학술논문
Optical and Infrared Photometry of the Type Ia Supernovae 1991T, 1991bg, 1999ek, 2001bt, 2001cn, 2001cz, and 2002bo
Document Type
Working Paper
Author
Krisciunas, Kevin; Suntzeff, Nicholas B.; Phillips, Mark M.; Candia, Pablo; Prieto, Jose Luis; Antezana, R.; Chassagne, R.; Chen, H. -W.; Dickinson, M.; Eisenhardt, P. R.; Espinoza, J.; Garnavich, P. M.; Gonzalez, D.; Harrison, T. E.; Hamuy, M.; Ivanov, V. D.; Krzeminski, W.; Kulesa, C.; McCarthy, P.; Moro-Martin, A.; Muena, C.; Noriega-Crespo, A.; Persson, S. E.; Pinto, P. A.; Roth, M.; Rubenstein, E. P.; Stanford, S. A.; Stringfellow, G. S.; Zapata, A.; Porter, Alain; Wischnjewsky, Marina
Source
Subject
Language
Abstract
We present optical and/or infrared photometry of the Type Ia supernovae SN 1991T, SN 1991bg, SN 1999ek, SN 2001bt, SN 2001cn, SN 2001cz, and SN 2002bo. All but one of these supernovae have decline rate parameters Delta m_15(B) close to the median value of 1.1 for the whole class of Type Ia supernovae. The addition of these supernovae to the relationship between the near-infrared absolute magnitudes and Delta m_15(B) strengthens the previous relationships we have found, in that the maximum light absolute magnitudes are essentially independent of the decline rate parameter. (SN 1991bg, the prototype of the subclass of fast declining Type Ia supernovae, is a special case.) The dispersion in the Hubble diagram in JHK is only ~0.15 mag. The near-infrared properties of Type Ia supernovae continue to be excellent measures of the luminosity distances to the supernova host galaxies, due to the need for only small corrections from the epoch of observation to maximum light, low dispersion in absolute magnitudes at maximum light, and the minimal reddening effects in the near-infrared.
Comment: Astron. J., 128, 3034 (Dec. 2004). This version with updated author list, addresses, acknowledgments, references
Comment: Astron. J., 128, 3034 (Dec. 2004). This version with updated author list, addresses, acknowledgments, references