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    RELICS: A Strong Lens Model for SPT-CLJ0615-5746, a z=0.972 Cluster

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    Paterno-Mahler_2018_ApJ_863_154.pdf
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    Final Published version
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    Author
    Paterno-Mahler, Rachel
    Sharon, Keren
    Coe, Dan
    Mahler, Guillaume
    Cerny, Catherine
    Johnson, Traci L.
    Schrabback, Tim
    Andrade-Santos, Felipe
    Avila, Roberto J.
    Bradač, Maruša
    Bradley, Larry D.
    Carrasco, Daniela
    Czakon, Nicole G.
    Dawson, William A.
    Frye, Brenda L.
    Hoag, Austin T.
    Huang, Kuang-Han
    Jones, Christine
    Lam, Daniel
    Livermore, Rachael
    Lovisari, Lorenzo
    Mainali, Ramesh cc
    Oesch, Pascal A.
    Ogaz, Sara
    Past, Matthew
    Peterson, Avery
    Ryan, Russell E.
    Salmon, Brett cc
    Sendra-Server, Irene
    Stark, Daniel P.
    Umetsu, Keiichi
    Vulcani, Benedetta
    Zitrin, A. cc
    Show allShow less
    Affiliation
    Univ Arizona, Steward Observ
    Univ Arizona, Dept Astron
    Issue Date
    2018-08-20
    Keywords
    clusters: individual (SPT-CLJ0615-5746)
    gravitational lensing: strong
    
    Metadata
    Show full item record
    Publisher
    IOP PUBLISHING LTD
    Citation
    Rachel Paterno-Mahler et al 2018 ApJ 863 154
    Journal
    ASTROPHYSICAL JOURNAL
    Rights
    © 2018. The American Astronomical Society. All rights reserved.
    Collection Information
    This item from the UA Faculty Publications collection is made available by the University of Arizona with support from the University of Arizona Libraries. If you have questions, please contact us at repository@u.library.arizona.edu.
    Abstract
    We present a lens model for the cluster SPT-CLJ0615-5746, which is the highest-redshift (z = 0.972) system in the Reionization of Lensing Clusters Survey, making it the highest-redshift cluster for which a full, strong lens model is published. We identify three systems of multiply imaged lensed galaxies, two of which we spectroscopically confirm at z = 1.358 and z = 4.013, which we use as constraints for the model. We find a foreground structure at z similar to 0.4, which we include as a second cluster-sized halo in one of our models; however, two different statistical tests find the best-fit model consists of one cluster-sized halo combined with three individually optimized galaxy-sized halos, as well as contributions from the cluster galaxies themselves. We find the total projected mass density within r = 26.'' 7 (the region where the strong lensing constraints exist) to be M = 2.51(-0.09)(+0.15) x 10(14) M-circle dot. If we extrapolate out to r(500), our projected mass density is consistent with the mass inferred from weak lensing and from the Sunyaev-Zel'dovich effect (M similar to 10(15)M(circle dot)). This cluster is lensing a previously reported z similar to 10 galaxy, which, if spectroscopically confirmed, will be the highest-redshift strongly lensed galaxy known.
    ISSN
    1538-4357
    DOI
    10.3847/1538-4357/aad239
    Version
    Final published version
    Sponsors
    NASA through a grant from the Space Telescope Science Institute [GO14096]; NASA [NAS 5-26555]; [GO12757]; [GO12477]
    Additional Links
    http://stacks.iop.org/0004-637X/863/i=2/a=154?key=crossref.f55ee4fc904de82eaf2fec4b0acbb5dc
    ae974a485f413a2113503eed53cd6c53
    10.3847/1538-4357/aad239
    Scopus Count
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    UA Faculty Publications

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