JWST's PEARLS: 119 multiply imaged galaxies behind MACS0416, lensing properties of caustic crossing galaxies, and the relation between halo mass and number of globular clusters at z = 0.4
We present a new lens model for the ɀ = 0.396 galaxy cluster MACS J0416.1 –2403 based on a previously known set of 77 spectroscop-ically confirmed, multiply imaged galaxies plus an additional set of 42 candidate multiply imaged galaxies from past HST and new JWST data. The new galaxies lack spectros...
| Autores: | , , , , , , , , , , , , , , , , , , , , , , , , , , , , |
|---|---|
| Tipo de recurso: | artículo |
| Estado: | Versión publicada |
| Fecha de publicación: | 2024 |
| País: | España |
| Institución: | Consejo Superior de Investigaciones Científicas (CSIC) |
| Repositorio: | DIGITAL.CSIC. Repositorio Institucional del CSIC |
| OAI Identifier: | oai:digital.csic.es:10261/375060 |
| Acceso en línea: | http://hdl.handle.net/10261/375060 |
| Access Level: | acceso abierto |
| Palabra clave: | Gravitational lensing: strong Galaxies: clusters: intracluster medium Galaxies: clusters: individual: MACS J0416.1-2403 (MACS0416) Dark matter |
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| dc.title.none.fl_str_mv |
JWST's PEARLS: 119 multiply imaged galaxies behind MACS0416, lensing properties of caustic crossing galaxies, and the relation between halo mass and number of globular clusters at z = 0.4 |
| title |
JWST's PEARLS: 119 multiply imaged galaxies behind MACS0416, lensing properties of caustic crossing galaxies, and the relation between halo mass and number of globular clusters at z = 0.4 |
| spellingShingle |
JWST's PEARLS: 119 multiply imaged galaxies behind MACS0416, lensing properties of caustic crossing galaxies, and the relation between halo mass and number of globular clusters at z = 0.4 Diego, José María Gravitational lensing: strong Galaxies: clusters: intracluster medium Galaxies: clusters: individual: MACS J0416.1-2403 (MACS0416) Dark matter |
| title_short |
JWST's PEARLS: 119 multiply imaged galaxies behind MACS0416, lensing properties of caustic crossing galaxies, and the relation between halo mass and number of globular clusters at z = 0.4 |
| title_full |
JWST's PEARLS: 119 multiply imaged galaxies behind MACS0416, lensing properties of caustic crossing galaxies, and the relation between halo mass and number of globular clusters at z = 0.4 |
| title_fullStr |
JWST's PEARLS: 119 multiply imaged galaxies behind MACS0416, lensing properties of caustic crossing galaxies, and the relation between halo mass and number of globular clusters at z = 0.4 |
| title_full_unstemmed |
JWST's PEARLS: 119 multiply imaged galaxies behind MACS0416, lensing properties of caustic crossing galaxies, and the relation between halo mass and number of globular clusters at z = 0.4 |
| title_sort |
JWST's PEARLS: 119 multiply imaged galaxies behind MACS0416, lensing properties of caustic crossing galaxies, and the relation between halo mass and number of globular clusters at z = 0.4 |
| dc.creator.none.fl_str_mv |
Diego, José María Adams, Nathan Willner, Steven P. Harvey, Thomas Broadhurst, Tom Cohen, Seth Jansen, Rolf A. Summers, Jake Windhorst, Rogier A. D’Silva, Jordan C. J. Koekemoer, Anton M. Coe, Dan Conselice, Christopher J. Driver, Simon P. Frye, Brenda Grogin, Norman A. Marshall, Madeline A. Nonino, Mario Ortiz III, Rafael Pirzkal, Nor Robotham, Aaron Ryan Jr., Russell E. Willmer, Christopher N. A. Yan, Haojing Sun, Fengwu Hainline, Kevin Berkheimer, Jessica Polleta, Maria del Carmen Zitrin, Adi |
| author |
Diego, José María |
| author_facet |
Diego, José María Adams, Nathan Willner, Steven P. Harvey, Thomas Broadhurst, Tom Cohen, Seth Jansen, Rolf A. Summers, Jake Windhorst, Rogier A. D’Silva, Jordan C. J. Koekemoer, Anton M. Coe, Dan Conselice, Christopher J. Driver, Simon P. Frye, Brenda Grogin, Norman A. Marshall, Madeline A. Nonino, Mario Ortiz III, Rafael Pirzkal, Nor Robotham, Aaron Ryan Jr., Russell E. Willmer, Christopher N. A. Yan, Haojing Sun, Fengwu Hainline, Kevin Berkheimer, Jessica Polleta, Maria del Carmen Zitrin, Adi |
| author_role |
author |
| author2 |
Adams, Nathan Willner, Steven P. Harvey, Thomas Broadhurst, Tom Cohen, Seth Jansen, Rolf A. Summers, Jake Windhorst, Rogier A. D’Silva, Jordan C. J. Koekemoer, Anton M. Coe, Dan Conselice, Christopher J. Driver, Simon P. Frye, Brenda Grogin, Norman A. Marshall, Madeline A. Nonino, Mario Ortiz III, Rafael Pirzkal, Nor Robotham, Aaron Ryan Jr., Russell E. Willmer, Christopher N. A. Yan, Haojing Sun, Fengwu Hainline, Kevin Berkheimer, Jessica Polleta, Maria del Carmen Zitrin, Adi |
