COSMOS-Web: An Overview of the JWST Cosmic Origins Survey

被引：164

作者：

Casey, Caitlin M. ^{[1
,2
]}

Kartaltepe, Jeyhan S. ^{[3
]}

Drakos, Nicole E. ^{[4
]}

Franco, Maximilien ^{[1
]}

Harish, Santosh ^{[3
]}

Paquereau, Louise ^{[5
,6
]}

Ilbert, Olivier ^{[7
]}

Rose, Caitlin ^{[3
]}

Cox, Isabella G. ^{[3
]}

Nightingale, James W. ^{[8
]}

Robertson, Brant E. ^{[4
]}

Silverman, John D. ^{[9
,10
]}

Koekemoer, Anton M. ^{[11
]}

Massey, Richard ^{[12
]}

McCracken, Henry Joy ^{[5
,6
]}

Rhodes, Jason ^{[13
]}

Akins, Hollis B. ^{[1
]}

Allen, Natalie ^{[2
,14
]}

Amvrosiadis, Aristeidis ^{[8
]}

Arango-Toro, Rafael C. ^{[7
]}

Bagley, Micaela B. ^{[1
]}

Bongiorno, Angela ^{[15
]}

Capak, Peter L. ^{[2
]}

Champagne, Jaclyn B. ^{[16
]}

Chartab, Nima ^{[17
]}

Ortiz, Oscar A. Chavez ^{[1
]}

Chworowsky, Katherine ^{[1
]}

Cooke, Kevin C. ^{[18
]}

Cooper, Olivia R. ^{[1
]}

Darvish, Behnam ^{[19
]}

Ding, Xuheng ^{[9
]}

Faisst, Andreas L. ^{[20
]}

Finkelstein, Steven L. ^{[1
]}

Fujimoto, Seiji ^{[1
]}

Gentile, Fabrizio ^{[21
,22
]}

Gillman, Steven ^{[2
,23
]}

Gould, Katriona M. L. ^{[2
]}

Gozaliasl, Ghassem ^{[24
]}

Hayward, Christopher C. ^{[25
]}

He, Qiuhan ^{[8
]}

Hemmati, Shoubaneh ^{[27
]}

Hirschmann, Michaela ^{[26
,39
]}

Jahnke, Knud ^{[28
]}

Jin, Shuowen ^{[2
]}

Khostovan, Ali Ahmad ^{[3
]}

Kokorev, Vasily ^{[29
]}

Lambrides, Erini ^{[30
]}

Laigle, Clotilde ^{[5
,6
]}

Larson, Rebecca L. ^{[1
]}

Leung, Gene C. K. ^{[1
]}

机构：

[1] Univ Texas Austin, 2515 Speedway Blvd Stop,C1400, Austin, TX 78712 USA

[2] Cosm Dawn Ctr DAWN, Copenhagen, Denmark

[3] Rochester Inst Technol, Sch Phys & Astron, Lab Multiwavelength Astrophys, 84 Lomb Mem Dr, Rochester, NY 14623 USA

[4] Univ Calif Santa Cruz, Dept Astron & Astrophys, 1156 High St, Santa Cruz, CA 95064 USA

[5] Inst Astrophys Paris, UMR 7095, CNRS, 98 Bis Blvd Arago, F-75014 Paris, France

[6] Sorbonne Univ, 98 Bis Blvd Arago, F-75014 Paris, France

[7] Aix Marseille Univ, CNRS, CNES, LAM, Marseille, France

[8] Univ Durham, Inst Computat Cosmol, Dept Phys, South Rd, Durham DH1 3LE, England

[9] Univ Tokyo, Kavli Inst Phys & Math Universe WPI, Kashiwa, Chiba 2778583, Japan

[10] Univ Tokyo, Sch Sci, Dept Astron, 7-3-1 Hongo, Bunkyo, Tokyo 1130033, Japan

[11] Space Telescope Sci Inst, 3700 San Martin Dr, Baltimore, MD 21218 USA

[12] Univ Durham, Ctr Extragalact Astron, Dept Phys, South Rd, Durham DH1 3LE, England

[13] CALTECH, Jet Prop Lab, 4800 Oak Grove Dr, Pasadena, CA 91001 USA

[14] Univ Copenhagen, Niels Bohr Inst, Jagtvej 128, DK-2200 Copenhagen, Denmark

[15] Observ Rome, INAF, Via Frascati 33, I-00074 Monte Porzio Catone, Italy

[16] Univ Arizona, Steward Observ, 933 N Cherry Ave, Tucson, AZ 85721 USA

[17] Observ Carnegie Inst Sci, 813 Santa Barbara St, Pasadena, CA 91101 USA

[18] Assoc Publ & Land Grant Univ, 1220 L St NW,Suite 1000, Washington, DC 20005 USA

[19] Univ Calif Riverside, Dept Phys & Astron, 900 Univ Ave, Riverside, CA 92521 USA

