RELICS: Strong Lensing Analysis of MACS J0417.5–1154 and Predictions for Observing the Magnified High-redshift Universe with JWST
Abstract
Strong gravitational lensing by clusters of galaxies probes the mass distribution at the core of each cluster and magnifies the universe behind it. MACS J0417.5–1154 at z = 0.443 is one of the most massive clusters known based on weak lensing, X-ray, and Sunyaev–Zel'dovich analyses. In this work we compute a strong lens model of MACS J0417 based on Hubble Space Telescope imaging observations collected, in part, by the Reionization Lensing Cluster Survey (RELICS), and recently reported spectroscopic redshifts from the MUSE instrument on the Very Large Telescope (VLT). We measure an Einstein radius of $${\theta }_{E}\simeq 36^{\prime\prime} $$ at z = 9 and a mass projected within 200 kpc of $${M}_{(200\mathrm{kpc})}={1.78}_{-0.03}^{+0.01}\times {10}^{14}$$ M $${}_{\odot }$$. Using this model, we measure a ratio between the mass attributed to cluster-member galaxy halos and the main cluster halo of order 1:100. We assess the probability to detect magnified high-redshift galaxies in the field of this cluster, both for comparison with RELICS HST results and as a prediction for the James Webb Space Telescope (JWST) Guaranteed Time Observations upcoming for this cluster. Our lensing analysis suggests that this cluster has similar lensing strength to other clusters in the RELICS program. Our lensing analysis predicts a detection of at least a few z ~ 6–8 galaxies behind this cluster, at odds with a recent analysis that yielded no such candidates in this field. Reliable strong lensing models are important for accurately predicting the intrinsic properties of lensed galaxies. As part of the RELICS program, our strong lensing model produced with the Lenstool parametric method is publicly available through the Mikulski Archive for Space Telescopes.
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- Univ. of Michigan, Ann Arbor, MI (United States)
- Space Telescope Science Inst., Baltimore, MD (United States)
- Durham Univ. (United Kingdom); Univ. of KwaZulu-Natal, Durban (South Africa)
- Univ. of California, Davis, CA (United States)
- Durham Univ. (United Kingdom)
- Ben-Gurion Univ. of the Negev, Beer-Sheva (Israel)
- Harvard-Smithsonian Center for Astrophysics, Cambridge, MA (United States)
- Univ. of Melbourne (Australia)
- Boston Univ., MA (United States)
- Academia Sinica, Taipei (Taiwan)
- Lawrence Livermore National Lab. (LLNL), Livermore, CA (United States)
- Univ. of Arizona, Tucson, AZ (United States)
- Univ. of Tokyo (Japan)
- Leiden Univ. (Netherlands)
- Univ. of Melbourne (Australia); ARC Centre of Excellence for All Sky Astrophysics in 3 Dimensions (ASTRO 3D) (Australia)
- Univ. of Tokyo (Japan); Leiden Univ. (Netherlands)
- Univ. of Michigan, Ann Arbor, MI (United States); Joint Inst. for Nuclear Astrophysics (JINA), East Lansing, MI (United States). Center for the Evolution of the Elements (JINA-CEE)
- California Inst. of Technology (CalTech), Pasadena, CA (United States)
- Univ. of Copenhagen (Denmark)
- Univ. of Melbourne (Australia); ARC Centre of Excellence for All Sky Astrophysics in 3 Dimensions (ASTRO 3D) (Australia)
- Publication Date:
- Research Org.:
- Lawrence Livermore National Lab. (LLNL), Livermore, CA (United States)
- Sponsoring Org.:
- USDOE Office of Science (SC); USDOE National Nuclear Security Administration (NNSA)
- OSTI Identifier:
- 1545279
- Alternate Identifier(s):
- OSTI ID: 1862743
- Report Number(s):
- LLNL-JRNL-831919
Journal ID: ISSN 1538-4357
- Grant/Contract Number:
- AC52-07NA27344
- Resource Type:
- Accepted Manuscript
- Journal Name:
- The Astrophysical Journal (Online)
- Additional Journal Information:
- Journal Name: The Astrophysical Journal (Online); Journal Volume: 873; Journal Issue: 1; Journal ID: ISSN 1538-4357
- Publisher:
- IOP Publishing
- Country of Publication:
- United States
- Language:
- English
- Subject:
- 79 ASTRONOMY AND ASTROPHYSICS; galaxies: clusters: individual (MACSJ0417.5–1154); gravitational lensing: strong
Citation Formats
Mahler, Guillaume, Sharon, Keren, Fox, Carter, Coe, Dan, Jauzac, Mathilde, Strait, Victoria, Edge, Alastair, Acebron, Ana, Andrade-Santos, Felipe, Avila, Roberto J., Bradač, Maruša, Bradley, Larry D., Carrasco, Daniela, Cerny, Catherine, Cibirka, Nathália, Czakon, Nicole G., Dawson, William A., Frye, Brenda L., Hoag, Austin T., Huang, Kuang-Han, Johnson, Traci L., Jones, Christine, Kikuchihara, Shotaro, Lam, Daniel, Livermore, Rachael, Lovisari, Lorenzo, Mainali, Ramesh, Ogaz, Sara, Ouchi, Masami, Paterno-Mahler, Rachel, Roederer, Ian U., Ryan, Russell E., Salmon, Brett, Sendra-Server, Irene, Stark, Daniel P., Toft, Sune, Trenti, Michele, Umetsu, Keiichi, Vulcani, Benedetta, and Zitrin, Adi. RELICS: Strong Lensing Analysis of MACS J0417.5–1154 and Predictions for Observing the Magnified High-redshift Universe with JWST. United States: N. p., 2019.
