS, Italy, M. BaldiDipartimento di Fisica e Astronomia, Università di Bologna, Via Gobetti 93/2, 40129 Bologna, ItalyINAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Via Piero Gobetti 93/3, 40129 Bologna, ItalyINFN-Sezione di Bologna, Viale Berti Pichat 6/2, 40127 Bologna, Italy, S. BardelliINAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Via Piero Gobetti 93/3, 40129 Bologna, Italy, F. BellagambaDipartimento di Fisica e Astronomia, Università di Bologna, Via Gobetti 93/2, 40129 Bologna, ItalyINAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Via Piero Gobetti 93/3, 40129 Bologna, Italy, R. BenderMax Planck Institute for Extraterrestrial Physics, Giessenbachstr. 1, 85748 Garching, GermanyUniversitäts-Sternwarte München, Fakultät für Physik, Ludwig-Maximilians-Universität München, Scheinerstrasse 1, 81679 München, Germany, F. BernardeauInstitut de Physique Théorique, CEA, CNRS, Université Paris-Saclay 91191 Gif-sur-Yvette Cedex, FranceInstitut d'Astrophysique de Paris, UMR 7095, CNRS, and Sorbonne Université, 98 bis boulevard Arago, 75014 Paris, France, D. BoninoINAF-Osservatorio Astrofisico di Torino, Via Osservatorio 20, 10025 Pino Torinese, E. BranchiniDipartimento di Fisica, Università di Genova, Via Dodecaneso 33, 16146, Genova, ItalyINFN-Sezione di Genova, Via Dodecaneso 33, 16146, Genova, ItalyINAF-Osservatorio Astronomico di Brera, Via Brera 28, 20122 Milano, Italy, M. BresciaDepartment of Physics \"E. Pancini\", University Federico II, Via Cinthia 6, 80126, Napoli, ItalyINAF-Osservatorio Astronomico di Capodimonte, Via Moiariello 16, 80131 Napoli, ItalyINFN section of Naples, Via Cinthia 6, 80126, Napoli, Italy, J. BrinchmannInstituto de Astrofísica e Ciências do Espaço, Universidade do Porto, CAUP, Rua das Estrelas, PT4150-762 Porto, PortugalFaculdade de Ciências da Universidade do Porto, Rua do Campo de Alegre, 4150-007 Porto, Portugal, S. CameraDipartimento di Fisica, Università degli Studi di Torino, Via P. Giuria 1, 10125 Torino, ItalyINFN-Sezione di Torino, Via P. Giuria 1, 10125 Torino, ItalyINAF-Osservatorio Astrofisico di Torino, Via Osservatorio 20, 10025 Pino Torinese, V. CapobiancoINAF-Osservatorio Astrofisico di Torino, Via Osservatorio 20, 10025 Pino Torinese, J. CarreteroCentro de Investigaciones Energéticas, Medioambientales y TecnológicasPort d'Informació Científica, Campus UAB, C. Albareda s/n, 08193 Bellaterra, S. CasasInstitute for Theoretical Particle Physics and Cosmology, M. CastellanoINAF-Osservatorio Astronomico di Roma, Via Frascati 33, 00078 Monteporzio Catone, Italy, G. CastignaniINAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Via Piero Gobetti 93/3, 40129 Bologna, Italy, S. CavuotiINAF-Osservatorio Astronomico di Capodimonte, Via Moiariello 16, 80131 Napoli, ItalyINFN section of Naples, Via Cinthia 6, 80126, Napoli, Italy, A. CimattiDipartimento di Fisica e Astronomia \"Augusto Righi\" - Alma Mater Studiorum Università di Bologna, Viale Berti Pichat 6/2, 40127 Bologna, Italy, C. Colodro-CondeInstituto de Astrofísica de Canarias, Calle Vía Láctea s/n, 38204, San Cristóbal de La Laguna, Tenerife, Spain, G. CongedoInstitute for Astronomy, University of Edinburgh, Royal Observatory, Blackford Hill, Edinburgh EH9 3HJ, UK, C. J. ConseliceJodrell Bank Centre for Astrophysics, Department of Physics and Astronomy, University of Manchester, Oxford Road, Manchester M13 9PL, UK, L. ConversiEuropean Space Agency/ESRIN, Largo Galileo Galilei 1, 00044 Frascati, Roma, ItalyESAC/ESA, Camino Bajo del Castillo, s/n., Urb. Villafranca del Castillo, 28692 Villanueva de la Cañada, Madrid, Spain, Y. CopinUniversité Claude Bernard Lyon 1, CNRS/IN2P3, IP2I Lyon, UMR 5822, Villeurbanne, F-69100, France, F. CourbinInstitute of Physics, Laboratory of Astrophysics, Ecole Polytechnique Fédérale de LausanneInstitut de Ciències del CosmosInstitució Catalana de Recerca i Estudis Avançats, H. M. CourtoisUCB Lyon 1, CNRS/IN2P3, IUF, IP2I Lyon, 4 rue Enrico Fermi, 69622 Villeurbanne, France, M. CropperMullard Space Science Laboratory, University College London, Holmbury St Mary, Dorking, Surrey RH5 6NT, UK, A. Da SilvaDepartamento de Física, Faculdade de Ciências, Universidade de Lisboa, Edifício C8, Campo Grande, PT1749-016 Lisboa, PortugalInstituto de Astrofísica e Ciências do Espaço, Faculdade de Ciências, Universidade de Lisboa, Campo Grande, 1749-016 Lisboa, Portugal, H. DegaudenziDepartment of Astronomy, University of Geneva, ch. d'Ecogia 16, 1290 Versoix, Switzerland, G. De LuciaINAF-Osservatorio Astronomico di Trieste, Via G. B. Tiepolo 11, 34143 Trieste, Italy, J. DinisDepartamento de Física, Faculdade de Ciências, Universidade de Lisboa, Edifício C8, Campo Grande, PT1749-016 Lisboa, PortugalInstituto de Astrofísica e Ciências do Espaço, Faculdade de Ciências, Universidade de Lisboa, Campo Grande, 1749-016 Lisboa, Portugal, F. DubathDepartment of Astronomy, University of Geneva, ch. d'Ecogia 16, 1290 Versoix, Switzerland, C. A. J. DuncanJodrell Bank Centre for Astrophysics, Department of Physics and Astronomy, University of Manchester, Oxford Road, Manchester M13 9PL, UK, X. DupacESAC/ESA, Camino Bajo del Castillo, s/n., Urb. Villafranca del Castillo, 28692 Villanueva de la Cañada, Madrid, Spain, S. DusiniINFN-Padova, Via Marzolo 8, 35131 Padova, Italy, A. EaletUniversité Claude Bernard Lyon 1, CNRS/IN2P3, IP2I Lyon, UMR 5822, Villeurbanne, F-69100, France, M. FarinaINAF-Istituto di Astrofisica e Planetologia Spaziali, via del Fosso del Cavaliere, 100, 00100 Roma, Italy, F. FaustiniSpace Science Data Center, Italian Space Agency, via del Politecnico snc, 00133 Roma, ItalyINAF-Osservatorio Astronomico di Roma, Via Frascati 33, 00078 Monteporzio Catone, Italy, S. FerriolUniversité Claude Bernard Lyon 1, CNRS/IN2P3, IP2I Lyon, UMR 5822, Villeurbanne, F-69100, France, P. FosalbaInstitut d'Estudis Espacials de CatalunyaInstitute of Space Sciences, M. FrailisINAF-Osservatorio Astronomico di Trieste, Via G. B. Tiepolo 11, 34143 Trieste, Italy, E. FranceschiINAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Via Piero Gobetti 93/3, 40129 Bologna, Italy, M. FumanaINAF-IASF Milano, Via Alfonso Corti 12, 20133 Milano, Italy, S. GaleottaINAF-Osservatorio Astronomico di Trieste, Via G. B. Tiepolo 11, 34143 Trieste, Italy, W. GillardAix-Marseille Université, CNRS/IN2P3, CPPM, Marseille, France, B. GillisInstitute for Astronomy, University of Edinburgh, Royal Observatory, Blackford Hill, Edinburgh EH9 3HJ, UK, P. Gómez-AlvarezFRACTAL S.L.N.E., calle Tulipán 2, Portal 13 1A, 28231, Las Rozas de Madrid, SpainESAC/ESA, Camino Bajo del Castillo, s/n., Urb. Villafranca del Castillo, 28692 Villanueva de la Cañada, Madrid, Spain, A. GrazianINAF-Osservatorio Astronomico di Padova, Via dell'Osservatorio 5, 35122 Padova, Italy, F. GruppMax Planck Institute for Extraterrestrial Physics, Giessenbachstr. 1, 85748 Garching, GermanyUniversitäts-Sternwarte München, Fakultät für Physik, Ludwig-Maximilians-Universität München, Scheinerstrasse 1, 81679 München, Germany, L. GuzzoDipartimento di Fisica \"Aldo Pontremoli\", Università degli Studi di Milano, Via Celoria 16, 20133 Milano, ItalyINAF-Osservatorio Astronomico di Brera, Via Brera 28, 20122 Milano, Italy, S. V. H. HauganInstitute of Theoretical Astrophysics, University of Oslo, P.O. Box 1029 Blindern, 0315 Oslo, Norway, W. HolmesJet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, CA, 91109, USA, F. HormuthFelix Hormuth Engineering, Goethestr. 