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J/MNRAS/357/1231    Texas-Oxford NVSS (TONS) radio galaxies  (Brand+, 2005)

The three-dimensional clustering of radio galaxies in the Texas-Oxford NVSS structure survey. Brand K., Rawlings S., Hill G.J., Tufts J.R. <Mon. Not. R. Astron. Soc., 357, 1231-1254 (2005)> =2005MNRAS.357.1231B
ADC_Keywords: Surveys ; Galaxies, radio ; Redshifts ; Galaxies, photometry Keywords: galaxies: active - cosmology: observations - large-scale structure of Universe - radio continuum: galaxies Abstract: We present a clustering analysis of the Texas-Oxford NVSS Structure (TONS) radio galaxy redshift survey. This complete flux-limited survey consists of 268 radio galaxies with spectroscopic redshifts in three separate regions of the sky covering a total of 165°2. By going to faint radio flux densities (S1.4≥3mJy) but imposing relatively bright optical limits (E∼R∼19.5), the TONS sample is optimized for looking at the clustering properties of low-luminosity radio galaxies in a region of moderate (0≤z≤0.5) redshifts. Description: Description: Optical spectra were obtained during the period 2000 October-2003 May on the 2.6-m Nordic Optical Telescope (NOT) using the Andalucia faint object spectrograph, the 4.2-m William Herschel telescope (WHT) using ISIS, the 2.7-m Smith reflector at McDonald with the Imaging Grism Instrument (IGI), and the Hobby-Eberly Telescope (HET) using the Marcario low-resolution spectrograph (LRS). File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table4.dat 117 107 A summary of key information on the TONS12 sample table5.dat 117 47 A summary of key information on the TONS08w sample table6.dat 117 40 A summary of key information on the TONS16 sample
See also: VIII/71 : The FIRST Survey Catalog, Version 03Apr11 (Becker+ 2003) VII/226 : The 2dF Galaxy Redshift Survey 100k Data Release (2dFGRS Team, 2001) VIII/65 : 1.4GHz NRAO VLA Sky Survey (NVSS) (Condon+ 1998) J/AJ/126/2579 : SDSS quasar catalog. II. First data release (Schneider+, 2003) Table 1. The RA and Dec. limits for the different TONS subsamples. ---------------------------------------------------------------------- Sample RA DE ---------------------------------------------------------------------- TONS08 08:10:20 ≤ RA ≤ 08:29:20 24:10:00 ≤ DE ≤ 29:30:00 TONS12 12:48:00 ≤ RA ≤ 13:12:00 33:00:00 ≤ DE ≤ 38:00:00 TONS08w 08:00:00 ≤ RA ≤ 08:41:00 21:50:00 ≤ DE ≤ 31:50:00 TONS16w 16:24:00 ≤ RA ≤ 16:56:00 42:00:00 ≤ DE ≤ 51:00:00 Byte-by-byte Description of file: table4.dat table5.dat table6.dat
Bytes Format Units Label Explanations
1- 4 A4 --- --- [TONS] 6- 13 A8 --- TONS TONS designation 15- 17 A3 --- Tel Telescope identification (1) 19- 22 I4 yr ObsY ? Year of observation 24- 30 A7 --- ObsM Months of observation (MMM/MMM) 32- 33 I2 h RAh Right ascension (J2000.0) (2) 35- 36 I2 min RAm Right ascension (J2000.0) (2) 38- 42 F5.2 s RAs Right ascension (J2000.0) (2) 44 A1 --- DE- Declination sign (J2000.0) (2) 45- 46 I2 deg DEd Declination sign (J2000.0) (2) 48- 49 I2 arcmin DEm Declination sign (J2000.0) (2) 51- 55 F5.2 arcsec DEs Declination sign (J2000.0) (2) 57- 62 F6.1 mJy SNVSS Integrated radio flux in NVSS catalog (VIII/65) 64- 70 F7.2 mJy SFIRST ? Integrated radio flux in FIRST (VIII/71) (3) 72- 76 F5.2 mag Emag APM E magnitude 78- 82 F5.2 mag Omag APM O magnitude 84- 88 F5.3 --- zest Estimated redshift 90- 95 F6.4 --- zc ? Redshift obtained by cross-correlating the spectra with the combined de-redshifted spectra model 97-102 F6.4 --- zsed ? Redshift obtained by cross-correlating the spectra with the GISSEL model 104-117 A14 --- Notes Name of the object in other samples (4)
Note (1): Telescopes are designated as follows: 2.7 = 2.7-m Smith reflector at McDonald HET = Hobby-Eberly Telescope WHT = 4.2-m William Herschel telescope Note (2): The positions are that of the radio positions except in the case of multiple sources where the positions are from APM. Note (3): In cases where FIRST resolves out multiple components, SFIRST is the total integrated flux density. Note (4): Spectra for the TOOT objects will be presented in Rawlings et al. (in preparation). Spectra denoted by Benn are from Benn (private communication). Other redshifts were obtained from the literature.
History: From electronic version of the journal
(End) Patricia Vannier [CDS] 11-Oct-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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