COSMOS-Web: An Overview of the JWST Cosmic Origins Survey
We present the survey design, implementation, and outlook for COSMOS-Web, a 255 hr treasury program conducted by the James Webb Space Telescope in its first cycle of observations. COSMOS-Web is a contiguous 0.54 deg 2 NIRCam imaging survey in four filters (F115W, F150W, F277W, and F444W) that will r...
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| Veröffentlicht in: | The Astrophysical journal Jg. 954; H. 1; S. 31 - 62 |
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| Format: | Journal Article |
| Sprache: | Englisch |
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The American Astronomical Society
01.09.2023
IOP Publishing |
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| ISSN: | 0004-637X, 1538-4357, 1538-4357 |
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| Abstract | We present the survey design, implementation, and outlook for COSMOS-Web, a 255 hr treasury program conducted by the James Webb Space Telescope in its first cycle of observations. COSMOS-Web is a contiguous 0.54 deg
2
NIRCam imaging survey in four filters (F115W, F150W, F277W, and F444W) that will reach 5
σ
point-source depths ranging ∼27.5–28.2 mag. In parallel, we will obtain 0.19 deg
2
of MIRI imaging in one filter (F770W) reaching 5
σ
point-source depths of ∼25.3–26.0 mag. COSMOS-Web will build on the rich heritage of multiwavelength observations and data products available in the COSMOS field. The design of COSMOS-Web is motivated by three primary science goals: (1) to discover thousands of galaxies in the Epoch of Reionization (6 ≲
z
≲ 11) and map reionization’s spatial distribution, environments, and drivers on scales sufficiently large to mitigate cosmic variance, (2) to identify hundreds of rare quiescent galaxies at
z
> 4 and place constraints on the formation of the universe’s most-massive galaxies (
M
⋆
> 10
10
M
⊙
), and (3) directly measure the evolution of the stellar-mass-to-halo-mass relation using weak gravitational lensing out to
z
∼ 2.5 and measure its variance with galaxies’ star formation histories and morphologies. In addition, we anticipate COSMOS-Web’s legacy value to reach far beyond these scientific goals, touching many other areas of astrophysics, such as the identification of the first direct collapse black hole candidates, ultracool subdwarf stars in the Galactic halo, and possibly the identification of
z
> 10 pair-instability supernovae. In this paper we provide an overview of the survey’s key measurements, specifications, goals, and prospects for new discovery. |
|---|---|
| AbstractList | We present the survey design, implementation, and outlook for COSMOS-Web, a 255 hr treasury program conducted by the James Webb Space Telescope in its first cycle of observations. COSMOS-Web is a contiguous 0.54 deg ^2 NIRCam imaging survey in four filters (F115W, F150W, F277W, and F444W) that will reach 5 σ point-source depths ranging ∼27.5–28.2 mag. In parallel, we will obtain 0.19 deg ^2 of MIRI imaging in one filter (F770W) reaching 5 σ point-source depths of ∼25.3–26.0 mag. COSMOS-Web will build on the rich heritage of multiwavelength observations and data products available in the COSMOS field. The design of COSMOS-Web is motivated by three primary science goals: (1) to discover thousands of galaxies in the Epoch of Reionization (6 ≲ z ≲ 11) and map reionization’s spatial distribution, environments, and drivers on scales sufficiently large to mitigate cosmic variance, (2) to identify hundreds of rare quiescent galaxies at z > 4 and place constraints on the formation of the universe’s most-massive galaxies ( M _⋆ > 10 ^10 M _⊙ ), and (3) directly measure the evolution of the stellar-mass-to-halo-mass relation using weak gravitational lensing out to z ∼ 2.5 and measure its variance with galaxies’ star formation histories and morphologies. In addition, we anticipate COSMOS-Web’s legacy value to reach far beyond these scientific goals, touching many other areas of astrophysics, such as the identification of the first direct collapse black hole candidates, ultracool subdwarf stars in the Galactic halo, and possibly the identification of z > 10 pair-instability supernovae. In this paper we provide an overview of the survey’s key measurements, specifications, goals, and prospects for new discovery. We present the survey design, implementation, and outlook for COSMOS-Web, a 255 hr treasury program conducted by the James Webb Space Telescope in its first cycle of observations. COSMOS-Web is a contiguous 0.54 deg2 NIRCam imaging survey in four filters (F115W, F150W, F277W, and F444W) that will reach 5σ point-source depths ranging ∼27.5–28.2 mag. In parallel, we will obtain 0.19 deg2 of MIRI imaging in one filter (F770W) reaching 5σ point-source depths of ∼25.3–26.0 mag. COSMOS-Web will build on the rich heritage of multiwavelength observations and data products available in the COSMOS field. The design of COSMOS-Web is motivated by three primary science goals: (1) to discover thousands of galaxies in the Epoch of Reionization (6 ≲ z ≲ 11) and map reionization’s spatial distribution, environments, and drivers on scales sufficiently large to mitigate cosmic variance, (2) to identify hundreds of rare quiescent galaxies at z > 4 and place constraints on the formation of the universe’s most-massive galaxies (M⋆ > 1010M⊙), and (3) directly measure the evolution of the stellar-mass-to-halo-mass relation using weak gravitational lensing out to z ∼ 2.5 and measure its variance with galaxies’ star