Web. doi:10.3847/1538-4357/ab042b.
Mahler, Guillaume, Sharon, Keren, Fox, Carter, Coe, Dan, Jauzac, Mathilde, Strait, Victoria, Edge, Alastair, Acebron, Ana, Andrade-Santos, Felipe, Avila, Roberto J., Bradač, Maruša, Bradley, Larry D., Carrasco, Daniela, Cerny, Catherine, Cibirka, Nathália, Czakon, Nicole G., Dawson, William A., Frye, Brenda L., Hoag, Austin T., Huang, Kuang-Han, Johnson, Traci L., Jones, Christine, Kikuchihara, Shotaro, Lam, Daniel, Livermore, Rachael, Lovisari, Lorenzo, Mainali, Ramesh, Ogaz, Sara, Ouchi, Masami, Paterno-Mahler, Rachel, Roederer, Ian U., Ryan, Russell E., Salmon, Brett, Sendra-Server, Irene, Stark, Daniel P., Toft, Sune, Trenti, Michele, Umetsu, Keiichi, Vulcani, Benedetta, & Zitrin, Adi. RELICS: Strong Lensing Analysis of MACS J0417.5–1154 and Predictions for Observing the Magnified High-redshift Universe with JWST. United States. https://doi.org/10.3847/1538-4357/ab042b
Mahler, Guillaume, Sharon, Keren, Fox, Carter, Coe, Dan, Jauzac, Mathilde, Strait, Victoria, Edge, Alastair, Acebron, Ana, Andrade-Santos, Felipe, Avila, Roberto J., Bradač, Maruša, Bradley, Larry D., Carrasco, Daniela, Cerny, Catherine, Cibirka, Nathália, Czakon, Nicole G., Dawson, William A., Frye, Brenda L., Hoag, Austin T., Huang, Kuang-Han, Johnson, Traci L., Jones, Christine, Kikuchihara, Shotaro, Lam, Daniel, Livermore, Rachael, Lovisari, Lorenzo, Mainali, Ramesh, Ogaz, Sara, Ouchi, Masami, Paterno-Mahler, Rachel, Roederer, Ian U., Ryan, Russell E., Salmon, Brett, Sendra-Server, Irene, Stark, Daniel P., Toft, Sune, Trenti, Michele, Umetsu, Keiichi, Vulcani, Benedetta, and Zitrin, Adi. Thu .
"RELICS: Strong Lensing Analysis of MACS J0417.5–1154 and Predictions for Observing the Magnified High-redshift Universe with JWST". United States. https://doi.org/10.3847/1538-4357/ab042b. https://www.osti.gov/servlets/purl/1545279.
