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J/ApJ/563/629 VIK' photometry and redshifts of galaxy clusters (Nelson+, 2001)
Cluster galaxy evolution from a new sample of galaxy clusters at 0.3<z<0.9. Nelson A.E., Gonzalez A.H., Zaritsky D., Dalcanton J.J. <Astrophys. J. 563, 629 (2001)> =2001ApJ...563..629N
ADC_Keywords: Clusters, galaxy ; Redshifts ; Photometry ; Photometry, infrared Keywords: galaxies: clusters: general - galaxies: evolution - galaxies: formation - galaxies: photometry - surveys Abstract: We analyze photometry and spectroscopy of a sample of 63 clusters at 0.3≤z≤0.9 drawn from the Las Campanas Distant Cluster Survey to empirically constrain models of cluster galaxy evolution. Our data originate from a variety of telescopes and instruments. The candidate galaxy clusters are identified using drift-scan images and techniques described briefly below for context but in full detail by Gonzalez et al. (2001, Cat. J/ApJS/137/117). File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table1.dat 73 75 Observations table2.dat 78 75 Redshift data
See also: VII/203 : Las Campanas Redshift Survey (Shectman+ 1996) J/AJ/119/2598 : u'g'r'i'z' photometry of LCRS galaxies (Sowards-Emmerd+ 2000) J/ApJS/123/41 : Radio galaxies in LCRS (Machalski+, 1999) J/ApJS/130/237 : LCRS loose groups of galaxies (Tucker+, 2000) J/ApJS/137/117 : Las Campanas Distant Cluster Survey (LCDCS) (Gonzales+, 2001) J/MNRAS/327/588 : Las Campanas/AAT Rich Cluster Survey - I (Pimbblet+, 2001) J/AN/321/101 : Compact groups of galaxies in LCRS (Allam+, 2000) Byte-by-byte Description of file: table1.dat
Bytes Format Units Label Explanations
1- 11 A11 --- Cluster Cluster designation 13- 14 I2 h RAh Right ascension (J2000.0) 16- 17 I2 min RAm Right ascension (J2000.0) 19- 23 F5.2 s RAs Right ascension (J2000.0) 25 A1 --- DE- Declination sign (J2000.0) 26- 27 I2 deg DEd Declination (J2000.0) 29- 30 I2 arcmin DEm Declination (J2000.0) 32- 35 F4.1 arcsec DEs Declination (J2000.0) 37- 39 I3 min TexpV ? Exposure time in V band 40 A1 --- r_TexpV [abcd] Telescope used for observations (1) 42- 44 F3.1 arcsec SeeingV ? Seeing in V band 46- 48 I3 min TexpI ? Exposure time in I band 49 A1 --- r_TexpI [abcd] Telescope used for observations (1) 51- 53 F3.1 arcsec SeeingI ? Seeing in I band 55- 57 I3 min TexpK' ? Exposure time in K' (2.5µm) band 58 A1 --- r_TexpK' [abcd] Telescope used for observations (1) 60- 62 F3.1 arcsec SeeingK' ? Seeing in K' (2.5µm) band
Note (1): Telescope used: a: Palomar 1.5m b: Lick 3m c: Las Campanas 1m d: Las Campanas 2.5m
Byte-by-byte Description of file: table2.dat
Bytes Format Units Label Explanations
1- 11 A11 --- Cluster Cluster candidate name 13- 16 F4.2 --- zSpec ? The spectroscopic redshift 18- 21 F4.2 --- zLum ? Redshift from the I band luminosity function 23- 26 F4.2 --- e_zLum ? Error in zLum 28- 31 F4.2 --- zCol ? Redshift from the the cluster's `red-envelope' location in the color-magnitude diagram 33- 36 F4.2 --- e_zCol ? Error in zCol 38- 41 F4.2 --- zBGC ? Redshift from the brightest cluster galaxy 43- 46 F4.2 --- e_zBGC ? Error in zBGC 48- 52 F5.2 mag I*mag ? I band m* magnitude (1) 54- 57 F4.2 mag e_I*mag ? Error in I*mag 59- 62 F4.2 mag V-I ? The (V-I) color of the `red-envelope' 64- 67 F4.2 mag e_V-I ? Error in V-I 69- 72 F4.2 mag I-K' ? The (I-K') color of the `red-envelope' 74- 77 F4.2 mag e_I-K' ? Error in I-K'
Note (1): m* is the characteristic magnitude, see Schechter, 1976ApJ...203..297S
History: From electronic version of the journal
(End) Greg Schwarz [AAS], Patricia Bauer [CDS] 18-Feb-2002
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