activity
19942011
most citedOptical Design of the Atacama Cosmology Telescope and the Millimeter Bolometric Array Camera

188 citations · 895 across the 18 of their papers we have counts for

collaborators

18 papers

astro-ph.CO2011★ 165 cited

Evidence for dark energy from the cosmic microwave background alone using the Atacama Cosmology Telescope lensing measurements

Blake D. Sherwin, Joanna Dunkley, Sudeep Das +35

For the first time, measurements of the cosmic microwave background radiation (CMB) alone favor cosmologies with dark energy over models without dark energy at a 3.2-sigma l…

astro-ph.CO2011

New High-Resolution Sunyaev-Zel'dovich Observations with GBT+MUSTANG

Tony Mroczkowski, Mark Devlin, Simon Dicker +7

We present recent high angular resolution (9") Sunyaev-Zel'dovich effect (SZE) observations with MUSTANG, a 90-GHz bolometric receiver on the Green Bank Telescope. MUSTANG has now…

astro-ph.CO2009★ 184 cited

Over half of the far-infrared background light comes from galaxies at z >= 1.2

Mark J. Devlin, Peter A. R. Ade, Itziar Aretxaga +26

Submillimetre surveys during the past decade have discovered a population of luminous, high-redshift, dusty starburst galaxies. In the redshift range 1 <= z <= 4, these massive sub…

astro-ph.CO2009★ 45 cited

Radio and mid-infrared identification of BLAST source counterparts in the Chandra Deep Field South

Simon Dye, Peter A. R. Ade, James J. Bock +28

We have identified radio and/or mid-infrared counterparts to 198 out of 350 sources detected at >=5 sigma over ~ 9 square degrees centered on the Chandra Deep Field South (CDFS) by…

astro-ph.CO2009★ 15 cited

A Bright Submillimeter Source in the Bullet Cluster (1E0657--56) Field Detected with BLAST

Marie Rex, Peter A. R. Ade, Itziar Aretxaga +26

We present the 250, 350, and 500 micron detection of bright submillimeter emission in the direction of the Bullet Cluster measured by the Balloon-borne Large Aperture Submillimeter…

astro-ph.CO2009★ 4 cited

Observing the Evolution of the Universe

James Aguirre, Alexandre Amblard, Amjad Ashoorioon +172

How did the universe evolve? The fine angular scale (l>1000) temperature and polarization anisotropies in the CMB are a Rosetta stone for understanding the evolution of the univers…