J/MNRAS/396/223     QSO candidates selection in VO era     (D'Abrusco+, 2009)

Quasar candidates selection in the Virtual Observatory era. D'Abrusco R., Longo G., Walton N.A. <Mon. Not. R. Astron. Soc., 396, 223-262 (2009)> =2009MNRAS.396..223D 2009MNRAS.396..223D
ADC_Keywords: QSOs ; Surveys ; Photometry, SDSS Keywords: methods: data analysis - methods: observational - methods: statistical - catalogues - surveys - quasars: general Abstract: We present a method for the photometric selection of candidate quasars in multiband surveys. The method makes use of a priori knowledge derived from a subsample of spectroscopic confirmed quasi-stellar objects (QSOs) to map the parameter space. The disentanglement of QSOs candidates and stars is performed in the colour space through the combined use of two algorithms, the probabilistic principal surfaces and the negative entropy clustering, which are for the first time used in an astronomical context. Both methods have been implemented in the voneural package on the Astrogrid Virtual Observatory platform. Even though they belong to the class of the unsupervised clustering tools, the performances of the method are optimized by using the available sample of confirmed quasars and it is therefore possible to learn from any improvement in the available 'base of knowledge'. The method has been applied and tested on both optical and optical plus near-infrared data extracted from the visible Sloan Digital Sky Survey (SDSS) and infrared United Kingdom Infrared Deep Sky Survey-Large Area Survey public data bases. In all cases, the experiments lead to high values of both efficiency and completeness, comparable if not better than the methods already known in the literature. A catalogue of optical candidate QSOs extracted from the SDSS Data Release 7 Legacy photometric data set has been produced. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file list.dat 25 37 List of the stripe files data/* . 37 Ascii stripe files fits/* . 37 Files in FITS format -------------------------------------------------------------------------------- See also: II/294 : The SDSS Photometric Catalog, Release 7 (Adelman-McCarthy+, 2009) http://www.sdss.org : SDSS Home Page Byte-by-byte Description of file: list.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 12 A12 --- FileName Name of the file in subdirectory data 16- 20 I5 --- Nqsos Number of QSOs in the file 24- 25 I2 --- Stripe [9/86] Stripe number -------------------------------------------------------------------------------- Byte-by-byte Description of file: data/* -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 7 I7 --- Seq Candidate ID 9- 26 A18 --- objID SDSS objID of the source 28- 36 F9.5 deg RAdeg Right ascension in decimal degrees (J2000) 38- 46 F9.5 deg DEdeg Declination in decimal degrees (J2000) 48- 53 F6.3 mag umag PSF magnitude in SDSS/u' band 55- 60 F6.3 mag gmag PSF magnitude in SDSS/g' band 62- 67 F6.3 mag rmag PSF magnitude in SDSS/r' band 69- 74 F6.3 mag imag PSF magnitude in SDSS/i' band 76- 81 F6.3 mag zmag PSF magnitude in SDSS/z' band 83- 84 I2 --- cl [1,10] Cluster index (generation number of 'goal-successful' cluster) -------------------------------------------------------------------------------- History: Copied at http://voneural.na.infn.it/qso.html
(End) Patricia Vannier [CDS] 31-Jan-2011
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