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J/MNRAS/352/1245 Faint 1.4GHz radio sources in 2dFGRS (Chan+, 2004)
Faint 1.4-GHz radio sources in the 2dF Galaxy Redshift Survey. Chan B.H.P., Cram L.E., Sadler E.M., Killeen N.E.B., Jackson C.A., Mobasher B., Ekers R.D. <Mon. Not. R. Astron. Soc., 352, 1245-1254 (2004)> =2004MNRAS.352.1245C
ADC_Keywords: Radio sources ; Redshifts Keywords: surveys - galaxies: distances and redshifts - galaxies: evolution - galaxies: fundamental parameters - galaxies: statistics - radio continuum: galaxies Abstract: We have used the Australia Telescope Compact Array (ATCA) to search for faint radio sources in a ∼3deg2 region of sky covered by the 2dF Galaxy Redshift Survey (2dFGRS, Cat. VII/226). Over the region surveyed, the 1σ noise level at 1.4GHz ranges from 20Jy to 1mJy. The survey region includes 365 2dFGRS galaxies, of which 316 have good-quality spectra (176 early-type galaxies or active galactic nuclei, and 140 star-forming galaxies). The fraction of 2dFGRS galaxies detected as radio sources in our survey rises from ∼4% at a 3σ detection limit of 0.3mJy to 12% at 75µJy, with roughly equal numbers of star-forming galaxies and active galactic nuclei (AGNs) being detected. File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table3.dat 124 34 2dFGRS radio identifications table4.dat 62 331 2dFGRS radio upper limits
See also: VII/226 : The 2dF Galaxy Redshift Survey 100k Data Release (2dFGRS Team, 2001) Byte-by-byte Description of file: table3.dat
Bytes Format Units Label Explanations
1- 2 I2 h RAh 2dFGRS right ascension (J2000) 4- 5 I2 min RAm 2dFGRS right ascension (J2000) 7- 11 F5.2 s RAs 2dFGRS right ascension (J2000) 13 A1 --- DE- 2dFGRS declination sign (J2000) 14- 15 I2 deg DEd 2dFGRS declination (J2000) 17- 18 I2 arcmin DEm 2dFGRS declination (J2000) 20- 23 F4.1 arcsec DEs 2dFGRS declination (J2000) 25- 34 A10 --- 2dFGRS 2dFGRS (VII/226) name 36- 41 F6.4 --- z 2dFGRS Redshift 43- 47 F5.2 mag Bjmag Final Bj magnitude used in 2dFGRS 49 I1 --- q_z [1/5] 2dFGRS redshift measurement quality (G1) 51- 54 A4 --- Class Visual spectral classification (G2) 56 I1 --- FM [1/3] Fitting method used to derive the radio flux density (1) 58- 59 I2 h RAVh ? VSAD-5σ radio right ascension (J2000) 61- 62 I2 min RAVm ? VSAD-5σ radio right ascension (J2000) 64- 68 F5.2 s RAVs ? VSAD-5σ radio right ascension (J2000) 70 A1 --- DEV- VSAD-5σ radio declination sign (J2000) 71- 72 I2 deg DEVd ? VSAD-5σ radio declination (J2000) 74- 75 I2 arcmin DEVm ? VSAD-5σ radio declination (J2000) 77- 80 F4.1 arcsec DEVs ? VSAD-5σ radio declination (J2000) 82- 84 F3.1 arcsec Delta ? Estimated VSAD fitted positional uncertainty 86- 90 F5.3 arcsec Sep ? Radio-optical angular separation 92- 97 F6.3 mJy Speak ? Peak 1.4GHz radio flux density (2) 99-104 F6.3 mJy Stot ? Integrated 1.4GHz radio flux density (2) 106-107 I2 % e_S Percentage radio flux uncertainty (3) 109-113 F5.3 mJy e_Speak Actual radio flux uncertainty (3) 115-120 F6.4 mJy sigma-n Estimated local noise 122-124 I3 --- S/N Signal-to-noise ratio (Speak/σn)
Note (1): The fitting method used to derive the radio flux density: 1 = VSAD≥ 5σ match; 2 = IMFIT≥ 3σ match, and 3 = pixel summation. Note (2): Determined using the corresponding fitting method Note (3): When the local noise exceeds the fitting uncertainty, the larger value was used
Byte-by-byte Description of file: table4.dat
Bytes Format Units Label Explanations
1- 2 I2 h RAh 2dFGRS right ascension (J2000) 4- 5 I2 min RAm 2dFGRS right ascension (J2000) 7- 11 F5.2 s RAs 2dFGRS right ascension (J2000) 13 A1 --- DE- 2dFGRS declination sign (J2000) 14- 15 I2 deg DEd 2dFGRS declination (J2000) 17- 18 I2 arcmin DEm 2dFGRS declination (J2000) 20- 23 F4.1 arcsec DEs 2dFGRS declination (J2000) 25- 34 A10 --- 2dFGRS 2dFGRS (VII/226) name 35 A1 --- n_2dFGRS [a] upper limit (1) 37- 42 F6.4 --- z ? 2dFGRS Redshift 44- 48 F5.2 mag Bjmag Final Bj magnitude used in 2dFGRS 50 I1 --- q_z [1/5] 2dFGRS redshift measurement quality (G1) 52- 55 A4 --- Class Visual spectral classification (G2) 58- 62 F5.3 mJy UL 3σ upper limit
Note (1): 'a' indicates a radio upper limit represented by the average of the nearest four pixels to the 2dFGRS position
Global notes: Note (G1): The 2dFGRS redshift quality (Q) ranges from '1' for unlikely/poor quality spectra to '5' indicating a secure redshift Note (G2): Visual spectral classification use the following abbreviations: abs = absorption-line spectrum em = emission-line spectrum with dominant forbidden lines (e.g. [OIII]) a+e = combined absorption- and emission-line spectrum SF = emission-line spectrum with dominant recombination lines (e.g. Hα) ??? = spectrum with inadequate signal-to-noise ratio (S/N) or otherwise unclassifiable
History: From electronic version of the journal
(End) Patricia Vannier [CDS] 28-Feb-2005
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