Journal article icon

Journal article : Review

Strong Lensing by Galaxies

Abstract:
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.
Publication status:
Published
Peer review status:
Peer reviewed

Actions


Access Document


Files:
Publisher copy:
10.1007/s11214-024-01105-x

Authors


More by this author
Role:
Author
ORCID:
0000-0002-5558-888X
More by this author
Role:
Author
ORCID:
0000-0001-8554-7248



Publisher:
Springer
Journal:
Space Science Reviews More from this journal
Volume:
220
Issue:
8
Article number:
87
Publication date:
2024-11-08
Acceptance date:
2024-08-26
DOI:
EISSN:
1572-9672
ISSN:
0038-6308


Language:
English
Keywords:
Subtype:
Review
Source identifiers:
2406060
Deposit date:
2024-11-08
This ORA record was generated from metadata provided by an external service. It has not been edited by the ORA Team.

Terms of use



Views and Downloads






If you are the owner of this record, you can report an update to it here: Report update to this record

TO TOP