J/MNRAS/327/588 Las Campanas/AAT Rich Cluster Survey - I (Pimbblet+, 2001)
The Las Campanas/AAT Rich Cluster Survey -
I. Precision and reliability of the photometric catalogue.
Pimbblet K.A., Smail I., Edge A.C., Couch W.J., O'Hely E., Zabludoff A.I.
<Mon. Not. R. Astron. Soc. 327, 588 (2001)>
=2001MNRAS.327..588P 2001MNRAS.327..588P
ADC_Keywords: Galaxy catalogs ; Clusters, galaxy ; Redshifts
Keywords: catalogues - surveys - galaxies: photometry
Abstract:
The Las Campanas Observatory and Anglo-Australian Telescope Rich
Cluster Survey (LARCS) is a panoramic imaging and spectroscopic survey
of an X-ray luminosity-selected sample of 21 clusters of galaxies at
0.97<z<0.16. Charge-coupled device (CCD) imaging was obtained in B and
R of typically 2° wide regions centred on the 21 clusters, and the
galaxy sample selected from the imaging is being used for an on-going
spectroscopic survey of the clusters with the 2dF spectrograph on the
Anglo-Australian Telescope.
File Summary:
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FileName Lrecl Records Explanations
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ReadMe 80 . This file
table1.dat 67 21 Details of the 21 clusters in the LARCS sample
and the multiwavelength observations of those
so far obtained
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See also:
VII/203 : Las Campanas Redshift Survey (Shectman+ 1996)
J/ApJS/130/237 : LCRS loose groups of galaxies (Tucker+, 2000)
J/ApJS/137/117 : Las Campanas Distant Cluster Survey (LCDCS) (Gonzales+, 2001)
J/AN/321/101 : Compact groups of galaxies in LCRS (Allam+, 2000)
Byte-by-byte Description of file: table1.dat
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Bytes Format Units Label Explanations
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1- 5 A5 --- Cluster Cluster name (ANNNN)
7- 8 I2 h RAh Right ascension (J2000)
10- 11 I2 min RAm Right ascension (J2000)
13- 17 F5.2 s RAs Right ascension (J2000)
19 A1 --- DE- Declination sign (J2000)
20- 21 I2 deg DEd Declination (J2000)
23- 24 I2 arcmin DEm Declination (J2000)
26- 27 I2 arcsec DEs Declination (J2000)
29- 33 F5.3 --- z Redshift
35- 39 F5.2 10+37W LX X-ray luminosity (1044 erg/s)
41- 47 A7 --- Band Broad-band filters used to observe each cluster
49- 51 F3.1 deg Diam ? Diameter
53- 67 A15 --- Obs Other observations (1)
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Note (1): Other observations indicate ROSAT imaging (with the PSPC or HRI
instruments), XMM-Newton EPIC time which has been allocated and
observations undertaken with the 2dF spectrograph at the AAT
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History:
From electronic version of the journal
(End) Patricia Bauer [CDS] 17-Jan-2002