RELICS: A Very Large (θE ~ 40") Cluster Lens—RXC J0032.1+1808
Journal Article
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· The Astrophysical Journal (Online)
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- Ben Gurion Univ. of the Negev, Beer Sheva (Israel)
- Space Telescope Science Inst., Baltimore, MD (United States)
- Univ. of Michigan, Ann Arbor, MI (United States)
- Univ. of Tokyo (Japan). Research Center for the Early Universe; Univ. of Tokyo (Japan); Univ. of Tokyo (Japan). Kavli Institute for the Physics and Mathematics of the Universe (WPI)
- Univ. of California, Davis, CA (United States)
- Univ. of Arizona, Tucson, AZ (United States). Steward Observatory
- Harvard-Smithsonian Center for Astrophysics, Cambridge, MA (United States)
- Univ. of Kentucky, Lexington, KY (United States)
- Academia Sinica Inst. of Astronomy and Astrophysics (ASIAA), Taipei (Taiwan)
- Univ. of Melbourne, VIC (Australia)
- Boston Univ., MA (United States). Inst. for Astrophysical Research
- Lawrence Livermore National Lab. (LLNL), Livermore, CA (United States)
- Univ. of Tokyo (Japan). Inst. for Cosmic Ray Research; Univ. of Tokyo
- Leiden Univ. (Netherlands). Leiden Observatory
- Istituto Nazionale di Astrofisica (INAF), Trieste (Italy). Osservatorio Astronomico di Trieste
- Univ. of Geneva, Versoix (Switzerland)
- Univ. of Tokyo (Japan). Kavli Institute for the Physics and Mathematics of the Universe (WPI); Univ. of Tokyo (Japan). Inst. for Cosmic Ray Research
- Cosmic Dawn Center (DAWN) (Denmark); Univ. of Copenhagen (Denmark). Niels Bohr Inst.
- Univ. of Melbourne, VIC (Australia); Australian Research Council Centre of Excellence for All Sky Astrophysics in 3 Dimensions (ASTRO 3D), Melbourne, VIC (Australia)
- Istituto Nazionale di Astrofisica (INAF), Padova (Italy). Osservatorio Astronomico di Padova
- Johns Hopkins Univ., Baltimore, MD (United States)
Extensive surveys with the Hubble Space Telescope over the past decade, targeting some of the most massive clusters in the sky, have uncovered dozens of galaxy cluster strong lenses. The massive cluster strong-lens scale is typically θE ~ 10'' to ~30''–35'', with only a handful of clusters known with Einstein radii θE ~ 40'' or above (for zsource = 2, nominally). Here we report another very large cluster lens, RXC J0032.1+1808 (z = 0.3956), the second-richest cluster in the redMapper cluster catalog and the 85th most massive cluster in the Planck Sunyaev–Zel'dovich catalog. With our light-traces-mass and fully parametric approaches, we construct strong-lensing models based on 18 multiple images of five background galaxies newly identified in the Hubble data, mainly from the Reionization Lensing Cluster Survey (RELICS), in addition to a known sextuply imaged system in this cluster. Furthermore, we compare these models to Lenstool and GLAFIC models that were produced independently as part of the RELICS program. All models reveal a large effective Einstein radius of θE ≃ 40'' (zsource = 2), owing to the obvious concentration of substructures near the cluster center. Although RXC J0032.1+1808 has a very large critical area and high lensing strength, only three magnified high-redshift candidates are found within the field targeted by RELICS. Nevertheless, we expect many more high-redshift candidates will be seen in wider and deeper observations with Hubble or the James Webb Space Telescope. Finally, the comparison between several algorithms demonstrates that the total error budget is largely dominated by systematic uncertainties.
- Research Organization:
- Lawrence Livermore National Laboratory (LLNL), Livermore, CA (United States)
- Sponsoring Organization:
- European Research Council (ERC); JSPS KAKENHI; Ministry of Science and Technology (MOST) Taiwan; National Aeronautic and Space Administration (NASA); USDOE National Nuclear Security Administration (NNSA)
- Grant/Contract Number:
- AC52-07NA27344
- OSTI ID:
- 1862745
- Report Number(s):
- LLNL-JRNL-831921; 1049238
- Journal Information:
- The Astrophysical Journal (Online), Journal Name: The Astrophysical Journal (Online) Journal Issue: 1 Vol. 898; ISSN 1538-4357
- Publisher:
- IOP PublishingCopyright Statement
- Country of Publication:
- United States
- Language:
- English
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OSTI ID:22869135