The Type Ia Supernova 1999aw: a Probable 1999aa-like Event In a Low-Luminosity Host Galaxy

• Published in: arXiv.org 2002-07
• Main Authors: L -G Strolger, Smith, R C, Suntzeff, N B, Phillips, M M, Aldering, G, Nugent, P, Knop, R, Perlmutter, S, Schommer, R A, Ho, L C, Hamuy, M, Krisciunas, K, Germany, L M, Covarrubias, R, Candia, P, Athey, A, Blanc, G, Bonacic, A, Bowers, T, Conley, A, Dahlen, T, Freedman, W, Galaz, G, Gates, E, Goldhaber, G, Goobar, A, Groom, D, Hook, I M, Marzke, R, Mateo, M, McCarthy, P, Mendez, J, Muena, C, Persson, S E, Quimby, R, Roth, M, Ruiz-Lapuente, P, Seguel, J, Szentgyorgyi, A, K von Braun, Wood-Vasey, W M, York, T
• Format: Article
• Language: English
• Subjects: Bolometers; Galaxies; Light curve; Luminosity; Photometry; Space telescopes; Supernovae
• ISSN: 2331-8422
• DOI: 10.48550/arxiv.0207409

SN 1999aw was discovered during the first campaign of the Nearby Galaxies Supernova Search (NGSS) project. This luminous, slow-declining (Delta m_{15} (B) = 0.81 \pm 0.03) Type Ia supernova was noteworthy in at least two respects. First, it occurred in an extremely low luminosity host galaxy that was not visible in the template images, nor in initial subsequent deep imaging. Secondly, the photometric and spectral properties of this supernova indicate that it very likely was similar to the subclass of Type Ia supernovae whose prototype is SN 1999aa. This paper presents the BVRI and J_{s} HK_{s} lightcurves of SN 1999aw (through 100 days past maximum light), as well as several epochs of optical spectra. From these data we calculate the bolometric light curve, and give estimates of the luminosity at maximum light and the initial ^{56}Ni mass. In addition, we present deep BVI images obtained recently with the Baade 6.5-meter telescope at Las Campanas Observatory which reveal the remarkably low-luminosity host galaxy.