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J/AJ/129/26       A deep radio survey of Abell 2125. I             (Owen+, 2005)

A deep radio survey of Abell 2125. I. Radio, optical, and near-infrared observations. Owen F.N., Keel W.C., Ledlow M.J., Morrison G.E., Windhorst R.A. <Astron. J., 129, 26-30 (2005)> =2005AJ....129...26O
ADC_Keywords: Clusters, galaxy ; Radio sources Keywords: cosmology: observations - galaxies: clusters: individual (Abell 2125) - galaxies: evolution - galaxies: starburst - infrared: galaxies Abstract: We present a description of deep radio, optical, and near-IR observations taken with the VLA, the KPNO 2m telescope, and the KPNO 4m telescope of the region containing the rich cluster of galaxies Abell 2125. The reduction of each data set is described. A catalog of radio sources apparently not associated with members of A2125 and the associated R-band magnitudes is presented. Description: Observations were made with the VLA for 3.5hr in the 1997 B configuration and for 27.5hr in the 1998 A configuration. The data were all taken in spectral line mode 4, which provides seven 3.125MHz channels in each of two intermediate frequencies (IFs; centered at 1365 and 1435MHz) and each of two polarizations. File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table1.dat 86 357 Non-cluster member radio sources
See also: J/AJ/129/31 : A deep radio survey of Abell 2125. II (Owen+, 2005) J/ApJ/613/841 : Redshifts in A2125 (Miller+, 2004) J/AJ/118/625 : Radio sources in Abell 2125 and 2645 (Dwarakanath+, 1999) J/ApJ/611/821 : X-raying A2125 (Wang+, 2004) Byte-by-byte Description of file: table1.dat
Bytes Format Units Label Explanations
1- 5 I5 --- [OKL2005] Source name (1) 7- 8 I2 h RAh Hour of Right Ascension (J2000) 10- 11 I2 min RAm Minute of Right Ascension (J2000) 13- 17 F5.2 s RAs Second of Right Ascension (J2000) 19- 22 F4.2 s e_RAs Estimated error in RAs 24- 25 I2 deg DEd Degree of Declination (J2000) 27- 28 I2 arcmin DEm Arcminute of Declination (J2000) 30- 33 F4.1 arcsec DEs Arcsecond of Declination (J2000) 35- 37 F3.1 arcsec e_DEs Estimated error in DEs 39- 42 F4.1 arcmin Dist Angular distance from the pointing center (2) 44- 50 F7.1 uJy Sp20cm Uncorrected peak flux density at 20cm in units of µJy/beam size 52- 58 F7.1 uJy S20cm Corrected total flux density at 20cm 60- 64 F5.0 uJy e_S20cm Estimated error in S20cm 66 A1 --- l_Size [<] Limit flag in Size 67- 70 F4.1 arcsec Size Best fit size, major axis (3) 71 A1 --- --- [x] 72- 74 F3.1 arcsec Size1 ? Best fit size, minor axis (3) 76- 78 I3 deg PA ? Best fit, position angle (3) 80- 84 F5.2 mag Rmag ?=0.00 The R band optical magnitude 86 A1 --- n_Rmag [ibc] Optical/NIR identification status (4)
Note (1): The first two digits are the facet number and the last three a sequence number. Note (2): Where the center is RA=15:41:14.00 and DE=66:15:00.0. Note (3): If a two dimensional Gaussian was the best fit, we give the major and minor axis size (FWHM) and the position angle. Upper limits are given for sources which were unresolved. Sources with sizes only were estimated directly from the maps using the AIPS task, TVSTAT. Note (4): Optical/NIR identification status, defined as follows: i = identifications in at least one of the 10 observed bands; b = a blank field; c = an optical field which is too confused to be sure of the identification.
History: From electronic version of the journal References: Owen et al., Paper II 2005AJ....129...31O, Cat. J/AJ/129/31
(End) Greg Schwarz [AAS], Marianne Brouty [CDS] 06-Jul-2005
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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