BVI photometry in NGC 300 (Pietrzynski+, 2002)

Details BVI photometry in NGC 300 (Pietrzynski+, 2002) BVI photometry in NGC 300 (Pietrzynski+, 2002)

Apr 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002ycat..61140298p&link_type=abstract

VizieR On-line Data Catalog: J/PASP/114/298. Originally published in: 2002PASP..114..298P

Other

Galaxies: Photometry, Stars: Standard, Photometry: Ubvri

Scientific paper

Based on 13 nights of observations of four fields in NGC 300, we have set up an extensive sequence of stars with accurate BVI photometry covering a relatively large (25'x25') region centered on this galaxy. This sequence of standard stars is very useful for calibrating the photometry of variable stars and other objects in NGC 300 and other galaxies obtained from wide-field mosaic images. Our standard-star list contains B, V, and I measurements for 390 stars. The accuracy of the zero points in the V filter and B-V color is better than 0.02mag, and about 0.03mag for the V-I color. We found very good agreement between our measurements and those previously obtained by Walker for 26 stars near NGC 300.
(1 data file).

Affiliated with

Also associated with

No associations

Rating

BVI photometry in NGC 300 (Pietrzynski+, 2002) 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 BVI photometry in NGC 300 (Pietrzynski+, 2002), we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and BVI photometry in NGC 300 (Pietrzynski+, 2002) will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1590253