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J/AJ/122/2205       HDF-South K photometric redshift catalog (Rudnick+, 2001)

A K-band-selected photometric redshift catalog in the Hubble Deep Field South: sampling the rest-frame V band to z=3. Rudnick G., Franx M., Rix H.-W., Moorwood A., Kuijken K., van Starkenburg L., van der Werf P., Rottgering H., van Dokkum P., Labbe I. <Astron. J. 122, 2205 (2001)> =2001AJ....122.2205R
ADC_Keywords: Galaxy catalogs; Photometry, infrared; Photometry, UBV; Redshifts Keywords: galaxies: distances and redshifts - galaxies: evolution - galaxies: formation - galaxies: high-redshift - galaxies: photometry Abstract: We present the first results from the Faint Infra-Red Extragalactic Survey of the Hubble Deep Field South (HDF-S). Using a combination of deep near-infrared (NIR) data obtained with the Infrared Spectrograph and Array Camera at the VLT and the WFPC2 Hubble Space Telescope data, we construct a K-band-selected sample which is 50% and 90% complete for Ks,AB≤23.5 and Ks,AB≤22.0, respectively, where the magnitudes are measured over a 2.0" diameter aperture. For z≤3, our selection by the K-band flux chooses galaxies based on wavelengths redder than the rest-frame V band, and so selects them in a way that is less dependent on their current star formation rates than selection in the rest-frame UV. File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table1.dat 103 136 Photometric Catalog table3.dat 109 136 Photometric Redshift Catalog
See also: J/A+AS/145/111 : HDF-South catalogue of galaxies (Volonteri+, 2000) J/AJ/119/486 : HDF-South: STIS imaging (Gardner+, 2000) J/AJ/120/2747 : HDF-South WFPC2 observations (Casertano+, 2000) J/AJ/122/2190 : HDF-South multicolor observations (Vanzella+, 2001) Byte-by-byte Description of file: table1.dat
Bytes Format Units Label Explanations
1- 9 A9 --- [RFR2001] Object identification 11- 15 F5.1 10-34W/m2/Hz F300W The WFPC2 F300W (U) filter flux (1) 17- 19 F3.1 10-34W/m2/Hz e_F300W Uncertainty in F300W 21- 25 F5.1 10-34W/m2/Hz F450W The WFPC2 F450W (B) filter flux (1) 27- 29 F3.1 10-34W/m2/Hz e_F450W Uncertainty in F450W 31- 36 F6.1 10-34W/m2/Hz F606W The WFPC2 F606W (V) filter flux (1) 38- 40 F3.1 10-34W/m2/Hz e_F606W Uncertainty in F606W 42- 47 F6.1 10-34W/m2/Hz F814W The WFPC2 F814W (I) filter flux (1) 49- 51 F3.1 10-34W/m2/Hz e_F814W Uncertainty in F814W 53- 58 F6.1 10-34W/m2/Hz Jflux The Js band (1.24±0.16um) flux (1) 60- 63 F4.1 10-34W/m2/Hz e_Jflux Uncertainty in Jflux 65- 71 F7.1 10-34W/m2/Hz Hflux The H band (1.65±0.30um) flux (1) 73- 76 F4.1 10-34W/m2/Hz e_Hflux Uncertainty in Hflux 78- 84 F7.1 10-34W/m2/Hz Kflux The Ks band (2.16±0.27um) flux (1) 86- 89 F4.1 10-34W/m2/Hz e_Kflux Uncertainty in Kflux 91- 97 F7.1 10-34W/m2/Hz Ktot The total Ks flux (2) 99-102 F4.1 10-34W/m2/Hz e_Ktot Uncertainty in Ktot
Note (1): In units of 10-31ergs/cm2/s/Hz. Fluxes measured over a 2.0" diameter aperture. Note (2): In units of 10-31ergs/cm2/s/Hz. The "AUTO" flux from SExtractor with a minimum 2" diameter aperture.
Byte-by-byte Description of file: table3.dat
Bytes Format Units Label Explanations
1- 9 A9 --- [RFR2001] Object identification 11 A1 --- f_[RFR2001] [b] Flag on ID (1) 13- 14 I2 h RAh Right Ascension (J2000) 16- 17 I2 min RAm Right Ascension (J2000) 19- 23 F5.2 s RAs Right Ascension (J2000) 25 A1 --- DE- Declination sign (J2000) 26- 27 I2 deg DEd Declination (J2000) 29- 30 I2 arcmin DEm Declination (J2000) 32- 35 F4.1 arcsec DEs Declination (J2000) 37- 40 F4.2 --- z Photometric redshift 42- 45 F4.2 --- E_z Upper error in z 47- 50 F4.2 --- e_z Lower error in z 52 A1 --- f_z [a] Flag on z (2) 54- 58 F5.2 10+10solLum ULum Rest frame U band luminosity 60- 64 F5.2 10+10solLum E_ULum Upper error in ULum 66- 70 F5.2 10+10solLum e_ULum Lower error in ULum 72- 76 F5.2 10+10solLum BLum Rest frame Bband luminosity 78- 81 F4.2 10+10solLum E_BLum Upper error in BLum 83- 87 F5.2 10+10solLum e_BLum Lower error in BLum 89- 93 F5.2 10+10solLum VLum Rest frame V band luminosity 95- 98 F4.2 10+10solLum E_VLum Upper error in VLum 100-104 F5.2 10+10solLum e_VLum Lower error in VLum
Note (1): Indicates that the photometric redshift may be discrepant. Note (2): Indicates ≥1% of Monte-Carlo realizations have z more than unity away from the photometric redshift.
History: From electronic version of the journal
(End) Greg Schwarz [AAS], Patricia Bauer [CDS] 14-Jan-2002
The document above follows the rules of the Standard Description for Astronomical Catalogues.From this documentation it is possible to generate f77 program to load files into arrays or line by line

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