142 citations · 327 across the 7 of their papers we have counts for
7 papers
The Spatial Distribution of Type Ia Supernovae within Host Galaxies
Christopher Pritchet, Karun Thanjavur, Connor Bottrell +1
We study how type Ia supernovae (SNe Ia) are spatially distributed within their host galaxies, using data taken from the Sloan Digital Sky Survey (SDSS). This paper specifically te…
Photometric classification of type Ia supernovae in the SuperNova Legacy Survey with supervised learning
A. Möller, V. Ruhlmann-Kleider, C. Leloup +6
In the era of large astronomical surveys, photometric classification of supernovae (SNe) has become an important research field due to limited spectroscopic resources for candidate…
Evidence for Type Ia Supernova Diversity from Ultraviolet Observations with the Hubble Space Telescope
Xiaofeng Wang, Lifan Wang, Alexei V. Filippenko +93
We present ultraviolet (UV) spectroscopy and photometry of four Type Ia supernovae (SNe 2004dt, 2004ef, 2005M, and 2005cf) obtained with the UV prism of the Advanced Camera for Sur…
Very Red and Extremely Red Galaxies in the Fields of z ~ 1.5 Radio-Loud Quasars
Patrick B. Hall, Marcin Sawicki, Paul Martini +7
We previously identified an excess of mostly red galaxies around 31 RLQs at z=1-2. These fields have an ERO (extremely red object, R-K>6) density 2.7 times higher than the field. A…
The Evolution of Blue Stragglers Formed Via Stellar Collisions
J. A. Ouellette, C. J. Pritchet
We have used the results of recent smoothed particle hydrodynamic simulations of colliding stars to create models appropriate for input into a stellar evolution code. In evolving t…
The CNOC Cluster Survey: Omega, sigma_8, Phi(L,z) Results, and Prospects for Lambda Measurement
R. G. Carlberg, H. K. C. Yee, H. Lin +14
Rich galaxy clusters are powerful probes of both cosmological and galaxy evolution parameters. The CNOC cluster survey was primarily designed to distinguish between Omega=1 and Ome…
Close Pairs of Field Galaxies in the CNOC1 Redshift Survey
D. R. Patton, C. J. Pritchet, H. K. C. Yee +2
A redshift sample of 545 field galaxies is used to examine how the galaxy merger rate changes with redshift, and how mergers affect the observed properties of galaxies in close pai…