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J/AZh/87/760  Astrophysical catalog of clusters of galaxies (Kuvshinova+, 2010)

The physical properties of the intergalactic gas in rich clusters of galaxies. Kuvshinova I.B., Rozgacheva I. K. <Astron. Zh. 87, 760 (2010)> =2010AZh....87..760K =2010ARep...54..696K
ADC_Keywords: Clusters, galaxy; Combined data; X-ray sources Description: This catalog of rich clusters of galaxies contains information about the astrometric and physical characteristics of the 213 clusters of galaxies and data about evidences of the presence of cooling flows and filaments in selected clusters. The catalog lists also the references to the sources of the data. File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table1.dat 100 213 Physical characteristics of clusters of galaxies table2.dat 97 236 Processes and phenomenon in clusters of galaxies table3.dat 88 213 Physical parameters of clusters of galaxies in X-ray table4.dat 67 213 X-ray, optical and IR luminosities of clusters of galaxies refs.dat 158 237 References
Byte-by-byte Description of file: table1.dat
Bytes Format Units Label Explanations
1- 16 A16 --- Name Name of cluster 18- 19 I2 h RAh Right ascension (J2000.0) 21- 22 I2 min RAm Right ascension (J2000.0) 24- 27 F4.1 s RAs Right ascension (J2000.0) 29 A1 --- DE- Declination sign (J2000.0) 30- 31 I2 deg DEd Declination (J2000.0) 33- 34 I2 arcmin DEm Declination (J2000.0) 36- 37 I2 arcsec DEs [0/60] Declination (J2000.0) 39- 43 A5 --- r_Pos Reference of RA and DE, in refs.dat file 45- 50 F6.4 --- z Redshift 52- 59 A8 --- r_z Reference of redshift, in refs.dat file 61- 64 F4.1 mag mag ? Magnitude 66- 67 A2 --- r_mag Reference of magnitude, in refs.dat file 69- 74 F6.2 mag MAG ? Absolute magnitude 76- 78 A3 --- R ? Richness of clusters of galaxies 80- 83 I4 km/s sigma ? Velocity dispersion 85- 92 A8 --- r_sigma Reference of velocity dispersion, in refs.dat file 94- 96 I3 km/s E_sigma ? Error on sigma (upper limit) 98-100 I3 km/s e_sigma ? Error on sigma (lower limit)
Byte-by-byte Description of file: table2.dat
Bytes Format Units Label Explanations
1- 16 A16 --- Name Name of cluster 19 A1 --- CF [±?] cooling flows (CF) detection flag (1) 21- 74 A54 --- r_CF References for evidence of the presence of cooling flows (CF) in clusters of galaxies, in refs.dat file 77 A1 --- Fil [±?] Filaments datection flag (1) 79- 97 A19 --- r_Fil References for evidence of the presence of filaments in clusters of galaxies in refs.dat file
Note (1): the flag is as follows: + = found - = not detected ? = no data
Byte-by-byte Description of file: table3.dat
Bytes Format Units Label Explanations
1- 16 A16 --- Name Name of cluster 19- 24 F6.2 fW/m2 FX ? X-ray flux (10-12erg/cm2/s) 26- 32 A7 --- r_FX Reference of FX, in refs.dat file 34- 40 F7.3 10+37W LX ? X-ray luminosity (10+44erg/s) 42- 48 A7 --- r_LX Reference of LX, in refs.dat file 49- 54 F6.3 10+37W E_LX ? Error on X-ray luminosity (upper limit) 56- 60 F5.3 10+37W e_LX ? Error on X-ray luminosity (lower limit) 62- 66 F5.2 keV TX ? Temperature of the intracluster gas 68- 78 A11 --- r_TX Reference of TX, in refs.dat file 80- 83 F4.2 keV E_TX ? Error on TX (upper limit) 85- 88 F4.2 keV e_TX ? Error on TX (lower limit)
Byte-by-byte Description of file: table4.dat
Bytes Format Units Label Explanations
1- 16 A16 --- Name Name of cluster 18- 23 F6.2 10+37W LX ? X-ray luminosity (in 10+44erg/s) 25- 31 A7 --- r_LX ? Reference of LX, in refs.dat file 33- 39 F7.2 10+33W LHa ? Halpha luminosity (in 10+40erg/s) 41- 43 I3 --- r_LHa ? Reference of LHa, in refs.dat file 45- 50 F6.2 10+33W E_LHa ? Error on LHa (upper limit) 52- 57 F6.2 10+33W e_LHa ? Error on LHa (lower limit) 59- 63 F5.2 10+37W LIR ? IR-luminosity 65- 67 I3 --- r_LIR ? Reference of LIR, in refs.dat file
Byte-by-byte Description of file: refs.dat
Bytes Format Units Label Explanations
1- 3 I3 --- Ref Reference number 5- 23 A19 --- BibCode BibCode 25- 54 A30 --- Aut Author's name 55-158 A104 --- Com Comments

(End) Veta Avedisova (INASAN) 14-Oct-2010
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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