17, 69181 Leimen, Germany, A. HornstrupTechnical University of Denmark, Elektrovej 327, 2800 Kgs. Lyngby, DenmarkCosmic Dawn Center, P. HudelotInstitut d'Astrophysique de Paris, UMR 7095, CNRS, and Sorbonne Université, 98 bis boulevard Arago, 75014 Paris, France, S. IlićUniversité Paris-Saclay, CNRS/IN2P3, IJCLab, 91405 Orsay, FranceInstitut de Recherche en Astrophysique et Planétologie, K. JahnkeMax-Planck-Institut für Astronomie, Königstuhl 17, 69117 Heidelberg, Germany, M. JhabvalaNASA Goddard Space Flight Center, Greenbelt, MD 20771, USA, B. JoachimiDepartment of Physics and Astronomy, University College London, Gower Street, London WC1E 6BT, UK, E. KeihänenDepartment of Physics and Helsinki Institute of Physics, Gustaf Hällströmin katu 2, 00014 University of Helsinki, Finland, S. KermicheAix-Marseille Université, CNRS/IN2P3, CPPM, Marseille, France, A. KiesslingJet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, CA, 91109, USA, M. KilbingerUniversité Paris-Saclay, Université Paris Cité, CEA, CNRS, AIM, 91191, Gif-sur-Yvette, France, B. KubikUniversité Claude Bernard Lyon 1, CNRS/IN2P3, IP2I Lyon, UMR 5822, Villeurbanne, F-69100, France, M. KümmelUniversitäts-Sternwarte München, Fakultät für Physik, Ludwig-Maximilians-Universität München, Scheinerstrasse 1, 81679 München, Germany, M. KunzUniversité de Genève, Département de Physique Théorique and Centre for Astroparticle Physics, 24 quai Ernest-Ansermet, CH-1211 Genève 4, Switzerland, H. Kurki-SuonioDepartment of Physics, P.O. Box 64, 00014 University of Helsinki, FinlandHelsinki Institute of Physics, Gustaf Hällströmin katu 2, University of Helsinki, Helsinki, Finland, S. LigoriINAF-Osservatorio Astrofisico di Torino, Via Osservatorio 20, 10025 Pino Torinese, P. B. LiljeInstitute of Theoretical Astrophysics, University of Oslo, P.O. Box 1029 Blindern, 0315 Oslo, Norway, V. LindholmDepartment of Physics, P.O. Box 64, 00014 University of Helsinki, FinlandHelsinki Institute of Physics, Gustaf Hällströmin katu 2, University of Helsinki, Helsinki, Finland, I. LloroNOVA optical infrared instrumentation group at ASTRON, Oude Hoogeveensedijk 4, 7991PD, Dwingeloo, The Netherlands, G. MainettiCentre de Calcul de l'IN2P3/CNRS, 21 avenue Pierre de Coubertin 69627 Villeurbanne Cedex, France, E. MaioranoINAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Via Piero Gobetti 93/3, 40129 Bologna, Italy, O. MansuttiINAF-Osservatorio Astronomico di Trieste, Via G. B. Tiepolo 11, 34143 Trieste, Italy, S. MarcinUniversity of Applied Sciences and Arts of Northwestern Switzerland, School of Engineering, 5210 Windisch, Switzerland, O. MarggrafUniversität Bonn, Argelander-Institut für Astronomie, Auf dem Hügel 71, 53121 Bonn, Germany, K. MarkovicJet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, CA, 91109, USA, M. MartinelliINAF-Osservatorio Astronomico di Roma, Via Frascati 33, 00078 Monteporzio Catone, ItalyINFN-Sezione di Roma, Piazzale Aldo Moro, 2 - c/o Dipartimento di Fisica, Edificio G. Marconi, 00185 Roma, Italy, N. MartinetAix-Marseille Université, CNRS, CNES, LAM, Marseille, France, F. MarulliDipartimento di Fisica e Astronomia \"Augusto Righi\" - Alma Mater Studiorum Università di Bologna, via Piero Gobetti 93/2, 40129 Bologna, ItalyINAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Via Piero Gobetti 93/3, 40129 Bologna, ItalyINFN-Sezione di Bologna, Viale Berti Pichat 6/2, 40127 Bologna, Italy, R. MasseyDepartment of Physics, Institute for Computational Cosmology, Durham University, South Road, DH1 3LE, UK, E. MedinaceliINAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Via Piero Gobetti 93/3, 40129 Bologna, Italy, S. MeiUniversité Paris Cité, CNRS, Astroparticule et Cosmologie, 75013 Paris, France, M. MelchiorUniversity of Applied Sciences and Arts of Northwestern Switzerland, School of Engineering, 5210 Windisch, Switzerland, Y. MellierInstitut d'Astrophysique de Paris, 98bis Boulevard Arago, 75014, Paris, FranceInstitut d'Astrophysique de Paris, UMR 7095, CNRS, and Sorbonne Université, 98 bis boulevard Arago, 75014 Paris, France, E. MerlinINAF-Osservatorio Astronomico di Roma, Via Frascati 33, 00078 Monteporzio Catone, Italy, G. MeylanInstitute of Physics, Laboratory of Astrophysics, Ecole Polytechnique Fédérale de Lausanne, M. MorescoDipartimento di Fisica e Astronomia \"Augusto Righi\" - Alma Mater Studiorum Università di Bologna, via Piero Gobetti 93/2, 40129 Bologna, ItalyINAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Via Piero Gobetti 93/3, 40129 Bologna, Italy, E. MunariINAF-Osservatorio Astronomico di Trieste, Via G. B. Tiepolo 11, 34143 Trieste, ItalyIFPU, Institute for Fundamental Physics of the Universe, via Beirut 2, 34151 Trieste, Italy, S. -M. NiemiEuropean Space Agency/ESTEC, Keplerlaan 1, 2201 AZ Noordwijk, The Netherlands, C. PadillaInstitut de Física d'Altes Energies, K. PaechMax Planck Institute for Extraterrestrial Physics, Giessenbachstr. 1, 85748 Garching, Germany, S. PaltaniDepartment of Astronomy, University of Geneva, ch. d'Ecogia 16, 1290 Versoix, Switzerland, F. PasianINAF-Osservatorio Astronomico di Trieste, Via G. B. Tiepolo 11, 34143 Trieste, Italy, K. PedersenDARK, Niels Bohr Institute, University of Copenhagen, Jagtvej 155, 2200 Copenhagen, Denmark, W. J. PercivalWaterloo Centre for Astrophysics, University of Waterloo, Waterloo, Ontario N2L 3G1, CanadaDepartment of Physics and Astronomy, University of Waterloo, Waterloo, Ontario N2L 3G1, CanadaPerimeter Institute for Theoretical Physics, Waterloo, Ontario N2L 2Y5, Canada, V. PettorinoEuropean Space Agency/ESTEC, Keplerlaan 1, 2201 AZ Noordwijk, The Netherlands, S. PiresUniversité Paris-Saclay, Université Paris Cité, CEA, CNRS, AIM, 91191, Gif-sur-Yvette, France, G. PolentaSpace Science Data Center, Italian Space Agency, via del Politecnico snc, 00133 Roma, Italy, M. PoncetCentre National d'Etudes Spatiales -- Centre spatial de Toulouse, 18 avenue Edouard Belin, 31401 Toulouse Cedex 9, France, L. A. PopaInstitute of Space Science, Str. Atomistilor, nr. 409 Măgurele, Ilfov, 077125, Romania, L. PozzettiINAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Via Piero Gobetti 93/3, 40129 Bologna, Italy, F. RaisonMax Planck Institute for Extraterrestrial Physics, Giessenbachstr. 1, 85748 Garching, Germany, A. RenziDipartimento di Fisica e Astronomia \"G. Galilei\", Università di Padova, Via Marzolo 8, 35131 Padova, ItalyINFN-Padova, Via Marzolo 8, 35131 Padova, Italy, J. RhodesJet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, CA, 91109, USA, G. RiccioINAF-Osservatorio Astronomico di Capodimonte, Via Moiariello 16, 80131 Napoli, Italy, E. RomelliINAF-Osservatorio Astronomico di Trieste, Via G. B. Tiepolo 11, 34143 Trieste, Italy, M. RoncarelliINAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Via Piero Gobetti 93/3, 40129 Bologna, Italy, E. RossettiDipartimento di Fisica e Astronomia, Università di Bologna, Via Gobetti 93/2, 40129 Bologna, Italy, R. SagliaUniversitäts-Sternwarte München, Fakultät für Physik, Ludwig-Maximilians-Universität München, Scheinerstrasse 1, 81679 München, GermanyMax Planck Institute for Extraterrestrial Physics, Giessenbachstr. 1, 85748 Garching, Germany, Z. SakrInstitut für Theoretische Physik, University of Heidelberg, Philosophenweg 16, 69120 Heidelberg, GermanyInstitut de Recherche en Astrophysique et PlanétologieUniversité St Joseph, Faculty of Sciences, Beirut, Lebanon, J. -C. SalvignolEuropean Space Agency/ESTEC, Keplerlaan 1, 2201 AZ Noordwijk, The Netherlands, A. G. SánchezMax Planck Institute for Extraterrestrial Physics, Giessenbachstr. 1, 85748 Garching, Germany, D. SaponeDepartamento de Física, FCFM, Universidad de Chile, Blanco Encalada 2008, Santiago, Chile, B. SartorisUniversitäts-Sternwarte München, Fakultät für Physik, Ludwig-Maximilians-Universität München, Scheinerstrasse 1, 81679 München, GermanyINAF-Osservatorio Astronomico di Trieste, Via G. B. Tiepolo 11, 34143 Trieste, Italy, M. SchirmerMax-Planck-Institut für Astronomie, Königstuhl 17, 69117 Heidelberg, Germany, P. SchneiderUniversität Bonn, Argelander-Institut für Astronomie, Auf dem Hügel 71, 53121 Bonn, Germany, A. SecrounAix-Marseille Université, CNRS/IN2P3, CPPM, Marseille, France, G. SeidelMax-Planck-Institut für Astronomie, Königstuhl 17, 69117 Heidelberg, Germany, S. SerranoInstitut d'Estudis Espacials de CatalunyaSatlantis, University Science Park, Sede Bld 48940, Leioa-Bilbao, SpainInstitute of Space Sciences, C. SirignanoDipartimento di Fisica e Astronomia \"G. Galilei\", Università di Padova, Via Marzolo 8, 35131 Padova, ItalyINFN-Padova, Via Marzolo 8, 35131 Padova, Italy, G. SirriINFN-Sezione di Bologna, Viale Berti Pichat 6/2, 40127 Bologna, Italy, L. StancoINFN-Padova, Via Marzolo 8, 35131 Padova, Italy, J. SteinwagnerMax Planck Institute for Extraterrestrial Physics, Giessenbachstr. 