Radio and mid-IR counterpart of submm galaxies (Biggs+, 2011)

Details Radio and mid-IR counterpart of submm galaxies (Biggs+, 2011) Radio and mid-IR counterpart of submm galaxies (Biggs+, 2011)

Nov 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011ycat..74132314b&link_type=abstract

VizieR On-line Data Catalog: J/MNRAS/413/2314. Originally published in: 2011MNRAS.413.2314B

Physics

Millimetric/Submm Sources, Galaxies: Ir, Galaxies: Radio

Scientific paper

We present radio and infrared (3.6-24um) counterparts to submillimetre galaxies (SMGs) detected in the Extended Chandra Deep Field-South with the Large APEX Bolometer Camera (LABOCA) 870um bolometer camera on the 12m Atacama Pathfinder Experiment. Using the Very Large Array at .4GHz and Spitzer, we have identified secure counterparts to 79 of the 126 SMGs [signal-to-noise ratio (S/N)>3.7, S870>4.4mJy] in the field, 62 via their radio and/or 24um emission, the remainder using a colour-flux cut on Infrared Array Camera 3.6um and 5.8um sources chosen to maximize the number of secure, coincident radio and 24um counterparts.
(4 data files).

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