formation histories and morphologies. In addition, we anticipate COSMOS-Web’s legacy value to reach far beyond these scientific goals, touching many other areas of astrophysics, such as the identification of the first direct collapse black hole candidates, ultracool subdwarf stars in the Galactic halo, and possibly the identification of z > 10 pair-instability supernovae. In this paper we provide an overview of the survey’s key measurements, specifications, goals, and prospects for new discovery. We present the survey design, implementation, and outlook for COSMOS-Web, a 255 hr treasury program conducted by the James Webb Space Telescope in its first cycle of observations. COSMOS-Web is a contiguous 0.54 deg 2 NIRCam imaging survey in four filters (F115W, F150W, F277W, and F444W) that will reach 5 σ point-source depths ranging ∼27.5–28.2 mag. In parallel, we will obtain 0.19 deg 2 of MIRI imaging in one filter (F770W) reaching 5 σ point-source depths of ∼25.3–26.0 mag. COSMOS-Web will build on the rich heritage of multiwavelength observations and data products available in the COSMOS field. The design of COSMOS-Web is motivated by three primary science goals: (1) to discover thousands of galaxies in the Epoch of Reionization (6 ≲ z ≲ 11) and map reionization’s spatial distribution, environments, and drivers on scales sufficiently large to mitigate cosmic variance, (2) to identify hundreds of rare quiescent galaxies at z > 4 and place constraints on the formation of the universe’s most-massive galaxies ( M ⋆ > 10 10 M ⊙ ), and (3) directly measure the evolution of the stellar-mass-to-halo-mass relation using weak gravitational lensing out to z ∼ 2.5 and measure its variance with galaxies’ star formation histories and morphologies. In addition, we anticipate COSMOS-Web’s legacy value to reach far beyond these scientific goals, touching many other areas of astrophysics, such as the identification of the first direct collapse black hole candidates, ultracool subdwarf stars in the Galactic halo, and possibly the identification of z > 10 pair-instability supernovae. In this paper we provide an overview of the survey’s key measurements, specifications, goals, and prospects for new discovery. |
| Author | Massey, Richard Bagley, Micaela B. McPartland, Conor J. R. Mainieri, Vincenzo Zavala, Jorge A. Yang, Lilan Casey, Caitlin M. Chartab, Nima Paquereau, Louise Magdis, Georgios Leung, Gene C. K. Urry, C. Megan Ilbert, Olivier He, Qiuhan Vardoulaki, Eleni Fujimoto, Seiji Jahnke, Knud Akins, Hollis B. Liaudat, Tobias Mobasher, Bahram Chávez Ortiz, Óscar A. Allen, Natalie Champagne, Jaclyn B. Khostovan, Ali Ahmad Nightingale, James W. Capak, Peter L. Gozaliasl, Ghassem Manning, Sinclaire M. Rose, Caitlin Hemmati, Shoubaneh Cooke, Kevin C. Long, Arianna S. Sheth, Kartik Rich, R. Michael Talia, Margherita Shuntov, Marko Bongiorno, Angela Martin, Crystal L. Faisst, Andreas L. Sparre, Martin Laigle, Clotilde Mahler, Guillaume Sattari, Zahra Robertson, Brant E. Silverman, John D. Scoville, Nick Rhodes, Jason Kokorev, Vasily Kartaltepe, Jeyhan S. Trakhtenbrot, Benny McCleary, Jacqueline E. Finkelstein, Steven L. Larson, Rebecca L. Darvish, Behnam Whitaker, Katherine E. Harish, Santosh Jin, Shuowen Koekemoer, Anton M. McCracken, Henry Joy Vanderhoof, Britt |
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Megan orcidid: 0000-0002-0745-9792 surname: Urry fullname: Urry, C. Megan organization: Yale University Physics Department and Yale Center for Astronomy & Astrophysics, P.O. Box 208120, CT 06520, USA – sequence: 79 givenname: Francesco orcidid: 0000-0001-6477-4011 surname: Valentino fullname: Valentino, Francesco organization: University of Copenhagen Niels Bohr Institute, Jagtvej 128, DK-2200, Copenhagen, Denmark – sequence: 80 givenname: Brittany N. orcidid: 0000-0002-8163-0172 surname: Vanderhoof fullname: Vanderhoof, Brittany N. organization: School of Physics and Astronomy Laboratory for Multiwavelength Astrophysics, Rochester Institute of Technology, 84 Lomb Memorial Drive, Rochester, NY 14623, USA – sequence: 81 givenname: Eleni orcidid: 0000-0002-4437-1773 surname: Vardoulaki fullname: Vardoulaki, Eleni organization: Thüringer Landessternwarte , Sternwarte 5, D-07778 Tautenburg, Germany – sequence: 82 givenname: John R. orcidid: 0000-0003-1614-196X surname: Weaver fullname: Weaver, John R. organization: University of Massachusetts Amherst Department of Astronomy, 710 N Pleasant Street, Amherst, MA 01003, USA – sequence: 83 givenname: Katherine E. orcidid: 0000-0001-7160-3632 surname: Whitaker fullname: Whitaker, Katherine E. organization: University of Massachusetts Amherst Department of Astronomy, 710 N Pleasant Street, Amherst, MA 01003, USA – sequence: 84 givenname: Stephen M. orcidid: 0000-0003-3903-6935 surname: Wilkins fullname: Wilkins, Stephen M. organization: University of Malta Institute of Space Sciences and Astronomy, Msida MSD 2080, Malta – sequence: 85 givenname: Lilan orcidid: 0000-0002-8434-880X surname: Yang fullname: Yang, Lilan organization: The University of Tokyo Kavli Institute for the Physics and Mathematics of the Universe (WPI), Kashiwa, Chiba 277-8583, Japan – sequence: 86 givenname: Jorge A. orcidid: 0000-0002-7051-1100 surname: Zavala fullname: Zavala, Jorge A. organization: National Astronomical Observatory of Japan , 2-21-1 Osawa, Mitaka, Tokyo 181-8588, Japan |
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| Title | COSMOS-Web: An Overview of the JWST Cosmic Origins Survey |
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