Using rest-frame optical and NIR data from the RAISIN survey to explore the redshift evolution of dust laws in SN Ia host galaxies

被引：6

作者：

Thorp, Stephen ^{[1
,2
,3
]}

Mandel, Kaisey S. ^{[2
,3
,4
]}

Jones, David O. ^{[5
]}

Kirshner, Robert P. ^{[6
,7
]}

Challis, Peter M. ^{[8
]}

机构：

[1] Stockholm Univ, AlbaNova Univ Ctr, Oskar Klein Ctr, Dept Phys, SE-10691 Stockholm, Sweden

[2] Inst Astron, Madingley Rd, Cambridge CB3 0HA, England

[3] Kavli Inst Cosmol, Madingley Rd, Cambridge CB3 0HA, England

[4] Univ Cambridge, Stat Lab, DPMMS, Wilberforce Rd, Cambridge CB3 0WB, England

[5] Univ Hawaii, Inst Astron, 640 N Aohoku Pl, Hilo, HI 96720 USA

[6] TMT Int Observ, 100 West Walnut St, Pasadena, CA 91124 USA

[7] CALTECH, 1200 East Calif Blvd, Pasadena, CA 91125 USA

[8] Harvard Smithsonian Ctr Astrophys, 60 Garden St, Cambridge, MA 02138 USA

来源：

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | 2024年 / 530卷 / 04期

基金：

欧洲研究理事会; 英国科学技术设施理事会;

关键词：

methods: statistical; supernovae: general; dust; extinction; distance scale; PHOTOMETRY DATA RELEASE; 2-PARAMETER LUMINOSITY CORRECTION; SUPERNOVA LIGHT CURVES; PANTHEON PLUS ANALYSIS; HUBBLE DIAGRAM; COSMOLOGICAL CONSTRAINTS; SYSTEMATIC UNCERTAINTIES; STELLAR MASS; INTERGALACTIC DUST; INTRINSIC SCATTER;

D O I：

10.1093/mnras/stae1111

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We use rest-frame optical and near-infrared (NIR) observations of 42 Type Ia supernovae (SNe Ia) from the Carnegie Supernova Project at low-z and 37 from the RAISIN (SNIA in the IR) Survey at high-z to investigate correlations between SN Ia host galaxy dust, host mass, and redshift. This is the first time the SN Ia host galaxy dust extinction law at high-z has been estimated using combined optical and rest-frame NIR data (YJ band). We use the BayeSN hierarchical model to leverage the data's wide rest-frame wavelength range (extending to similar to 1.0-1.2 mu m for the RAISIN sample at 0.2 less than or similar to z less than or similar to 0.6). By contrasting the RAISIN and Carnegie Supernova Project (CSP) data, we constrain the population distributions of the host dust RV parameter for both redshift ranges. We place a limit on the difference in population mean RV between RAISIN and CSP of -1.16 < Delta mu(RV) < 1.38 with 95 per cent posterior probability. For RAISIN we estimate mu(RV) = 2.58 +/- 0.57, and constrain the population standard deviation to sigma(RV) < 0.90 [2.42] at the 68 [95] per cent level. Given that we are only able to constrain the size of the low- to high-z shift in mu(RV) to less than or similar to 1.4 - which could still propagate to a substantial bias in the equation-of-state parameter w - these and other recent results motivate continued effort to obtain rest-frame NIR data at low- and high-redshifts (e.g. using the Roman Space Telescope).

引用

页码：4016 / 4031

页数：16

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