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J/PAZh/27/170 BR photometry of the UMa galaxy supercluster (Kopylov+, 2001)
The Ursa Major supercluster of galaxies - I. The luminosity function. Kopylov A.I., Kopylova F.G. <Pis'ma Astron. Zh. 27, 170 (2001)> =2001PAZh...27..170K =2001AstL...27..140K
ADC_Keywords: Clusters, galaxy ; Photometry Description: A catalogue of 1192 galaxies in the central regions (30' x 30') of 11 clusters in the Ursa Major supercluster is presented. For each galaxy equatorial and relative coordinates and total B and Rc magnitudes and B-Rc colour are given. Plates taken with the 2-m Tautenburg Observatory telescope and CCD images obtained with the 6-m and 1-m SAO telescopes are used. File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table1.dat 41 11 Coordinates of cluster centers table2.dat 76 1192 Galaxy catalogue in the Ursa Major supercluster
Byte-by-byte Description of file: table1.dat
Bytes Format Units Label Explanations
1- 5 A5 --- Cluster Cluster name 7- 8 I2 h RAh Right ascension (J2000.0) 10- 11 I2 min RAm Right ascension (J2000.0) 13- 16 F4.1 s RAs Right ascension (J2000.0) 18 A1 --- DE- Declination sign (J2000.0) 19- 20 I2 deg DEd Declination (J2000.0) 22- 23 I2 arcmin DEm Declination (J2000.0) 25- 26 I2 arcsec DEs Declination (J2000.0) 29- 40 A12 --- SName Simbad name
Byte-by-byte Description of file: table2.dat
Bytes Format Units Label Explanations
1- 5 A5 --- Cluster Cluster name 7- 9 I3 --- Galaxy Galaxy number in the cluster 12- 13 I2 h RAh Right Ascension B1950.0 15- 16 I2 min RAm Right Ascension B1950.0 18- 22 F5.2 s RAs Right Ascension B1950.0 24 A1 --- DE- Declination sign B1950.0 25- 26 I2 deg DEd Declination B1950.0 28- 29 I2 arcmin DEm Declination B1950.0 31- 34 F4.1 arcsec DEs Declination B1950.0 37- 43 F7.2 arcsec Xpos X-position (1) 45- 51 F7.2 arcsec Ypos Y-position (1) 54- 58 F5.2 mag Bmag Asymptotic magnitude in B band 61- 65 F5.2 mag Rmag ? Asymptotic magnitude in Rc band 67- 71 F5.2 mag B-R ? B-R colour index 74 I1 --- Notes ? Notes (2) 76 A1 --- Rem [c] c: Asymptotic magnitude in Rc band measured with CCD
Note (1): X and Y positions in arcseconds relative to the approximate center of cluster (table 1), increasing westwards and northwards, respectively. Note (2): Notes: 1 = cluster galaxy with measured redshift, 2 = foreground or background galaxy with measured redshift, 3 = probable foreground or background galaxy,
(End) Flera Kopylova [SAO, Russia], Veta Avedisova [INASAN] 29-March-2001
| 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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