1, 85748 Garching, Germany, P. Tallada-CrespíCentro de Investigaciones Energéticas, Medioambientales y TecnológicasPort d'Informació Científica, Campus UAB, C. Albareda s/n, 08193 Bellaterra, D. TavagnaccoINAF-Osservatorio Astronomico di Trieste, Via G. B. Tiepolo 11, 34143 Trieste, Italy, A. N. TaylorInstitute for Astronomy, University of Edinburgh, Royal Observatory, Blackford Hill, Edinburgh EH9 3HJ, UK, I. TerenoDepartamento de Física, Faculdade de Ciências, Universidade de Lisboa, Edifício C8, Campo Grande, PT1749-016 Lisboa, PortugalInstituto de Astrofísica e Ciências do Espaço, Faculdade de Ciências, Universidade de Lisboa, Tapada da Ajuda, 1349-018 Lisboa, Portugal, R. Toledo-MoreoUniversidad Politécnica de Cartagena, Departamento de Electrónica y Tecnología de Computadoras, Plaza del Hospital 1, 30202 Cartagena, Spain, F. TorradeflotPort d'Informació Científica, Campus UAB, C. Albareda s/n, 08193 BellaterraCentro de Investigaciones Energéticas, Medioambientales y Tecnológicas, I. TutusausInstitut de Recherche en Astrophysique et Planétologie, L. ValenzianoINAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Via Piero Gobetti 93/3, 40129 Bologna, ItalyINFN-Bologna, Via Irnerio 46, 40126 Bologna, Italy, T. VassalloUniversitäts-Sternwarte München, Fakultät für Physik, Ludwig-Maximilians-Universität München, Scheinerstrasse 1, 81679 München, GermanyINAF-Osservatorio Astronomico di Trieste, Via G. B. Tiepolo 11, 34143 Trieste, Italy, G. Verdoes KleijnKapteyn Astronomical Institute, University of Groningen, PO Box 800, 9700 AV Groningen, The Netherlands, A. VeropalumboINAF-Osservatorio Astronomico di Brera, Via Brera 28, 20122 Milano, ItalyINFN-Sezione di Genova, Via Dodecaneso 33, 16146, Genova, ItalyDipartimento di Fisica, Università degli studi di Genova, and INFN-Sezione di Genova, via Dodecaneso 33, 16146, Genova, Italy, Y. WangInfrared Processing and Analysis Center, California Institute of Technology, Pasadena, CA 91125, USA, J. WellerUniversitäts-Sternwarte München, Fakultät für Physik, Ludwig-Maximilians-Universität München, Scheinerstrasse 1, 81679 München, GermanyMax Planck Institute for Extraterrestrial Physics, Giessenbachstr. 1, 85748 Garching, Germany, G. ZamoraniINAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Via Piero Gobetti 93/3, 40129 Bologna, Italy, E. ZuccaINAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Via Piero Gobetti 93/3, 40129 Bologna, Italy, M. BolzonellaINAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Via Piero Gobetti 93/3, 40129 Bologna, Italy, E. BozzoDepartment of Astronomy, University of Geneva, ch. d'Ecogia 16, 1290 Versoix, Switzerland, C. BuriganaINAF, Istituto di Radioastronomia, Via Piero Gobetti 101, 40129 Bologna, ItalyINFN-Bologna, Via Irnerio 46, 40126 Bologna, Italy, M. CalabreseAstronomical Observatory of the Autonomous Region of the Aosta ValleyINAF-IASF Milano, Via Alfonso Corti 12, 20133 Milano, Italy, D. Di FerdinandoINFN-Sezione di Bologna, Viale Berti Pichat 6/2, 40127 Bologna, Italy, J. A. Escartin VigoMax Planck Institute for Extraterrestrial Physics, Giessenbachstr. 1, 85748 Garching, Germany, R. FarinelliINAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Via Piero Gobetti 93/3, 40129 Bologna, Italy, F. FinelliINAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Via Piero Gobetti 93/3, 40129 Bologna, ItalyINFN-Bologna, Via Irnerio 46, 40126 Bologna, Italy, J. Gracia-CarpioMax Planck Institute for Extraterrestrial Physics, Giessenbachstr. 1, 85748 Garching, Germany, S. MatthewInstitute for Astronomy, University of Edinburgh, Royal Observatory, Blackford Hill, Edinburgh EH9 3HJ, UK, A. PezzottaMax Planck Institute for Extraterrestrial Physics, Giessenbachstr. 1, 85748 Garching, Germany, M. PöntinenDepartment of Physics, P.O. Box 64, 00014 University of Helsinki, Finland, V. ScottezInstitut d'Astrophysique de Paris, 98bis Boulevard Arago, 75014, Paris, FranceJunia, EPA department, 41 Bd Vauban, 59800 Lille, France, M. TentiINFN-Sezione di Bologna, Viale Berti Pichat 6/2, 40127 Bologna, Italy, M. VielIFPU, Institute for Fundamental Physics of the Universe, via Beirut 2, 34151 Trieste, ItalyINAF-Osservatorio Astronomico di Trieste, Via G. B. Tiepolo 11, 34143 Trieste, ItalySISSA, International School for Advanced Studies, Via Bonomea 265, 34136 Trieste TS, ItalyINFN, Sezione di Trieste, Via Valerio 2, 34127 Trieste TS, ItalyICSC - Centro Nazionale di Ricerca in High Performance Computing, Big Data e Quantum Computing, Via Magnanelli 2, Bologna, Italy, M. WiesmannInstitute of Theoretical Astrophysics, University of Oslo, P.O. Box 1029 Blindern, 0315 Oslo, Norway, Y. AkramiInstituto de Física Teórica UAM-CSIC, Campus de Cantoblanco, 28049 Madrid, SpainCERCA/ISO, Department of Physics, Case Western Reserve University, 10900 Euclid Avenue, Cleveland, OH 44106, USA, V. AllevatoINAF-Osservatorio Astronomico di Capodimonte, Via Moiariello 16, 80131 Napoli, Italy, S. AnselmiINFN-Padova, Via Marzolo 8, 35131 Padova, ItalyDipartimento di Fisica e Astronomia \"G. Galilei\", Università di Padova, Via Marzolo 8, 35131 Padova, ItalyLaboratoire Univers et Théorie, Observatoire de Paris, Université PSL, Université Paris Cité, CNRS, 92190 Meudon, France, M. ArchidiaconoDipartimento di Fisica \"Aldo Pontremoli\", Università degli Studi di Milano, Via Celoria 16, 20133 Milano, ItalyINFN-Sezione di Milano, Via Celoria 16, 20133 Milano, Italy, F. Atrio-BarandelaDepartamento de Física Fundamental. Universidad de Salamanca. Plaza de la Merced s/n. 37008 Salamanca, Spain, M. BallardiniDipartimento di Fisica e Scienze della Terra, Università degli Studi di Ferrara, Via Giuseppe Saragat 1, 44122 Ferrara, ItalyINAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Via Piero Gobetti 93/3, 40129 Bologna, ItalyIstituto Nazionale di Fisica Nucleare, Sezione di Ferrara, Via Giuseppe Saragat 1, 44122 Ferrara, Italy, D. BertaccaDipartimento di Fisica e Astronomia \"G. Galilei\", Università di Padova, Via Marzolo 8, 35131 Padova, ItalyINAF-Osservatorio Astronomico di Padova, Via dell'Osservatorio 5, 35122 Padova, ItalyINFN-Padova, Via Marzolo 8, 35131 Padova, Italy, M. BetherminUniversité de Strasbourg, CNRS, Observatoire astronomique de Strasbourg, UMR 7550, 67000 Strasbourg, FranceAix-Marseille Université, CNRS, CNES, LAM, Marseille, France, A. BlanchardInstitut de Recherche en Astrophysique et Planétologie, L. BlotCenter for Data-Driven Discovery, Kavli IPMULaboratoire Univers et Théorie, Observatoire de Paris, Université PSL, Université Paris Cité, CNRS, 92190 Meudon, France, H. BöhringerMax Planck Institute for Extraterrestrial Physics, Giessenbachstr. 1, 85748 Garching, GermanyLudwig-Maximilians-University, Schellingstrasse 4, 80799 Munich, GermanyMax-Planck-Institut für Physik, Boltzmannstr. 