ZTF SN Ia DR2: Exploring SN Ia properties in the vicinity of under-dense environments

IF 5.8 2区 物理与天体物理 Q1 ASTRONOMY & ASTROPHYSICS Astronomy & Astrophysics Pub Date : 2025-02-14 DOI:10.1051/0004-6361/202450951
M. Aubert, P. Rosnet, B. Popovic, F. Ruppin, M. Smith, M. Rigault, G. Dimitriadis, A. Goobar, J. Johansson, C. Barjou-Delayre, U. Burgaz, B. Carreres, F. Feinstein, D. Fouchez, L. Galbany, M. Ginolin, T. de Jaeger, M. M. Kasliwal, Y.-L. Kim, L. Lacroix, F. J. Masci, T. E. Müller-Bravo, B. Racine, C. Ravoux, N. Regnault, R. L. Riddle, D. Rosselli, B. Rusholme, R. Smith, J. Sollerman, J. H. Terwel, A. Townsend
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Abstract

Context. The unprecedented statistics of detected Type Ia supernovae (SNe Ia) brought by the Zwicky Transient Facility (ZTF) enable us to probe the impact of the large-scale structure (LSS) on the properties of these objects.Aims. The goal of this paper is to explore the possible impact of the under-dense part of the LSS on the intrinsic SALT2 light-curve properties of SNe Ia and uncover possible biases in SN Ia analyses.Methods. With a volume-limited selection of ZTF-Cosmo-DR2 SNe Ia overlapping with the SDSS-DR7 survey footprint, we investigated the distribution of their properties with regard to voids detected in the SDSS-DR7 galaxy sample. We further used Voronoi volumes as a proxy for local density environments within the LSS.Results. We find a moderate dependency of the stretch on the localisation around the void centre and none when considering colour. The local Voronoi volumes mostly affect the fraction of low- and high-stretch supernovae.Conclusions. With the presently available statistics, we consider that the impact of high- or low-local-density environment can be considered as a proxy for the colour of the host galaxy. Under-dense environments should not cause any biases in analyses of supernova.
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ZTF SN Ia DR2:探索低密度环境附近的SN Ia性质
上下文。兹威基瞬变设施(ZTF)带来的Ia型超新星(SNe Ia)的前所未有的统计数据使我们能够探索大尺度结构(LSS)对这些天体性质的影响。本文的目的是探讨LSS的低密度部分对SN Ia的固有SALT2光曲线性质的可能影响,并揭示SN Ia分析中可能存在的偏差。通过与SDSS-DR7调查足迹重叠的ztf - cosmos - dr2 snia的体积有限选择,我们研究了它们在SDSS-DR7星系样本中检测到的空洞的性质分布。我们进一步使用Voronoi体积作为lss内局部密度环境的代理。我们发现拉伸适度依赖于空洞中心周围的局部,而在考虑颜色时则没有。局部Voronoi体积主要影响低伸展和高伸展超新星的比例。根据目前可用的统计数据,我们认为高或低局部密度环境的影响可以被认为是宿主星系颜色的代理。低密度环境不应该在超新星分析中造成任何偏差。
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来源期刊
Astronomy & Astrophysics
Astronomy & Astrophysics 地学天文-天文与天体物理
CiteScore
10.20
自引率
27.70%
发文量
2105
审稿时长
1-2 weeks
期刊介绍: Astronomy & Astrophysics is an international Journal that publishes papers on all aspects of astronomy and astrophysics (theoretical, observational, and instrumental) independently of the techniques used to obtain the results.
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