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The First Data Release of CNIa0.02-A Complete Nearby (Redshift <0.02) Sample of Type Ia Supernova Light Curves

Autor
Elias-Rosa, N.
Kankare, Erkki
Lundqvist, P.
Prieto, J. L.
Shappee, B. J.
Muñoz, J. A.
Natusch, Tim
Koff, Robert
Buckley, David A. H.
Cappellaro, Enrico
Data publikacji
2022
Abstrakt (EN)

The CNIa0.02 project aims to collect a complete, nearby sample of Type Ia supernovae (SNe Ia) light curves, and the SNe are volume-limited with host-galaxy redshifts z <SUB>host</SUB> < 0.02. The main scientific goal is to infer the distributions of key properties (e.g., the luminosity function) of local SNe Ia in a complete and unbiased fashion in order to study SN explosion physics. We spectroscopically classify any SN candidate detected by the All-Sky Automated Survey for Supernovae (ASAS-SN) that reaches a peak brightness <16.5 mag. Since ASAS-SN scans the full sky and does not target specific galaxies, our target selection is effectively unbiased by host-galaxy properties. We perform multiband photometric observations starting from the time of discovery. In the first data release (DR1), we present the optical light curves obtained for 247 SNe from our project (including 148 SNe in the complete sample), and we derive parameters such as the peak fluxes, Δm <SUB>15</SUB>, and s <SUB>BV</SUB> . <SUP>*</SUP> This paper includes data gathered with the 6.5 m Magellan Telescopes located at Las Campanas Observatory, Chile.

Dyscyplina PBN
astronomia
Czasopismo
Astrophysical Journal, Supplement Series
Tom
259
Zeszyt
2
Strony od-do
53
ISSN
0067-0049
Data udostępnienia w otwartym dostępie
2022-03-30
Licencja otwartego dostępu
Uznanie autorstwa