8, 85748 Garching, Germany, S. BorganiDipartimento di Fisica - Sezione di Astronomia, Università di Trieste, Via Tiepolo 11, 34131 Trieste, ItalyIFPU, Institute for Fundamental Physics of the Universe, via Beirut 2, 34151 Trieste, ItalyINAF-Osservatorio Astronomico di Trieste, Via G. B. Tiepolo 11, 34143 Trieste, ItalyINFN, Sezione di Trieste, Via Valerio 2, 34127 Trieste TS, Italy, S. BrutonMinnesota Institute for Astrophysics, University of Minnesota, 116 Church St SE, Minneapolis, MN 55455, USA, R. CabanacInstitut de Recherche en Astrophysique et Planétologie, A. CalabroINAF-Osservatorio Astronomico di Roma, Via Frascati 33, 00078 Monteporzio Catone, Italy, G. Cañas-HerreraEuropean Space Agency/ESTEC, Keplerlaan 1, 2201 AZ Noordwijk, The NetherlandsInstitute Lorentz, Leiden University, Niels Bohrweg 2, 2333 CA Leiden, The Netherlands, A. CappiINAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Via Piero Gobetti 93/3, 40129 Bologna, ItalyUniversité Côte d'Azur, Observatoire de la Côte d'Azur, CNRS, Laboratoire Lagrange, Bd de l'Observatoire, CS 34229, 06304 Nice cedex 4, France, F. CaroINAF-Osservatorio Astronomico di Roma, Via Frascati 33, 00078 Monteporzio Catone, Italy, C. S. CarvalhoInstituto de Astrofísica e Ciências do Espaço, Faculdade de Ciências, Universidade de Lisboa, Tapada da Ajuda, 1349-018 Lisboa, Portugal, T. CastroINAF-Osservatorio Astronomico di Trieste, Via G. B. Tiepolo 11, 34143 Trieste, ItalyINFN, Sezione di Trieste, Via Valerio 2, 34127 Trieste TS, ItalyIFPU, Institute for Fundamental Physics of the Universe, via Beirut 2, 34151 Trieste, ItalyICSC - Centro Nazionale di Ricerca in High Performance Computing, Big Data e Quantum Computing, Via Magnanelli 2, Bologna, Italy, K. C. ChambersInstitute for Astronomy, University of Hawaii, 2680 Woodlawn Drive, Honolulu, HI 96822, USA, S. ContariniMax Planck Institute for Extraterrestrial Physics, Giessenbachstr. 1, 85748 Garching, Germany, A. R. CoorayDepartment of Physics & Astronomy, University of California Irvine, Irvine CA 92697, USA, M. CostanziDipartimento di Fisica - Sezione di Astronomia, Università di Trieste, Via Tiepolo 11, 34131 Trieste, ItalyINAF-Osservatorio Astronomico di Trieste, Via G. B. Tiepolo 11, 34143 Trieste, ItalyIFPU, Institute for Fundamental Physics of the Universe, via Beirut 2, 34151 Trieste, Italy, O. CucciatiINAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Via Piero Gobetti 93/3, 40129 Bologna, Italy, G. DesprezDepartment of Astronomy & Physics and Institute for Computational Astrophysics, Saint Mary's University, 923 Robie Street, Halifax, Nova Scotia, B3H 3C3, Canada, A. Díaz-SánchezDepartamento Física Aplicada, Universidad Politécnica de Cartagena, Campus Muralla del Mar, 30202 Cartagena, Murcia, Spain, J. J. DiazInstituto de Astrofísica de Canarias, S. Di DomizioDipartimento di Fisica, Università di Genova, Via Dodecaneso 33, 16146, Genova, ItalyINFN-Sezione di Genova, Via Dodecaneso 33, 16146, Genova, Italy, H. DoleUniversité Paris-Saclay, CNRS, Institut d'astrophysique spatiale, 91405, Orsay, France, S. EscoffierAix-Marseille Université, CNRS/IN2P3, CPPM, Marseille, France, M. EzziatiAix-Marseille Université, CNRS, CNES, LAM, Marseille, France, A. G. FerrariDipartimento di Fisica e Astronomia \"Augusto Righi\" - Alma Mater Studiorum Università di Bologna, Viale Berti Pichat 6/2, 40127 Bologna, ItalyINFN-Sezione di Bologna, Viale Berti Pichat 6/2, 40127 Bologna, Italy, P. G. FerreiraDepartment of Physics, Oxford University, Keble Road, Oxford OX1 3RH, UK, I. FerreroInstitute of Theoretical Astrophysics, University of Oslo, P.O. Box 1029 Blindern, 0315 Oslo, Norway, A. FinoguenovDepartment of Physics, P.O. Box 64, 00014 University of Helsinki, Finland, A. FontanaINAF-Osservatorio Astronomico di Roma, Via Frascati 33, 00078 Monteporzio Catone, Italy, F. FornariINFN-Bologna, Via Irnerio 46, 40126 Bologna, Italy, L. GabarraDepartment of Physics, Oxford University, Keble Road, Oxford OX1 3RH, UK, K. GangaUniversité Paris Cité, CNRS, Astroparticule et Cosmologie, 75013 Paris, France, J. García-BellidoInstituto de Física Teórica UAM-CSIC, Campus de Cantoblanco, 28049 Madrid, Spain, T. GasparettoINAF-Osservatorio Astronomico di Trieste, Via G. B. Tiepolo 11, 34143 Trieste, Italy, V. GautardCEA Saclay, DFR/IRFU, Service d'Astrophysique, Bat. 709, 91191 Gif-sur-Yvette, France, E. GaztanagaInstitute of Space SciencesInstitut d'Estudis Espacials de CatalunyaInstitute of Cosmology and Gravitation, University of Portsmouth, Portsmouth PO1 3FX, UK, F. GiacominiINFN-Sezione di Bologna, Viale Berti Pichat 6/2, 40127 Bologna, Italy, F. GianottiINAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Via Piero Gobetti 93/3, 40129 Bologna, Italy, G. GozaliaslDepartment of Computer Science, Aalto University, PO Box 15400, Espoo, FI-00 076, FinlandDepartment of Physics, P.O. Box 64, 00014 University of Helsinki, Finland, C. M. GutierrezInstituto de Astrofísica de Canarias, c/ Via Lactea s/n, La Laguna E-38200, Spain. Departamento de Astrofí sica de la Universidad de La Laguna, Avda. Francisco Sanchez, La Laguna, E-38200, Spain, A. HallInstitute for Astronomy, University of Edinburgh, Royal Observatory, Blackford Hill, Edinburgh EH9 3HJ, UK, H. HildebrandtRuhr University Bochum, Faculty of Physics and Astronomy, Astronomical Institute, J. HjorthDARK, Niels Bohr Institute, University of Copenhagen, Jagtvej 155, 2200 Copenhagen, Denmark, A. Jimenez MuñozUniv. Grenoble Alpes, CNRS, Grenoble INP, LPSC-IN2P3, 53, Avenue des Martyrs, 38000, Grenoble, France, J. J. E. KajavaDepartment of Physics and Astronomy, Vesilinnantie 5, 20014 University of Turku, FinlandSerco for European Space Agency, V. KansalARC Centre of Excellence for Dark Matter Particle Physics, Melbourne, AustraliaCentre for Astrophysics & Supercomputing, Swinburne University of Technology, Hawthorn, Victoria 3122, Australia, D. KaragiannisSchool of Physics and Astronomy, Queen Mary University of London, Mile End Road, London E1 4NS, UKDepartment of Physics and Astronomy, University of the Western Cape, Bellville, Cape Town, 7535, South Africa, C. C. KirkpatrickDepartment of Physics and Helsinki Institute of Physics, Gustaf Hällströmin katu 2, 00014 University of Helsinki, Finland, A. M. C. Le BrunLaboratoire Univers et Théorie, Observatoire de Paris, Université PSL, Université Paris Cité, CNRS, 92190 Meudon, France, J. Le GraetAix-Marseille Université, CNRS/IN2P3, CPPM, Marseille, France, L. LegrandICTP South American Institute for Fundamental Research, Instituto de Física Teórica, Universidade Estadual Paulista, São Paulo, Brazil, J. LesgourguesInstitute for Theoretical Particle Physics and Cosmology, T. I. LiaudatIRFU, CEA, Université Paris-Saclay 91191 Gif-sur-Yvette Cedex, France, A. LoureiroOskar Klein Centre for Cosmoparticle Physics, Department of Physics, Stockholm University, Stockholm, SE-106 91, SwedenAstrophysics Group, Blackett Laboratory, Imperial College London, London SW7 2AZ, UK, J. Macias-PerezUniv. Grenoble Alpes, CNRS, Grenoble INP, LPSC-IN2P3, 53, Avenue des Martyrs, 38000, Grenoble, France, G. MaggioINAF-Osservatorio Astronomico di Trieste, Via G. B. Tiepolo 11, 34143 Trieste, Italy, M. MagliocchettiINAF-Istituto di Astrofisica e Planetologia Spaziali, via del Fosso del Cavaliere, 100, 00100 Roma, Italy, F. MannucciINAF-Osservatorio Astrofisico di Arcetri, Largo E. Fermi 5, 50125, Firenze, Italy, R. MaoliDipartimento di Fisica, Sapienza Università di Roma, Piazzale Aldo Moro 2, 00185 Roma, ItalyINAF-Osservatorio Astronomico di Roma, Via Frascati 33, 00078 Monteporzio Catone, Italy, J. Martín-FleitasAurora Technology for European Space Agency, C. J. A. P. MartinsCentro de Astrofísica da Universidade do Porto, Rua das Estrelas, 4150-762 Porto, PortugalInstituto de Astrofísica e Ciências do Espaço, Universidade do Porto, CAUP, Rua das Estrelas, PT4150-762 Porto, Portugal, L. MaurinUniversité Paris-Saclay, CNRS, Institut d'astrophysique spatiale, 91405, Orsay, France, R. B. MetcalfDipartimento di Fisica e Astronomia \"Augusto Righi\" - Alma Mater Studiorum Università di Bologna, via Piero Gobetti 93/2, 40129 Bologna, ItalyINAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Via Piero Gobetti 93/3, 40129 Bologna, Italy, M. MiluzioESAC/ESA, Camino Bajo del Castillo, s/n., Urb. Villafranca del Castillo, 28692 Villanueva de la Cañada, Madrid, SpainHE Space for European Space Agency, P. MonacoDipartimento di Fisica - Sezione di Astronomia, Università di Trieste, Via Tiepolo 11, 34131 Trieste, ItalyINAF-Osservatorio Astronomico di Trieste, Via G. B. Tiepolo 11, 34143 Trieste, ItalyINFN, Sezione di Trieste, Via Valerio 2, 34127 Trieste TS, ItalyIFPU, Institute for Fundamental Physics of the Universe, via Beirut 2, 34151 Trieste, Italy, A. MontoroInstitute of Space SciencesInstitut d'Estudis Espacials de Catalunya, A. MoraAurora Technology for European Space Agency, C. MorettiSISSA, International