Cosmological parameters; Galaxies: elliptical and lenticular, cD; Galaxies: evolution; Galaxies: structure; Gravitational lensing: strong; Elliptical galaxies; Galaxy evolution; Gravitational lensing; Initial mass; Mass structure; Stellars; Astronomy and Astrophysics; Space and Planetary Science
Abstract :
[en] Strong gravitational lensing at the galaxy scale is a valuable tool for various applications in astrophysics and cosmology. Some of the primary uses of galaxy-scale lensing are to study elliptical galaxies' mass structure and evolution, constrain the stellar initial mass function, and measure cosmological parameters. Since the discovery of the first galaxy-scale lens in the 1980s, this field has made significant advancements in data quality and modeling techniques. In this review, we describe the most common methods for modeling lensing observables, especially imaging data, as they are the most accessible and informative source of lensing observables. We then summarize the primary findings from the literature on the astrophysical and cosmological applications of galaxy-scale lenses. We also discuss the current limitations of the data and methodologies and provide an outlook on the expected improvements in both areas in the near future.
Research Center/Unit :
STAR - Space sciences, Technologies and Astrophysics Research - ULiège
Disciplines :
Space science, astronomy & astrophysics
Author, co-author :
Shajib, A J ; Department of Astronomy and Astrophysics, University of Chicago, Chicago, IL 60637 USA ; Kavli Institute for Cosmological Physics, University of Chicago, Chicago, IL 60637 USA
Vernardos, G ; Institute of Physics, Laboratory of Astrophysics, Ecole Polytechnique Fédérale de Lausanne (EPFL), Observatoire de Sauverny, 1290 Versoix, Switzerland ; Department of Astrophysics, American Museum of Natural History, Central Park West and 79th Street, New York, NY 10024-5192 USA ; Department of Physics and Astronomy, Lehman College of the CUNY, Bronx, NY 10468 USA
Collett, T E; Institute of Cosmology and Gravitation, University of Portsmouth, Burnaby Rd, Portsmouth, PO1 3FX UK
Motta, V; Instituto de Fisica y Astronomia, Facultad de Ciencias, Universidad de Valparaiso, Avda. Gran Bretana 1111, Valparaiso, Chile
Sluse, Dominique ; Université de Liège - ULiège > Département d'astrophysique, géophysique et océanographie (AGO) ; STAR Institute, Quartier Agora - Allée du six Aout, 19c B-4000 Liége, Belgium
Williams, L L R; School of Physics and Astronomy, University of Minnesota, 116 Church Street SE, Minneapolis, MN 55455 USA
Saha, P; Physik-Institut, University of Zurich, Winterthurerstrasse 190, 8057 Zurich, Switzerland
Birrer, S; Kavli Institute for Particle Astrophysics and Cosmology and Department of Physics, Stanford University, Stanford, CA 94305 USA ; SLAC National Accelerator Laboratory, Menlo Park, CA 94025 USA ; Department of Physics and Astronomy, Stony Brook University, Stony Brook, NY 11794 USA
Spiniello, C; Department of Physics, University of Oxford, Denys Wilkinson Building, Keble Road, Oxford, OX1 3RH UK ; INAF - Osservatorio Astronomico di Capodimonte, Via Moiariello 16, 80131 Naples, Italy
Treu, T; Department of Physics and Astronomy, University of California, Los Angeles, 430 Portola Plaza, Los Angeles, CA 90095 USA
Language :
English
Title :
Strong Lensing by Galaxies.
Publication date :
2024
Journal title :
Space Science Reviews
ISSN :
0038-6308
eISSN :
1572-9672
Publisher :
Springer Science and Business Media B.V., Netherlands
NASA - National Aeronautics and Space Administration EU - European Union EPFL - École Polytechnique Fédérale de Lausanne
Funding text :
The authors thank the anonymous referees for helpful comments that improved the content and quality of the manuscript. The authors also thank Caro Derkenne and Nandini Sahu for providing a compilation of measurements from the literature, which was used in Fig. . The authors thank the International Space Science Institute in Bern (ISSI) for their hospitality and the conveners for organizing the stimulating workshop on \u201CStrong Gravitational Lensing\u201D. Support for this work was provided by NASA through the NASA Hubble Fellowship grant HST-HF2-51492 awarded to AJS by the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Inc., for NASA, under contract NAS5-26555. This work was also supported by the U.S. Department of Energy (DOE) Office of Science Distinguished Scientist Fellow Program. GV has received funding from the European Union\u2019s Horizon 2020 research and innovation program under the Marie Sk\u0142odowska-Curie grant agreement No 897124. This research was made possible by the generosity of Eric and Wendy Schmidt by recommendation of the Schmidt Futures program. VM acknowledges partial support from Centro de Astrof\u00EDsica de Valpara\u00EDso and project \u201CFortalecimiento del Sistema de Investigaci\u00F3n e Innovaci\u00F3n de la Universidad de Valpara\u00EDso\u201D (UVA20993). This article made use of lenstronomy (Birrer and Amara ; Birrer et al. ), astropy (Astropy Collaboration , , ), numpy (Oliphant ), scipy (Jones et al. ), matplotlib (Hunter ), seaborn (Waskom et al. ), and ChainConsumer (Hinton ).The authors thank the anonymous referees for helpful comments that improved the content and quality of the manuscript. The authors also thank Caro Derkenne and Nandini Sahu for providing a compilation of measurements from the literature, which was used in Fig.\u00A010. The authors thank the International Space Science Institute in Bern (ISSI) for their hospitality and the conveners for organizing the stimulating workshop on \u201CStrong Gravitational Lensing\u201D. Support for this work was provided by NASA through the NASA Hubble Fellowship grant HST-HF2-51492 awarded to AJS by the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Inc., for NASA, under contract NAS5-26555. This work was also supported by the U.S. Department of Energy (DOE) Office of Science Distinguished Scientist Fellow Program. GV has received funding from the European Union\u2019s Horizon 2020 research and innovation program under the Marie Sk\u0142odowska-Curie grant agreement No 897124. This research was made possible by the generosity of Eric and Wendy Schmidt by recommendation of the Schmidt Futures program. VM acknowledges partial support from Centro de Astrof\u00EDsica de Valpara\u00EDso and project \u201CFortalecimiento del Sistema de Investigaci\u00F3n e Innovaci\u00F3n de la Universidad de Valpara\u00EDso\u201D (UVA20993). This article made use of lenstronomy (Birrer and Amara 2018 ; Birrer et\u00A0al. 2021), astropy (Astropy Collaboration 2013, 2018, 2022), numpy (Oliphant 2015), scipy (Jones et\u00A0al. 2001), matplotlib (Hunter 2007), seaborn (Waskom et\u00A0al. 2014), and ChainConsumer (Hinton 2016).
Commentary :
Originally published is Space Science Reviews, Vol 220 - Book review dedicated to Strong Gravitational Lensing
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