RELICS: Strong Lens Models for Five Galaxy Clusters from the Reionization Lensing Cluster Survey
Abstract
Strong gravitational lensing by galaxy clusters magnifies background galaxies, enhancing our ability to discover statistically significant samples of galaxies at $${\boldsymbol{z}}\gt 6$$, in order to constrain the high-redshift galaxy luminosity functions. In this study, we present the first five lens models out of the Reionization Lensing Cluster Survey (RELICS) Hubble Treasury Program, based on new HST WFC3/IR and ACS imaging of the clusters RXC J0142.9+4438, Abell 2537, Abell 2163, RXC J2211.7–0349, and ACT-CLJ0102–49151. The derived lensing magnification is essential for estimating the intrinsic properties of high-redshift galaxy candidates, and properly accounting for the survey volume. We report on new spectroscopic redshifts of multiply imaged lensed galaxies behind these clusters, which are used as constraints, and detail our strategy to reduce systematic uncertainties due to lack of spectroscopic information. In addition, we quantify the uncertainty on the lensing magnification due to statistical and systematic errors related to the lens modeling process, and find that in all but one cluster, the magnification is constrained to better than 20% in at least 80% of the field of view, including statistical and systematic uncertainties. The five clusters presented in this paper span the range of masses and redshifts of the clusters in the RELICS program. We find that they exhibit similar strong lensing efficiencies to the clusters targeted by the Hubble Frontier Fields within the WFC3/IR field of view. Outputs of the lens models are made available to the community through the Mikulski Archive for Space Telescopes.
- Authors:
-
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- Univ. of Michigan, Ann Arbor, MI (United States). Dept. of Astronomy
- Harvard-Smithsonian Center for Astrophysics, Cambridge, MA (United States)
- Space Telescope Science Inst., Baltimore, MD (United States)
- Univ. of California, Davis, CA (United States). Dept. of Physics
- Univ. of Melbourne (Australia). School of Physics
- Academia Sinica, Taipei (Taiwan). Inst. of Astronomy and Astrophysics
- Lawrence Livermore National Lab. (LLNL), Livermore, CA (United States)
- Univ. of Arizona, Tucson, AZ (United States). Dept. of Astronomy
- Leiden Univ. (Netherlands). Leiden Observatory
- Yale Univ., New Haven, CT (United States). Dept. of Astronomy
- Univ. of Michigan, Ann Arbor, MI (United States). Dept. of Astronomy; Univ. of California, Irvine, CA (United States). Dept. of Physics and Astronomy
- Univ. of South Carolina, Columbia, SC (United States). Dept. of Physics and Astronomy
- American School of Warsaw, Bielawa (Poland); Univ. of Basque Country, Bilbao (Spain). Dept. of Theoretical Physics
- Ben-Gurion Univ. of the Negev, Beer-Sheva (Israel). Physics Dept.
- Publication Date:
- Research Org.:
- Lawrence Livermore National Lab. (LLNL), Livermore, CA (United States)
- Sponsoring Org.:
- USDOE National Nuclear Security Administration (NNSA); National Aeronautics and Space Administration (NASA)
- OSTI Identifier:
- 1660520
- Report Number(s):
- LLNL-JRNL-748251
Journal ID: ISSN 1538-4357; 933345; TRN: US2203524
- Grant/Contract Number:
- AC52-07NA27344; NAS 5-26555
- Resource Type:
- Accepted Manuscript
- Journal Name:
- The Astrophysical Journal (Online)
- Additional Journal Information:
- Journal Name: The Astrophysical Journal (Online); Journal Volume: 859; Journal Issue: 2; Journal ID: ISSN 1538-4357
- Publisher:
- Institute of Physics (IOP)
- Country of Publication:
- United States
- Language:
- English
- Subject:
- 79 ASTRONOMY AND ASTROPHYSICS; galaxies: clusters: individual (RXC J0142.9+4438; Abell 2537; Abell 2163; RXC J2211.7-0349; ACT-CLJ0102-49151 – gravitational lensing: strong
Citation Formats
Cerny, Catherine, Sharon, Keren, Andrade-Santos, Felipe, Avila, Roberto J., Bradač, Maruša, Bradley, Larry D., Carrasco, Daniela, Coe, Dan, Czakon, Nicole G., Dawson, William A., Frye, Brenda L., Hoag, Austin, Huang, Kuang-Han, Johnson, Traci L., Jones, Christine, Lam, Daniel, Lovisari, Lorenzo, Mainali, Ramesh, Oesch, Pascal A., Ogaz, Sara, Past, Matthew, Paterno-Mahler, Rachel, Peterson, Avery, Riess, Adam G., Rodney, Steven A., Ryan, Russell E., Salmon, Brett, Sendra-Server, Irene, Stark, Daniel P., Strolger, Louis-Gregory, Trenti, Michele, Umetsu, Keiichi, Vulcani, Benedetta, and Zitrin, Adi. RELICS: Strong Lens Models for Five Galaxy Clusters from the Reionization Lensing Cluster Survey. United States: N. p., 2018.
Web. doi:10.3847/1538-4357/aabe7b.
