A1 Refereed original research article in a scientific journal
Photometric study of the late-time near-infrared plateau in Type Ia supernovae
Authors: Deckers M, Graur O, Maguire K, Shingles L, Brennan SJ, Anderson JP, Burke J, Chen TW, Galbany L, Grayling MJP, Gutierrez CP, Harvey L, Hiramatsu D, Howell DA, Inserra C, Killestein T, McCully C, Muller-Bravo TE, Nicholl M, Newsome M, Gonzalez EP, Pellegrino C, Terreran G, Terwel JH, Toy M, Young DR
Publisher: OXFORD UNIV PRESS
Publication year: 2023
Journal:Monthly Notices of the Royal Astronomical Society
Journal name in sourceMONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
Journal acronym: MON NOT R ASTRON SOC
Volume: 521
Issue: 3
First page : 4414
Last page: 4430
Number of pages: 17
ISSN: 0035-8711
DOI: https://doi.org/10.1093/mnras/stad841
Web address : https://doi.org/10.1093/mnras/stad841
Self-archived copy’s web address: https://research.utu.fi/converis/portal/detail/Publication/179780162
We present an in-depth study of the late-time near-infrared plateau in Type Ia supernovae (SNe Ia), which occurs between 70 and 500 d. We double the existing sample of SNe Ia observed during the late-time near-infrared plateau with new observations taken with the Hubble Space Telescope, Gemini, New Technology Telescope, the 3.5-m Calar Alto Telescope, and the Nordic Optical Telescope. Our sample consists of 24 nearby SNe Ia at redshift < 0.025. We are able to confirm that no plateau exists in the K-s band for most normal SNe Ia. SNe Ia with broader optical light curves at peak tend to have a higher average brightness on the plateau in J and H, most likely due to a shallower decline in the preceding 100 d. SNe Ia that are more luminous at peak also show a steeper decline during the plateau phase in H. We compare our data to state-of-the-art radiative transfer models of nebular SNe Ia in the near-infrared. We find good agreement with the sub-M-ch model that has reduced non-thermal ionization rates, but no physical justification for reducing these rates has yet been proposed. An analysis of the spectral evolution during the plateau demonstrates that the ratio of [Fe ii] to [Fe iii] contribution in a near-infrared filter determines the light curve evolution in said filter. We find that overluminous SNe decline slower during the plateau than expected from the trend seen for normal SNe Ia.
Downloadable publication This is an electronic reprint of the original article. |  |
