Integral-field spectroscopy of SLACS lenses
Oliver Czoske, Matteo Barnabe, Leon Koopmans (Kapteyn Astronomical, Institute, Groningen, NL)

TL;DR
This study combines integral-field spectroscopy and gravitational lens modeling to analyze the internal structure and dark matter distribution of 17 early-type galaxies at moderate redshifts, enhancing understanding of galaxy evolution.
Contribution
It introduces a comprehensive approach integrating VIMOS integral-field data with HST imaging to study galaxy kinematics and dark matter in SLACS lenses.
Findings
Detailed phase-space reconstructions of early-type galaxies.
Constraints on dark matter distribution in galaxy cores.
Enhanced understanding of galaxy structure at intermediate redshifts.
Abstract
The combination of two-dimensional kinematics and gravitational lens modelling permits detailed reconstruction of the phase-space structure of early-type galaxies and sets constraints on the dark-matter distribution in their inner regions. We describe a project which combines integral-field spectroscopy from an ESO Large Programme using VIMOS on the VLT with deep HST ACS and NICMOS images to study a sample of 17 early-type lens galaxies at redshifts between 0.1 and 0.3, drawn from the Sloan Lens ACS survey (SLACS).
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
Taxonomy
TopicsAstronomy and Astrophysical Research · Adaptive optics and wavefront sensing · Stellar, planetary, and galactic studies
