The Astrophysical Journal (Jan 2025)

COOL-LAMPS. VII. Quantifying Strong-lens Scaling Relations with 177 Cluster-scale Strong Gravitational Lenses in DECaLS

  • Simon D. Mork,
  • Michael D. Gladders,
  • Gourav Khullar,
  • Keren Sharon,
  • Nathalie Chicoine,
  • Aidan P. Cloonan,
  • Håkon Dahle,
  • Diego Garza,
  • Rowen Glusman,
  • Katya Gozman,
  • Gabriela Horwath,
  • Benjamin C. Levine,
  • Olina Liang,
  • Daniel Mahronic,
  • Viraj Manwadkar,
  • Michael N. Martinez,
  • Alexandra Masegian,
  • Owen S. Matthews Acuña,
  • Kaiya Merz,
  • Yue Pan,
  • Jorge A. Sanchez,
  • Isaac Sierra,
  • Daniel J. Kavin Stein,
  • Ezra Sukay,
  • Marcos Tamargo-Arizmendi,
  • Kiyan Tavangar,
  • Ruoyang Tu,
  • Grace Wagner,
  • Erik A. Zaborowski,
  • Yunchong Zhang,
  • (COOL-LAMPS Collaboration)

DOI
https://doi.org/10.3847/1538-4357/ada24c
Journal volume & issue
Vol. 979, no. 2
p. 184

Abstract

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We estimate the Einstein-radius-enclosed total mass for 177 cluster-scale strong gravitational lenses identified by the ChicagO Optically selected Lenses Located At the Margins of Public Surveys (COOL-LAMPS) collaboration with lens redshifts ranging from 0.2 ⪅ z ⪅ 1.0 using the brightest-cluster-galaxy (BCG) redshift and an observable proxy for the Einstein radius. We constrain the Einstein-radius-enclosed luminosity and stellar mass by fitting parametric spectral energy distributions to aperture photometry from the Dark Energy Camera Legacy Survey (DECaLS) in the g -, r -, and z -band Dark Energy Camera filters. We find that the BCG redshift, enclosed total mass, and enclosed luminosity are strongly correlated and well described by a planar relationship in 3D space. We find that the enclosed total mass and stellar mass are correlated with a logarithmic slope of $0.50{0}_{-0.031}^{+0.029}$ , and the enclosed total mass and stellar-to-total mass fraction are correlated with a logarithmic slope of $-0.49{5}_{-0.033}^{+0.032}$ . In tandem with the small radii within which these slopes are constrained, this may suggest invariance in baryon conversion efficiency and feedback strength as a function of cluster-centric radii in galaxy clusters. Additionally, the correlations described here should have utility in ranking strong-lensing candidates in upcoming imaging surveys—such as Rubin/Legacy Survey of Space and Time—in which an algorithmic treatment of strong lenses will be needed due to the sheer volume of data these surveys will produce.

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