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, Δm_(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 Δm_(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-infr...
Artículo de publicación ISIWe analyze the standardizability of Type Ia supernovae (SNe Ia) in the ne...
We present first-season infrared (IR) and optical photometry and spectroscopy of the Type Ia Superno...
Accepted. Received; in original form In this third paper in a series we compare spectral feature mea...
Artículo de publicación ISI.We present optical and/or infrared photometry of the Type Ia supernovae ...
We present near-infrared photometry of the Type Ia supernova (SN) 1999ee; also, optical and infrared...
Artículo de publicación ISI.We present near-infrared photometry of the Type Ia supernova (SN) 1999ee...
We present well-sampled optical (UBVRI) and infrared (JHK) light curves of the nearby (≈18.0 Mpc) Ty...
We present optical and near-infrared photometric and spectroscopic observations of the fast-declinin...
We present optical and near-infrared photometry, as well as ground-based optical spectra and Hubble ...
We present optical and infrared photometry of the unusual Type Ia supernova 2000cx. With the data of...
From observations of 7 Type Ia supernovae obtained during the last four years at the Las Campanas an...
We obtained optical photometry of SN 2003gs on 49 nights, from 2 to 494 days after T(B max). We also...
We present optical (UBVRI) and near-IR (YJHK) photometry of the normal Type Ia supernova (SN) 2004S....
We obtained optical photometry of SN 2003gs on 49 nights, from 2 to 494 days after T(B(max)). We als...
New infrared data for 11 Type I supernovae are presented. These results, when combined with other pu...
Artículo de publicación ISIWe analyze the standardizability of Type Ia supernovae (SNe Ia) in the ne...
We present first-season infrared (IR) and optical photometry and spectroscopy of the Type Ia Superno...
Accepted. Received; in original form In this third paper in a series we compare spectral feature mea...
Artículo de publicación ISI.We present optical and/or infrared photometry of the Type Ia supernovae ...
We present near-infrared photometry of the Type Ia supernova (SN) 1999ee; also, optical and infrared...
Artículo de publicación ISI.We present near-infrared photometry of the Type Ia supernova (SN) 1999ee...
We present well-sampled optical (UBVRI) and infrared (JHK) light curves of the nearby (≈18.0 Mpc) Ty...
We present optical and near-infrared photometric and spectroscopic observations of the fast-declinin...
We present optical and near-infrared photometry, as well as ground-based optical spectra and Hubble ...
We present optical and infrared photometry of the unusual Type Ia supernova 2000cx. With the data of...
From observations of 7 Type Ia supernovae obtained during the last four years at the Las Campanas an...
We obtained optical photometry of SN 2003gs on 49 nights, from 2 to 494 days after T(B max). We also...
We present optical (UBVRI) and near-IR (YJHK) photometry of the normal Type Ia supernova (SN) 2004S....
We obtained optical photometry of SN 2003gs on 49 nights, from 2 to 494 days after T(B(max)). We als...
New infrared data for 11 Type I supernovae are presented. These results, when combined with other pu...
Artículo de publicación ISIWe analyze the standardizability of Type Ia supernovae (SNe Ia) in the ne...
We present first-season infrared (IR) and optical photometry and spectroscopy of the Type Ia Superno...
Accepted. Received; in original form In this third paper in a series we compare spectral feature mea...