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J/MNRAS/306/592 UBVR CCD sequences for wide-field surveys. II. (Croom+, 1999)
Faint UBVRI CCD sequences for wide-field surveys. II. UBVR sequences at δ=-30° Croom S.M., Ratcliffe A., Parker Q.A., Shanks T., Boyle B.J., Smith R.J. <Mon. Not. R. Astron. Soc. 306, 592 (1999)> =1999MNRAS.306..592C (SIMBAD/NED BibCode)
ADC_Keywords: Photometry, UBVRI ; Surveys Keywords: techniques: photometric - catalogues Abstract: We present results from a continuing campaign to secure deep multi-colour CCD sequences for photoelectric calibration in UK Schmidt fields with galactic latitudes |b|>50°. In this paper, we present UBVR photometry in 12 fields and BR photometry in a further 14 fields observed within UK Schmidt survey fields centered at δ=-30°. Our observations were carried out with the 0.9m Telecope at the Cerro-Tololo Inter-American Observatory. File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file tables.dat 107 1323 UBVR photometry
See also: J/MNRAS/276/33 : UBVRI CCD sequences for wide-field surveys. I. (Boyle+ 1995) Byte-by-byte Description of file: tables.dat
Bytes Format Units Label Explanations
1- 9 A9 --- Object Object designation (fNNNN-NNN) 11- 12 I2 h RAh Right ascension (J2000.0) 14- 15 I2 min RAm Right ascension (J2000.0) 17- 21 F5.2 s RAs Right ascension (J2000.0) 23 A1 --- DE- Declination sign (J2000.0) 24- 25 I2 deg DEd Declination (J2000.0) 27- 28 I2 arcmin DEm Declination (J2000.0) 30- 33 F4.1 arcsec DEs Declination (J2000.0) 35- 39 F5.2 mag Bmag B magnitude 41- 44 F4.2 mag e_Bmag rms uncertainty on Bmag 46- 50 F5.2 mag B25mag B 25 pixel aperture magnitude (1) 52- 56 F5.2 --- s/g Star galaxy separation parameter b_10_-b_6_ (2) 58- 62 F5.2 mag Umag U magnitude 64- 67 F4.2 mag e_Umag rms uncertainty on Umag 69- 73 F5.2 mag U25mag U 25 pixel aperture magnitude (1) 75- 79 F5.2 mag Vmag V magnitude 81- 84 F4.2 mag e_Vmag rms uncertainty on Vmag 86- 90 F5.2 mag V25mag V 25 pixel aperture magnitude (1) 92- 96 F5.2 mag Rmag R magnitude 98-101 F4.2 mag e_Rmag rms uncertainty on Rmag 103-107 F5.2 mag R25mag R 25 pixel aperture magnitude (1)
Note (1): 25 pixel aperture magnitudes give good estimates of total galaxy magnitude for galaxies with isophotal diameter less than 20". Note (2): Generally, objects with b10-b6 < -0.2 will be galaxies, although this does vary somewhat from field to field, depending on the seeing in each observation.
History: Copied on 22-Apr-1999 at http://icstar5.ph.ic.ac.uk:80/~scroom/phot/photom.html
(End) Patricia Bauer [CDS] 21-Apr-1999
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