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dc.contributor.authorCoppin, Kristenen_US
dc.contributor.authorHalpern, Marken_US
dc.contributor.authorScott, Douglasen_US
dc.contributor.authorBorys, Colinen_US
dc.contributor.authorChapman, Scotten_US
dc.date.accessioned2014-03-12T19:20:49Z
dc.date.available2014-03-12T19:20:49Z
dc.date.issued2005-03en_US
dc.identifier.citationCoppin, Kristen, Mark Halpern, Douglas Scott, Colin Borys, et al. 2005. "An 850-micron SCUBA map of the Groth Strip and reliable source extraction." Monthly Notices of the Royal Astronomical Society 357(3): 1022-1028en_US
dc.identifier.issn0035-8711en_US
dc.identifier.urihttp://dx.doi.org/10.1111/j.1365-2966.2005.08723.xen_US
dc.identifier.urihttp://hdl.handle.net/10222/45285
dc.description.abstractWe present an 850-micron map and list of candidate sources in a 70 arcmin^2 sub-area of the Groth Strip observed using SCUBA. We initially detect 7 candidate sources with signal-to-noise ratios (SNRs) between 3.0 and 3.5 and 4 candidate sources with SNR > 3.5. Simulations suggest that on average in a map this size one expects 1.6 false positive sources for SNR > 3.5 and 4.5 for 3 3.5 which has a reasonable chance of being real.en_US
dc.titleAn 850-micron SCUBA map of the Groth Strip and reliable source extractionen_US
dc.title.alternativeMonthly Notices of the Royal Astronomical Societyen_US
dc.typearticleen_US
dc.identifier.volume357en_US
dc.identifier.issue3en_US
dc.identifier.startpage1022en_US
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