COOL-LAMPS. VII. Quantifying Strong-lens Scaling Relations with 177 Cluster-scale Strong Gravitational Lenses in DECaLS
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-gal...
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| author | 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) |
| author_facet | 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) |
| author_sort | Simon D. Mork |
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| description | 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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| spelling | doaj-art-4c797dbff928484ab6c9fef834a261402025-01-27T13:18:25ZengIOP PublishingThe Astrophysical Journal1538-43572025-01-01979218410.3847/1538-4357/ada24cCOOL-LAMPS. VII. Quantifying Strong-lens Scaling Relations with 177 Cluster-scale Strong Gravitational Lenses in DECaLSSimon D. Mork0https://orcid.org/0000-0002-5573-9131Michael D. Gladders1https://orcid.org/0000-0003-1370-5010Gourav Khullar2https://orcid.org/0000-0002-3475-7648Keren Sharon3https://orcid.org/0000-0002-7559-0864Nathalie Chicoine4https://orcid.org/0009-0005-1143-495XAidan P. Cloonan5https://orcid.org/0000-0001-9978-2601Håkon Dahle6https://orcid.org/0000-0003-2200-5606Diego Garza7https://orcid.org/0009-0003-0226-6988Rowen Glusman8https://orcid.org/0000-0001-9816-0878Katya Gozman9https://orcid.org/0000-0003-2294-4187Gabriela Horwath10https://orcid.org/0009-0006-6950-6351Benjamin C. Levine11https://orcid.org/0000-0001-8000-1959Olina Liang12Daniel Mahronic13Viraj Manwadkar14https://orcid.org/0000-0002-7113-0262Michael N. Martinez15https://orcid.org/0000-0002-8397-8412Alexandra Masegian16https://orcid.org/0000-0002-3361-2893Owen S. Matthews Acuña17https://orcid.org/0000-0001-9225-972XKaiya Merz18https://orcid.org/0000-0001-5931-5056Yue Pan19https://orcid.org/0000-0002-7922-9726Jorge A. Sanchez20https://orcid.org/0000-0002-9142-6378Isaac Sierra21https://orcid.org/0000-0002-2323-303XDaniel J. Kavin Stein22https://orcid.org/0000-0001-8008-7270Ezra Sukay23https://orcid.org/0000-0002-1106-4881Marcos Tamargo-Arizmendi24https://orcid.org/0009-0008-0518-8045Kiyan Tavangar25https://orcid.org/0000-0001-6584-6144Ruoyang Tu26https://orcid.org/0009-0002-9963-7564Grace Wagner27https://orcid.org/0000-0003-0295-875XErik A. Zaborowski28https://orcid.org/0000-0002-6779-4277Yunchong Zhang29https://orcid.org/0000-0001-6454-1699(COOL-LAMPS Collaboration)Department of Astronomy and Astrophysics, University of Chicago , 5640 S. Ellis Avenue, Chicago, IL 60637, USA ; sdmork@asu.edu; School of Earth and Space Exploration, Arizona State University , 781 Terrace Mall, Tempe, AZ 85287, USA; Beus Center for Cosmic Foundations, Arizona State University , 781 Terrace Mall, Tempe, AZ 85287, USADepartment of Astronomy and Astrophysics, University of Chicago , 5640 S. Ellis Avenue, Chicago, IL 60637, USA ; sdmork@asu.edu; Kavli Institute for Cosmological Physics, University of Chicago , 5640 S. Ellis Avenue, Chicago, IL 60637, USADepartment of Physics and Astronomy, University of Pittsburgh , 3941 O’Hara Street, Pittsburgh, PA 15260, USA; Pittsburgh Particle Physics Astrophysics and Cosmology Center, University of Pittsburgh , 3941 O’Hara Street, Pittsburgh, PA 15260, USADepartment of Astronomy, University of Michigan , 1085 S. University Avenue, Ann Arbor, MI 48109, USADepartment of Astronomy and