activity
19952012
most citedThe Infrared Array Camera (IRAC) for the Spitzer Space Telescope

3.3k citations · 8.8k across the 53 of their papers we have counts for

collaborators

53 papers

astro-ph.CO2012★ 229 cited

CfA4: Light Curves for 94 Type Ia Supernovae

Malcolm Hicken, Peter Challis, Robert P. Kirshner +36

We present multi-band optical photometry of 94 spectroscopically-confirmed Type Ia supernovae (SN Ia) in the redshift range 0.0055 to 0.073, obtained between 2006 and 2011. There a…

astro-ph.CO2009★ 524 cited

CfA3: 185 Type Ia Supernova Light Curves from the CfA

Malcolm Hicken, Peter Challis, Saurabh Jha +5

We present multi-band photometry of 185 type-Ia supernovae (SN Ia), with over 11500 observations. These were acquired between 2001 and 2008 at the F. L. Whipple Observatory of the…

astro-ph2008★ 16 cited

A Direct Measurement of the Dust Extinction Curve in an Intermediate-Redshift Galaxy

Kevin Heng, Davide Lazzati, Rosalba Perna +5

We present a proof-of-concept study that dust extinction curves can be extracted from the infrared (IR), optical, ultraviolet (UV) and X-ray afterglow observations of GRBs without…

astro-ph2008★ 39 cited

The Mid-Infrared Properties of X-ray Sources

V. Gorjian, M. Brodwin, C. S. Kochanek +16

We combine the results of the Spitzer IRAC Shallow Survey and the Chandra XBootes Survey of the 8.5 square degrees Bootes field of the NOAO Deep Wide- Field Survey to produce the l…

astro-ph2007★ 186 cited

Long Gamma-Ray Bursts and Type Ic Core Collapse Supernovae Have Similar Locations in Hosts

P. L. Kelly, R. P. Kirshner, M. Pahre

When the afterglow fades at the site of a long-duration gamma-ray burst (LGRB), Type Ic supernovae (SN Ic) are the only type of core collapse supernova observed. Recent work found…

astro-ph2007★ 59 cited

The Local Galaxy 8 micron Luminosity Function

J. -S. Huang, M. L. N. Ashby, P. Barmby +18

A SST survey in the NOAO Deep-Wide Field in Boötes provides a complete, 8-micron-selected sample of galaxies to a limiting (Vega) magnitude of 13.5. In the 6.88 deg field sampl…