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The ALPINE-ALMA [CII] Survey: Exploring the Dark Side of Normal Galaxies at the End of Reionisation ALPINE-ALMA [CII]调查:在再电离结束时探索正常星系的黑暗面
IF 0.4 Q4 COMMUNICATION Pub Date : 2020-06-01 DOI: 10.18727/0722-6691/5198
M. Béthermin, M. Dessauges-Zavadsky, A. Faisst, M. Ginolfi, C. Gruppioni, G. Jones, Y. Khusanova, B. Lemaux, P. Capak, P. Cassata, O. Fèvre, D. Schaerer, J. Silverman, Lin Yan
1 Aix Marseille Université, CNRS, CNES, LAM, Marseille, France 2 Département d’Astronomie, Université de Genève, Versoix, Switzerland 3 IPAC, M/C 314-6, California Institute of Technology, Pasadena, USA 4 INAF – Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Italy 5 Cavendish Laboratory, University of Cambridge, UK 6 Kavli Institute for Cosmology, University of Cambridge, UK 7 Max-Planck-Institut für Astronomie, Heidelberg, Germany 8 Department of Physics, University of California Davis, USA 9 The Cosmic Dawn Center (DAWN), University of Copenhagen, Denmark 10 Niels Bohr Institute, University of Copenhagen, Denmark 11 Dipartimento di Fisica e Astronomia, Università di Padova, Italy 12 INAF – Osservatorio Astronomico di Padova, Italy 13 Kavli Institute for the Physics and Mathematics of the Universe (Kavli IPMU, WPI), The University of Tokyo, Kashiwa, Japan 14 Department of Astronomy, School of Science, The University of Tokyo, Japan 15 The Caltech Optical Observatories, California Institute of Technology, Pasadena, USA
1、大学Aix Marseille, CNRS CNES、大学d’Astronomie LAM,马赛,法国2省,IPAC 3 - de Versoix, Switzerland, M / C 314-6,加州理工学院,美国帕萨迪纳4 INAF博洛尼亚—天体物理学和空间科学观测站,意大利5剑桥大学卡文迪许实验室,英国6研究所(Kavli Institute for Cosmology,剑桥大学,英国7天für Astronomie、海德堡,Germany 8 Department of物理,加州大学戴维斯,美国9 The cosmos Dawn Center (Dawn)、10,丹麦哥本哈根大学尼尔斯·玻尔研究所,11,丹麦哥本哈根大学物理系和天文学、帕多瓦大学、意大利INAF 12—13帕多瓦、意大利天文观测台研究所(Kavli Institute for The物理和服装of The宇宙(Kavli IPMU, WPI), The University of 14日本东京,Kashiwa Department of天文学,School of Science, The University of东京日本加州理工学院光学天文台,帕萨迪纳,美国
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引用次数: 0
Report on the ESO Summer School “La Silla Observing Summer School 2020” ESO暑期学校“2020年拉新罗观察暑期学校”报告
IF 0.4 Q4 COMMUNICATION Pub Date : 2020-06-01 DOI: 10.18727/0722-6691/5201
E. Pompei, J. Hartke, H. Korhonen, C. Mazzucchelli, C. Navarrete, A. Pala, L. Sbordone, L. Schmidtobreick
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引用次数: 0
A Rare Pair of Eclipsing Brown Dwarfs Identified by the SPECULOOS Telescopes 由SPECULOOS望远镜发现的一对罕见的食棕矮星
IF 0.4 Q4 COMMUNICATION Pub Date : 2020-06-01 DOI: 10.18727/0722-6691/5199
A. Triaud, A. Burgasser, A. Burdanov, V. Hodžić, R. Alonso, D. B. Gagliuffi, L. Delrez, B. Demory, J. Wit, E. Ducrot, F. Hessman, T. Husser, E. Jehin, P. P. Pedersen, D. Queloz, J. McCormac, C. Murray, D. Sebastian, S. Thompson, V. Grootel, M. Gillon
The Messenger 180 – Quarter 2 | 2020 Amaury H. M. J. Triaud 1 Adam J. Burgasser 2 Artem Burdanov 3 Vedad Kunovac Hodžić 1 Roi Alonso 4 Daniella Bardalez Gagliuffi 5 Laetitia Delrez 6 Brice-Olivier Demory 7 Julien de Wit 8 Elsa Ducrot 3 Frederic V. Hessman 9 Tim-Oliver Husser 9 Emmanuël Jehin10 Peter P. Pedersen 6 Didier Queloz 6 James McCormac 11 Catriona Murray 6 Daniel Sebastian 3 Samantha Thompson 6 Valérie Van Grootel 10 Michaël Gillon 3
