activity
19972022
most citedThe Supernova Legacy Survey: Measurement of Omega_M, Omega_Lambda and w from the First Year Data Set

2.4k citations · 5.9k across the 26 of their papers we have counts for

collaborators

26 papers

astro-ph.GA2022

New limits from microlensing on Galactic Black Holes in the mass range

T. Blaineau, M. Moniez, C. Afonso +17

We have searched for long duration microlensing events originating from intermediate mass Black Holes (BH) in the halo of the Milky Way, using archival data from EROS-2 and MACHO p…

astro-ph.CO2012★ 86 cited

Evolution in the Volumetric Type Ia Supernova Rate from the Supernova Legacy Survey

K. Perrett, M. Sullivan, A. Conley +23

We present a measurement of the volumetric Type Ia supernova (SN Ia) rate (SNR_Ia) as a function of redshift for the first four years of data from the Canada-France-Hawaii Telescop…

astro-ph.CO2011★ 51 cited

21 cm observation of LSS at z~1 Instrument sensitivity and foreground subtraction

R. Ansari, J. E. Campagne, P. Colom +6

Large Scale Structures (LSS) in the universe can be traced using the neutral atomic hydrogen HI through its 21cm emission. Such a 3D matter distribution map can be used to test the…

astro-ph.CO2011★ 78 cited

Constraining Type Ia Supernovae progenitors from three years of SNLS data

F. B. Bianco, D. A. Howell, M. Sullivan +20

While it is generally accepted that Type Ia supernovae are the result of the explosion of a carbon-oxygen White Dwarf accreting mass in a binary system, the details of their genesi…

astro-ph.CO2010★ 147 cited

The Fine-Scale Structure of the neutral Interstellar Medium in nearby Galaxies

I. Bagetakos, E. Brinks, F. Walter +5

We present an analysis of the properties of HI holes detected in 20 galaxies that are part of "The HI Nearby Galaxy Survey" (THINGS). We detected more than 1000 holes in total in t…

astro-ph.CO2009★ 2 cited

QSO Selection and Photometric Redshifts with Neural Networks

Ch. Yeche, P. Petitjean, J. Rich +9

Baryonic Acoustic Oscillations (BAO) and their effects on the matter power spectrum can be studied by using the Lyman-alpha absorption signature of the matter density field along q…