Photometric properties of intermediate-redshift Type Ia supernovae observed by the Sloan Digital Sky Survey-II Supernova Survey

Takanashi, N.; Doi, M.; Yasuda, N.; Kuncarayakti, H.; Konishi, K.; Schneider, D. P.; Cinabro, D.; Marriner, J.

doi:10.1093/mnras/stw2730

Title: Photometric properties of intermediate-redshift Type Ia supernovae observed by the Sloan Digital Sky Survey-II Supernova Survey

Journal Article · Tue Dec 06 00:00:00 EST 2016 · Monthly Notices of the Royal Astronomical Society

DOI:https://doi.org/10.1093/mnras/stw2730· OSTI ID:1343972

Takanashi, N. ^[1]; Doi, M. ^[2]; Yasuda, N. ^[3]; Kuncarayakti, H. ^[4]; Konishi, K. ^[5]; Schneider, D. P. ^[6]; Cinabro, D. ^[7]; Marriner, J. ^[8]

Univ. of Tokyo, Tokyo (Japan)
Univ. of Tokyo, Tokyo (Japan); Univ. of Tokyo, Chiba (Japan)
Univ. of Tokyo, Chiba (Japan)
Millennium Institute of Astrophysics, Santiago (Chile); Univ. de Chile, Santiago (Chile)
Nikon Corp., Kanagawa (Japan)
Pennsylvania State Univ., University Park, PA (United States)
Wayne State Univ., Detroit, MI (United States)
Fermi National Accelerator Lab. (FNAL), Batavia, IL (United States)

We have analyzed multi-band light curves of 328 intermediate redshift (0.05 <= z < 0.24) type Ia supernovae (SNe Ia) observed by the Sloan Digital Sky Survey-II Supernova Survey (SDSS-II SN Survey). The multi-band light curves were parameterized by using the Multi-band Stretch Method, which can simply parameterize light curve shapes and peak brightness without dust extinction models. We found that most of the SNe Ia which appeared in red host galaxies (u - r > 2.5) don't have a broad light curve width and the SNe Ia which appeared in blue host galaxies (u - r < 2.0) have a variety of light curve widths. The Kolmogorov-Smirnov test shows that the colour distribution of SNe Ia appeared in red / blue host galaxies is different (significance level of 99.9%). We also investigate the extinction law of host galaxy dust. As a result, we find the value of Rv derived from SNe Ia with medium light curve width is consistent with the standard Galactic value. On the other hand, the value of Rv derived from SNe Ia that appeared in red host galaxies becomes significantly smaller. Furthermore, these results indicate that there may be two types of SNe Ia with different intrinsic colours, and they are obscured by host galaxy dust with two different properties.

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Research Organization:: Fermi National Accelerator Laboratory (FNAL), Batavia, IL (United States)

Sponsoring Organization:: USDOE Office of Science (SC), High Energy Physics (HEP)

Grant/Contract Number:: AC02-07CH11359

OSTI ID:: 1343972

Report Number(s):: arXiv:1610.06396; FERMILAB-PUB-16-645-CD; 1492947; TRN: US1701173

Journal Information:: Monthly Notices of the Royal Astronomical Society, Vol. 465, Issue 2; ISSN 0035-8711

Publisher:: Royal Astronomical SocietyCopyright Statement

Country of Publication:: United States

Language:: English

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Cited by: 2 works

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79 ASTRONOMY AND ASTROPHYSICS
supernovae: general
dust
extinction
galaxies: ISM

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