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
Author
Paterno-Mahler, RachelSharon, 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
Oesch, Pascal A.
Ogaz, Sara
Past, Matthew
Peterson, Avery
Ryan, Russell E.
Salmon, Brett
Sendra-Server, Irene
Stark, Daniel P.
Umetsu, Keiichi
Vulcani, Benedetta
Zitrin, A.
Affiliation
Univ Arizona, Steward ObservUniv Arizona, Dept Astron
Issue Date
2018-08-20
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IOP PUBLISHING LTDCitation
Rachel Paterno-Mahler et al 2018 ApJ 863 154Journal
ASTROPHYSICAL JOURNALRights
© 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
1538-4357Version
Final published versionSponsors
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.f55ee4fc904de82eaf2fec4b0acbb5dcae974a485f413a2113503eed53cd6c53
10.3847/1538-4357/aad239
