VII/241 The 2dF QSO Redshift Survey (Croom+ 2004) ================================================================================ The 2dF QSO Redshift Survey (2QZ) Croom S.M., Smith R.J., Boyle B.J., Shanks T., Miller L., Outram P.J., Loaring N.S. =2004MNRAS.349.1397C ================================================================================ ADC_Keywords: Active gal. nuclei; QSOs; Redshifts; Spectroscopy; Stars, white dwarf; Stars, normal; Galaxies, spectra Keywords: catalogues - surveys - white dwarfs - galaxies: active - quasars: general - galaxies: Seyfert Abstract: The final catalogue of the 2dF QSO Redshift Survey (2QZ) is based on Anglo-Australian Telescope 2dF spectroscopic observations of 44576 colour-selected (ub_J_r) objects with 18.25 Note (3): 1.4GHz radio flux is taken from the NRAO VLA Sky Survey (NVSS), Condon et al., 1998AJ....115.1693C, Cat. Note (4): The X-ray flux is taken from the ROSAT All Sky Survey, Voges et al., 1999A&A...349..389V, Cat. ; Voges et al., 2000IAUC.7432R...1V. Counts/s in the 0.1 to 2.4keV band were converted to flux in 10^-13^erg/s/cm^2^ (or equivalently 10^-13^mW/m^2^) assuming a photon index of -2 giving a conversion factor of 5.6x10^-12^. -------------------------------------------------------------------------------- Byte-by-byte Description of file: ngp_rep.dat sgp_rep.dat 6qz_rep.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 16 A16 --- 2QZ Name of the source in 2QZ (JHHMMSS.S+DDMMSS) 18- 19 I2 h RAh Right ascension (J2000) 21- 22 I2 min RAm Right ascension (J2000) 24- 28 F5.2 s RAs Right ascension (J2000) 30 A1 --- DE- Declination sign 31- 32 I2 deg DEd Declination (J2000) 34- 35 I2 arcmin DEm Declination (J2000) 37- 40 F4.1 arcsec DEs Declination (J2000) 42- 51 A10 --- intName Internal name of the object 53- 58 F6.3 mag bJmag b_J_ magnitude 61- 66 F6.3 mag u-bJ u-b_J_ colour index 68- 74 F7.3 mag bJ-r b_J_-r colour index (G1) 76- 81 F6.4 --- z Redshift from first spectrum 83- 84 I2 --- q_z Quality flag for first spectrum (G3) 86- 94 A9 --- ID Identification for first spectrum (G4) 97-104 I8 "YYYYMMDD" Date ? Date of observation for first spectrum 106-109 I4 --- Field field and spectrograph for first spectrum (G2) 111-113 I3 --- Fiber 2dF fiber number 115-120 F6.2 --- S/N1 Signal-to-noise ratio for first spectrum (G5) 121 A1 --- --- [0] 124 I1 --- No [3,6] Observation number 126-145 A20 --- Com Comment on observation -------------------------------------------------------------------------------- Gloval Notes: Note (G1): In the case of an object having only an upper limit in the r-band, the b_J_-r colour is defined as (b_J_-r_lim_)-10. All r-band detections have b_J_-r>-1.5 while this definition gives all upper limits b_J_-r<-9.8. Note (G2): The number is defined as 2dF field number x10 + 2dF spectrograph number e.g. field number 218 and spectrograph 2 gives 2182. (the spectrograph number is 1 or 2) Note (G3): Both redshift and identification are given separate quality flags (1 = high-quality, 2 = low-quality, 3 = unclassifiable). The quality number is set as identification quality x 10 + redshift quality Note (G4): The spectra are classified in six main categories: QSO = for a spectrum with broad emission lines NELG = (narrow-emission line galaxy) for a spectrum with narrow emission lines gal = a galaxy spectrum with no emission lines star = a Galactic star spectrum cont = a high signal-to-noise (S/N>10) spectrum with no identifiable emission of absorption features ?? = an unclassifiable spectrum Sub-classes are contained within parentheses after the main classifications: DA = a DA white dwarf DB = a DB white dwarf DO = a DO white dwarf DZ = a DZ white dwarf CV = a star with strong hydrogen Balmer emission lines DAM = a DA white dwarf - M-dwarf binary DBM = a DB white dwarf - M-dwarf binary BAL = a broad absorption line QSO For example QSO(BAL), star(DA), star(CV). If the identification has a class 2 quality then there is a ? appended to the end of the identification. Note (G5): Signal-to-noise calculated in a 400-490nm band -------------------------------------------------------------------------------- History: From the 2QZ site at http://www.2dfquasar.org/ ================================================================================ (End) Francois Ochsenbein [CDS] 01-Jun-2006