4.7 Article

THE BOSS EMISSION-LINE LENS SURVEY (BELLS). I. A LARGE SPECTROSCOPICALLY SELECTED SAMPLE OF LENS GALAXIES AT REDSHIFT ∼0.5

Journal

ASTROPHYSICAL JOURNAL
Volume 744, Issue 1, Pages -

Publisher

IOP Publishing Ltd
DOI: 10.1088/0004-637X/744/1/41

Keywords

galaxies: distances and redshifts; galaxies: evolution; galaxies: high-redshift; gravitational lensing: strong; large-scale structure of universe; surveys

Funding

  1. NASA/ESA Hubble Space Telescope
  2. Space Telescope Science Institute
  3. NASA [NAS 5-26555]
  4. NASA from the Space Telescope Science Institute
  5. NSF [AST-1004756]
  6. STFC [ST/I001204/1] Funding Source: UKRI
  7. Science and Technology Facilities Council [ST/I001204/1] Funding Source: researchfish
  8. Direct For Mathematical & Physical Scien
  9. Division Of Astronomical Sciences [1009756] Funding Source: National Science Foundation

Ask authors/readers for more resources

We present a catalog of 25 definite and 11 probable strong galaxy-galaxy gravitational lens systems with lens redshifts 0.4 less than or similar to z less than or similar to 0.7, discovered spectroscopically by the presence of higher-redshift emission lines within the Baryon Oscillation Spectroscopic Survey (BOSS) of luminous galaxies, and confirmed with high-resolution Hubble Space Telescope (HST) images of 44 candidates. Our survey extends the methodology of the Sloan Lens Advanced Camera for Surveys survey (SLACS) to higher redshift. We describe the details of the BOSS spectroscopic candidate detections, our HST ACS image processing and analysis methods, and our strong gravitational lens modeling procedure. We report BOSS spectroscopic parameters and ACS photometric parameters for all candidates, and mass-distribution parameters for the best-fit singular isothermal ellipsoid models of definite lenses. Our sample to date was selected using only the first six months of BOSS survey-quality spectroscopic data. The full five-year BOSS database should produce a sample of several hundred strong galaxy-galaxy lenses and in combination with SLACS lenses at lower redshift, strongly constrain the redshift evolution of the structure of elliptical, bulgedominated galaxies as a function of luminosity, stellar mass, and rest-frame color, thereby providing a powerful test for competing theories of galaxy formation and evolution.

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