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J/MNRAS/356/331  QSO-candidates in OGLE-II Galactic bulge fields   (Sumi+, 2005)

Variability-selected QSO candidates in OGLE-II Galactic bulge fields. Sumi T., Wozniak P.R., Eyer L., Dobrzycki A., Udalski A., Szymanski M.K., Kubiak M., Pietrzynski G., Soszynski I., Zebrun K., Szewczyk O., Wyrzykowski L. <Mon. Not. R. Astron. Soc., 356, 331-335 (2005)> =2005MNRAS.356..331S
ADC_Keywords: QSOs ; Photometry, CCD Keywords: stars: variables: other - Galaxy: bulge - Galaxy: centre - quasars: general Abstract: We present 97 QSO candidates in 48 Galactic bulge fields of the Optical Gravitational Lensing Experiment II (OGLE-II) covering ∼11deg2, which are selected via their variability. We extend light curves of variable objects which were detected in a 3-yr baseline in the OGLE-II variable star catalogue to fourth year. We search for objects that are faint (16<I0<18.5) and slowly variable over 4-yr in this catalogue by using the variogram/structure function. Finding the QSOs in such stellar-crowded and high extinction fields is challenging, but should be useful for the astrometric reference frame. Spectroscopic follow-up observations are required to confirm these QSO candidates. Follow-up observations are being prepared for four of these fields (BUL_SC1, 2, 32 and 45). Follow-up observations for other fields are strongly encouraged. The complete list and light curves of all 97 candidates are available in electronic format at http://www.astro.princeton.edu/sumi/QSO-OGLEII/ . File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table2.dat 89 97 The list of the 97 QSO candidates
See also: ftp://sirius.astrouw.edu.pl/ogle : OGLE DataBase http://www.astro.princeton.edu/~sumi/QSO-OGLEII : Home Page of the paper J/AcA/52/129 : DIA OGLE2 candidate variable stars catalog (Wozniak+ 2002) Byte-by-byte Description of file: table2.dat
Bytes Format Units Label Explanations
1- 2 I2 --- Field Field number (field name is BUL_SC NN) 4- 7 I4 ---- VID Variable number, in the field (1) 10- 15 I6 --- ID Identification number, in the field (2) 17- 23 F7.2 pix Xpos X position 25- 31 F7.2 pix Ypos Y position 33- 34 I2 h RAh Right ascension (J2000) 36- 37 I2 min RAm Right ascension (J2000) 39- 43 F5.2 s RAs Right ascension (J2000) 45 A1 --- DE- Declination sign (J2000) 46- 47 I2 deg DEd Declination (J2000) 49- 50 I2 arcmin DEm Declination (J2000) 52- 55 F4.1 arcsec DEs Declination (J2000) 58- 63 F6.3 mag Imag I magnitude 65- 69 F5.3 mag V-I ?=9.999 V-I colour index 71- 76 F6.3 mag Icmag ?=99.999 Extinction corrected I magnitude 78- 83 F6.3 mag (V-I)c ?=9.999 Extinction corrected V-I colour index 85- 89 F5.3 --- Svar Variogram slope (3)
Note (1): Numbering of Udalski et al, 2002, Cat. J/AcA/52/217, OGLEII DIA BUL-SCNN NNNN in Simbad Note (2): OGLE BUL-SCNN NNNNNN in Simbad Note (3): The larger Svar, the larger the variability on larger time-scales.
History: * 07-Feb-2006: Copied at http://www.astro.princeton.edu/~sumi/QSO-OGLEII
(End) Patricia Vannier [CDS] 07-Feb-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

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