activity
19942023
most citedThe Simons Observatory: Science goals and forecasts

1.5k citations · 15.6k across the 200 of their papers we have counts for

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Showing 2009Show all

13 papers · 1 filter

astro-ph.IM2009★ 5 cited

A Vigorous Explorer Program

Martin Elvis, Matthew Beasley, Roger Brissenden +47

Explorers have made breakthroughs in many fields of astrophysics. The science from both these missions contributed to three Nobel Prizes - Giacconi (2002), Mather, and Smoot (2006)…

astro-ph.GA2009★ 29 cited

The BLAST Survey of the Vela Molecular Cloud: Physical Properties of the Dense Cores in Vela-D

Luca Olmi, Peter A. R. Ade, Daniel Angles-Alcazar +34

The Balloon-borne Large-Aperture Submillimeter Telescope (BLAST) carried out a 250, 350 and 500 micron survey of the galactic plane encompassing the Vela Molecular Ridge, with the…

astro-ph.CO2009★ 153 cited

BLAST: the far-infrared/radio correlation in distant galaxies

R. J. Ivison, David M. Alexander, Andy D. Biggs +32

We investigate the correlation between far-infrared (FIR) and radio luminosities in distant galaxies, a lynchpin of modern astronomy. We use data from the Balloon-borne Large Apert…

astro-ph.GA2009★ 25 cited

BLAST05: Power Spectra of Bright Galactic Cirrus at Submillimeter Wavelengths

Arabindo Roy, Peter A. R. Ade, James J. Bock +25

We report multi-wavelength power spectra of diffuse Galactic dust emission from BLAST observations at 250, 350, and 500 microns in Galactic Plane fields in Cygnus X and Aquila. The…

astro-ph.CO2009★ 21 cited

The BLAST 250-micron selected galaxy population in GOODS-South

J. S. Dunlop, P. A. R. Ade, J. J. Bock +33

We identify and investigate the nature of the 20 brightest 250-micron sources detected by the BLAST within the central 150 sq. arcmin of the GOODS-South field. Aided by the availab…

astro-ph.CO2009★ 46 cited

Lensing Magnification: Implications for Counts of Submillimeter Galaxies and SZ Clusters

Marcos Lima, Bhuvnesh Jain, Mark Devlin

We study lensing magnification of source galaxies by intervening galaxy groups and clusters using a halo model. Halos are modeled with truncated NFW profiles with ellipticity added…