Cerny, Catherine, Sharon, Keren, Andrade-Santos, Felipe, Avila, Roberto J., Bradač, Maruša, Bradley, Larry D., Carrasco, Daniela, Coe, Dan, Czakon, Nicole G., Dawson, William A., Frye, Brenda L., Hoag, Austin, Huang, Kuang-Han, Johnson, Traci L., Jones, Christine, Lam, Daniel, Lovisari, Lorenzo, Mainali, Ramesh, Oesch, Pascal A., Ogaz, Sara, Past, Matthew, Paterno-Mahler, Rachel, Peterson, Avery, Riess, Adam G., Rodney, Steven A., Ryan, Russell E., Salmon, Brett, Sendra-Server, Irene, Stark, Daniel P., Strolger, Louis-Gregory, Trenti, Michele, Umetsu, Keiichi, Vulcani, Benedetta, & Zitrin, Adi. RELICS: Strong Lens Models for Five Galaxy Clusters from the Reionization Lensing Cluster Survey. United States. https://doi.org/10.3847/1538-4357/aabe7b
Cerny, Catherine, Sharon, Keren, Andrade-Santos, Felipe, Avila, Roberto J., Bradač, Maruša, Bradley, Larry D., Carrasco, Daniela, Coe, Dan, Czakon, Nicole G., Dawson, William A., Frye, Brenda L., Hoag, Austin, Huang, Kuang-Han, Johnson, Traci L., Jones, Christine, Lam, Daniel, Lovisari, Lorenzo, Mainali, Ramesh, Oesch, Pascal A., Ogaz, Sara, Past, Matthew, Paterno-Mahler, Rachel, Peterson, Avery, Riess, Adam G., Rodney, Steven A., Ryan, Russell E., Salmon, Brett, Sendra-Server, Irene, Stark, Daniel P., Strolger, Louis-Gregory, Trenti, Michele, Umetsu, Keiichi, Vulcani, Benedetta, and Zitrin, Adi. Mon .
"RELICS: Strong Lens Models for Five Galaxy Clusters from the Reionization Lensing Cluster Survey". United States. https://doi.org/10.3847/1538-4357/aabe7b. https://www.osti.gov/servlets/purl/1660520.
@article{osti_1660520,
title = {RELICS: Strong Lens Models for Five Galaxy Clusters from the Reionization Lensing Cluster Survey},
author = {Cerny, Catherine and Sharon, Keren and Andrade-Santos, Felipe and Avila, Roberto J. and Bradač, Maruša and Bradley, Larry D. and Carrasco, Daniela and Coe, Dan and Czakon, Nicole G. and Dawson, William A. and Frye, Brenda L. and Hoag, Austin and Huang, Kuang-Han and Johnson, Traci L. and Jones, Christine and Lam, Daniel and Lovisari, Lorenzo and Mainali, Ramesh and Oesch, Pascal A. and Ogaz, Sara and Past, Matthew and Paterno-Mahler, Rachel and Peterson, Avery and Riess, Adam G. and Rodney, Steven A. and Ryan, Russell E. and Salmon, Brett and Sendra-Server, Irene and Stark, Daniel P. and Strolger, Louis-Gregory and Trenti, Michele and Umetsu, Keiichi and Vulcani, Benedetta and Zitrin, Adi},
abstractNote = {Strong gravitational lensing by galaxy clusters magnifies background galaxies, enhancing our ability to discover statistically significant samples of galaxies at ${\boldsymbol{z}}\gt 6$, in order to constrain the high-redshift galaxy luminosity functions. In this study, we present the first five lens models out of the Reionization Lensing Cluster Survey (RELICS) Hubble Treasury Program, based on new HST WFC3/IR and ACS imaging of the clusters RXC J0142.9+4438, Abell 2537, Abell 2163, RXC J2211.7–0349, and ACT-CLJ0102–49151. The derived lensing magnification is essential for estimating the intrinsic properties of high-redshift galaxy candidates, and properly accounting for the survey volume. We report on new spectroscopic redshifts of multiply imaged lensed galaxies behind these clusters, which are used as constraints, and detail our strategy to reduce systematic uncertainties due to lack of spectroscopic information. In addition, we quantify the uncertainty on the lensing magnification due to statistical and systematic errors related to the lens modeling process, and find that in all but one cluster, the magnification is constrained to better than 20% in at least 80% of the field of view, including statistical and systematic uncertainties. The five clusters presented in this paper span the range of masses and redshifts of the clusters in the RELICS program. We find that they exhibit similar strong lensing efficiencies to the clusters targeted by the Hubble Frontier Fields within the WFC3/IR field of view. Outputs of the lens models are made available to the community through the Mikulski Archive for Space Telescopes.},
doi = {10.3847/1538-4357/aabe7b},
journal = {The Astrophysical Journal (Online)},
number = 2,
volume = 859,
place = {United States},
year = {Mon Jun 04 00:00:00 EDT 2018},
month = {Mon Jun 04 00:00:00 EDT 2018}
}
Web of Science
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Works referencing / citing this record:
An Evaluation of 10 Lensing Models of the Frontier Fields Cluster MACS J0416.1-2403
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The core of the massive cluster merger MACS J0417.5-1154 as seen by VLT/MUSE
text, January 2018
- Jauzac, Mathilde; Mahler, Guillaume; Edge, Alastair C.
- arXiv
A new Einstein Cross gravitational lens of a Lyman-break galaxy
text, January 2019
- Bettoni, D.; Falomo, R.; Scarpa, R.
- arXiv