Variable point sources in SDSS stripe 82. I. (Bhatti+, 2010)

Details Variable point sources in SDSS stripe 82. I. (Bhatti+, 2010) Variable point sources in SDSS stripe 82. I. (Bhatti+, 2010)

Apr 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010ycat..21860233b&link_type=abstract

VizieR On-line Data Catalog: J/ApJS/186/233. Originally published in: 2010ApJS..186..233B

Physics

Binaries: Eclipsing, Stars: Variable, Surveys, Photometry: Ugriz, Photometry: Sdss

Scientific paper

The SDSS uses a dedicated 2.5m telescope located at the Apache Point Observatory in New Mexico. Stripe 82 is on the celestial equator, ranging from 20hr to 4hr in right ascension and -1.27° to +1.27° in declination, for a total area of about 300deg2. The Stripe has been observed many times over the 10 years of operation of SDSS and SDSS-II, mostly during the fall (September-December).
(3 data files).

Affiliated with

Also associated with

No associations

Rating

Variable point sources in SDSS stripe 82. I. (Bhatti+, 2010) 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 Variable point sources in SDSS stripe 82. I. (Bhatti+, 2010), we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Variable point sources in SDSS stripe 82. I. (Bhatti+, 2010) will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1191520