activity
20052015
most citedThe Supernova Legacy Survey: Measurement of Omega_M, Omega_Lambda and w from the First Year Data Set

2.4k citations · 8.5k across the 18 of their papers we have counts for

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8 papers · 1 filter

astro-ph2008★ 2 cited

Initial Hubble Diagram Results from the Nearby Supernova Factory

S. Bailey, G. Aldering, P. Antilogus +22

The use of Type Ia supernovae as distance indicators led to the discovery of the accelerating expansion of the universe a decade ago. Now that large second generation surveys have…

astro-ph2008★ 39 cited

Type Ia Supernovae Rates and Galaxy Clustering from the CFHT Supernova Legacy Survey

M. L. Graham, C. J. Pritchet, M. Sullivan +25

The Canada-France-Hawaii Telescope Supernova Legacy Survey (SNLS) has created a large homogeneous database of intermediate redshift (0.2 < z < 1.0) type Ia supernovae (SNe Ia). The…

astro-ph2007★ 887 cited

SALT2: using distant supernovae to improve the use of Type Ia supernovae as distance indicators

J. Guy, P. Astier, S. Baumont +22

We present an empirical model of Type Ia supernovae spectro-photometric evolution with time. The model is built using a large data set including light-curves and spectra of both ne…

astro-ph2007★ 6 cited

The Supernova Type Ia Rate Evolution with SNLS

J. D. Neill, M. Sullivan, D. Balam +36

We present a progress report on a project to derive the evolution of the volumetric supernova Type Ia rate from the Supernova Legacy Survey. Our preliminary estimate of the rate ev…

astro-ph2006★ 107 cited

The Rise Time of Type Ia Supernovae from the Supernova Legacy Survey

A. Conley, D. A. Howell, A. Howes +24

We compare the rise times of nearby and distant Type Ia supernovae (SNe Ia) as a test for evolution using 73 high-redshift spectroscopically-confirmed SNe Ia from the first two yea…

astro-ph2006★ 562 cited

Rates and properties of type Ia supernovae as a function of mass and star-formation in their host galaxies

M. Sullivan, D. Le Borgne, C. J. Pritchet +27

(ABRIDGED) We show that Type Ia supernovae (SNe Ia) are formed within both very young and old stellar populations, with observed rates that depend on the stellar mass and mean star…