| author2_role |
author author author author author author author author author author author author author author author author author author author author author author author author author author author author |
| dc.contributor.none.fl_str_mv |
NASA European Space Agency Universities Space Research Association (US) Agencia Estatal de Investigación (España) Ministerio de Ciencia, Innovación y Universidades (España) European Commission European Research Council Australian Research Council National Research Council of Canada United States-Israel Binational Science Foundation Ministry of Science, Technology and Space (Israel) University of Arizona Israel Science Foundation Consejo Superior de Investigaciones Científicas [https://ror.org/02gfc7t72] |
| dc.subject.none.fl_str_mv |
Gravitational lensing: strong Galaxies: clusters: intracluster medium Galaxies: clusters: individual: MACS J0416.1-2403 (MACS0416) Dark matter |
| topic |
Gravitational lensing: strong Galaxies: clusters: intracluster medium Galaxies: clusters: individual: MACS J0416.1-2403 (MACS0416) Dark matter |
| description |
We present a new lens model for the ɀ = 0.396 galaxy cluster MACS J0416.1 –2403 based on a previously known set of 77 spectroscop-ically confirmed, multiply imaged galaxies plus an additional set of 42 candidate multiply imaged galaxies from past HST and new JWST data. The new galaxies lack spectroscopic redshifts but have geometric and/or photometric redshift estimates that are presented here. The new model predicts magnifications and time delays for all multiple images. The full set of constraints totals 343, constituting the largest sample of multiple images lensed by a single cluster to date. Caustic-crossing galaxies lensed by this cluster are especially interesting. Some of these galaxies show transient events, most of which are interpreted as micro-lensing of stars at cosmological distances. These caustic-crossing arcs are expected to show similar events in future, deeper JWST observations. We provide time delay and magnification models for all these arcs. The time delays and the magnifications for different arcs are generally anti-correlated. In the major sub-halos of the cluster, the dark-matter mass from our lens model correlates well with the observed number of globular clusters, as expected from N-body simulations. This confirms earlier results, derived at lower redshifts, which suggest that globular clusters can be used as powerful mass proxies for the halo masses when lensing constraints are scarce or not available. |
| publishDate |
2024 |
| dc.date.none.fl_str_mv |
2024 2024 2024 |
| dc.type.none.fl_str_mv |
info:eu-repo/semantics/article http://purl.org/coar/resource_type/c_6501 Publisher's version info:eu-repo/semantics/publishedVersion |
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article |
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publishedVersion |
| dc.identifier.none.fl_str_mv |
http://hdl.handle.net/10261/375060 |
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http://hdl.handle.net/10261/375060 |
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Inglés |
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Inglés |
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info:eu-repo/semantics/openAccess |
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openAccess |
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application/pdf |
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EDP Sciences |
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EDP Sciences |
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reponame:DIGITAL.CSIC. Repositorio Institucional del CSIC instname:Consejo Superior de Investigaciones Científicas (CSIC) |
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1869410413971505152 |
