We present 65 optical spectra of the Type Ia SN 2012fr, 33 of which were obtained before maximum light. At early times, SN 2012fr shows clear evidence of a high-velocity feature (HVF) in the Si lambda 6355 line that can be cleanly decoupled from the lower velocity "photospheric" component. This Si lambda 6355 HVF fades by phase - 5; subsequently, the photospheric component exhibits a very narrow velocity width and remains at a nearly constant velocity of similar to 12,000 km s(-1) until at least five weeks after maximum brightness. The Ca II infrared triplet exhibits similar evidence for both a photospheric component at v approximate to 12,000 km s(-1) with narrow line width and long velocity plateau, as well as an HVF beginning at v approx...
Artículo de publicación ISIAs part of the European Supernova Collaboration, we obtained extensive ph...
We present photometry and time-series spectroscopy of the nearby type Ia supernova (SN Ia) SN 2015F ...
The UBVRI photometric follow-up of SN 2011fu has been initiated a few days after the explosion, show...
We present 65 optical spectra of the Type Ia SN 2012fr, 33 of which were obtained before maximum lig...
We present 65 optical spectra of the Type Ia SN 2012fr, 33 of which were obtained before maximum lig...
We present 65 optical spectra of the Type Ia SN 2012fr, 33 of which were obtained before maximum lig...
We present detailed ultraviolet, optical, and near-infrared light curves of the Type Ia supernova (S...
We report measurements and analysis of high-velocity (HVF) (>20,000 km s(-1)) and photospheric absor...
We present an investigation of the optical spectra of 264 low-redshift (z < 0.2) Type Ia supernov...
We present extensive u{prime}g{prime}r{prime}i{prime} BV RIY JHK{sub s} photometry and optical spect...
Accepted for publication in AJ Extensive optical and ultraviolet (UV) observations of the type Ia su...
We present extensive u'g'r'i'BVRIYJHKs photometry and optical spectroscopy of SN 2005hk. These data ...
We present early-time optical and near-infrared photometry of supernova (SN) 2005cf. The observation...
We present optical and infrared observations of the unusual Type Ia supernova (SN) 2004eo. The light...
Aims. We present and study the spectroscopic and photometric evolution of the type Ia supernova (SN ...
Artículo de publicación ISIAs part of the European Supernova Collaboration, we obtained extensive ph...
We present photometry and time-series spectroscopy of the nearby type Ia supernova (SN Ia) SN 2015F ...
The UBVRI photometric follow-up of SN 2011fu has been initiated a few days after the explosion, show...
We present 65 optical spectra of the Type Ia SN 2012fr, 33 of which were obtained before maximum lig...
We present 65 optical spectra of the Type Ia SN 2012fr, 33 of which were obtained before maximum lig...
We present 65 optical spectra of the Type Ia SN 2012fr, 33 of which were obtained before maximum lig...
We present detailed ultraviolet, optical, and near-infrared light curves of the Type Ia supernova (S...
We report measurements and analysis of high-velocity (HVF) (>20,000 km s(-1)) and photospheric absor...
We present an investigation of the optical spectra of 264 low-redshift (z < 0.2) Type Ia supernov...
We present extensive u{prime}g{prime}r{prime}i{prime} BV RIY JHK{sub s} photometry and optical spect...
Accepted for publication in AJ Extensive optical and ultraviolet (UV) observations of the type Ia su...
We present extensive u'g'r'i'BVRIYJHKs photometry and optical spectroscopy of SN 2005hk. These data ...
We present early-time optical and near-infrared photometry of supernova (SN) 2005cf. The observation...
We present optical and infrared observations of the unusual Type Ia supernova (SN) 2004eo. The light...
Aims. We present and study the spectroscopic and photometric evolution of the type Ia supernova (SN ...
Artículo de publicación ISIAs part of the European Supernova Collaboration, we obtained extensive ph...
We present photometry and time-series spectroscopy of the nearby type Ia supernova (SN Ia) SN 2015F ...
The UBVRI photometric follow-up of SN 2011fu has been initiated a few days after the explosion, show...