RR Lyrae Stars in the SDSS-II Supernova Survey

Other

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

1

Scientific paper

This report details the ongoing search for RR Lyrae stars in the Supernova Survey of the Sloan Digital Sky Survey (SDSS). The SDSS-II SN Survey covers a 2.5 degree equatorial stripe ranging from -60 to +60 degrees in RA. This corresponds to relatively high southern galactic latitudes in the anti-center direction. There are currently over five million detected objects in this survey. Many of these have nearly concurrent observations in all five ugriz filters. The current work contains data from SDSS-I calibration runs and the first year of the three year SN Survey. This represents on average roughly 20 epochs per object.
Using this sample, we explore spatial and period distributions of the RR Lyrae stars in the Galactic Halo. These distributions are compared to other surveys of RR Lyrae stars which concentrate on other components of the Galaxy. We will discuss the results to date and consider further analyses that will be conducted as this survey continues.
We would like to thank the NSF for partial support from grants AST 0607249 and AST 0406784 to Michigan State University.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

RR Lyrae Stars in the SDSS-II Supernova Survey 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 RR Lyrae Stars in the SDSS-II Supernova Survey, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and RR Lyrae Stars in the SDSS-II Supernova Survey will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-1162504

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.