activity
19952011
most citedThe Cosmic Microwave Background Spectrum from the Full COBE/FIRAS Data Set

1.7k citations · 4.6k across the 15 of their papers we have counts for

collaborators

15 papers

astro-ph.CO2011★ 54 cited

High Resolution XMM-Newton Spectroscopy of the Cooling Flow Cluster A3112

Esra Bulbul, Randall Smith, Adam Foster +4

We examine high signal to noise XMM-Newton European Photon Imaging Camera (EPIC) and Reflection Grating Spectrometer (RGS) observations to determine the physical characteristics of…

astro-ph.CO2009★ 2 cited

On the nature of the first galaxies selected at 350 microns

Sophia A. Khan, Pierre F. Chanial, S. P. Willner +18

[abridged] We present constraints on the nature of the first galaxies selected at 350 microns. The sample includes galaxies discovered in the deepest blank-field survey at 350 micr…

astro-ph2007★ 18 cited

First Constraints on Source Counts at 350 Microns

Sophia A. Khan, Richard A. Shafer, Stephen Serjeant +16

We have imaged a 6 arcminute region in the Boötes Deep Field using the 350 m-optimised second generation Submillimeter High Angular Resolution Camera (SHARC II), achie…

astro-ph2005★ 10 cited

On the discovery of the first 350 micron-selected galaxy

Sophia A. Khan, Richard A. Shafer, Dominic J. Benford +17

We report the detection of a 3.6sigma 350micron-selected source in the Bootes Deep Field. The source, the first Short-wavelength Submillimeter-selected Galaxy (SSG 1), was discover…

astro-ph2005★ 7 cited

Resolving IRAS 09111-1007 at 350 microns - a different path to ULIRG formation?

Sophia A. Khan, Dominic J. Benford, David L. Clements +3

We have resolved the ultraluminous infrared galaxy (ULIRG), IRAS 09111-1007, with the new 350 micron-optimised Second Generation Submillimeter High Angular Resolution Camera (SHARC…

astro-ph2002★ 68 cited

The X-ray Halo of GX 13+1

Randall K. Smith, Richard J. Edgar, Richard A. Shafer

We present observations of the X-ray halo around the LMXB GX 13+1 from the Chandra X-ray telescope. The halo is caused by scattering in interstellar dust grains, and we use it to d…