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J/A+AS/130/359 Faint photometric BVR CCD sequences (Spagna+ 1998)
Faint photometric BVRc CCD sequences. The North Galactic Pole (b=85 deg) and the anticenter (l=133.2, b=-1.6 deg) Spagna A., Lattanzi M.G., McLean B.J., Massone G., Lasker B.M. <Astron. Astrophys. Suppl. Ser. 130, 359 (1998)> =1998A&AS..130..359S (SIMBAD/NED BibCode)
ADC_Keywords: Photometry, CCD ; Photometry, standards Keywords: catalogs - Galaxy: structure - techniques: photometric Description: CCD photometric standard stars in the BVRc system of Johnson and Cousins are presented for two regions of importance in studies of galactic structure and kinematics: the North galactic pole (NGP), and a second galactic plane region (GPR) toward the anticenter. Precision and accuracy are better than 0.05mag down to V=18-18.5. These data are part of the Second Guide Photometric Catalog (GSPC-II). File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table3.dat 67 56 NGP: photometry and position of the CCD standards in fields I, II, III table4.dat 67 207 GPR: photometry and position of the CCD standards tables.tex 94 334 LaTeX version of tables 3 and 4
Byte-by-byte Description of file: table3.dat table4.dat
Bytes Format Units Label Explanations
1- 14 A14 --- IdPOSS Identifier on POSS plate 17- 22 A6 --- IdCCD Identifier on CCD frames (1) 24- 30 F7.3 mag Vmag V Johnson magnitude 32- 37 F6.3 mag B-V B-V Johnson color index 39- 44 F6.3 mag V-R V-R Johnson-Cousins color index 47- 48 I2 h RAh Right Ascension (J2000) 50- 51 I2 min RAm Right Ascension (J2000) 53- 56 F4.1 s RAs Right Ascension (J2000) 59 A1 --- DE- Declination sign 60- 61 I2 deg DEd Declination (J2000) 63- 64 I2 arcmin DEm Declination (J2000) 66- 67 I2 arcsec DEs Declination (J2000)
Note (1): The format of the CCD identifier is nnn-N, where nnn is a progressive index, while N = I,II,III identifies three different close CCD fields.
Acknowledgements: Alessandro Spagna Historical Notes: CCD data were taken at Mt. Hopkins using the 1.2m telescope. The GPR (table4) was observed on October 15 1993, while the NGP fields (table3) were imaged on June 5 1994. References: Krzeminski W., Serkowski K., 1967ApJ...147..988K Postman M., et al., 1992, Digitalized Optical Sky Surveys, Mac Gillivray and Thomson eds., 61-63 Reid N., et al., 1991PASP..103..661R Spagna A. et al., 1996A&A...311..758S Straizys V., Multicolor stellar photometry, 1992, Ed. Pachart Publishing House
(End) A. Spagna [Obs. Astron. Torino] 5-Jan-1998
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