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J/ApJ/723/1119    Optical properties of radio galaxies at z<0.3    (Lin+, 2010)

On the populations of radio galaxies with extended morphology at z < 0.3. Lin Y.-T., Shen Y., Strauss M.A., Richards G.T., Lunnan R. <Astrophys. J., 723, 1119-1138 (2010)> =2010ApJ...723.1119L
ADC_Keywords: Galaxies, radio ; Morphology ; Photometry, SDSS ; Active gal. nuclei ; Radio continuum Keywords: galaxies: active - galaxies: elliptical and lenticular, cD - radio continuum: galaxies Abstract: Extended extragalactic radio sources have traditionally been classified into Fanaroff & Riley (FR) I and II types, based on the ratio rs of the separation S between the brightest regions on either sides of the host galaxy and the total size T of the radio source (rs∼S/T). In this paper, we examine the distribution of various physical properties as a function of rs of 1040 luminous (L≳L*) extended radio galaxies (RGs) at z<0.3 selected with well-defined criteria from the SDSS (Strauss et al. 2002AJ....124.1810S), NVSS (Condon et al. 1998, Cat. VIII/65), and FIRST (Becker et al. 1995+, Cat. VIII/71) surveys. About 2/3 of the RGs are lobe dominated (LD) and 1/3 have prominent jets. If we follow the original definition of the FR types, i.e., a division based solely on rs, FRI and FRII RGs overlap in their host galaxy properties. File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table4.dat 103 1040 Basic properties of radio galaxies
See also: II/306 : The SDSS Photometric Catalog, Release 8 (Adelman-McCarthy+, 2011) III/255 : Spectroscopy of SDSS Data Release (SDSS-DR6) (ARC, 2007) VIII/71 : The FIRST Survey Catalog, Version 03Apr11 (Becker+ 2003) VIII/65 : 1.4GHz NRAO VLA Sky Survey (NVSS) (Condon+ 1998) J/MNRAS/415/1013 : FR II radio galaxies in SDSS (Koziel-Wierzbowska+, 2011) J/MNRAS/404/1719 : Combined NVSS-FIRST galaxies (CoNFIG) sample II (Gendre+, 2010) J/ApJ/699/L43 : FIRST-NVSS-SDSS AGN sample catalog (Smolcic+, 2009) J/ApJS/179/306 : Radio galaxy morphologies (Russell+, 2008) J/MNRAS/390/819 : CoNFIG sample (Gendre+, 2008) : MPA-JHU DR7 spectrum measurements : NYU Value-Added Galaxy Catalog : SDSS home page Byte-by-byte Description of file: table4.dat
Bytes Format Units Label Explanations
1- 18 A18 --- ObjId SDSS identification number 20- 26 I7 --- VAGC NYU VAGC DR6 object number 28 A1 --- Class [a-e] Class (1) 30- 39 F10.6 deg RAdeg Right Ascension in decimal degrees (J2000) 41- 50 F10.6 deg DEdeg Declination in decimal degrees (J2000) 52- 57 F6.4 --- z SDSS redshift 59- 63 F5.2 [W/Hz] logP1.4 Log of the 1.4GHz power 65- 71 F7.3 mag r0.1Mag Absolute SDSS r band magnitude (2) 73- 75 I3 km/s sigma Stellar velocity dispersion (3) 77- 80 F4.1 kpc Reff Effective radius 82- 85 I4 kpc T Total physical size 87- 90 F4.2 --- rs Ratio of separation and total size (4) 92- 98 F7.3 10+6Lsun LOIII ? The [OIII](5007Å) line luminosity 100-103 F4.1 --- Sig0.5 Excess number of neighbors within 0.5Mpc
Note (1): Classification, as in table 1 (with S = the angular separation between the highest surface brightness (HSB) spots on either sides of the galaxy), as follows: a = HSB spots: opposite sides of RG; Central source: not HSB; S: distance between two HSB spots; Number: 667 = Fraction: 64.1% b = HSB spot: center; Central source: extended, ≥0.1ftot; S: size of the HSB spot; Number: 289 = fraction: 27.7% c = HSB spot: center; Central source: extended, <0.1ftot; S: Distance between secondary HSB spots; Number: 38 = Fraction: 3.6% d = HSB spot: center; Central source: compact, ≥0.3ftot; S: Distance between secondary HSB spots; Number: 9 = Fraction: 0.9% e = HSB spot: center; Central source: compact, <0.3ftot; S: Distance between secondary HSB spots; Number: 37 = Fraction: 3.6% See section 3 for further details. Note (2): Where the r band has been shifted blueward by a factor of 1.1 in wavelength. Note (3): A zero sigma value indicates that SDSS didn't measure the redshift for the object, and we used the redshift from the nearest neighbor with a spectrum. Note (4): The separation between the brightest regions on either sides of the host galaxy and the total size of the radio source (rs=S/T).
History: From electronic version of the journal
(End) Greg Schwarz [AAS], Emmanuelle Perret [CDS] 25-Jul-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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