Most Strong Lensing Deflectors in the AGEL Survey Are in Group and Cluster Environments
William J. Gottemoller, Nandini Sahu, Rodrigo Cordova-Rosado, Leena Iwamoto, Courtney B. Watson, Kim-Vy H. Tran, A. Makai Baker, Tania M. Barone, Duncan J. Bowden, Karl Glazebrook, Anishya Harshan, Tucker Jones, Glenn G. Kacprzak, and Camryn M. Neches

TL;DR
This study analyzes the environments of strong lensing deflectors in the AGEL survey, revealing many are in dense group and cluster environments, which impacts lens modeling and cosmological tests.
Contribution
It provides the first comprehensive measurement of deflector environments and Einstein masses for a large sample of strong lenses, highlighting environmental effects on lens properties.
Findings
47.2% of deflectors are in cluster environments
Weak correlation (r=0.38) between Einstein mass and galaxy surface density
AGEL deflectors are in denser environments than control fields
Abstract
The environments of deflectors in strong lensing systems affect our ability to test cosmological models and constrain evolutionary properties of galaxies. Here we measure the deflector scale (Einstein mass) and deflector environment (halo mass) of 89 spectroscopically confirmed strong lenses in the ASTRO3D Galaxy Evolution With Lenses (AGEL) survey. We classify deflector scale by measuring to determine the mass enclosed by the Einstein radius, . We quantify deflector environment by using photometric redshifts to determine the galaxy surface density to the fifth-nearest neighbor . We find that 47.2% of our deflectors are embedded in cluster environments, whereas only 9.0% have cluster-scale Einstein radii (masses). We measure a weak correlation () between Einstein mass and , suggesting that the assumption of…
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Taxonomy
TopicsGalaxies: Formation, Evolution, Phenomena · Astronomy and Astrophysical Research · Stellar, planetary, and galactic studies
