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J/MNRAS/327/601     OGLE-II High proper motion stars          (Eyer+, 2001)

Photometric detection of high proper motions in dense stellar fields using Difference Image Analysis. Eyer L., Wozniak P.R. <Mon. Not. R. Astron. Soc. 327, 601 (2001)> =2001MNRAS.327..601E
ADC_Keywords: Stars, variable ; Proper motions Keywords: methods: data analysis - techniques: photometric - astrometry - stars: variables: other Abstract: The difference image analysis (DIA) of the images obtained by the Optical Gravitational Lensing Experiment (OGLE-II) revealed a peculiar artefact in the sample of stars proposed as variable by Woniak in one of the Galactic bulge fields: the occurrence of pairs of candidate variables showing anti-correlated light curves monotonic over a period of 3 yr. This effect can be understood, quantified and related to the stellar proper motions. DIA photometry supplemented with a simple model offers an effective and easy way to detect high proper motion stars in very dense stellar fields, where conventional astrometric searches are extremely inefficient. File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table1.dat 68 74 HPM stars found in the OGLE bulge field SC1
See also: J/AcA/51/175 : OGLE-II DIA microlensing events (Wozniak+, 2001) J/AcA/50/421 : OGLE-II DIA data (Wozniak+, 2000) Byte-by-byte Description of file: table1.dat
Bytes Format Units Label Explanations
1- 4 I4 --- Name1 First OGLE BUL-SC1 number of the pair 5 A1 --- --- [-] 6- 9 I4 --- Name2 Second OGLE BUL-SC1 number of the pair 11- 15 F5.2 mag Imag I magnitude 17- 18 I2 h RAh Right ascension (J2000) 20- 21 I2 min RAm Right ascension (J2000) 23- 27 F5.2 s RAs Right ascension (J2000) 29 A1 --- DE- Declination sign (J2000) 30- 31 I2 deg DEd Declination (J2000) 33- 34 I2 arcmin DEm Declination (J2000) 36- 39 F4.1 arcsec DEs Declination (J2000) 41- 45 F5.1 mas/yr pmRA Proper motion in right ascension 47- 49 F3.1 mas/yr e_pmRA rms uncertainty on pmRA 51- 55 F5.1 mas/yr pmDE Proper motion in declination 57- 59 F3.1 mas/yr e_pmDE rms uncertainty on pmDE 61- 64 F4.1 mas/yr pm Total proper motion 66- 68 F3.1 mas/yr e_pm rms uncertainty on pm
History: From electronic version of the journal
(End) James Marcout, Patricia Bauer [CDS] 20-Jan-2003
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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