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J/A+A/469/861       Radial velocities of A115 galaxies       (Barrena+, 2007)

The dynamical status of the galaxy cluster Abell 115. Barrena R., Boschin W., Girardi M., Spolaor M. <Astron. Astrophys., 469, 861-872 (2007)> =2007A&A...469..861B
ADC_Keywords: Clusters, galaxy ; Radial velocities Keywords: galaxies: clusters: general - galaxies: clusters: individual: Abell 115 - galaxies: distances and redshifts - cosmology: observations Abstract: We present the results of a new spectroscopic and photometric survey of the hot, binary X-ray cluster A115 at z=0.193, containing a radio relic. Our analysis is based on new spectroscopic data obtained at the Telescopio Nazionale Galileo for 115 galaxies and on new photometric data obtained at the Isaac Newton Telescope in a large field. We combine galaxy velocity and position information to select 85 galaxies recognized as cluster members, determine global dynamical properties and detect substructures. Description: Multi-object spectroscopic observations of A115 were carried out at the TNG telescope in December 2003 during the program of proposal AOT8/CAT-G6. File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table1.dat 78 115 Velocity catalogue of 115 spectroscopically measured galaxies
Byte-by-byte Description of file: table1.dat
Bytes Format Units Label Explanations
1- 3 I3 --- [BBG2007b] Sequential number 4 A1 --- n_[BBG2007b] [F*] Field or bright member (1) 6- 21 A16 --- Name IAU designation (JHHMMSS.s+DDMMSS) 23- 24 I2 h RAh Right ascension (J2000) 26- 27 I2 min RAm Right ascension (J2000) 29- 33 F5.2 s RAs Right ascension (J2000) 35 A1 --- DE- Declination sign (J2000) 36- 37 I2 deg DEd Declination (J2000) 39- 40 I2 arcmin DEm Declination (J2000) 42- 45 F4.1 arcsec DEs Declination (J2000) 47- 51 F5.2 mag Bmag Harris B magnitude 53- 57 F5.2 mag Rmag Harris R magnitude 59- 64 I6 km/s RV Radial velocity 66- 68 I3 km/s e_RV rms uncertainty on RV 70- 78 A9 --- SpClass Spectral classification (2)
Note (1): Notes as follows: F = non-cluster galaxies * = highlight the three brightest cluster members: BCM-A = 3C28 = 21, BCM-B = 54, BCM-C = 104 (corresponding to Beers et al. 1983ApJ...264..356B, groups) and a fourth bright cluster member BCM-D = 81 (see text). Note (2): Spectral classification as follows: e(a) = galaxies having EW(Hdelta)≥4Å e(b) = galaxies having EW([OII])≤-40Å (likely starburst galaxies) EW(Hdelta)<4Å (likely spiral galaxies) e(c) = galaxies having moderate emission lines and EW(Hdelta)<4Å (likely spiral galaxies) k = passive galaxies a = active galaxies k+a = galaxies having 4≤EW(Hdelta)≤8Å a+k = galaxies having EW(Hdelta)>8Å
History: From electronic version of the journal
(End) Patricia Vannier [CDS] 30-Oct-2007
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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