First Data Release of the COSMOS Ly α Mapping and Tomography Observations: 3D Ly α Forest Tomography at 2.05 < z < 2.55
Journal Article
·
· The Astrophysical Journal. Supplement Series (Online)
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- Lawrence Berkeley National Lab. (LBNL), Berkeley, CA (United States)
- Univ. of California, Berkeley, CA (United States). Dept. of Astronomy
- Lawrence Berkeley National Lab. (LBNL), Berkeley, CA (United States); Univ. of California, Berkeley, CA (United States). Dept. of Astronomy
- Univ. of California, Santa Barbara, CA (United States). Dept. of Physics
- Max Planck Inst. for Astronomy, Heidelberg (Germany)
- Univ. of California, Santa Cruz, CA (United States). Dept. of Astronomy and Astrophysics; University of California Observatories, Santa Cruz, CA (United States). Lick Observatory
- Univ. College London, London (United Kingdom). Dept. of Physics and Astronomy
- Univ. of Tokyo (Japan). Kavli Inst. for the Physics and Mathematics of the Universe (IPMU)
- Swinburne Univ. of Technology, Victoria (Australia)
- Rochester Inst. of Technology, Rochester, NY (United States). School of Physics and Astronomy
- Space Telescope Science Inst., Baltimore MD (United States)
- Aix Marseille Univ., Marseille (France). Laboratoire d'Astrophysique de Marseille (LAM)
- Aix Marseille Univ., Marseille (France). Laboratoire d'Astrophysique de Marseille (LAM); Univ. of California, Davis, CA (United States). Dept. of Physics
- Univ. of Vienna (Austria). Dept. of Astrophysics
- Leiden Univ. (Netherlands). Leiden Observatory
- Univ. of California, Los Angeles, CA (United States). Dept. of Physics and Astronomy
- Univ. of Hawaii, Honolulu, HI (United States). Inst. for Astronomy
- Max Planck Inst. for Extraterrestrial Physics, Garching (Germany)
- Univ. of New South Wales, Sydney, NSW (Australia). School of Physics; Texas A & M Univ., College Station, TX (United States). George P. and Cynthia Woods Mitchell Insti. for Fundamental Physics and Astronomy, and Dept. of Physics and Astronomy
Faint star-forming galaxies at $$z\sim 2-3$$ can be used as alternative background sources to probe the Lyman-α forest in addition to quasars, yielding high sightline densities that enable 3D tomographic reconstruction of the foreground absorption field. Here, we present the first data release from the COSMOS Lyman-Alpha Mapping And Mapping Observations (CLAMATO) Survey, which was conducted with the LRIS spectrograph on the Keck-I telescope. Over an observational footprint of 0.157$$\mathrm{deg}^2$$ within the COSMOS field, we used 240 galaxies and quasars at 2.17
- Research Organization:
- Lawrence Berkeley National Laboratory (LBNL), Berkeley, CA (United States)
- Sponsoring Organization:
- USDOE Office of Science (SC), Advanced Scientific Computing Research (ASCR)
- Grant/Contract Number:
- AC02-05CH11231
- OSTI ID:
- 1456980
- Journal Information:
- The Astrophysical Journal. Supplement Series (Online), Vol. 237, Issue 2; Related Information: https://arxiv.org/abs/1710.02894; ISSN 1538-4365
- Publisher:
- American Astronomical Society/IOPCopyright Statement
- Country of Publication:
- United States
- Language:
- English
Cited by: 70 works
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