2014/05/30 by Zuzanna Kostrzewa-Rutkowska, Z. Kostrzewa-Rutkowska, Ł. Wyrzykowski +4 · 2 citations
Physics and Astronomy · #Astronomy #Astronomy and Astrophysical Research #Astrophysics #Galaxies: Formation, Evolution, Phenomena #Galaxy #Galaxy formation and evolution #Luminosity #Luminosity function #Physics #Redshift #Sky #Stellar, planetary, and galactic studies #Weak gravitational lensing #astro-ph.GA
paper · pdf · doi:10.1093/mnras/stu783
published as MNRAS (2014) 441, 3238
openalex publication_date 2014/05/30 · arxiv created 2014/06/04 · arxiv updated 2014/06/05 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05
We explore the properties of lensing galaxies and lensed faint sources at redshifts between 1.5 and 3.0. Our sample consists of nine, carefully selected strongly lensed galaxies discovered by the CASSOWARY (Cambridge And Sloan Survey Of Wide ARcs in the skY) survey in the Sloan Digital Sky Survey (SDSS) data. We find that, despite some limitations of the original SDSS data, the homogeneous sample of lensing systems can provide a useful insight into lens and source properties. We also explore the limitations of using low-resolution data to model and analyse galaxy–galaxy lensing. We derive the relative alignment of mass and light in fitted lens profiles. The range of magnification extends above 5; hence, we are able to analyse potentially small and low-mass galaxies at high redshifts. We confirm the likely evolution of the size–luminosity relation for blue star-forming galaxies as a function of redshift.