The Carousel Lens I: A Spectroscopic Survey of the Carousel Lens Field
astro-ph.GA, astro-ph.CO
Submitted: 2026-01-20
Updated: 2026-09-08
Comments: 17 pages, 10 figures, 4 tables. Published in the Open Journal of Astrophysics
License: http://creativecommons.org/licenses/by/4.0/
The gist: We present a spectroscopic survey of field galaxies and lensed sources in the vicinity of the strong lensing galaxy cluster known as the Carousel lens at z=0.49.
Terminology
Abstract
We present a spectroscopic survey of field galaxies and lensed sources in the vicinity of the strong lensing galaxy cluster known as the Carousel lens at z=0.49. Using both Gemini/GMOS slitmask spectra and deep VLT/MUSE observations, we bring the total number of lensed sources up to 12, including three which were not previously known from imaging observations but are apparent in the MUSE data as emission-line sources. Of these sources, 10 have confident redshifts, and an additional 2 have tentative redshifts from likely Ly α emission (including seven new redshifts determined here adding to those presented previously in). In total, we identify 42 images of these 12 sources. This lens system is remarkably symmetric and well-modeled by a simpler lens model than typical cluster lenses, and the large number of sources and their large range of redshifts make this cluster ideal for constraining cosmological parameters such as w and Ω m as well as the cluster density profile. Additionally, we present a catalog of 57 unlensed field galaxies with confident redshifts, of which 49 are associated with the cluster. We measure a cluster velocity dispersion of about 1100 km s-1 from which we estimate a halo mass M 200c about 1.2 times 10 15 M.
Sources
- Constraining the dark energy equation of state with double source plane strong lenses
- Cosmological Constraints from Strong Gravitational Lensing in Galaxy Clusters
- CLASH-VLT: A Highly Precise Strong Lensing Model of the Galaxy Cluster RXC J2248.7-4431 (Abell S1063) and Prospects for Cosmography
- Galaxy cluster strong lensing cosmography: cosmological constraints from a sample of regular galaxy clusters
- Cosmography from accurate mass modeling of the lens group SDSS J0100+1818: five sources at three different redshifts
- Cosmological Constraints from the double source plane lens SDSSJ0946+1006
- Cosmography with the Double Source Plane Strong Gravitational Lens AGEL150745+052256
- Constraining Cosmology with Double-source-plane Strong Gravitational Lenses from the AGEL Survey
- Discovering New Strong Gravitational Lenses in the DESI Legacy Imaging Surveys
- The DES Bright Arcs Survey: Candidate Strongly Lensed Galaxy Systems from the Dark Energy Survey 5,000 Sq. Deg. Footprint
- The MUSE second-generation VLT instrument
- ZAP -- Enhanced PCA Sky Subtraction for Integral Field Spectroscopy
- Gaia Data Release 3: Summary of the content and survey properties
- Velocity Dispersions of Clusters in the Dark Energy Survey Y3 redMaPPer Catalog
- Spectroscopic and X-ray Modeling of the Strong Lensing Galaxy Cluster MACS J0138.0-2155
- The serendipitous observation of a gravitationally lensed galaxy at z = 0.9057 from the Blanco Cosmology Survey: The Elliot Arc
- The Kaleidoscope Survey: Strong Gravitational Lensing in Galaxy Clusters with Radial Arcs
Related papers
- Apparent Stability in Self-Gravitating Turbulence and the Evolution of Molecular Clouds
- Two sets of potential-density basis pairs for the study of radial perturbations in collisionless spherical stellar systems
- Constraining reionization-era Ly alpha escape with JELS-MUSE: a highly complete H alpha-selected sample at z about6.1
- Deriving volume density profiles of filaments from observed surface densities
- Little Red Dots and Supermassive Black Hole Seed Formation in Ultralight Dark Matter Halos
- MEGATRON: how the first stars can create an iron metallicity plateau in the smallest dwarf galaxies