activity
20082019
most citedThe Carnegie Supernova Project: Light Curve Fitting with SNooPy

314 citations · 649 across the 7 of their papers we have counts for

collaborators

7 papers

astro-ph.GA2019★ 155 cited

Mapping the Stellar Halo with the H3 Spectroscopic Survey

Charlie Conroy, Ana Bonaca, Phillip Cargile +8

Modern theories of galaxy formation predict that the Galactic stellar halo was hierarchically assembled from the accretion and disruption of smaller systems. This hierarchical asse…

astro-ph.CO2012★ 64 cited

The Standardizability of Type Ia Supernovae in the Near-Infrared: Evidence for a Peak Luminosity-Decline Rate Relation in the Near-Infrared

ShiAnne Kattner, Douglas C. Leonard, Christopher R. Burns +9

We analyze the standardizability of Type Ia supernovae (SNe Ia) in the near-infrared (NIR) by investigating the correlation between observed peak NIR absolute magnitude and post-ma…

astro-ph.CO2010★ 314 cited

The Carnegie Supernova Project: Light Curve Fitting with SNooPy

Christopher R. Burns, Maximilian Stritzinger, M. M. Phillips +13

In providing an independent measure of the expansion history of the Universe, the Carnegie Supernova Project (CSP) has observed 71 high-z Type Ia supernovae (SNe Ia) in the near-in…

astro-ph.CO2010★ 98 cited

The Distance to NGC 1316 (Fornax A) From Observations of Four Type Ia Supernovae

Maximilian Stritzinger, Chris Burns, Mark Phillips +13

The giant elliptical galaxy NGC 1316 (Fornax A) is a well-studied member of the Fornax Cluster and a prolific producer of Type Ia supernovae, having hosted four observed events sin…

astro-ph.CO2010★ 3 cited

The Wyoming Survey for H-alpha. III. A Multi-wavelength Look at Attenuation by Dust in Galaxies out to z~0.4

Carolynn A. Moore, Daniel A. Dale, Rebecca J. Barlow +6

We report results from the Wyoming Survey for H-alpha (WySH), a comprehensive four-square degree survey to probe the evolution of star-forming galaxies over the latter half of the…

astro-ph2008★ 6 cited

Time-Resolved Photometry of the Optical Counterpart of Swift J2319.4+2619

A. W. Shafter, J. R. A. Davenport, T. Güth +3

Time-resolved CCD photometry is presented of the V~17 optical counterpart of the newly-discovered, hard-X-ray-emitting polar Swift J2619.4+2619. A total of ~20 hr of data obtained…