Search catalogue
J/MNRAS/391/369 New z≥3.6 QSOs from FIRST-SDSS DR5 (Carballo+, 2008)
Use of neural networks for the identification of new z ≥ 3.6 QSOs from FIRST-SDSS DR5. Carballo R., Gonzalez-Serrano J.I., Benn C.R., Jimenez-Lujan F. <Mon. Not. R. Astron. Soc., 391, 369-382 (2008)> =2008MNRAS.391..369C
ADC_Keywords: QSOs ; Redshifts ; Radio sources ; Photometry, SDSS Keywords: methods: data analysis - surveys - galaxies: high-redshift - quasars: general - early Universe - radio continuum: galaxies Abstract: We aim to obtain a complete sample of redshift z≥3.6 radio quasi-stellar objects (QSOs) from the Faint Images of the Radio Sky at Twenty cm survey (FIRST) sources (S1.4GHz>1mJy) having star-like counterparts in the Sloan Digital Sky Survey (SDSS) Data Release 5 (DR5) photometric survey (rAB≤20.2). Our starting sample of 8665 FIRST-DR5 pairs includes 4250 objects with spectra in DR5, 52 of these being z≥3.6 QSOs. We found that simple supervised neural networks, trained on the sources with DR5 spectra, and using optical photometry and radio data, are very effective for identifying high-z QSOs in a sample without spectra. For the sources with DR5 spectra the technique yields a completeness (fraction of actual high-z QSOs classified as such by the neural network) of 96 per cent, and an efficiency (fraction of objects selected by the neural network as high-z QSOs that actually are high-z QSOs) of 62 per cent. Applying the trained networks to the 4415 sources without DR5 spectra we found 58 z≥3.6 QSO candidates. We obtained spectra of 27 of them, and 17 are confirmed as high-z QSOs. Spectra of 13 additional candidates from the literature and from SDSS Data Release 6 (DR6) revealed seven more z≥3.6 QSOs, giving an overall efficiency of 60 per cent (24/40). File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table2.dat 62 52 FIRST-DR5 sources with SDSS spectra, and classified by SDSS as z≥3.6 QSOs table5.dat 79 58 z≥3.6 QSO candidates identified by the NN in the FIRST-SDSS DR5 unlabelled sample
See also: II/276 : The SDSS Photometric Catalog, Release 5 (Adelman-McCarthy+, 2007) J/MNRAS/348/857 : Radio-loud QSOs at z∼4 (Holt+, 2004) J/MNRAS/370/1034 : FIRST-APM-SDSS survey for high-z radio QSOs (Carballo+, 2006) Byte-by-byte Description of file: table2.dat
Bytes Format Units Label Explanations
1- 2 I2 h RAh SDSS Right ascension (J2000) 4- 5 I2 min RAm SDSS Right ascension (J2000) 7- 11 F5.2 s RAs SDSS Right ascension (J2000) 13 A1 --- DE- SDSS Declination sign (J2000) 14- 15 I2 deg DEd SDSS Declination (J2000) 17- 18 I2 arcmin DEm SDSS Declination (J2000) 20- 23 F4.1 arcsec DEs SDSS Declination (J2000) 25- 29 F5.2 mag rmag SDSS dereddened PSF rAB magnitude 31- 36 F6.2 mJy S1.4GHz FIRST total radio flux density 39- 43 F5.3 --- z SDSS redshift 44 A1 --- n_z [a] a = revised redshift from DR5Q, see Section 2 47- 50 F4.2 --- NN [0.1,1] Neuronal network (NN) output (ymed≥.01) see Section 4.2) 52- 58 A7 --- PSamp Included in previous samples (1) 60- 62 A3 --- Notes Notes (G1)
Note (1): Previous samples are: 1 = QSOs included in the samples of Benn et al. (2002MNRAS.329..221B) 2 = QSOs included in the samples of Holt et al. 2004, Cat. J/MNRAS/348/857 3 = QSOs included in the samples of Carballo et al. 2006, Cat. J/MNRAS/370/1034
Byte-by-byte Description of file: table5.dat
Bytes Format Units Label Explanations
1- 2 I2 h RAh SDSS Right ascension (J2000) 4- 5 I2 min RAm SDSS Right ascension (J2000) 7- 11 F5.2 s RAs SDSS Right ascension (J2000) 13 A1 --- DE- SDSS Declination sign (J2000) 14- 15 I2 deg DEd SDSS Declination (J2000) 17- 18 I2 arcmin DEm SDSS Declination (J2000) 20- 23 F4.1 arcsec DEs SDSS Declination (J2000) 25- 29 F5.2 mag rmag SDSS dereddened PSF rAB magnitude 31- 36 F6.2 mJy S1.4GHz FIRST total radio flux density 38- 41 F4.2 --- NN [0.1,1] Neuronal network (NN) output (ymed≥.01) see Section 4.2) 43- 47 F5.3 --- zNED ? Redshift from NED 48- 51 F4.2 --- z ? Redshift from William Herschel Telescope 53- 57 F5.3 --- zDR6 ? Redshift from SDSS DR6 59- 75 A17 --- Notes Notes (G1) 77- 79 A3 --- Flag [Yes] indicates sources located within the spectroscopic plates available in DR6
Note (G1): Notes include: BAL = broad absorption line QSO abs = Lyα line appears to be self-absorbed
History: From electronic version of the journal
(End) Patricia Vannier [CDS] 27-Mar-2009
| 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 |
© UDS/CNRS