VII/249             6dF-DR2 Galaxy Survey                        (Jones+, 2005)

Second Data Release of the 6dF Galaxy Survey. Jones D.H., Saunders W., Read M., Colless M. <Publications - Astron. Soc. Australia, 22, 277 (2005)> =2005PASA...22..277J 2005PASA...22..277J
ADC_Keywords: Surveys; Galaxy catalogs; Redshifts Keywords: galaxies: statistics, luminosity function - cosmology: large-scale structure of universe Abstract: The 6dF Galaxy Survey is measuring around 150000 redshifts and 15000 peculiar velocities from galaxies over the southern sky at |b|>10°. When complete, it will be the largest survey of its kind by more than an order of magnitude. A total of 83014 sources now have their spectra, redshifts, and near-infrared and optical photometry available online and searchable through an Structured Query Language at www.wfau.roe.ac.uk/6dFGS/ . File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file master.dat 127 179262 Master config file used to form the target table (version April 2005) spectra.dat 212 89211 Table of spectral observations (subset of parameters) -------------------------------------------------------------------------------- See also: http://www-wfau.roe.ac.uk/6dfgs/ : the 6dFGS Home page VII/226 : The 2dF Galaxy Redshift Survey 100k Data Release (2dFGRS Team, 2001) Byte-by-byte Description of file: master.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 15 A15 --- TargName Galaxy survey target ID 17- 18 I2 h RAh Right ascension (J2000) 20- 21 I2 min RAm Right ascension (J2000) 23- 27 F5.2 s RAs Right ascension (J2000) 29 A1 --- DE- Declination sign (J2000) 30- 31 I2 deg DEd Declination (J2000) 33- 34 I2 arcmin DEm Declination (J2000) 36- 39 F4.1 arcsec DEs Declination (J2000) 41 A1 --- P [P] 'P' for programme objects 43 I1 --- W Weight assigned in future fibre allocation 45- 49 F5.2 mag bJmag ?=0 Recalibrated bJ magnitude (BMAG) 51- 53 I3 --- PrID Programme ID number (PROGID in database) (1) 55- 59 F5.2 mag rFmag ?=0 Recalibrated rF magnitude (RMAG) 61 I1 --- S/G [0/4] SuperCOSMOS star/galaxy classifier (2) 63 I1 --- Tile Tile weighting 65- 71 I7 km/s cz Recession velocity cz 73- 75 I3 km/s e_cz Nominal uncertainty in cz 77- 80 I4 --- r_cz Code identifying source of redshift (3) 82 I1 --- q_cz Redshift quality value (4) 84- 91 F8.4 deg GLON Galactic longitude 93-100 F8.4 deg GLAT Galactic latitude 102-106 F5.2 mag AV Galactic extinction in V magnitudes (from Schlegel et al., 1998ApJ...500..525S 1998ApJ...500..525S) 108 I1 --- w0 Original weight source had for first round of fibre allocation 110-127 A18 --- File Name of redshift field file containing the redshift if from 6dFGS (5) -------------------------------------------------------------------------------- Note (1): ProgID as follows: 1 = 2MASS Ks<12.75 3 = 2MASS H <13.00 4 = 2MASS J <13.75 5 = DENIS J <14.00 6 = DENIS I <14.00 7 = SuperCOSMOS rF<15.60 8 = SuperCOSMOS bJ<16.75 78 = Durham/UKST Galaxy Survey sources 90 = Shapley 109 = Not precised 113 = ROSAT All-Sky Survey 116 = 2MASS AGN 119 = HIPASS (>4sigma) 125 = SUMSS sources 126 = IRAS FSC 6sigma 129 = Hamburg-ESO Survey 130 = NRAO-VLA Sky Survey 999 = orphaned sources Note (2): SuperCOSMOS star/galaxy classifier as follows: 1 = star 2 = galaxy 3 = unclassifiable 4 = noise Note (3): Code identifying source of redshift as follows: 0 = no measure -1 to 68 = reference code of ZCAT (Cat. VII/193) 126 = 6dFGS 392 = 2dFGRS Note (4): Quality flag as follows: 2 = 6dFGS/2dFGRS, possible, but doubtful, redshift estimate 3 = 6dFGS/2dFGRS, 'probable' redshift (notionally 90% confidence) 4 = 6dFGS/2dFGRS, reliable redshift (notionally 99% confidence) 6 = 6dFGS confirmed Galactic source (not all), 8 = Other sources except ZCAT (not a measure of quality) 9 = ZCAT sources (not a measure of quality) redshift quality schemes used by 6dFGS and 2dFGRS respectively.) Note (5): word "2dFGRS" if from that survey. -------------------------------------------------------------------------------- Byte-by-byte Description of file: spectra.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 5 I5 --- SpecID Unique ID number used to generate GIF image of spectrum 7- 12 I6 --- TargID ID number in Target table 14- 28 A15 --- TargName Matching name in target table, used to name FITS files and generate thumbnail images 31- 32 I2 h RAh Observed right ascension (J2000) 33 A1 --- --- [:] 34- 35 I2 min RAm Observed right ascension (J2000) 36 A1 --- --- [:] 37- 41 F5.2 s RAs [0/60] Observed right ascension (J2000) 43 A1 --- DE- Observed Declination sign (J2000) 44- 45 I2 deg DEd Observed Declination (J2000) 46 A1 --- --- [:] 47- 48 I2 arcmin DEm Observed Declination (J2000) 49 A1 --- --- [:] 50- 53 F4.1 arcsec DEs [0/60] Observed Declination (J2000) 56- 70 E15.9 arcsec dr ?=-9.99 Position match error (arcsec) 72- 85 E14.7 --- zraw ?=-9.999 Raw measured redshift 87-100 E14.7 --- z ?=-9.999 Heliocentric redshift 103 I1 --- q_z [0/6] Redshift measurement quality: 4=good to 1=bad (6=star) 109-118 F10.6 --- Rcor ?=-9.99 Cross-correlation peak 122-133 F12.6 s ExpV V reference frame exposure time seconds 136-150 E15.9 d MJD.V MJD of observation in V band 154-165 E12.9 s ExpR R reference frame exposure time seconds 168-182 E15.9 d MJD.R ?=0 MJD of observation in R band 184-212 A29 --- Com Comments on redshift -------------------------------------------------------------------------------- History: Copied at http://www.aao.gov.au/local/www/6df/
(End) Patricia Vannier [CDS] 22-Jun-2006
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