Astrophysics, University of Chicago , 5640 S. Ellis Avenue, Chicago, IL 60637, USA ; sdmork@asu.eduDepartment of Astronomy and Astrophysics, University of Chicago , 5640 S. Ellis Avenue, Chicago, IL 60637, USA ; sdmork@asu.edu; Department of Astronomy , University of Massachusetts Amherst, 710 N. Pleasant Street, Amherst, MA 01003, USAInstitute of Theoretical Astrophysics, University of Oslo , P.O. Box 1029, Blindern, NO-0315 Oslo, NorwayDepartment of Astronomy and Astrophysics, University of Chicago , 5640 S. Ellis Avenue, Chicago, IL 60637, USA ; sdmork@asu.edu; Department of Astronomy and Astrophysics, University of California , Santa Cruz, CA 95064, USADepartment of Astronomy and Astrophysics, University of Chicago , 5640 S. Ellis Avenue, Chicago, IL 60637, USA ; sdmork@asu.edu; Gravitation & Astroparticle Physics, University of Amsterdam , Science Park 904, 1098 XH Amsterdam, The NetherlandsDepartment of Astronomy and Astrophysics, University of Chicago , 5640 S. Ellis Avenue, Chicago, IL 60637, USA ; sdmork@asu.edu; Department of Astronomy, University of Michigan , 1085 S. University Avenue, Ann Arbor, MI 48109, USADepartment of Astronomy and Astrophysics, University of Chicago , 5640 S. Ellis Avenue, Chicago, IL 60637, USA ; sdmork@asu.eduDepartment of Astronomy and Astrophysics, University of Chicago , 5640 S. Ellis Avenue, Chicago, IL 60637, USA ; sdmork@asu.edu; Department of Physics and Astronomy, Stony Brook University , 100 Nicolls Road, Stony Brook, NY 11794, USADepartment of Astronomy and Astrophysics, University of Chicago , 5640 S. Ellis Avenue, Chicago, IL 60637, USA ; sdmork@asu.eduDepartment of Astronomy and Astrophysics, University of Chicago , 5640 S. Ellis Avenue, Chicago, IL 60637, USA ; sdmork@asu.eduDepartment of Astronomy and Astrophysics, University of Chicago , 5640 S. Ellis Avenue, Chicago, IL 60637, USA ; sdmork@asu.edu; Department of Physics, Stanford University , 382 Via Pueblo, Stanford, CA 94305, USA; Kavli Institute for Particle Astrophysics and Cosmology, Stanford University , 382 Via Pueblo, Stanford, CA 94305, USADepartment of Astronomy and Astrophysics, University of Chicago , 5640 S. Ellis Avenue, Chicago, IL 60637, USA ; sdmork@asu.edu; Department of Physics, University of Wisconsin , Madison, 1150 University Avenue, Madison, WI 53706, USADepartment of Astronomy and Astrophysics, University of Chicago , 5640 S. Ellis Avenue, Chicago, IL 60637, USA ; sdmork@asu.edu; Department of Astronomy, Columbia University , 538 W. 120th Street, New York, NY 10027, USADepartment of Astronomy and Astrophysics, University of Chicago , 5640 S. Ellis Avenue, Chicago, IL 60637, USA ; sdmork@asu.edu; Department of Astronomy, University of Wisconsin—Madison , 475 N. Charter Street, Madison, WI 53706, USADepartment of Astronomy and Astrophysics, University of Chicago , 5640 S. Ellis Avenue, Chicago, IL 60637, USA ; sdmork@asu.eduDepartment of Astronomy and Astrophysics, University of Chicago , 5640 S. Ellis Avenue, Chicago, IL 60637, USA ; sdmork@asu.edu; Department of Astrophysical Sciences, Princeton University , 4 Ivy Lane, Princeton, NJ 08544, USADepartment of Astronomy and Astrophysics, University of Chicago , 5640 S. Ellis Avenue, Chicago, IL 60637, USA ; sdmork@asu.edu; School of Earth and Space Exploration, Arizona State University , 781 Terrace Mall, Tempe, AZ 85287, USADepartment of Astronomy and