J/MNRAS/428/226     High-redshift quasar candidates          (Polsterer+, 2013)

Finding new high-redshift quasars by asking the neighbours. Polsterer K.L., Zinn P.-C., Gieseke F. <Mon. Not. R. Astron. Soc., 428, 226-235 (2013)> =2013MNRAS.428..226P 2013MNRAS.428..226P
ADC_Keywords: QSOs ; Redshifts Keywords: methods: statistical - techniques: photometric - catalogues - surveys - galaxies: distances and redshifts - quasars: general Abstract: Quasars with a high redshift (z) are important to understand the evolution processes of galaxies in the early Universe. However, only a few of these distant objects are known to this date. The costs of building and operating a 10-m class telescope limit the number of facilities and, thus, the available observation time. Therefore, an efficient selection of candidates is mandatory. This paper presents a new approach to select quasar candidates with high redshift (z>4.8) based on photometric catalogues. We have chosen to use the z>4.8 limit for our approach because the dominant Lyman α emission line of a quasar can only be found in the Sloan i- and z-band filters. As part of the candidate selection approach, a photometric redshift estimator is presented, too. Three of the 120000 generated candidates have been spectroscopically analysed in follow-up observations and a new z=5.0 quasar was found. This result is consistent with the estimated detection ratio of about 50% and we expect 60000 high-redshift quasars to be part of our candidate sample. The created candidates are available for download at MNRAS or at http://www.astro.rub.de/polsterer/quasar-candidates.csv. Description: The presented method of photometrically selecting high-redshift quasar candidates is based on the Sloan Digital Sky Survey Data Release 6. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file qsocand.dat 150 121909 Quasar candidate data from SDSS photometry -------------------------------------------------------------------------------- See also: V/139 : The SDSS Photometric Catalog, Release 9 (Adelman-McCarthy+, 2012) http://www.sdss.org : SDSS Home Page Byte-by-byte Description of file: qsocand.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 18 I18 --- SDSS SDSS objID number 20- 37 F18.14 deg RAdeg Right ascension (J2000) 39- 56 E18.14 deg DEdeg Declination (J2000) 58- 62 F5.3 --- z [2.5/6.2] Redshift photometric estimate 64- 70 F7.5 --- e_z Standard deviation in redshift 72- 85 F14.12 --- Class [0.83/1] Coarse classifier rate (separates quasars, galaxies and stars) 87-100 F14.12 --- Rej* [0/.471] Cool star rejection rate (separates cool stars and quasars) 102-115 F14.12 --- Dist [0.63/1] Modified distance rate (separates quasars, galaxies and stars) 117-122 F6.3 mag umag psf SDSS u magnitude 124-129 F6.3 mag gmag psf SDSS g magnitude 131-136 F6.3 mag rmag psf SDSS r magnitude 138-143 F6.3 mag imag psf SDSS i magnitude 145-150 F6.3 mag zmag psf SDSS z magnitude -------------------------------------------------------------------------------- History: From electronic version of the journal
(End) Patricia Vannier [CDS] 03-Dec-2013
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