A Blind Test of Photometric Redshift Prediction

Results of a blind test of photometric redshift predictions against spectroscopic galaxy redshifts obtained in the Hubble Deep Field with the Keck Telescope are presented. The best photometric redshift schemes predict spectroscopic redshifts with a redshift accuracy of Delta z less than 0.1 for more...

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Veröffentlicht in:The Astronomical journal 1998-04, Vol.115 (4), p.1418-1422
Hauptverfasser: Hogg, David W, Cohen, Judith G, Blandford, Roger, Gwyn, Stephen D. J, Hartwick, F. D. A, Mobasher, B, Mazzei, Paula, Sawicki, Marcin, Lin, Huan, Yee, H. K. C, Connolly, Andrew J, Brunner, Robert J, Csabai, Istvan, Dickinson, Mark, SubbaRao, Mark U, Szalay, Alexander S, Fernández-Soto, Alberto, Lanzetta, Kenneth M, Yahil, Amos
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Sprache:eng
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Zusammenfassung:Results of a blind test of photometric redshift predictions against spectroscopic galaxy redshifts obtained in the Hubble Deep Field with the Keck Telescope are presented. The best photometric redshift schemes predict spectroscopic redshifts with a redshift accuracy of Delta z less than 0.1 for more than 68 percent of sources and with Delta z less than 0.3 for 100 percent, when single-feature spectroscopic redshifts are removed from consideration. This test shows that photometric redshift schemes work well, at least when the photometric data are of high quality and when the sources are at moderate redshifts. (Author)
ISSN:1538-3881
0004-6256
1538-3881
DOI:10.1086/300277