Astrophysics, University of Chicago , 5640 S. Ellis Avenue, Chicago, IL 60637, USA ; sdmork@asu.eduDepartment of Astronomy and Astrophysics, University of Chicago , 5640 S. Ellis Avenue, Chicago, IL 60637, USA ; sdmork@asu.eduDepartment of Astronomy and Astrophysics, University of Chicago , 5640 S. Ellis Avenue, Chicago, IL 60637, USA ; sdmork@asu.edu; Department of Physics and Astronomy, Johns Hopkins University , 3400 N. Charles Street, Baltimore, MD 21218, USADepartment of Astronomy and Astrophysics, University of Chicago , 5640 S. Ellis Avenue, Chicago, IL 60637, USA ; sdmork@asu.eduDepartment of Astronomy and Astrophysics, University of Chicago , 5640 S. Ellis Avenue, Chicago, IL 60637, USA ; sdmork@asu.edu; Department of Astronomy, Columbia University , 538 W. 120th Street, New York, NY 10027, USADepartment of Astronomy and Astrophysics, University of Chicago , 5640 S. Ellis Avenue, Chicago, IL 60637, USA ; sdmork@asu.edu; Department of Anthropology, Yale University , 10 Sachem Street, New Haven, CT 06520, USADepartment of Astronomy and Astrophysics, University of Chicago , 5640 S. Ellis Avenue, Chicago, IL 60637, USA ; sdmork@asu.eduDepartment of Astronomy and Astrophysics, University of Chicago , 5640 S. Ellis Avenue, Chicago, IL 60637, USA ; sdmork@asu.edu; Department of Physics, The Ohio State University , 191 W. Woodruff Avenue, Columbus, OH 43210, USA; Center for Cosmology and Astro-Particle Physics, The Ohio State University , 191 W. Woodruff Avenue, Columbus, OH 43210, USADepartment of Astronomy and Astrophysics, University of Chicago , 5640 S. Ellis Avenue, Chicago, IL 60637, USA ; sdmork@asu.edu; Department of Physics and Astronomy, University of Pittsburgh , 3941 O’Hara Street, Pittsburgh, PA 15260, USAWe 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.https://doi.org/10.3847/1538-4357/ada24cGalaxy clustersHigh-redshift galaxy clustersScaling relationsSpectral energy distributionStrong gravitational lensing |
| spellingShingle | 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) COOL-LAMPS. VII. Quantifying Strong-lens Scaling Relations with 177 Cluster-scale Strong Gravitational Lenses in DECaLS The Astrophysical Journal Galaxy clusters High-redshift galaxy clusters Scaling relations Spectral energy distribution Strong gravitational lensing |
| title | COOL-LAMPS. VII. Quantifying Strong-lens Scaling Relations with 177 Cluster-scale Strong Gravitational Lenses in DECaLS |
| title_full | COOL-LAMPS. VII. Quantifying Strong-lens Scaling Relations with 177 Cluster-scale Strong Gravitational Lenses in DECaLS |
| title_fullStr | COOL-LAMPS. VII. Quantifying Strong-lens Scaling Relations with 177 Cluster-scale Strong Gravitational Lenses in DECaLS |
| title_full_unstemmed | COOL-LAMPS. VII. Quantifying Strong-lens Scaling Relations with 177 Cluster-scale Strong Gravitational Lenses in DECaLS |
| title_short | COOL-LAMPS. VII. Quantifying Strong-lens Scaling Relations with 177 Cluster-scale Strong Gravitational Lenses in DECaLS |
| title_sort | cool lamps vii quantifying strong lens scaling relations with 177 cluster scale strong gravitational lenses in decals |
| topic | Galaxy clusters High-redshift galaxy clusters Scaling relations Spectral energy distribution Strong gravitational lensing |
| url | https://doi.org/10.3847/1538-4357/ada24c |
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