activity
20002010
most citedHigh Resolution Rotation Curves of Low Surface Brightness Galaxies

195 citations · 758 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.GA2010★ 179 cited

Mid-Infrared Spectral Diagnostics of Luminous Infrared Galaxies

A. O. Petric, L. Armus, J. Howell +22

We present a statistical analysis of the mid-infrared (MIR) spectra of 248 luminous infrared (IR) galaxies (LIRGs) which comprise the Great Observatories All-sky LIRG Survey (GOALS…

astro-ph.CO2010★ 129 cited

Galaxy and Mass Assembly (GAMA): FUV, NUV, ugrizYJHK Petrosian, Kron and Sèrsic photometry

David T. Hill, Lee S. Kelvin, Simon P. Driver +33

In order to generate credible 0.1-2 μm SEDs, the GAMA project requires many Gigabytes of imaging data from a number of instruments to be re-processed into a standard format. In thi…

astro-ph.CO2009★ 123 cited

The Carnegie Supernova Project: First Near-Infrared Hubble Diagram to z~0.7

Wendy L. Freedman, Christopher R. Burns, M. M. Phillips +37

The Carnegie Supernova Project (CSP) is designed to measure the luminosity distance for Type Ia supernovae (SNe Ia) as a function of redshift, and to set observational constraints…

astro-ph2008★ 25 cited

A Survey for Fast Transients in the Fornax Cluster of Galaxies

A. Rau, E. O. Ofek, S. R. Kulkarni +3

The luminosity gap between novae (M_R < -10) and supernovae (M_R > -14) is well known since the pioneering research of Zwicky and Hubble. Nearby galaxy clusters and concentrations…

astro-ph2004★ 107 cited

Number Counts of GALEX Sources in FUV (1530A) and NUV (2310A) Bands

C. Kevin Xu, Jose Donas, Stephane Arnouts +21

Number Counts of galaxies in two GALEX bands (FUV: 1530A and NUV: 2310A, both in AB magnitudes) are reported. They provide for the first time in the literature homogeneously calibr…

astro-ph2000★ 195 cited

High Resolution Rotation Curves of Low Surface Brightness Galaxies

R. A. Swaters, B. F. Madore, M. Trewhella

High resolution Halpha rotation curves are presented for five low surface brightness galaxies. These Halpha rotation curves have shapes different from those previously derived from…