The Sloan Bright Arcs Survey: Four Strongly Lensed Galaxies with Redshift >2
arXiv:0910.4600 · doi:10.1088/0004-637X/707/1/686
Abstract
We report the discovery of four very bright, strongly-lensed galaxies found via systematic searches for arcs in Sloan Digital Sky Survey Data Release 5 and 6. These were followed-up with spectroscopy and imaging data from the Astrophysical Research Consortium 3.5m telescope at Apache Point Observatory and found to have redshift . With isophotal magnitudes and $3\arcsec$-diameter magnitudes , these systems are some of the brightest and highest surface brightness lensed galaxies known in this redshift range. In addition to the magnitudes and redshifts, we present estimates of the Einstein radii, which range from $5.0 \arcsec$ to $12.7 \arcsec$, and use those to derive the enclosed masses of the lensing galaxies.
References in corpus (12)
- The Sloan Lens ACS Survey. V. The Full ACS Strong-Lens Sample
- The CFHTLS Strong Lensing Legacy Survey: I. Survey overview and T0002 release sample
- Rest-Frame Optical Spectra of Three Strongly Lensed Galaxies at z~2
- First catalog of strong lens candidates in the COSMOS field
- A New Survey for Giant Arcs
- A very bright, highly magnified Lyman-break galaxy at z=3.07
- Two New Large Separation Gravitational Lenses from SDSS
- Gravitational lenses and lens candidates identified from the COSMOS field
- Discovery of A Very Bright, Strongly-Lensed z=2 Galaxy in the SDSS DR5
- The Sloan Bright Arcs Survey : Six Strongly Lensed Galaxies at z=0.4-1.4
- The OLS-lens survey: The discovery of five new galaxy-galaxy strong lenses from the SDSS
- Discovery of four gravitational lensing systems by clusters in the SDSS DR6
Cited by in corpus (43)
- The Cosmic BPT Diagram: Confronting Theory with Observations
- Cluster Lenses
- Validation of the equilibrium model for galaxy evolution to z~3 through molecular gas and dust observations of lensed star-forming galaxies
- Combined strong and weak lensing analysis of 28 clusters from the Sloan Giant Arcs Survey
- Evidence for Wide-Spread AGN Driven Outflows in the Most Massive z~1-2 Star Forming Galaxies
- Ultraviolet Emission Lines in Young Low Mass Galaxies at z~2: Physical Properties and Implications for Studies at z>7
- Constraining the metallicities, ages, star formation histories, and ionizing continua of extragalactic massive star populations
- Gravitationally Lensed Galaxies at 2<z<3.5: Direct Abundance Measurements of Lya Emitters
- Space Warps: I. Crowd-sourcing the Discovery of Gravitational Lenses
- The Physical Conditions, Metallicity and Metal Abundance Ratios In a Highly Magnified Galaxy at z = 3.6252
- The Low Mass End of the Fundamental Relation for Gravitationally Lensed Star Forming Galaxies at 1<z<6
- The CASSOWARY spectroscopy survey: A new sample of gravitationally lensed galaxies in SDSS
- Rest-frame ultraviolet spectrum of the gravitationally lensed galaxy `the 8 o'clock arc': stellar and interstellar medium properties
- Gemini/GMOS Spectroscopy of 26 Strong Lensing Selected Galaxy Cluster Cores
- Strong Lens Models for 37 Clusters of Galaxies from the SDSS Giant Arcs Survey
- LBT/LUCIFER Observations of the z~2 Lensed Galaxy J0900+2234
- Arc Statistics
- The Magellan Evolution of Galaxies Spectroscopic and Ultraviolet Reference Atlas (MEGaSaURA) I: The Sample and the Spectra
- Broadband Photometry of 105 Giant Arcs: Redshift Constraints and Implications for Giant Arc Statistics
- Discovery of the Lensed Quasar System DES J0408-5354
- The Sloan Bright Arcs Survey : Discovery of Seven New Strongly Lensed Galaxies from z=0.66-2.94
- From Nuclear to Circumgalactic: Zooming in on AGN-Driven Outflows at z~2.2 with SINFONI
- Observation and Confirmation of Six Strong Lensing Systems in The Dark Energy Survey Science Verification Data
- Resolved Molecular Gas and Star Formation Properties of the Strongly Lensed z=2.26 Galaxy SDSS J0901+1814
- Two Lensed Lyman-alpha Emitting Galaxies at z~5
- The Sloan Bright Arcs Survey: Ten Strong Gravitational Lensing Clusters and Evidence of Overconcentration
- A ~600 pc view of the strongly-lensed, massive main sequence galaxy J0901: a baryon-dominated, thick turbulent rotating disk with a clumpy cold gas ring at z = 2.259
- Lensing clusters of galaxies in the SDSS-III
- The serendipitous observation of a gravitationally lensed galaxy at z = 0.9057 from the Blanco Cosmology Survey: The Elliot Arc
- Identification of Galaxy-Galaxy Strong Lens Candidates in the DECam Local Volume Exploration Survey Using Machine Learning
- Mid-Infrared Spectroscopy of Two Lensed Star-forming Galaxies
- The DES Bright Arcs Survey: Candidate Strongly Lensed Galaxy Systems from the Dark Energy Survey 5,000 Sq. Deg. Footprint
- Spectroscopy of CASSOWARY gravitationally-lensed galaxies in SDSS: characterisation of an extremely bright reionization-era analog at
- Herschel Extreme Lensing Line Observations: Dynamics of two strongly lensed star forming galaxies near redshift z = 2
- A UV Ultra-luminous Lyman Break Galaxy at Z=2.78 in NDWFS Bootes Field
- Efficient Mass Estimate at the Core of Strong Lensing Galaxy Clusters Using the Einstein Radius
- Searching for Cooling Signatures in Strong Lensing Galaxy Clusters: Evidence Against Baryons Shaping the Matter Distribution in Cluster Cores
- LBT/ARGOS adaptive optics observations of z lensed galaxies
- Observation and Confirmation of Nine Strong Lensing Systems in Dark Energy Survey Year 1 Data
- Optimizing machine learning methods to discover strong gravitational lenses in the Deep Lens Survey
- Pixel-level modelling of group-scale strong lens CASSOWARY 19
- Molecular gas budget of strongly magnified low-mass star-forming galaxies at cosmic noon
- Core Mass Estimates in Strong Lensing Galaxy Clusters: a Comparison Between Masses Obtained from Detailed Lens Models, Single-Halo Lens Models, and Einstein Radii