The SDSS Discovery of a Strongly Lensed Post-Starburst Galaxy at z=0.766

Astronomy and Astrophysics – Astrophysics

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

Accepted for publication in AJ

Scientific paper

10.1088/0004-6256/136/1/44

We present the first result of a survey for strong galaxy-galaxy lenses in Sloan Digital Sky Survey (SDSS) images. SDSS J082728.70+223256.4 was selected as a lensing candidate using selection criteria based on the color and positions of objects in the SDSS photometric catalog. Follow-up imaging and spectroscopy showed this object to be a lensing system. The lensing galaxy is an elliptical at z = 0.349 in a galaxy cluster. The lensed galaxy has the spectrum of a post-starburst galaxy at z = 0.766. The lensing galaxy has an estimated mass of $\sim 1.2 \times 10^{12} M_{\odot}$ and the corresponding mass to light ratio in the B-band is $\sim 26 M_{\odot}/L_{\odot}$ inside 1.1 effective radii of the lensing galaxy. Our study shows how catalogs drawn from multi-band surveys can be used to find strong galaxy-galaxy lenses having multiple lens images. Our strong lensing candidate selection based on photometry-only catalogs will be useful in future multi-band imaging surveys such as SNAP and LSST.

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

The SDSS Discovery of a Strongly Lensed Post-Starburst Galaxy at z=0.766 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 The SDSS Discovery of a Strongly Lensed Post-Starburst Galaxy at z=0.766, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The SDSS Discovery of a Strongly Lensed Post-Starburst Galaxy at z=0.766 will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-574864

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