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

Fuente: arXiv
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Main Authors: Aubert, M., Rosnet, P., Popovic, B., Ruppin, F., Smith, M., Rigault, M., Dimitriadis, G., Goobar, A., Johansson, J., Barjou-Delayre, C., Burgaz, U., Carreres, B., Feinstein, F., Fouchez, D., Galbany, L., Ginolin, M., de Jaeger, T., Kasliwal, M. M., Kim, Y. -L., Lacroix, L., Masci, F. J., Müller-Bravo, T. E., Racine, B., Ravoux, C., Regnault, N., Riddle, R. L., Rosselli, D., Rusholme, B., Smith, R., Sollerman, J., Terwel, J. H., Townsend, A.
Format: Preprint
Published: 2024
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author Aubert, M.
Rosnet, P.
Popovic, B.
Ruppin, F.
Smith, M.
Rigault, M.
Dimitriadis, G.
Goobar, A.
Johansson, J.
Barjou-Delayre, C.
Burgaz, U.
Carreres, B.
Feinstein, F.
Fouchez, D.
Galbany, L.
Ginolin, M.
de Jaeger, T.
Kasliwal, M. M.
Kim, Y. -L.
Lacroix, L.
Masci, F. J.
Müller-Bravo, T. E.
Racine, B.
Ravoux, C.
Regnault, N.
Riddle, R. L.
Rosselli, D.
Rusholme, B.
Smith, R.
Sollerman, J.
Terwel, J. H.
Townsend, A.
author_facet Aubert, M.
Rosnet, P.
Popovic, B.
Ruppin, F.
Smith, M.
Rigault, M.
Dimitriadis, G.
Goobar, A.
Johansson, J.
Barjou-Delayre, C.
Burgaz, U.
Carreres, B.
Feinstein, F.
Fouchez, D.
Galbany, L.
Ginolin, M.
de Jaeger, T.
Kasliwal, M. M.
Kim, Y. -L.
Lacroix, L.
Masci, F. J.
Müller-Bravo, T. E.
Racine, B.
Ravoux, C.
Regnault, N.
Riddle, R. L.
Rosselli, D.
Rusholme, B.
Smith, R.
Sollerman, J.
Terwel, J. H.
Townsend, A.
contents The unprecedented statistics of detected Type Ia supernovae (SNe Ia) brought by the Zwicky Transient Facility enables us to probe the impact of the Large-Scale Structure on the properties of these objects. The goal of this paper is to explore the possible impact of the under-dense part of the large-scale structure on the intrinsic SALT2 light curve properties of SNe Ia and uncover possible biases in SN Ia analyses. With a volume-limited selection of ZTF-Cosmo-DR2 Type Ia supernovae overlapping with the SDSS-DR7 survey footprint, we investigate the distribution of their properties with regard to voids detected in the SDSS-DR7 galaxy sample. We further use Voronoi volumes as proxy for local density environments within the large-scale structure. We find a moderate dependency of the stretch toward the localisation around the void centre and none when considering colour. The local Voronoi volumes mostly affect the fraction of low/high stretch supernovae. With the current statistics available, 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 supernova analyses.
format Preprint
id arxiv_https___arxiv_org_abs_2406_11680
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle ZTF SN Ia DR2: Exploring SN Ia properties in the vicinity of under-dense environments
Aubert, M.
Rosnet, P.
Popovic, B.
Ruppin, F.
Smith, M.
Rigault, M.
Dimitriadis, G.
Goobar, A.
Johansson, J.
Barjou-Delayre, C.
Burgaz, U.
Carreres, B.
Feinstein, F.
Fouchez, D.
Galbany, L.
Ginolin, M.
de Jaeger, T.
Kasliwal, M. M.
Kim, Y. -L.
Lacroix, L.
Masci, F. J.
Müller-Bravo, T. E.
Racine, B.
Ravoux, C.
Regnault, N.
Riddle, R. L.
Rosselli, D.
Rusholme, B.
Smith, R.
Sollerman, J.
Terwel, J. H.
Townsend, A.
Cosmology and Nongalactic Astrophysics
The unprecedented statistics of detected Type Ia supernovae (SNe Ia) brought by the Zwicky Transient Facility enables us to probe the impact of the Large-Scale Structure on the properties of these objects. The goal of this paper is to explore the possible impact of the under-dense part of the large-scale structure on the intrinsic SALT2 light curve properties of SNe Ia and uncover possible biases in SN Ia analyses. With a volume-limited selection of ZTF-Cosmo-DR2 Type Ia supernovae overlapping with the SDSS-DR7 survey footprint, we investigate the distribution of their properties with regard to voids detected in the SDSS-DR7 galaxy sample. We further use Voronoi volumes as proxy for local density environments within the large-scale structure. We find a moderate dependency of the stretch toward the localisation around the void centre and none when considering colour. The local Voronoi volumes mostly affect the fraction of low/high stretch supernovae. With the current statistics available, 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 supernova analyses.
title ZTF SN Ia DR2: Exploring SN Ia properties in the vicinity of under-dense environments
topic Cosmology and Nongalactic Astrophysics
url https://arxiv.org/abs/2406.11680