Extremely red objects in the UKIDSS Ultra Deep Survey Early Data Release

We construct a sample of extremely red objects (EROs) within the UKIDSS Ultra Deep Survey by combining the Early Data Release with optical data from the Subaru/XMM-Newton Deep Field. We find a total of 3715 objects over 2013 sq. arcmin with R-K>5.3 and K<=20.3, which is a higher surfac...

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Main Authors: Simpson, C, Almaini, O, Cirasuolo, M, Dunlop, J, Foucaud, S, Hirst, P, Ivison, R, Page, M, Rawlings, S, Sekiguchi, K, Smail, I, Watson, M
Format: Journal article
Published: 2006
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author Simpson, C
Almaini, O
Cirasuolo, M
Dunlop, J
Foucaud, S
Hirst, P
Ivison, R
Page, M
Rawlings, S
Sekiguchi, K
Smail, I
Watson, M
author_facet Simpson, C
Almaini, O
Cirasuolo, M
Dunlop, J
Foucaud, S
Hirst, P
Ivison, R
Page, M
Rawlings, S
Sekiguchi, K
Smail, I
Watson, M
author_sort Simpson, C
collection OXFORD
description We construct a sample of extremely red objects (EROs) within the UKIDSS Ultra Deep Survey by combining the Early Data Release with optical data from the Subaru/XMM-Newton Deep Field. We find a total of 3715 objects over 2013 sq. arcmin with R-K>5.3 and K<=20.3, which is a higher surface density than found by previous studies. This is partly due to our ability to use a small aperture in which to measure colours, but is also the result of a genuine overdensity of objects compared to other fields. We separate our sample into passively-evolving and dusty star-forming galaxies using their RJK colours and investigate their radio properties using a deep radio map. The dusty population has a higher fraction of individually-detected radio sources and a higher mean radio flux density among the undetected objects, but the passive population has a higher fraction of bright radio sources, suggesting that AGNs are more prevalent among the passive ERO population.
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spelling oxford-uuid:78ea8f39-8928-428b-8703-50952dfc608b2022-03-26T20:33:47ZExtremely red objects in the UKIDSS Ultra Deep Survey Early Data ReleaseJournal articlehttp://purl.org/coar/resource_type/c_dcae04bcuuid:78ea8f39-8928-428b-8703-50952dfc608bSymplectic Elements at Oxford2006Simpson, CAlmaini, OCirasuolo, MDunlop, JFoucaud, SHirst, PIvison, RPage, MRawlings, SSekiguchi, KSmail, IWatson, MWe construct a sample of extremely red objects (EROs) within the UKIDSS Ultra Deep Survey by combining the Early Data Release with optical data from the Subaru/XMM-Newton Deep Field. We find a total of 3715 objects over 2013 sq. arcmin with R-K>5.3 and K<=20.3, which is a higher surface density than found by previous studies. This is partly due to our ability to use a small aperture in which to measure colours, but is also the result of a genuine overdensity of objects compared to other fields. We separate our sample into passively-evolving and dusty star-forming galaxies using their RJK colours and investigate their radio properties using a deep radio map. The dusty population has a higher fraction of individually-detected radio sources and a higher mean radio flux density among the undetected objects, but the passive population has a higher fraction of bright radio sources, suggesting that AGNs are more prevalent among the passive ERO population.
spellingShingle Simpson, C
Almaini, O
Cirasuolo, M
Dunlop, J
Foucaud, S
Hirst, P
Ivison, R
Page, M
Rawlings, S
Sekiguchi, K
Smail, I
Watson, M
Extremely red objects in the UKIDSS Ultra Deep Survey Early Data Release
title Extremely red objects in the UKIDSS Ultra Deep Survey Early Data Release
title_full Extremely red objects in the UKIDSS Ultra Deep Survey Early Data Release
title_fullStr Extremely red objects in the UKIDSS Ultra Deep Survey Early Data Release
title_full_unstemmed Extremely red objects in the UKIDSS Ultra Deep Survey Early Data Release
title_short Extremely red objects in the UKIDSS Ultra Deep Survey Early Data Release
title_sort extremely red objects in the ukidss ultra deep survey early data release
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