School for Advanced Studies, Via Bonomea 265, 34136 Trieste TS, ItalyICSC - Centro Nazionale di Ricerca in High Performance Computing, Big Data e Quantum Computing, Via Magnanelli 2, Bologna, ItalyINAF-Osservatorio Astronomico di Trieste, Via G. B. Tiepolo 11, 34143 Trieste, ItalyIFPU, Institute for Fundamental Physics of the Universe, via Beirut 2, 34151 Trieste, ItalyINFN, Sezione di Trieste, Via Valerio 2, 34127 Trieste TS, Italy, G. MorganteINAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Via Piero Gobetti 93/3, 40129 Bologna, Italy, S. NadathurInstitute of Cosmology and Gravitation, University of Portsmouth, Portsmouth PO1 3FX, UK, Nicholas A. WaltonInstitute of Astronomy, University of Cambridge, Madingley Road, Cambridge CB3 0HA, UK, L. PaganoDipartimento di Fisica e Scienze della Terra, Università degli Studi di Ferrara, Via Giuseppe Saragat 1, 44122 Ferrara, ItalyIstituto Nazionale di Fisica Nucleare, Sezione di Ferrara, Via Giuseppe Saragat 1, 44122 Ferrara, Italy, L. PatriziiINFN-Sezione di Bologna, Viale Berti Pichat 6/2, 40127 Bologna, Italy, V. PopaInstitute of Space Science, Str. Atomistilor, nr. 409 Măgurele, Ilfov, 077125, Romania, D. PotterDepartment of Astrophysics, University of Zurich, Winterthurerstrasse 190, 8057 Zurich, Switzerland, I. RissoINAF-Osservatorio Astronomico di Brera, Via Brera 28, 20122 Milano, Italy, and INFN-Sezione di Genova, Via Dodecaneso 33, 16146, Genova, Italy, P. -F. RocciUniversité Paris-Saclay, CNRS, Institut d'astrophysique spatiale, 91405, Orsay, France, M. SahlénTheoretical astrophysics, Department of Physics and Astronomy, Uppsala University, Box 515, 751 20 Uppsala, Sweden, E. SarpaSISSA, International School for Advanced Studies, Via Bonomea 265, 34136 Trieste TS, ItalyICSC - Centro Nazionale di Ricerca in High Performance Computing, Big Data e Quantum Computing, Via Magnanelli 2, Bologna, ItalyINFN, Sezione di Trieste, Via Valerio 2, 34127 Trieste TS, Italy, A. SchneiderDepartment of Astrophysics, University of Zurich, Winterthurerstrasse 190, 8057 Zurich, Switzerland, M. SchultheisUniversité Côte d'Azur, Observatoire de la Côte d'Azur, CNRS, Laboratoire Lagrange, Bd de l'Observatoire, CS 34229, 06304 Nice cedex 4, France, P. SimonUniversität Bonn, Argelander-Institut für Astronomie, Auf dem Hügel 71, 53121 Bonn, Germany, A. Spurio ManciniDepartment of Physics, Royal Holloway, University of London, TW20 0EX, UKMullard Space Science Laboratory, University College London, Holmbury St Mary, Dorking, Surrey RH5 6NT, UK, J. StadelDepartment of Astrophysics, University of Zurich, Winterthurerstrasse 190, 8057 Zurich, Switzerland, S. A. StanfordDepartment of Physics and Astronomy, University of California, Davis, CA 95616, USA, K. TanidisDepartment of Physics, Oxford University, Keble Road, Oxford OX1 3RH, UK, C. TaoAix-Marseille Université, CNRS/IN2P3, CPPM, Marseille, France, G. TesteraINFN-Sezione di Genova, Via Dodecaneso 33, 16146, Genova, Italy, R. TeyssierDepartment of Astrophysical Sciences, Peyton Hall, Princeton University, Princeton, NJ 08544, USA, S. ToftCosmic Dawn CenterNiels Bohr Institute, University of Copenhagen, Jagtvej 128, 2200 Copenhagen, Denmark, S. TosiDipartimento di Fisica, Università di Genova, Via Dodecaneso 33, 16146, Genova, ItalyINFN-Sezione di Genova, Via Dodecaneso 33, 16146, Genova, Italy, A. TrojaDipartimento di Fisica e Astronomia \"G. Galilei\", Università di Padova, Via Marzolo 8, 35131 Padova, ItalyINFN-Padova, Via Marzolo 8, 35131 Padova, Italy, M. TucciDepartment of Astronomy, University of Geneva, ch. d'Ecogia 16, 1290 Versoix, Switzerland, C. ValieriINFN-Sezione di Bologna, Viale Berti Pichat 6/2, 40127 Bologna, Italy, J. ValiviitaDepartment of Physics, P.O. Box 64, 00014 University of Helsinki, FinlandHelsinki Institute of Physics, Gustaf Hällströmin katu 2, University of Helsinki, Helsinki, Finland, D. VerganiINAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Via Piero Gobetti 93/3, 40129 Bologna, Italy, G. VerzaCenter for Cosmology and Particle Physics, Department of Physics, New York University, New York, NY 10003, USACenter for Computational Astrophysics, Flatiron Institute, 162 5th Avenue, 10010, New York, NY, USA, P. VielzeufAix-Marseille Université, CNRS/IN2P3, CPPM, Marseille, France","doi":"arxiv-2409.02783","DOIUrl":"https://doi.org/arxiv-2409.02783","url":null,"abstract":"We investigate the level of accuracy and precision of cluster weak-lensing\u0000(WL) masses measured with the Euclid data processing pipeline. We use the\u0000DEMNUni-Cov $N$-body simulations to assess how well the WL mass probes the true\u0000halo mass, and, then, how well WL masses can be recovered in the presence of\u0000measurement uncertainties. We consider different halo mass density models,\u0000priors, and mass point estimates. WL mass differs from true mass due to, e.g.,\u0000the intrinsic ellipticity of sources, correlated or uncorrelated matter and\u0000large-scale structure, halo triaxiality and orientation, and merging or\u0000irregular morphology. In an ideal scenario without observational or measurement\u0000errors, the maximum likelihood estimator is the most accurate, with WL masses\u0000biased low by $langle b_M rangle = -14.6 pm 1.7 , %$ on average over the\u0000full range $M_text{200c} > 5 times 10^{13} , M_odot$ and $z < 1$. Due to\u0000the stabilising effect of the prior, the biweight, mean, and median estimates\u0000are more precise. The scatter decreases with increasing mass and informative\u0000priors significantly reduce the scatter. Halo mass density profiles with a\u0000truncation provide better fits to the lensing signal, while the accuracy and\u0000precision are not significantly affected. We further investigate the impact of\u0000additional sources of systematic uncertainty on the WL mass, namely the impact\u0000of photometric redshift uncertainties and source selection, the expected\u0000performance of Euclid cluster detection algorithms, and the presence of masks.\u0000Taken in isolation, we find that the largest effect is induced by\u0000non-conservative source selection. This effect can be mostly removed with a\u0000robust selection. As a final Euclid-like test, we combine systematic effects\u0000in a realistic observational setting and find results similar to the ideal\u0000case, $langle b_M rangle = - 15.5 pm 2.4 , %$, under a robust selection.","PeriodicalId":501207,"journal":{"name":"arXiv - PHYS - Cosmology and Nongalactic Astrophysics","volume":"68 1","pages":""},"PeriodicalIF":0.0,"publicationDate":"2024-09-04","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"142192637","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":0,"RegionCategory":"","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
引用次数: 0
Star-Crossed Labours: Checking Consistency Between Current Supernovae Compilations 星际交叉的工作检查当前超新星汇编之间的一致性
Pub Date : 2024-09-04 DOI: arxiv-2409.02550
William L. Matthewson, Arman Shafieloo
We make use of model-independent statistical methods to assess theconsistency of three different supernova compilations: Union3, Pantheon+ andDES 5-year supernovae. We expand the available model space of each, usingCrossing Statistics, and test the compatibility of each dataset, against theother two. This is done using (I) a Flat $Lambda$CDM fitting to, and (II)Iterative Smoothing from, one particular dataset, and determining the level ofdeformation by required to fit the other two. This allows us to test the mutualconsistency of the datasets both within the standard model and in the case ofsome extended model, motivated by features present in a particular dataset. Wefind that, in both these cases, the data are only consistent with the point inthe parameter space corresponding to zero deformation, at around a $2sigma$level, with the DES compilation showing the largest disagreement. However, allthree datasets are still found to be consistent to within $1-2sigma$ for somesubset of the extended model space implied by the deformations.
