BVRI CCD photometry in the field of M 31 (Magnier+ 1992)

Details BVRI CCD photometry in the field of M 31 (Magnier+ 1992) BVRI CCD photometry in the field of M 31 (Magnier+ 1992)

Sep 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996ycat.2208....0m&link_type=abstract

VizieR On-line Data Catalog: II/208. Originally published in: 1992A&AS...96..379M; 1993A&A...272..695M; 1994A&A...286..725H

Astronomy and Astrophysics

Astronomy

Photometry: Ccd, Regional Catalog, Stars: Faint

Scientific paper

Deep BVRI CCD photometry was performed on a 1 square degree region of M31. The observations were made between September 12 and September 27, 1990, using the McGraw-Hill 1.3m telescope at the Michigan-Dartmouth-MIT (MDM) observatory at Kitt Peak. The catalogue has typical completion limits of 22.3Bmag, 22.2Vmag, 22.2Rmag and 20.9Imag. Photometric accuracy is about 2% at Vmag=19. The final astrometric calibrations take into account the systematic error discovered in the Berkhuijsen etal (1987) catalog (Magnier etal 1993). They are in the J2000 system and are eventually tied to the HST Guide Star Catalog. The final photometric calibrations are tied via the NGC 206 region to photometry taken at the Michigan-Dartmouth-MIT (MDM) 1.3m in September and October 1993. These are tied to the Landolt (1992) system of standard stars, and are in the Johnson-Kron-Cousins system (BVRcIc). (3 data files).

Affiliated with

Also associated with

No associations

Rating

BVRI CCD photometry in the field of M 31 (Magnier+ 1992) does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with BVRI CCD photometry in the field of M 31 (Magnier+ 1992), we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and BVRI CCD photometry in the field of M 31 (Magnier+ 1992) will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-998590