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引用次数: 0
Report on the ESO/ALMA Conference “ALMA 2019: Science Results and Cross-Facility Synergies” ESO/ALMA会议“ALMA 2019:科学成果和跨设施协同效应”报告
IF 0.4 Q4 COMMUNICATION Pub Date : 2020-06-01 DOI: 10.18727/0722-6691/5200
C. Kemper
The Atacama Large Millimeter/submillimeter Array (ALMA) is the largest and most sensitive millimetre/submillimetre array on the planet, with the highest spatial resolution. Since it began operating, ALMA has routinely been at the forefront of science in this wavelength regime, delivering groundbreaking discoveries. The ALMA 2019 science conference was organised as one of a series of meetings held at regular intervals for the worldwide ALMA community, the previous one being held in Indian Wells, USA in 2016. At the start of Cycle 7 of observations, the ALMA 2019 conference provided an opportunity for the community to reflect on the multitude of scientific results from the facility, with special emphasis on the results from the first rounds of ALMA Large Programmes, the long baselines and high-frequency capabilities, the new solar and very long baseline interferometry (VLBI) modes, as well as the synergy between ALMA and other observatories.
阿塔卡马大型毫米/亚毫米阵列(ALMA)是地球上最大、最灵敏的毫米/亚毫米阵列,具有最高的空间分辨率。自开始运行以来,ALMA一直处于该波长范围的科学前沿,提供突破性的发现。ALMA 2019科学会议是全球ALMA社区定期举行的一系列会议之一,上一届会议于2016年在美国印第安维尔斯举行。在观测周期7开始之际,ALMA 2019会议为科学界提供了一个反思该设施所取得的众多科学成果的机会,特别强调了ALMA大型计划第一轮的结果、长基线和高频能力、新的太阳和甚长基线干涉测量(VLBI)模式,以及ALMA与其他天文台之间的协同作用。
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引用次数: 1
Report on the ESO Workshop "ESOz-2020: The Build-up of Galaxies through Multiple Tracers and Facilities" ESO研讨会“esoz2020:通过多种示踪剂和设施构建星系”报告
IF 0.4 Q4 COMMUNICATION Pub Date : 2020-06-01 DOI: 10.18727/0722-6691/5202
C. Lagos, A. Robotham, C. Breuck
We report on the second joint Australia– ESO conference, held in Perth, Australia, following the successful Sydney conference in 2019. The conference was supported by ESO, the Centre of Excellence ASTRO 3D, the International Centre for Radio Astronomy Research, Macquarie University, CSIRO Astronomy and Space Science (CASS), and the Galaxies Journal. The scientific organising committee (SOC) focused on a programme that highlighted the complementarity between ESO and Australian instruments and the science breakthroughs enabled by this combination. In terms of demographics, we followed the same strategies as the previous meeting to tackle unconscious bias, and this again resulted in a wellbalanced programme in terms of gender, career stage and geography, proving its effectiveness. Given concerns about global warming and the COVID-19 pandemic, the local organising committee (LOC) allowed several talks to be delivered remotely, and we reflect on that experience here. Motivation
继2019年悉尼会议取得成功后,我们报道在澳大利亚珀斯举行的第二次澳大利亚- ESO联合会议。会议得到了ESO、卓越ASTRO 3D中心、国际射电天文学研究中心、麦考瑞大学、CSIRO天文学与空间科学(CASS)和《星系杂志》的支持。科学组织委员会(SOC)将重点放在强调ESO与澳大利亚仪器之间的互补性以及这种组合所带来的科学突破的计划上。在人口统计方面,我们遵循了与上次会议相同的策略来解决无意识偏见,这再次导致了在性别、职业阶段和地理方面平衡良好的方案,证明了其有效性。考虑到对全球变暖和COVID-19大流行的担忧,当地组委会(LOC)允许几次远程演讲,我们在这里反思这一经验。动机
