THE MID-INFRARED AND OPTICAL DECAY OF SN 2011fe

Testing supernovae Ia distance measurement methods with SN 2011fe

(2012) J. Vinkó et al.   ASTRONOMY & ASTROPHYSICS

ANALYSIS OF THE EARLY-TIME OPTICAL SPECTRA OF SN 2011fe IN M101

(2012) J. T. Parrent et al.   Astrophysical Journal Letters

THE FIRST MAXIMUM-LIGHT ULTRAVIOLET THROUGH NEAR-INFRARED SPECTRUM OF A TYPE Ia SUPERNOVA,

(2012) Ryan J. Foley et al.   Astrophysical Journal Letters

NO STRIPPED HYDROGEN IN THE NEBULAR SPECTRA OF NEARBY TYPE Ia SUPERNOVA 2011fe

(2012) Benjamin J. Shappee et al.   Astrophysical Journal Letters

BVRI lightcurves of supernovae SN 2011fe in M101, SN 2012aw in M95, and SN 2012cg in NGC 4424

(2012) U. Munari et al.   NEW ASTRONOMY

A NEW CEPHEID DISTANCE TO THE GIANT SPIRAL M101 BASED ON IMAGE SUBTRACTION OFHUBBLE SPACE TELESCOPE/ADVANCED CAMERA FOR SURVEYS OBSERVATIONS

(2011) Benjamin J. Shappee et al.   ASTROPHYSICAL JOURNAL

The nebular spectrum of the Type Ia supernova 2003hv: evidence for a non-standard event

(2011) Paolo A. Mazzali et al.   MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY

NEAR-ULTRAVIOLET PROPERTIES OF A LARGE SAMPLE OF TYPE Ia SUPERNOVAE AS OBSERVED WITH THESwiftUVOT

(2010) Peter A. Milne et al.   ASTROPHYSICAL JOURNAL

An asymmetric explosion as the origin of spectral evolution diversity in type Ia supernovae

(2010) K. Maeda et al.   NATURE

The normal Type Ia SN 2003hv out to very late phases

(2009) G. Leloudas et al.   ASTRONOMY & ASTROPHYSICS

NEBULAR SPECTRA AND EXPLOSION ASYMMETRY OF TYPE Ia SUPERNOVAE

(2009) K. Maeda et al.   ASTROPHYSICAL JOURNAL