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J/A+A/517/A65         Velocities of A2294 galaxies              (Girardi+, 2010)

Internal dynamics of Abell 2294: a massive, likely merging cluster. Girardi M., Boschin W., Barrena R. <Astron. Astrophys., 517, A65 (2010)> =2010A&A...517A..65G
ADC_Keywords: Clusters, galaxy ; Galaxies, photometry ; Radial velocities Keywords: galaxies: clusters: individual: Abell 2294 - galaxies: clusters: general - galaxies: kinematics and dynamics Abstract: The mechanisms giving rise to diffuse radio emission in galaxy clusters, and in particular their connection with cluster mergers, are still debated. We seek to explore the internal dynamics of the cluster Abell 2294, which has been shown to host a radio halo. Our analysis is mainly based on redshift data for 88 galaxies acquired at the Telescopio Nazionale Galileo. We combine galaxy velocities and positions to select 78 cluster galaxies and analyze its internal dynamics. We also use both photometric data acquired at the Isaac Newton Telescope and X-ray data from the Chandra archive. Description: Multi-object spectroscopic observations of A2294 were carried out at the TNG telescope in December 2007 and August 2008. File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table1.dat 82 88 Velocity catalog of 88 spectroscopically measured galaxies in the field of the cluster A2294
Byte-by-byte Description of file: table1.dat
Bytes Format Units Label Explanations
1- 2 I2 --- Seq [1/88] Sequential number, <[GBB2010b] NN> in Simbad 3 A1 --- n_Seq [*i] * for BCG, i for non-member galaxies 5- 6 I2 h RAh Right ascension (J2000) 8- 9 I2 min RAm Right ascension (J2000) 11- 15 F5.2 s RAs Right ascension (J2000) 17 A1 --- DE- Declination sign (J2000) 18- 19 I2 deg DEd Declination (J2000) 21- 22 I2 arcmin DEm Declination (J2000) 24- 27 F4.1 arcsec DEs Declination (J2000) 29- 33 F5.2 mag Bmag INT Harris B magnitude 35- 39 F5.2 mag Rmag INT Harris R magnitude 41- 46 I6 km/s HRV Heliocentric radial velocity 48- 50 I3 km/s e_HRV rms uncertainty on HRV 52- 82 A31 --- Em Emission lines
History: From electronic version of the journal
(End) Patricia Vannier [CDS] 28-Oct-2011
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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