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Title: RELICS: Strong Lensing Analysis of the Galaxy Clusters Abell S295, Abell 697, MACS J0025.4-1222, and MACS J0159.8-0849

Journal Article · · The Astrophysical Journal (Online)
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  1. Ben Gurion Univ. of the Negev, Beer Sheva (Israel)
  2. Space Telescope Science Inst., Baltimore, MD (United States)
  3. Univ. of Michigan, Ann Arbor, MI (United States)
  4. Univ. of Melbourne, VIC (Australia); ARC Centre of Excellence for All Sky Astrophysics in 3 Dimensions (ASTRO 3D), Melbourne, VIC (Australia)
  5. Academia Sinica Inst. for Astronomy and Astrophysics (ASIAA), Taipei (Taiwan)
  6. Univ. of Melbourne, VIC (Australia)
  7. Academia Sinica Inst. of Astronomy and Astrophysics (ASIAA), Taipei (Taiwan)
  8. Lawrence Livermore National Lab. (LLNL), Livermore, CA (United States)
  9. Univ. of California, Davis, CA (United States)
  10. Harvard-Smithsonian Center for Astrophysics, Cambridge, MA (United States)
  11. Univ. of Tokyo (Japan). Inst. for Cosmic Ray Research
  12. Leiden Univ. (Netherlands). Leiden Observatory
  13. Univ. of Arizona, Tucson, AZ (United States). Steward Observatory
  14. Univ. of Geneva, Versoix (Switzerland). Geneva Observatory
  15. Univ. of Toyko (Japan). Inst. for Cosmic Ray Research; Univ. of Tokyo (Japan). Kavli Institute for the Physics and Mathematics of the Universe (WPI)
  16. American School of Warsaw (Poland); Univ. of Basque Country, Bilbao (Spain)
  17. Univ. of Copenhagen (Denmark). Niels Bohr Inst., Cosmic Dawn Center (DAWN)

In this work, we present a strong lensing analysis of four massive galaxy clusters imaged with the Hubble Space Telescope in the Reionization Lensing Cluster Survey. We use a light-traces-mass technique to uncover sets of multiple images and constrain the mass distribution of the clusters. These mass models are the first published for Abell S295 and MACS J0159.8-0849 and are improvements over previous models for Abell 697 and MACS J0025.4-1222. Our analysis for MACS J0025.4-1222 and Abell S295 shows a bimodal mass distribution supporting the merger scenarios proposed for these clusters. The updated model for MACS J0025.4-1222 suggests a substantially smaller critical area than previously estimated. For MACS J0159.8-0849 and Abell 697, we find a single peak and relatively regular morphology revealing fairly relaxed clusters. Despite being less prominent lenses, three of these clusters seem to have lensing strengths, i.e., cumulative area above certain magnification, similar to those of the Hubble Frontier Fields clusters (e.g., A(μ > 5) ~ 1–3 arcmin2, A(μ > 10) ~ 0.5–1.5 arcmin2), which in part can be attributed to their merging configurations. We make our lens models publicly available through the Mikulski Archive for Space Telescopes. Finally, using Gemini-N/GMOS spectroscopic observations, we detect a single emission line from a high-redshift J125 ≃ 25.7 galaxy candidate lensed by Abell 697. While we cannot rule out a lower-redshift solution, we interpret the line as Lyα at z = 5.800 ± 0.001, in agreement with its photometric redshift and dropout nature. Within this scenario, we measure a Lyα rest-frame equivalent width of 52 ± 22 Å and an observed Gaussian width of 117 ± 15 km s-1.

Research Organization:
Lawrence Livermore National Laboratory (LLNL), Livermore, CA (United States)
Sponsoring Organization:
USDOE National Nuclear Security Administration (NNSA); JSPS KAKENHI; Ministry of Science and Technology (MOST) Taiwan; European Research Council (ERC)
Grant/Contract Number:
AC52-07NA27344; NAS5-26555; JP15H05892; JP18K03693; 106-2628-M-001-003-MY3; 648179
OSTI ID:
1862751
Report Number(s):
LLNL-JRNL-831916; 1049227; TRN: US2305548
Journal Information:
The Astrophysical Journal (Online), Vol. 863, Issue 2; ISSN 1538-4357
Publisher:
IOP PublishingCopyright Statement
Country of Publication:
United States
Language:
English

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