Estimating photometric redshifts with artificial neural networks
dc.contributor.author | Firth, Andrew E. | en_US |
dc.contributor.author | Lahav, Ofer | en_US |
dc.contributor.author | Somerville, Rachel S. | en_US |
dc.date.accessioned | 2010-06-01T21:17:23Z | |
dc.date.available | 2010-06-01T21:17:23Z | |
dc.date.issued | 2003-03 | en_US |
dc.identifier.citation | Firth, Andrew E.; Lahav, Ofer; Somerville, Rachel S. (2003). "Estimating photometric redshifts with artificial neural networks." Monthly Notices of the Royal Astronomical Society 339(4): 1195-1202. <http://hdl.handle.net/2027.42/74360> | en_US |
dc.identifier.issn | 0035-8711 | en_US |
dc.identifier.issn | 1365-2966 | en_US |
dc.identifier.uri | https://hdl.handle.net/2027.42/74360 | |
dc.description.abstract | A new approach to estimating photometric redshifts – using artificial neural networks (ANNs) – is investigated. Unlike the standard template-fitting photometric redshift technique, a large spectroscopically-identified training set is required but, where one is available, ANNs produce photometric redshift accuracies at least as good as and often better than the template-fitting method. The Bayesian priors on the underlying redshift distribution are automatically taken into account. Furthermore, inputs other than galaxy colours – such as morphology, angular size and surface brightness – may be easily incorporated, and their utility assessed. Different ANN architectures are tested on a semi-analytic model galaxy catalogue and the results are compared with the template-fitting method. Finally, the method is tested on a sample of ∼20 000 galaxies from the Sloan Digital Sky Survey. The rms redshift error in the range z ≲ 0.35 is Σ z ∼ 0.021 . | en_US |
dc.format.extent | 503472 bytes | |
dc.format.extent | 3109 bytes | |
dc.format.mimetype | application/pdf | |
dc.format.mimetype | text/plain | |
dc.publisher | Blackwell Science Ltd | en_US |
dc.rights | RAS | en_US |
dc.subject.other | Methods: Data Analysis | en_US |
dc.subject.other | Surveys | en_US |
dc.subject.other | Galaxies: Distances and Redshifts | en_US |
dc.title | Estimating photometric redshifts with artificial neural networks | en_US |
dc.type | Article | en_US |
dc.subject.hlbsecondlevel | Astronomy | en_US |
dc.subject.hlbtoplevel | Science | en_US |
dc.description.peerreviewed | Peer Reviewed | en_US |
dc.contributor.affiliationum | Department of Astronomy, University of Michigan, Ann Arbor, MI 48109-1090, USA | en_US |
dc.contributor.affiliationother | Institute of Astronomy, University of Cambridge, Cambridge CB3 0HA | en_US |
dc.description.bitstreamurl | http://deepblue.lib.umich.edu/bitstream/2027.42/74360/1/j.1365-8711.2003.06271.x.pdf | |
dc.identifier.doi | 10.1046/j.1365-8711.2003.06271.x | en_US |
dc.identifier.source | Monthly Notices of the Royal Astronomical Society | en_US |
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