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19952009
most citedRates and properties of type Ia supernovae as a function of mass and star-formation in their host galaxies

562 citations · 2k across the 14 of their papers we have counts for

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Showing 2005Show all

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astro-ph2005

An Overview of Extremely Large Telescopes Projects

R. G. Carlberg

IAU Symposium 232 allows a snapshot of ELTs at a stage when design work in several critical mass projects has been seriously underway for two to three years. The status and som eof…

astro-ph2005

Photometric selection of high-redshift type Ia supernovae

M. Sullivan, D. A. Howell, K. Perrett +26

We present a method for selecting high-redshift type Ia supernovae (SNe Ia) located via rolling SN searches. The technique, using both color and magnitude information of events fro…

astro-ph2005

Gemini Spectroscopy of Supernovae from SNLS: Improving High Redshift SN Selection and Classification

D. A. Howell, M. Sullivan, K. Perrett +22

We present new techiques for improving the efficiency of supernova (SN) classification at high redshift using 64 candidates observed at Gemini North and South during the first year…

astro-ph2005

Mass-to-Light Ratios of Galaxy Groups from Weak Lensing

Laura C. Parker, Michael J. Hudson, Ray G. Carlberg +1

We present the findings of our weak lensing study of a sample of 116 CNOC2 galaxy groups. The lensing signal is used to estimate the mass-to-light ratio of these galaxy groups. The…

astro-ph2005

A Hubble Space Telescope Snapshot Survey of Dynamically Close Galaxy Pairs in the CNOC2 Redshift Survey

D. R. Patton, J. K. Grant, L. Simard +3

We compare the structural properties of two classes of galaxies at intermediate redshift: those in dynamically close galaxy pairs, and those which are isolated. Both samples are se…

astro-ph2005

Gemini Deep Deep Survey VI: Massive Hdelta-strong galaxies at z=1

Damien Le Borgne, Roberto Abraham, Kathryne Daniel +11

We show that there has been a dramatic decline in the abundance of massive galaxies with strong Hdelta stellar absorption lines from z=1.2 to the present. These ``Hdelta-strong'',…