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JWST's PEARLS: 119 multiply imaged galaxies behind MACS0416, lensing properties of caustic crossing galaxies, and the relation between halo mass and number of globular clusters at z = 0.4Diego, José MaríaAdams, NathanWillner, Steven P.Harvey, ThomasBroadhurst, TomCohen, SethJansen, Rolf A.Summers, JakeWindhorst, Rogier A.D’Silva, Jordan C. J.Koekemoer, Anton M.Coe, DanConselice, Christopher J.Driver, Simon P.Frye, BrendaGrogin, Norman A.Marshall, Madeline A.Nonino, MarioOrtiz III, RafaelPirzkal, NorRobotham, AaronRyan Jr., Russell E.Willmer, Christopher N. A.Yan, HaojingSun, FengwuHainline, KevinBerkheimer, JessicaPolleta, Maria del CarmenZitrin, AdiGravitational lensing: strongGalaxies: clusters: intracluster mediumGalaxies: clusters: individual: MACS J0416.1-2403 (MACS0416)Dark matterWe present a new lens model for the ɀ = 0.396 galaxy cluster MACS J0416.1 –2403 based on a previously known set of 77 spectroscop-ically confirmed, multiply imaged galaxies plus an additional set of 42 candidate multiply imaged galaxies from past HST and new JWST data. The new galaxies lack spectroscopic redshifts but have geometric and/or photometric redshift estimates that are presented here. The new model predicts magnifications and time delays for all multiple images. The full set of constraints totals 343, constituting the largest sample of multiple images lensed by a single cluster to date. Caustic-crossing galaxies lensed by this cluster are especially interesting. Some of these galaxies show transient events, most of which are interpreted as micro-lensing of stars at cosmological distances. These caustic-crossing arcs are expected to show similar events in future, deeper JWST observations. We provide time delay and magnification models for all these arcs. The time delays and the magnifications for different arcs are generally anti-correlated. In the major sub-halos of the cluster, the dark-matter mass from our lens model correlates well with the observed number of globular clusters, as expected from N-body simulations. This confirms earlier results, derived at lower redshifts, which suggest that globular clusters can be used as powerful mass proxies for the halo masses when lensing constraints are scarce or not available.This work is based on observations made with the NASA/ESA/CSA James Webb Space Telescope. The data were obtained from the Mikulski Archive for Space Telescopes at the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS 5-03127 for JWST. These observations are associated with JWST programs 1176 and 2738. JMD acknowledges the support of project PID2022-138896NB-C51 (MCIU/AEI/MINECO/FEDER, UE) Ministerio de Ciencia, Investigación y Universidades. RAW, SHC, and RAJ acknowledge support from NASA JWST Interdisciplinary Scientist grants NAG5-12460, NNX14AN10G and 80NSSC18K0200 from GSFC. Work by CJC acknowledges support from the European Research Council (ERC) Advanced Investigator Grant EPOCHS (788113). BLF thanks the Berkeley Center for Theoretical Physics for their hospitality during the writing of this paper. MAM acknowledges the support of a National Research Council of Canada Plaskett Fellowship, and the Australian Research Council Centre of Excellence for All Sky Astrophysics in 3 Dimensions (ASTRO 3D), through project number CE17010001. CNAW acknowledges funding from the JWST/NIRCam contract NASS-0215 to the University of Arizona. We thank the CANUCS team for generously providing early access to their proprietary data of MACS0416. AZ acknowledges support by Grant No. 2020750 from the United States-Israel Binational Science Foundation (BSF) and Grant No. 2109066 from the United States National Science Foundation (NSF); by the Ministry of Science & Technology, Israel; and by the Israel Science Foundation Grant No. 864/23.Peer reviewedEDP SciencesNASAEuropean Space AgencyUniversities Space Research Association (US)Agencia Estatal de Investigación (España)Ministerio de Ciencia, Innovación y Universidades (España)European CommissionEuropean Research CouncilAustralian Research CouncilNational Research Council of CanadaUnited States-Israel Binational Science FoundationMinistry of Science, Technology and Space (Israel)University of ArizonaIsrael Science FoundationConsejo Superior de Investigaciones Científicas [https://ror.org/02gfc7t72]202420242024info:eu-repo/semantics/articlehttp://purl.org/coar/resource_type/c_6501Publisher's versioninfo:eu-repo/semantics/publishedVersionapplication/pdfhttp://hdl.handle.net/10261/375060reponame:DIGITAL.CSIC. Repositorio Institucional del CSICinstname:Consejo Superior de Investigaciones Científicas (CSIC)Inglés#PLACEHOLDER_PARENT_METADATA_VALUE##PLACEHOLDER_PARENT_METADATA_VALUE#info:eu-repo/grantAgreement/AEI/Plan Estatal de Investigación Científica y Técnica y de Innovación 2021-2023/PID2022-138896NB-C51info:eu-repo/grantAgreement/EC/H2020/788113https://doi.org/10.1051/0004-6361/202349119Síinfo:eu-repo/semantics/openAccessoai:digital.csic.es:10261/3750602026-05-22T06:33:51Z |
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