J/A+A/591/A96     Robust detection of CID double stars in SDSS (Pourbaix+, 2016)

Robust detection of CID double stars in SDSS. Pourbaix D., Knapp G.R., Gunn J.E., Lupton R.H., Ivezic Z., Siopis C., Rigaux M., Rubens A. <Astron. Astrophys. 591, A96 (2016)> =2016A&A...591A..96P 2016A&A...591A..96P (SIMBAD/NED BibCode)
ADC_Keywords: Stars, double and multiple ; Positional data ; Photometry, SDSS Keywords: binaries: general - astrometry - methods: data analysis Abstract: The Sloan Digital Sky Survey (SDSS) offers a unique possibility of not only detecting colour induced displacement (CID) double stars but also confirming these detections. Successive cuts are applied to the SDSS data release (DR) 12 database to reduce the size of the sample under consideration. The resulting dataset is then screened with a criterion based on the distance and orientation of the photocentres in different photometric bands. About 3200 distinct objects are classified as CID double stars, 40 of which are confirmed with at least a second detection. A consistency check further validates these detections. Description: Whereas the possibility of detecting CID double stars with SDSS has been known for more than a decade, the absence of repeated observation (in particular of CID candidates) has prevented the validation of the technique, despite its easy setup. We have shown here that some CID are confirmed by at least a second observation. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file catalog.dat 102 3212 Identified CID with their THING Id, position, and SDSS dereddened magnitude for the five photometric bands table2.dat 70 3273 Accepted CID observations for the candidates listed in Table 1 with their THING Id, objectId, date, and offsets in right ascension -------------------------------------------------------------------------------- See also: http://www.sdss.org : SDSS Home page Byte-by-byte Description of file: catalog.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 4 A4 --- --- [SDSS] 5- 23 A19 --- SDSS SDSS designation (JHHMMSS.ss+DDMMSS.s) 25- 33 I9 --- ID Primary key for any SDSS object, THING ID 35- 44 F10.6 deg RAdeg Right ascension (J2000) 46- 55 F10.6 deg DEdeg Declination (J2000) 57 I1 --- N Number of observations flagged as CID 59- 66 F8.4 mag u*mag0 Dereddened SDSS u* magnitude 68- 75 F8.4 mag g*mag0 Dereddened SDSS g* magnitude 77- 84 F8.4 mag r*mag0 Dereddened SDSS r* magnitude 86- 93 F8.4 mag i*mag0 Dereddened SDSS i* magnitude 95-102 F8.4 mag z*mag0 Dereddened SDSS z* magnitude -------------------------------------------------------------------------------- Byte-by-byte Description of file: table2.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 9 I9 --- ID Primary key for any SDSS object, THING ID 11- 29 I19 --- objID Unique identifier for any SDSS observation 31- 38 F8.2 d MJD epoch of the observation 40- 46 F7.4 arcsec oRAu Offset in right ascension in the u band (1) 48- 54 F7.4 arcsec oDEu Offset in declination in the u band (1) 56- 62 F7.4 arcsec oRAz Offset in right ascension in the z band (1) 64- 70 F7.4 arcsec oDEz Offset in declination in the z band (1) -------------------------------------------------------------------------------- Note (1): Offset in RA*cos(DE) and declination in the u and z bands with respect to the position in the r band. -------------------------------------------------------------------------------- Acknowledgements: Dimitri Pourbaix, pourbaix(at)astro.ulb.ac.be
(End) Dimitri Pourbaix [FNRS, ULB, Belgium], Patricia Vannier [CDS] 24-May-2016
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