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Sep 20, 2006 · Supernova SNLS-03D3bb is more than twice as bright as most Type Ia supernovae but has much less kinetic energy, and appears to be half again as massive as a …

Sep 25, 2006 · Supernova SNLS-03D3bb is more than twice as bright as most Type Ia supernovae but has much less kinetic energy, and appears to be half again as massive as a …

Sep 29, 2006 · Howell et al. have reported the discovery of SN Ia SN 2003fg (SNLS-03D3bb) and conclude that SN 2003fg is very likely a super-Chandrasekhar-mass SN Ia perhaps with a …

SNLS-03D3bb (SN 2003fg) was discovered on April 24, 2003 (UT) as part of the Supernova Legacy Survey (SNLS). Its redshift is z = 0.2440 ± 0.0003, determined from host galaxy [OII],

SN Location SNLS-03D3bb is located at RA: 14:16:18.920 Dec: +52:14:53.66 (J2000) in the D3 (extended Groth Strip) field of the Supernova Legacy Survey (SNLS), located in a satellite …

Sep 21, 2006 · Here we show that the high redshift supernova SNLS-03D3bb has an exceptionally high luminosity and low kinetic energy that both imply a super-Chandrasekhar …

SNLS-03D3bb is the first high redshift (z=0.244) Type Ia supernova (SN Ia) with no obvious analogue at low redshift. It is one of the brightest SNe ever observed, with M<SUB>V</SUB>= …

Feb 1, 2006 · Here we show that the high-redshift supernova SNLS-03D3bb has an exceptionally high luminosity and low kinetic energy that both imply a super-Chandrasekhar mass progenitor.

Jan 1, 1993 · Here we show that the high redshift supernova SNLS-03D3bb has an exceptionally high luminosity and low kinetic energy that both imply a super-Chandrasekhar mass progenitor.

Here we show that the high-redshift supernova SNLS-03D3bb has an exceptionally high luminosity and low kinetic energy that both imply a super-Chandrasekhar-mass progenitor.

Here we show that the high redshift supernova SNLS-03D3bb has an exceptionally high luminosity and low kinetic energy that both imply a super-Chandrasekhar mass progenitor.

redshift supernova SNLS-03D3bb has an exceptionally high luminosity and low kinetic energy that both imply a super-Chandrasekhar-mass progenitor. Super-Chandrasekhar-mass

Sep 21, 2006 · Nugent’s research enabled scientists to distinguish SNLS-03D3bb from previously known Type Ia supernovae. While working at NERSC, Nugent developed an algorithm that …

Howell et al. have reported the discovery of SN Ia SN 2003fg (SNLS-03D3bb) and conclude that SN 2003fg is very likely a super-Chandrasekhar-mass SN Ia perhaps with a mass ∼ 2 M⊙. …

Sep 20, 2006 · University of Toronto postdoctoral researcher Andy Howell, lead author of the study, identified a Type Ia supernova named SNLS-03D3bb in a distant galaxy 4 billion light …

Sep 20, 2006 · Supernova SNLS-03D3bb is more than twice as bright as most Type Ia supernovae but has much less kinetic energy, and appears to be half again as massive as a …

In April 2003, the Supernova Legacy Survey observed a type Ia supernova, designated SNLS-03D3bb, in a galaxy approximately 4 billion light years away. According to a group of …