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- W2065439923 abstract "We have undertaken a deep (sigma~1.1 mJy) 1.1-mm survey of the z=0.54 cluster MS 0451.6-0305 using the AzTEC camera on the James Clerk Maxwell Telescope. We detect 36 sources with S/N>3.5 in the central 0.10 deg^2 and present the AzTEC map, catalogue and number counts. We identify counterparts to 18 sources (50%) using radio, mid-infrared, Spitzer IRAC and Submillimeter Array data. Optical, near- and mid-infrared spectral energy distributions are compiled for the 14 of these galaxies with detectable counterparts, which are expected to contain all likely cluster members. We then use photometric redshifts and colour selection to separate background galaxies from potential cluster members and test the reliability of this technique using archival observations of submillimetre galaxies. We find two potential MS 0451-03 members, which, if they are both cluster galaxies have a total star-formation rate (SFR) of ~100 solar masses per year -- a significant fraction of the combined SFR of all the other galaxies in MS 0451-03. We also examine the stacked rest-frame mid-infrared, millimetre and radio emission of cluster members below our AzTEC detection limit and find that the SFRs of mid-IR selected galaxies in the cluster and redshift-matched field populations are comparable. In contrast, the average SFR of the morphologically classified late-type cluster population is ~3 times less than the corresponding redshift-matched field galaxies. This suggests that these galaxies may be in the process of being transformed on the red-sequence by the cluster environment. Our survey demonstrates that although the environment of MS 0451-03 appears to suppress star-formation in late-type galaxies, it can support active, dust-obscured mid-IR galaxies and potentially millimetre-detected LIRGs." @default.
- W2065439923 created "2016-06-24" @default.
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- W2065439923 date "2010-02-01" @default.
- W2065439923 modified "2023-09-25" @default.
- W2065439923 title "An AzTEC 1.1-mm survey for ULIRGs in the field of the Galaxy Cluster MS 0451.6−0305" @default.
- W2065439923 cites W1841113251 @default.
- W2065439923 cites W1906850129 @default.
- W2065439923 cites W1914598719 @default.
- W2065439923 cites W1917496003 @default.
- W2065439923 cites W1968661712 @default.
- W2065439923 cites W1970517322 @default.
- W2065439923 cites W1971014996 @default.
- W2065439923 cites W1973808059 @default.
- W2065439923 cites W1982051859 @default.
- W2065439923 cites W1983332987 @default.
- W2065439923 cites W1994931053 @default.
- W2065439923 cites W1996393524 @default.
- W2065439923 cites W1998277739 @default.
- W2065439923 cites W2002391812 @default.
- W2065439923 cites W2005774056 @default.
- W2065439923 cites W2006029146 @default.
- W2065439923 cites W2006676156 @default.
- W2065439923 cites W2007741717 @default.
- W2065439923 cites W2017100570 @default.
- W2065439923 cites W2017569741 @default.
- W2065439923 cites W2029438261 @default.
- W2065439923 cites W2030950885 @default.
- W2065439923 cites W2036453346 @default.
- W2065439923 cites W2043533977 @default.
- W2065439923 cites W2048758550 @default.
- W2065439923 cites W2049531400 @default.
- W2065439923 cites W2055686415 @default.
- W2065439923 cites W2059474548 @default.
- W2065439923 cites W2060792137 @default.
- W2065439923 cites W2063734901 @default.
- W2065439923 cites W2070952256 @default.
- W2065439923 cites W2073925265 @default.
- W2065439923 cites W2080291289 @default.
- W2065439923 cites W2099045931 @default.
- W2065439923 cites W2105847337 @default.
- W2065439923 cites W2106695331 @default.
- W2065439923 cites W2110294314 @default.
- W2065439923 cites W2116466430 @default.
- W2065439923 cites W2117357987 @default.
- W2065439923 cites W2119405390 @default.
- W2065439923 cites W2120875714 @default.
- W2065439923 cites W2123494985 @default.
- W2065439923 cites W2123709957 @default.
- W2065439923 cites W2125179005 @default.
- W2065439923 cites W2125728999 @default.
- W2065439923 cites W2127377568 @default.
- W2065439923 cites W2138158862 @default.
- W2065439923 cites W2142238829 @default.
- W2065439923 cites W2147223987 @default.
- W2065439923 cites W2148837568 @default.
- W2065439923 cites W2150130981 @default.
- W2065439923 cites W2151062050 @default.
- W2065439923 cites W2162125418 @default.
- W2065439923 cites W2167262338 @default.
- W2065439923 cites W2168126149 @default.
- W2065439923 cites W2169330880 @default.
- W2065439923 cites W2171494255 @default.
- W2065439923 cites W2761493623 @default.
- W2065439923 cites W2963552953 @default.
- W2065439923 cites W3098160327 @default.
- W2065439923 cites W3099311826 @default.
- W2065439923 cites W3099333906 @default.
- W2065439923 cites W3099590139 @default.
- W2065439923 cites W3100967694 @default.
- W2065439923 cites W3102420486 @default.
- W2065439923 cites W3102713922 @default.
- W2065439923 cites W3103136267 @default.
- W2065439923 cites W3103136928 @default.
- W2065439923 cites W3103212644 @default.
- W2065439923 cites W3103281616 @default.
- W2065439923 cites W3104203777 @default.
- W2065439923 cites W3104805127 @default.
- W2065439923 cites W3106448032 @default.