@article{osti_1545279,
title = {RELICS: Strong Lensing Analysis of MACS J0417.5–1154 and Predictions for Observing the Magnified High-redshift Universe with JWST},
author = {Mahler, Guillaume and Sharon, Keren and Fox, Carter and Coe, Dan and Jauzac, Mathilde and Strait, Victoria and Edge, Alastair and Acebron, Ana and Andrade-Santos, Felipe and Avila, Roberto J. and Bradač, Maruša and Bradley, Larry D. and Carrasco, Daniela and Cerny, Catherine and Cibirka, Nathália and Czakon, Nicole G. and Dawson, William A. and Frye, Brenda L. and Hoag, Austin T. and Huang, Kuang-Han and Johnson, Traci L. and Jones, Christine and Kikuchihara, Shotaro and Lam, Daniel and Livermore, Rachael and Lovisari, Lorenzo and Mainali, Ramesh and Ogaz, Sara and Ouchi, Masami and Paterno-Mahler, Rachel and Roederer, Ian U. and Ryan, Russell E. and Salmon, Brett and Sendra-Server, Irene and Stark, Daniel P. and Toft, Sune and Trenti, Michele and Umetsu, Keiichi and Vulcani, Benedetta and Zitrin, Adi},
abstractNote = {Strong gravitational lensing by clusters of galaxies probes the mass distribution at the core of each cluster and magnifies the universe behind it. MACS J0417.5–1154 at z = 0.443 is one of the most massive clusters known based on weak lensing, X-ray, and Sunyaev–Zel'dovich analyses. In this work we compute a strong lens model of MACS J0417 based on Hubble Space Telescope imaging observations collected, in part, by the Reionization Lensing Cluster Survey (RELICS), and recently reported spectroscopic redshifts from the MUSE instrument on the Very Large Telescope (VLT). We measure an Einstein radius of ${\theta }_{E}\simeq 36^{\prime\prime} $ at z = 9 and a mass projected within 200 kpc of ${M}_{(200\mathrm{kpc})}={1.78}_{-0.03}^{+0.01}\times {10}^{14}$ M ${}_{\odot }$. Using this model, we measure a ratio between the mass attributed to cluster-member galaxy halos and the main cluster halo of order 1:100. We assess the probability to detect magnified high-redshift galaxies in the field of this cluster, both for comparison with RELICS HST results and as a prediction for the James Webb Space Telescope (JWST) Guaranteed Time Observations upcoming for this cluster. Our lensing analysis suggests that this cluster has similar lensing strength to other clusters in the RELICS program. Our lensing analysis predicts a detection of at least a few z ~ 6–8 galaxies behind this cluster, at odds with a recent analysis that yielded no such candidates in this field. Reliable strong lensing models are important for accurately predicting the intrinsic properties of lensed galaxies. As part of the RELICS program, our strong lensing model produced with the Lenstool parametric method is publicly available through the Mikulski Archive for Space Telescopes.},
doi = {10.3847/1538-4357/ab042b},
journal = {The Astrophysical Journal (Online)},
number = 1,
volume = 873,
place = {United States},
year = {Thu Mar 07 00:00:00 EST 2019},
month = {Thu Mar 07 00:00:00 EST 2019}
}
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Accounting for Cosmic Variance in Studies of Gravitationally-Lensed High-Redshift Galaxies in the Hubble Frontier Field Clusters
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Hubble Space Telescope Combined Strong and Weak Lensing Analysis of the CLASH Sample: Mass and Magnification Models and Systematic Uncertainties
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- arXiv
T-PHOT: A new code for PSF-matched, prior-based, multiwavelength extragalactic deconfusion photometry
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The Frontier Fields Lens Modeling Comparison Project
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A study of diffuse radio sources and X-ray emission in six massive clusters
text, January 2016
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Full-Data Results of Hubble Frontier Fields: UV Luminosity Functions at $z\sim6-10$ and a Consistent Picture of Cosmic Reionization
text, January 2017
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- arXiv
RELICS: Strong Lens Models for Five Galaxy Clusters From the Reionization Lensing Cluster Survey
text, January 2017
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- arXiv
The Dearth of z~10 Galaxies in all HST Legacy Fields -- The Rapid Evolution of the Galaxy Population in the First 500 Myr
text, January 2017
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- arXiv
RELICS: Strong-lensing analysis of the massive clusters MACS J0308.9+2645 and PLCK G171.9-40.7
text, January 2018
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- arXiv
RELICS: Strong Lensing analysis of the galaxy clusters Abell S295, Abell 697, MACS J0025.4-1222, and MACS J0159.8-0849
text, January 2018
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- arXiv
The Extreme Faint End of the UV Luminosity Function at $z\sim6$ Through Gravitational Telescopes: a comprehensive assessment of strong lensing uncertainties
text, January 2018
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- arXiv
The peculiar cluster MACS J0417.5-1154 in the C and X-bands
text, January 2018
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- arXiv
RELICS: A Strong Lens Model for SPT-CLJ0615-5746, a z=0.972 Cluster
text, January 2018
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- arXiv
The core of the massive cluster merger MACS J0417.5-1154 as seen by VLT/MUSE
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A New Method For Galaxy Cluster Detection I: The Algorithm
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Galaxies in the Hubble Ultra Deep Field: I. Detection, Multiband Photometry, Photometric Redshifts, and Morphology
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Works referencing / citing this record:
RELICS: Reionization Lensing Cluster Survey
journal, October 2019
- Coe, Dan; Salmon, Brett; Bradač, Maruša
- The Astrophysical Journal, Vol. 884, Issue 1