THE SDSS DISCOVERY OF A STRONGLY LENSED POST-STARBURST GALAXY AT z=0.766

نویسندگان

  • Min-Su Shin
  • Michael A. Strauss
  • Masamune Oguri
  • Naohisa Inada
  • Emilio E. Falco
  • Tom Broadhurst
  • James E. Gunn
چکیده

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 poststarburst galaxy at z = 0.766. The lensing galaxy has an estimated mass of ∼ 1.2× 10 M⊙ and the corresponding mass to light ratio in the B-band is ∼ 26 M⊙/L⊙ 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. Subject headings: gravitational lensing — galaxies

برای دانلود رایگان متن کامل این مقاله و بیش از 32 میلیون مقاله دیگر ابتدا ثبت نام کنید

ثبت نام

اگر عضو سایت هستید لطفا وارد حساب کاربری خود شوید

منابع مشابه

A New Einstein Cross: a Highly Magnified, Intrinsically Faint Lyman-alpha Emitter at Z = 2.7

We report the discovery of a new Einstein cross at redshift zS = 2.701 based on Lyα emission in a cruciform configuration around an SDSS luminous red galaxy (zL = 0.331). The system was targeted as a possible lens based on an anomalous emission line in the SDSS spectrum. Imaging and spectroscopy from the W.M. Keck Observatory confirm the lensing nature of this system. This is one of the widest-...

متن کامل

A New Gravitational Lens Candidate with Large Image Separation in the SDSS DR5 Data

The discovery of a gravitational lens candidate is reported. The quasars SDSS J111611.73+411821.5 and SDSS J111610.68+411814.4 are recognized as two images of the same object, being strongly lensed by the closer galaxy SDSS J111611.03+411820.9. The source is located at a redshift of z ∼ 3, while the redshift of the lens galaxy is z ∼ 0.25. The separation of the images is large, ∼ 13 arcsec. Com...

متن کامل

Discovery of Multiply Imaged Galaxies behind the Cluster and Lensed Quasar

We have identified three multiply imaged galaxies in Hubble Space Telescope images of the redshift z = 0.68 cluster responsible for the large-separation quadruply lensed quasar, SDSS J1004+4112. Spectroscopic redshifts have been secured for two of these systems using the Keck I 10m telescope. The most distant lensed galaxy, at z = 3.332, forms at least four images, and an Einstein ring encompas...

متن کامل

Lyman Break Galaxies in the Sloan Digital Sky Survey First Data Release

We report the discovery of six compact, starburst galaxies with redshifts 2.3 < z < 2.8 and r-band magnitudes 19.8−20.5 in the Quasar Catalog of the Sloan Digital Sky Survey First Data Release (SDSS DR1). The SDSS spectra of these objects resemble the composite spectrum of Lyman Break Galaxies (LBGs) at z ≈ 3, but the galaxies are 4−5 magnitudes brighter than an “L∗” LBG and 2 − 3 magnitudes br...

متن کامل

A Redline Starburst: Co(2–1) Observations of an Eddington-limited Galaxy Reveal Star Formation at Its Most Extreme

We report observations of the CO(2–1) emission of SDSS J1506+54, a compact (re ≈ 135 pc) starburst galaxy at z = 0.6. SDSS J1506+54 appears to be forming stars close to the limit allowed by stellar radiation pressure feedback models: the measured LIR/L′CO ≈ 1500 is one of the highest measured for any galaxy. With its compact optical morphology but extended low surface brightness envelope, post-...

متن کامل

ذخیره در منابع من


  با ذخیره ی این منبع در منابع من، دسترسی به آن را برای استفاده های بعدی آسان تر کنید

عنوان ژورنال:

دوره   شماره 

صفحات  -

تاریخ انتشار 2008