[20] Caltech, IPAC, 1200 E Calif Blvd, Pasadena, CA 91125 USA

[21] Univ Bologna, Dept Phys & Astron Augusto Righi DIFA, Via Gobetti 93-2, I-40129 Bologna, Italy

[22] INAF, Osservatorio Astrofis & Sci Spazio, Via Gobetti 93-3, I-40129 Bologna, Italy

[23] Tech Univ Denmark, DTU Space, Elektrovej 327, DK-2800 Lyngby, Denmark

[24] Univ Helsinki, Dept Phys, POB 64, FI-00014 Helsinki, Finland

[25] Flatiron Inst, Ctr Computat Astrophys, 162 Fifth Ave, New York, NY 10010 USA

[26] Ecole Polytech Fed Lausanne, Inst Phys, GalSpec, Observ Sauverny, CH-1290 Versoix, Switzerland

[27] Astron Observ Trieste, INAF, Via Tiepolo 11, I-34131 Trieste, Italy

[28] Max Planck Inst Astron, Konigstuhl 17, D-69117 Heidelberg, Germany

[29] Univ Groningen, Kapteyn Astron Inst, POB 800, NL-9700 AB Groningen, Netherlands

[30] NASA Goddard Space Flight Ctr, Code 662, Greenbelt, MD 20771 USA

[31] Max Planck Inst Extraterrestr Phys MPE, Giessenbachstr 1, D-85748 Garching, Germany

[32] Univ Paris Saclay, Univ Paris Cite, CNRS, CEA, Gif sur Yvette, France

[33] European Southern Observ, Karl Schwarzschild Str 2, D-85748 Garching, Germany

[34] Univ Massachusetts Amherst, Dept Astron, 710 N Pleasant St, Amherst, MA 01003 USA

[35] Univ Portsmouth, Inst Cosmol & Gravitat, Dennis Sciama Bldg Rd, Burnaby, BC PO13FX, Canada

[36] Univ Calif Santa Barbara, Dept Phys, Santa Barbara, CA 93109 USA

[37] Northeastern Univ, Dept Phys, 360 Huntington Ave, Boston, MA 02115 USA

[38] Osserv Astron Padova, Ist Nazl Astrofis INAF, Vicolo Osservatorio 5, I-35122 Padua, Italy

[39] UCLA, Dept Phys & Astron, PAB 430 Portola Plaza,Box 951547, Los Angeles, CA 90095 USA

[40] Univ Hawaii Manoa, Inst Astron, 2680 Woodlawn Dr, Honolulu, HI 96822 USA

[41] Argelander Inst Astron, Hugel 71, D-53121 Bonn, Germany

[42] CALTECH, Dept Astron, 1200 Calif Blvd, Pasadena, CA 91125 USA

[43] NASA Headquarters, 300 Hidden Figures Way,SE,Mary W Jackson NASA HQ, Washington, DC 20546 USA

[44] Univ Potsdam, Inst Phys & Astron, Karl Liebknecht Str 24 25, D-14476 Golm, Germany

[45] Leibniz Inst Astrophys Potsdam AIP, Sternwarte 6, D-14482 Potsdam, Germany

[46] Tel Aviv Univ, Sch Phys & Astron, IL-69978 Tel Aviv, Israel

[47] Yale Univ, Phys Dept, POB 208120, New Haven, CT 06511 USA

[48] Yale Univ, Yale Ctr Astron & Astrophys, POB 208120, New Haven, CT 06511 USA

[49] Thuringer Landessternwarte, Sternwarte 5, D-07778 Tautenburg, Germany

[50] Univ Sussex, Ctr Astron, Brighton BN1 9QH, E Sussex, England

来源：

ASTROPHYSICAL JOURNAL | 2023年 / 954卷 / 01期

基金：

欧洲研究理事会; 美国国家科学基金会; 以色列科学基金会; 新加坡国家研究基金会;

关键词：

STAR-FORMING GALAXIES; HUBBLE-SPACE-TELESCOPE; MASSIVE QUIESCENT GALAXIES; ACTIVE GALACTIC NUCLEI; HIGH-REDSHIFT GALAXIES; DARK-MATTER HALOES; SIMILAR-TO; REMARKABLY LUMINOUS GALAXY; DUST-ATTENUATION LAW; GOODS NICMOS SURVEY;

D O I：

10.3847/1538-4357/acc2bc

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

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 & sigma; point-source depths ranging & SIM;27.5-28.2 mag. In parallel, we will obtain 0.19 deg(2) of MIRI imaging in one filter (F770W) reaching 5 & sigma; point-source depths of & SIM;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 & LSIM; z & LSIM; 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 (& ODOT;)), and (3) directly measure the evolution of the stellar-mass-to-halo-mass relation using weak gravitational lensing out to z & SIM; 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.

引用

页数：32

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