期刊
ASTROPHYSICAL JOURNAL
卷 926, 期 1, 页码 -出版社
IOP Publishing Ltd
DOI: 10.3847/1538-4357/ac404a
关键词
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资金
- NSF-AAG [1907697]
- National Science Foundation [PHY1607611]
- UCSC Chancellor's Fellowship
- National Aeronautics and Space Administration
- Alfred P. Sloan Foundation
- U.S. Department of Energy Office of Science
- University of Arizona
- Carnegie Mellon University
- University of Florida
- Harvard University
- Instituto de Astrofisica de Canarias
- Johns Hopkins University
- Lawrence Berkeley National Laboratory
- Max Planck Institute for Extraterrestrial Physics
- New Mexico State University
- New York University
- Ohio State University
- Pennsylvania State University
- University of Portsmouth
- Princeton University
- University of Tokyo
- University of Utah
- Vanderbilt University
- University of Virginia
- University of Washington
- Yale University
- National Science Foundation
- Brazilian Participation Group
- Brookhaven National Laboratory
- Max Planck Institute for Astrophysics
- French Participation Group
- German Participation Group
- Spanish Participation Group
- Michigan State/Notre Dame/JINA Participation Group
- Division Of Astronomical Sciences
- Direct For Mathematical & Physical Scien [1907697] Funding Source: National Science Foundation
We describe the SQuIGG (L→E) project that studies the quenching process in intermediate-redshift galaxies. This project investigates various aspects of the quenching process by studying a large sample of bright post-starburst galaxies. Specifically, the survey examines the molecular gas reservoirs, morphologies, kinematics, resolved stellar populations, active galactic nucleus incidence, and infrared properties of this unique sample in order to place definitive constraints on the quenching process.
We describe the Studying Quenching in Intermediate-z Galaxies: Gas, angu (L) over right arrow ar momentum, and Evolution (SQuIGG (L) over right arrowE 75% of SQuIGG (L) over right arrowE E z less than or similar to 1 post-starburst galaxy samples. This large sample of bright post-starburst galaxies at intermediate redshift opens a wide range of studies into the quenching process. In particular, the full SQuIGG (L) over right arrowE survey will investigate the molecular gas reservoirs, morphologies, kinematics, resolved stellar populations, active galactic nucleus incidence, and infrared properties of this unique sample of galaxies in order to place definitive constraints on the quenching process.
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