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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
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:
FileName Lrecl Records Explanations
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
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
Bytes Format Units Label Explanations
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)
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
History: From electronic version of the journal
(End) Patricia Bauer [CDS] 17-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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