我们利用与模型无关的统计方法来评估三种不同超新星汇编的一致性:Union3、Pantheon+ 和 DES 5 年超新星汇编的一致性。我们使用交叉统计(Crossing Statistics)方法扩展了每个数据集的可用模型空间,并测试了每个数据集与另外两个数据集的兼容性。这是通过(I)对一个特定数据集进行平$Lambda$CDM拟合,以及(II)对另两个数据集进行迭代平滑来完成的。这样,我们就可以测试数据集在标准模型中的相互一致性,以及在某些扩展模型中的相互一致性,这些扩展模型是由特定数据集中存在的特征激发的。我们发现,在这两种情况下,数据只与参数空间中对应于零形变的点相一致,大约在2美元(sigma$)的水平上,DES汇编显示出最大的不一致性。然而,对于变形所隐含的扩展模型空间的某个子集,所有三个数据集的一致性仍然在1-2(sigma$)美元之内。
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引用次数: 0
Impact of survey spatial variability on galaxy redshift distributions and the cosmological $3times2$-point statistics for the Rubin Legacy Survey of Space and Time (LSST) 鲁宾时空遗产巡天(LSST)的巡天空间变异性对星系红移分布和宇宙学3times2$点统计的影响
Pub Date : 2024-09-04 DOI: arxiv-2409.02501
Qianjun Hang, Benjamin Joachimi, Eric Charles, John Franklin Crenshaw, Patricia Larsen, Alex I. Malz, Sam Schmidt, Ziang Yan, Tianqing Zhang, the LSST Dark Energy Science Collaboration
We investigate the impact of spatial survey non-uniformity on the galaxyredshift distributions for forthcoming data releases of the Rubin ObservatoryLegacy Survey of Space and Time (LSST). Specifically, we construct a mockphotometry dataset degraded by the Rubin OpSim observing conditions, andestimate photometric redshifts of the sample using a template-fitting photo-$z$estimator, BPZ, and a machine learning method, FlexZBoost. We select the Goldsample, defined as $i<25.3$ for 10 year LSST data, with an adjusted magnitudecut for each year and divide it into five tomographic redshift bins for theweak lensing lens and source samples. We quantify the change in the number ofobjects, mean redshift, and width of each tomographic bin as a function of thecoadd $i$-band depth for 1-year (Y1), 3-year (Y3), and 5-year (Y5) data. Inparticular, Y3 and Y5 have large non-uniformity due to the rolling cadence ofLSST, hence provide a worst-case scenario of the impact from non-uniformity. Wefind that these quantities typically increase with depth, and the variation canbe $10-40%$ at extreme depth values. Based on these results and using Y3 as anexample, we propagate the variable depth effect to the weak lensing$3times2$pt data vector in harmonic space. We find that galaxy clustering ismost susceptible to variable depth, causing significant deviations at largescales if not corrected for, due to the depth-dependent number densityvariations. For galaxy-shear and shear-shear power spectra, we find littleimpact given the expected LSST Y3 noise.
我们研究了空间巡天的不均匀性对即将发布的鲁宾天文台时空联合巡天(LSST)数据的星系红移分布的影响。具体来说,我们构建了一个由鲁宾OpSim观测条件退化的模拟光度数据集,并使用模板拟合光度-$z$估计器BPZ和机器学习方法FlexZBoost估计了样本的光度红移。我们选取金样本(Goldsample),定义为 10 年 LSST 数据中的 $i<25.3$,每年都有一个调整后的星等,并将其划分为五个层析红移区,用于弱透镜和源样本。我们对 1 年(Y1)、3 年(Y3)和 5 年(Y5)数据中的天体数量、平均红移和每个层析进行宽度的变化进行了量化,并将其作为coadd $i$ 波段深度的函数。特别是 Y3 和 Y5,由于LSST 的滚动节奏,有很大的不均匀性,因此提供了不均匀性影响的最坏情况。我们发现,这些量通常随深度的增加而增加,在极端深度值上的变化可达 10-40%$ 。基于这些结果,并以Y3为例,我们将变深效应传播到谐波空间的弱透镜$3times2$pt数据矢量上。我们发现,星系聚类最容易受到变深效应的影响,由于与深度相关的数量密度变化,如果不加以校正,就会在大尺度上造成显著偏差。对于星系剪切和剪切-剪切功率谱,我们发现由于预期的 LSST Y3 噪声,影响不大。
{"title":"Impact of survey spatial variability on galaxy redshift distributions and the cosmological $3times2$-point statistics for the Rubin Legacy Survey of Space and Time (LSST)","authors":"Qianjun Hang, Benjamin Joachimi, Eric Charles, John Franklin Crenshaw, Patricia Larsen, Alex I. Malz, Sam Schmidt, Ziang Yan, Tianqing Zhang, the LSST Dark Energy Science Collaboration","doi":"arxiv-2409.02501","DOIUrl":"https://doi.org/arxiv-2409.02501","url":null,"abstract":"We investigate the impact of spatial survey non-uniformity on the galaxy\u0000redshift distributions for forthcoming data releases of the Rubin Observatory\u0000Legacy Survey of Space and Time (LSST). Specifically, we construct a mock\u0000photometry dataset degraded by the Rubin OpSim observing conditions, and\u0000estimate photometric redshifts of the sample using a template-fitting photo-$z$\u0000estimator, BPZ, and a machine learning method, FlexZBoost. We select the Gold\u0000sample, defined as $i<25.3$ for 10 year LSST data, with an adjusted magnitude\u0000cut for each year and divide it into five tomographic redshift bins for the\u0000weak lensing lens and source samples. We quantify the change in the number of\u0000objects, mean redshift, and width of each tomographic bin as a function of the\u0000coadd $i$-band depth for 1-year (Y1), 3-year (Y3), and 5-year (Y5) data. In\u0000particular, Y3 and Y5 have large non-uniformity due to the rolling cadence of\u0000LSST, hence provide a worst-case scenario of the impact from non-uniformity. We\u0000find that these quantities typically increase with depth, and the variation can\u0000be $10-40%$ at extreme depth values. Based on these results and using Y3 as an\u0000example, we propagate the variable depth effect to the weak lensing\u0000$3times2$pt data vector in harmonic space. We find that galaxy clustering is\u0000most susceptible to variable depth, causing significant deviations at large\u0000scales if not corrected for, due to the depth-dependent number density\u0000variations. For galaxy-shear and shear-shear power spectra, we find little\u0000impact given the expected LSST Y3 noise.","PeriodicalId":501207,"journal":{"name":"arXiv - PHYS - Cosmology and Nongalactic Astrophysics","volume":"10 1","pages":""},"PeriodicalIF":0.0,"publicationDate":"2024-09-04","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"142192642","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":0,"RegionCategory":"","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
引用次数: 0
Galaxy clustering in a new implementation of the GAEA semi-analytical galaxy formation model GAEA半分析星系形成模型新实施中的星系聚类
Pub Date : 2024-09-03 DOI: arxiv-2409.02194
Fabio FontanotINAF-OATs, IFPU, Gabriella De LuciaINAF-OATs, IFPU, Lizhi XieTianjin Normal University, Michaela HirschmannEPFL, INAF-OATs, Carlton BaughICC, Durham University, John C. HellyICC