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引用次数: 1
The 2018 Visiting Committee Report 2018年访问委员会报告
IF 0.4 Q4 COMMUNICATION Pub Date : 2020-03-01 DOI: 10.18727/0722-6691/5184
H. Rix
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引用次数: 0
Report on the ESO Workshop "The La Silla Observatory — From Inauguration to the Future" ESO研讨会“拉西拉天文台-从落成到未来”报告
IF 0.4 Q4 COMMUNICATION Pub Date : 2020-03-01 DOI: 10.18727/0722-6691/5192
I. Saviane, B. Leibundgut, L. Schmidtobreick
The historical context of astronomical observatories in Chile was given by Bárbara Silva from the Pontificia Universidad Católica de Chile. The earliest astronomical site explorations by US astronomers were carried out around the end of the 19th and the beginning of the 20th centuries and identified the Atacama Desert around Copiapó and north of La Serena as potentially excellent sites for nighttime observations. The International Geophysical Year in 1958 brought the Chilean sites to the attention of American astronomers again and site explorations by Jürgen Stock — originally for the University of Chicago and later for the Association of Universities for Research in Astronomy (AURA) — identified mountains around Vicuña as possible observatory sites. After the US National Science Foundation selected Cerro Tololo as their southern station, ESO also became interested (through Stock’s former advisor Otto Heckmann, then ESO Director General). This was a rather abrupt change from the original plan to place the ESO observatory in southern Africa. Within a few years the La Silla mountain was selected and developed. Silva finished her presentation by displaying a stamp showing the ESO 1-metre telescope, which was issued by the Chilean Postal Office in 1973.
智利天文台的历史背景是由Católica de Chile Pontificia university的Bárbara Silva给出的。美国天文学家最早的天文观测地点是在19世纪末和20世纪初进行的,他们确定了位于Copiapó附近和拉塞雷纳北部的阿塔卡马沙漠是夜间观测的潜在绝佳地点。1958年的国际地球物理年再次引起了美国天文学家的注意,j rgen Stock(最初为芝加哥大学工作,后来为天文学大学研究协会工作)进行的现场勘探发现,Vicuña周围的山脉可能是天文台的地点。在美国国家科学基金会选择Cerro Tololo作为他们的南站之后,ESO也产生了兴趣(通过Stock的前顾问Otto Heckmann,当时的ESO总干事)。这与把ESO天文台放在非洲南部的最初计划相比,是一个相当突然的变化。几年内,拉西拉山被选中并开发。席尔瓦在演讲结束时展示了一张邮票,邮票上是智利邮政于1973年发行的ESO 1米望远镜。
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引用次数: 0
SPHERE Unveils the True Face of the Largest Main Belt Asteroids SPHERE揭示了最大的主带小行星的真实面貌
IF 0.4 Q4 COMMUNICATION Pub Date : 2020-03-01 DOI: 10.18727/0722-6691/5187
P. Vernazza, L. Jorda, B. Carry, J. Hanuš, M. Marsset, M. Viikinkoski, F. Marchis, M. Brož, A. Drouard, T. Fusco, R. Fétick, M. Ferrais, Harissa Team
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引用次数: 1
Following Up on the Recommendations of the Visiting Committee 跟进访问委员会的建议
IF 0.4 Q4 COMMUNICATION Pub Date : 2020-03-01 DOI: 10.18727/0722-6691/5185
X. Barcons
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引用次数: 0
The ASPECS Survey: An ALMA Large Programme Targeting the Hubble Ultra-Deep Field ASPECS调查:一项针对哈勃超深视场的ALMA大型计划
IF 0.4 Q4 COMMUNICATION Pub Date : 2020-03-01 DOI: 10.18727/0722-6691/5188
M. Aravena, C. Carilli, R. Decarli, F. Walter
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引用次数: 1
期刊
Jurnal The Messenger
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