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J/A+A/536/A89     g'r'i' and redshift of Abell 2254 galaxies    (Girardi+, 2011)

Internal dynamics of Abell 2254: a merging galaxy cluster with a clumpy, diffuse radio emission. Girardi M., Bardelli S., Barrena R., Boschin W., Gastaldello F., Nonino M. <Astron. Astrophys., 536, A89 (2011)> =2011A&A...536A..89G
ADC_Keywords: Clusters, galaxy ; Galaxies, photometry ; Photometry, SDSS ; Radial velocities Keywords: X-rays: galaxies: clusters - galaxies: kinematics and dynamics - galaxies: clusters: general - galaxies: clusters: individual: Abell 2254 Abstract: The mechanisms giving rise to diffuse radio emission in galaxy clusters and, in particular, their connection with cluster mergers are still being debated. We explore the internal dynamics of Abell 2254, which has been shown to host a very clumpy and irregular radio halo. Our analysis is mainly based on redshift data for 128 galaxies acquired at the Telescopio Nazionale Galileo. We combined galaxy velocities and positions to select 110 cluster galaxies and analyze its internal dynamics. We also used new (g', r', i') photometric data acquired at the Isaac Newton Telescope, and (V, i') photometric data available in the Subaru Archive. X-ray data from the XMM-Newton Science Archive were analyzed to study the hot gas component. Description: Multi-object spectroscopic observations of A2254 were carried out at the TNG telescope in May and October 2009 and in March 2010. Our photometric observations were carried out with the Wide Field Camera (WFC), mounted at the prime focus of the 2.5m INT telescope. We observed A2254 in g', r', and i' SDSS filters in photometric conditions and a seeing of ∼1.6". Subaru Suprime-Cam data were retrieved from the SMOKA archive (http://smoka.nao.ac.jp/SUPsearch). File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table1.dat 60 128 Velocity catalog of 128 spectroscopically measured galaxies in the field of the cluster A2254
Byte-by-byte Description of file: table1.dat
Bytes Format Units Label Explanations
1- 3 I3 --- Seq [1/128] Sequential number of galaxy 5- 7 I3 --- IDm [1/110]? Sequential number of member galaxy 9- 10 I2 h RAh Right ascension (J2000) 12- 13 I2 min RAm Right ascension (J2000) 15- 19 F5.2 s RAs Right ascension (J2000) 21 A1 --- DE- Declination sign (J2000) 22- 23 I2 deg DEd Declination (J2000) 25- 26 I2 arcmin DEm Declination (J2000) 28- 31 F4.1 arcsec DEs Declination (J2000) 33- 37 F5.2 mag g'mag INT g' magnitude 39- 43 F5.2 mag r'mag INT r' magnitude 45- 49 F5.2 mag i'mag INT i' magnitude 51- 56 I6 km/s HRV Heliocentric radial velocity (cz) 58- 60 I3 km/s e_HRV rms uncertainty on HRV
History: From electronic version of the journal
(End) Patricia Vannier [CDS] 21-Feb-2012
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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