We present results from the latest version of the GAEA model of galaxyformation coupled with merger trees extracted from the P-Millennium Simulation(PMS), which provides a better mass resolution, a larger volume and assumescosmological parameters consistent with latest results from the Planck mission.The model includes, at the same time, a treatment for the partition of cold gasinto atomic and molecular (H$_2$) components; a better treatment forenvironmental processes acting on satellite galaxies; an updated modelling ofcold gas accretion on Super-Massive Black Hole and relative AGN feedback on thehost galaxy. We compare GAEA predictions based on the PMS, with modelrealizations based on other simulations in the Millennium Suite at differentresolution, showing that the new model provides a remarkable consistency in thestatistical properties of galaxy populations. We interpret this as due to theinterplay between AGN feedback and H$_2$-based SFR (both acting as regulatorsof the cold gas content). We then compare model predictions with available datafor the galaxy 2-point correlation function (2pCF) in the redshift range 0
我们展示了从 P-Millennium 模拟(PMS)中提取的最新版 GAEA 星系形成模型与合并树的结果,该模型提供了更好的质量分辨率、更大的体积,并假定了与普朗克任务最新结果一致的宇宙学参数。同时,该模型还包括将冷气体分成原子和分子(H$_2$)两部分的处理方法;对卫星星系所处环境过程的更好处理方法;超大质量黑洞冷气体吸积的最新模型以及 AGN 对宿主星系的相对反馈。我们比较了基于PMS的GAEA预测和基于不同分辨率的Millennium套件中其他模拟的模型实现,结果表明新模型在星系群的统计特性方面具有显著的一致性。我们认为这是由于 AGN 反馈和基于 H$_2$ 的 SFR(两者都是冷气体含量的调节器)之间的相互作用造成的。我们表明,GAEA运行能够正确地恢复2pCF作为恒星质量(M$_star$)、恒星形成活动、HI-含量和红移的函数的主要依赖关系,对于M$_star$ < 10$^{11}$ M$_odot$星系来说是如此。我们的模型正确地捕捉到了星系种群在大尺度结构中的分布,以及中心星系和卫星星系中调节其重子含量的主要物理过程之间的相互作用。在恒星质量较大时,GAEA对2pCF振幅的预测较低,这表明模型中的大质量星系生活在质量较小的暗物质晕中。模型预测的聚类振幅的红移演化相当小,最高可达z$sim$3,这与现有的观测证据是一致的。
{"title":"Galaxy clustering in a new implementation of the GAEA semi-analytical galaxy formation model","authors":"Fabio FontanotINAF-OATs, IFPU, Gabriella De LuciaINAF-OATs, IFPU, Lizhi XieTianjin Normal University, Michaela HirschmannEPFL, INAF-OATs, Carlton BaughICC, Durham University, John C. HellyICC","doi":"arxiv-2409.02194","DOIUrl":"https://doi.org/arxiv-2409.02194","url":null,"abstract":"We present results from the latest version of the GAEA model of galaxy\u0000formation coupled with merger trees extracted from the P-Millennium Simulation\u0000(PMS), which provides a better mass resolution, a larger volume and assumes\u0000cosmological parameters consistent with latest results from the Planck mission.\u0000The model includes, at the same time, a treatment for the partition of cold gas\u0000into atomic and molecular (H$_2$) components; a better treatment for\u0000environmental processes acting on satellite galaxies; an updated modelling of\u0000cold gas accretion on Super-Massive Black Hole and relative AGN feedback on the\u0000host galaxy. We compare GAEA predictions based on the PMS, with model\u0000realizations based on other simulations in the Millennium Suite at different\u0000resolution, showing that the new model provides a remarkable consistency in the\u0000statistical properties of galaxy populations. We interpret this as due to the\u0000interplay between AGN feedback and H$_2$-based SFR (both acting as regulators\u0000of the cold gas content). We then compare model predictions with available data\u0000for the galaxy 2-point correlation function (2pCF) in the redshift range 0<z<3.\u0000We show that GAEA runs are able to correctly recover the main dependencies of\u0000the 2pCF as a function of stellar mass (M$_star$), star formation activity,\u0000HI-content and redshift for M$_star$ < 10$^{11}$ M$_odot$ galaxies. Our model\u0000correctly captures both the distribution of galaxy populations in the Large\u0000Scale Structure and the interplay between the main physical processes\u0000regulating their baryonic content, both for central and satellite galaxies. At\u0000larger stellar masses GAEA underpredicts the 2pCF amplitude, suggesting that\u0000model massive galaxies live in less massive dark matter haloes. The model\u0000predicts a rather small redshift evolution of the clustering amplitude up to\u0000z$sim$3, consistent with available observational evidence.","PeriodicalId":501207,"journal":{"name":"arXiv - PHYS - Cosmology and Nongalactic Astrophysics","volume":"24 1","pages":""},"PeriodicalIF":0.0,"publicationDate":"2024-09-03","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"142192645","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":0,"RegionCategory":"","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
引用次数: 0
Inferring Cosmological Parameters on SDSS via Domain-Generalized Neural Networks and Lightcone Simulations 通过域广义神经网络和光锥模拟推断 SDSS 上的宇宙学参数
Pub Date : 2024-09-03 DOI: arxiv-2409.02256
Jun-Young Lee, Ji-hoon Kim, Minyong Jung, Boon Kiat Oh, Yongseok Jo, Songyoun Park, Jaehyun Lee, Yuan-Sen Ting, Ho Seong Hwang
We present a proof-of-concept simulation-based inference on $Omega_{rm m}$and $sigma_{8}$ from the SDSS BOSS LOWZ NGC catalog using neural networks anddomain generalization techniques without the need of summary statistics. Usingrapid lightcone simulations, ${rm L{scriptsize -PICOLA}}$, mock galaxycatalogs are produced that fully incorporate the observational effects. Thecollection of galaxies is fed as input to a point cloud-based network,${texttt{Minkowski-PointNet}}$. We also add relatively more accurate ${rmG{scriptsize ADGET}}$ mocks to obtain robust and generalizable neuralnetworks. By explicitly learning the representations which reduces thediscrepancies between the two different datasets via the semantic alignmentloss term, we show that the latent space configuration aligns into a singleplane in which the two cosmological parameters form clear axes. Consequently,during inference, the SDSS BOSS LOWZ NGC catalog maps onto the plane,demonstrating effective generalization and improving prediction accuracycompared to non-generalized models. Results from the ensemble of 25independently trained machines find $Omega_{rm m}=0.339 pm 0.056$ and$sigma_{8}=0.801 pm 0.061$, inferred only from the distribution of galaxiesin the lightcone slices without relying on any indirect summary statistics. Asingle machine that best adapts to the ${rm G{scriptsize ADGET}}$ mocksyields a tighter prediction of $Omega_{rm m}=0.282 pm 0.014$ and$sigma_{8}=0.786 pm 0.036$. We emphasize that adaptation across multipledomains can enhance the robustness of the neural networks in observationaldata.
我们利用神经网络和域泛化技术,在不需要汇总统计的情况下,对SDSS BOSS LOWZ NGC星表中的$Omega_{rm m}$和$sigma_{8}$进行了基于概念验证的模拟推断。利用快速光锥模拟(${rm Lscriptsize -PICOLA}}$),生成了完全包含观测效应的模拟星系目录。星系集合被输入到一个基于点云的网络中,${texttt{Minkowski-PointNet}}$。我们还添加了相对更精确的${rmG{scriptsize ADGET}}$模拟,以获得稳健且可泛化的神经网络。通过语义对齐损失项,我们明确地学习了减少两个不同数据集之间差异的表征,结果表明潜在空间配置对齐到了一个单一平面,其中两个宇宙学参数形成了清晰的轴线。因此,在推理过程中,SDSS BOSS LOWZ NGC 星表映射到该平面上,显示了有效的泛化,与非泛化模型相比,提高了预测精度。由25台独立训练过的机器组成的集合的结果显示:$Omega_{rm m}=0.339 pm 0.056$和$sigma_{8}=0.801 pm 0.061$,它们都是仅从光锥切片中的星系分布推断出来的,而不依赖任何间接的汇总统计。如果有一台机器能够最好地适应${/rm G{scriptsize ADGET}}$模拟,那么就能得到更精确的预测结果:$Omega_{/rm m}=0.282 pm 0.014$和$sigma_{8}=0.786 pm 0.036$。我们强调跨多域适应可以增强神经网络在观测数据中的稳健性。
{"title":"Inferring Cosmological Parameters on SDSS via Domain-Generalized Neural Networks and Lightcone Simulations","authors":"Jun-Young Lee, Ji-hoon Kim, Minyong Jung, Boon Kiat Oh, Yongseok Jo, Songyoun Park, Jaehyun Lee, Yuan-Sen Ting, Ho Seong Hwang","doi":"arxiv-2409.02256","DOIUrl":"https://doi.org/arxiv-2409.02256","url":null,"abstract":"We present a proof-of-concept simulation-based inference on $Omega_{rm m}$\u0000and $sigma_{8}$ from the SDSS BOSS LOWZ NGC catalog using neural networks and\u0000domain generalization techniques without the need of summary statistics. Using\u0000rapid lightcone simulations, ${rm L{scriptsize -PICOLA}}$, mock galaxy\u0000catalogs are produced that fully incorporate the observational effects. The\u0000collection of galaxies is fed as input to a point cloud-based network,\u0000${texttt{Minkowski-PointNet}}$. We also add relatively more accurate ${rm\u0000G{scriptsize ADGET}}$ mocks to obtain robust and generalizable neural\u0000networks. By explicitly learning the representations which reduces the\u0000discrepancies between the two different datasets via the semantic alignment\u0000loss term, we show that the latent space configuration aligns into a single\u0000plane in which the two cosmological parameters form clear axes. Consequently,\u0000during inference, the SDSS BOSS LOWZ NGC catalog maps onto the plane,\u0000demonstrating effective generalization and improving prediction accuracy\u0000compared to non-generalized models. Results from the ensemble of 25\u0000independently trained machines find $Omega_{rm m}=0.339 pm 0.056$ and\u0000$sigma_{8}=0.801 pm 0.061$, inferred only from the distribution of galaxies\u0000in the lightcone slices without relying on any indirect summary statistics. A\u0000single machine that best adapts to the ${rm G{scriptsize ADGET}}$ mocks\u0000yields a tighter prediction of $Omega_{rm m}=0.282 pm 0.014$ and\u0000$sigma_{8}=0.786 pm 0.036$. We emphasize that adaptation across multiple\u0000domains can enhance the robustness of the neural networks in observational\u0000data.","PeriodicalId":501207,"journal":{"name":"arXiv - PHYS - Cosmology and Nongalactic Astrophysics","volume":"75 1","pages":""},"PeriodicalIF":0.0,"publicationDate":"2024-09-03","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"142192643","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":0,"RegionCategory":"","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
引用次数: 0
The evolving role of astrophysical modelling in dark matter halo relaxation response 天体物理建模在暗物质晕弛豫响应中不断演变的作用
Pub Date : 2024-08-09 DOI: arxiv-2408.04864
Premvijay Velmani, Aseem Paranjape
We study the change in the radial distribution of dark matter within haloesin response to baryonic astrophysical processes in galaxies at differentepochs, investigating the role of astrophysical modeling in cosmologicalhydrodynamic simulations in producing the response. We find that the linearquasi-adiabatic relaxation with additional dependence on the halo-centricdistance provides a good description not only at $z=0$, but also at an earlierepoch ($z=1$) in the IllustrisTNG simulation suite, with parameters being moreuniversal across a much larger variety of haloes at $z=1$ than at $z=0$.Through systematic analysis of a large collection of simulations from theCAMELS project, we find that the baryonic prescriptions for both AGN andstellar feedbacks have a strong influence on the relaxation response of thedark matter halo. In particular, only the parameters controlling the overallfeedback energy flux have an effect on the relaxation response, while the windspeed and burstiness have negligible effect on the relaxation at a fixed amountof energy flux. However, the exact role of these parameters on the relaxationdepends on the redshift. We also study the role of a variety of baryonicastrophysical processes through the EAGLE physics variation simulations. Whilethese depict a similar picture regarding the importance of feedback effects,they also reveal that the gas equation of state has one of the strongestinfluences on the relaxation response, consistent with the expectation fromself-similar analyses.
我们研究了不同时点星系中暗物质在光环内径向分布的变化对重子天体物理过程的响应,研究了宇宙流体力学模拟中的天体物理建模在产生响应中的作用。我们发现,在IllustrisTNG模拟套件中,线性类绝热弛豫(linearquasi-adiabatic relaxation)附加了对光环中心距离的依赖,不仅在$z=0$时提供了良好的描述,而且在早期($z=1$)也提供了良好的描述,在$z=1$时比在$z=0$时参数在更多的光环中更为普遍。通过对CAMELS项目的大量模拟进行系统分析,我们发现AGN和恒星反馈的重子参数对暗物质晕的弛豫响应有很大影响。特别是,只有控制总体反馈能量通量的参数才会对弛豫响应产生影响,而风速和爆发度在固定能量通量下对弛豫的影响可以忽略不计。然而,这些参数对弛豫的确切作用取决于红移。我们还通过 EAGLE 物理变异模拟研究了各种重子物理过程的作用。虽然这些模拟在反馈效应的重要性方面描述了类似的情况,但也揭示出气体状态方程对弛豫响应的影响是最强的,这与自相似分析的预期是一致的。
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引用次数: 0
Third-order corrections to the slow-roll expansion: calculation and constraints with Planck, ACT, SPT, and BICEP/Keck 慢滚扩展的三阶修正:普朗克、ACT、SPT 和 BICEP/Keck 的计算与约束
Pub Date : 2024-08-09 DOI: arxiv-2408.05210
Mario Ballardini, Alessandro Davoli, Salvatore Samuele Sirletti
We investigate the primordial power spectra (PPS) of scalar and tensorperturbations, derived through the slow-roll approximation. By solving theMukhanov-Sasaki equation and the tensor perturbation equation with Green'sfunction techniques, we extend the PPS calculations to third-order corrections,providing a comprehensive perturbative expansion in terms of slow-rollparameters. We investigate the accuracy of the analytic predictions with thenumerical solutions of the perturbation equations for a selection ofsingle-field slow-roll inflationary models. We derive the constraints on theHubble flow functions $epsilon_i$ from Planck, ACT, SPT, and BICEP/Keck data.We find an upper bound $epsilon_1 lesssim 0.002$ at 95% CL dominated byBICEP/Keck data and robust to all the different combination of datasets. Wederive the constraint $epsilon_2 simeq 0.031 pm 0.004$ at 68% confidencelevel (CL) from the combination of Planck data and late-time probes such asbaryon acoustic oscillations, redshift space distortions, and supernovae dataat first order in the slow-roll expansion. The uncertainty on $epsilon_2$ getslarger including second- and third-order corrections, allowing for anon-vanishing running and running of the running respectively, leading to$epsilon_2 simeq 0.034 pm 0.007$ at 68% CL. We find $epsilon_3 simeq 0.1pm 0.4$ at 95% CL both at second and at third order in the slow-rollexpansion of the spectra. $epsilon_4$ remains always unconstrained. Thecombination of Planck and SPT data leads to slightly tighter constraints on$epsilon_2$ and $epsilon_3$. On the contrary, the combination of Planck datawith ACT measurements, which point to higher values of the scalar spectralindex compared to Planck findings, leads to shifts in the means and maximumlikelihood values for $epsilon_2$ and $epsilon_3$.
我们研究了标量和张量扰动的原始功率谱(PPS),它是通过慢滚近似得到的。通过用格林函数技术求解穆哈诺夫-萨崎方程和张量扰动方程,我们将 PPS 计算扩展到三阶修正,提供了以慢滚参数为基础的全面扰动扩展。我们研究了单场慢滚暴胀模型的扰动方程数值解的分析预测的准确性。我们从普朗克、ACT、SPT和BICEP/Keck数据中推导出哈勃流函数$epsilon_i$的约束条件。我们发现在95%CL时,$epsilon_1 lesssim 0.002$的上界由BICEP/Keck数据主导,并且对所有不同的数据集组合都是稳健的。在68%置信水平(CL)下,我们从普朗克数据和重子声振荡、红移空间扭曲和超新星数据等晚期探测器的组合中,得出了慢卷膨胀一阶的约束$epsilon_2 simeq 0.031 pm 0.004$。包括二阶和三阶修正在内的$epsilon_2$的不确定性变大了,分别允许了非消失运行和运行的运行,导致在68% CL时$epsilon_2 simeq 0.034 pm 0.007$。我们发现在 95% CL 时,在光谱的慢速滚动扩展中,$epsilon_3 在二阶和三阶都是 0.1pm 0.4$。epsilon_4$始终是无约束的。将普朗克数据和 SPT 数据结合起来,对 $epsilon_2$ 和 $epsilon_3$ 的约束会稍微严格一些。与此相反,普朗克数据与ACT测量结果的结合(与普朗克的发现相比,ACT测量结果指向更高的标量光谱指数值)导致了$epsilon_2$和$epsilon_3$的均值和最大似然值的移动。
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引用次数: 0
期刊
arXiv - PHYS - Cosmology and Nongalactic Astrophysics
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