The GLASS-JWST Early Release Science Program. I. Survey Design and Release Plans

被引：212

作者：

Treu, T. ^{[1
]}

Roberts-Borsani, G. ^{[1
]}

Bradac, M. ^{[2
,3
]}

Brammer, G. ^{[4
,5
]}

Fontana, A. ^{[6
]}

Henry, A. ^{[7
,8
]}

Mason, C. ^{[4
,5
]}

Morishita, T. ^{[9
]}

Pentericci, L. ^{[6
]}

Wang, X. ^{[9
]}

Acebron, A. ^{[10
,11
]}

Bagley, M. ^{[12
]}

Bergamini, P. ^{[10
,13
]}

Belfiori, D. ^{[6
]}

Bonchi, A. ^{[6
,14
]}

Boyett, K. ^{[15
,16
]}

Boutsia, K. ^{[17
]}

Calabro, A. ^{[6
]}

Caminha, G. B. ^{[18
]}

Castellano, M. ^{[6
]}

Dressler, A. ^{[19
]}

Glazebrook, K. ^{[16
,20
]}

Grillo, C. ^{[10
,11
]}

Jacobs, C. ^{[16
,20
]}

Jones, T. ^{[3
]}

Kelly, P. L. ^{[21
]}

Leethochawalit, N. ^{[15
,16
]}

Malkan, M. A. ^{[1
]}

Marchesini, D. ^{[22
]}

Mascia, S. ^{[6
]}

Mercurio, A. ^{[23
]}

Merlin, E. ^{[6
]}

Nanayakkara, T. ^{[16
,20
]}

Nonino, M. ^{[24
]}

Paris, D. ^{[6
]}

Poggianti, B. ^{[25
]}

Rosati, P. ^{[13
,26
]}

Santini, P. ^{[6
]}

Scarlata, C. ^{[27
]}

Shipley, H., V ^{[22
]}

Strait, V ^{[4
,5
]}

Trenti, M. ^{[15
,16
]}

Tubthong, C. ^{[22
]}

Vanzella, E. ^{[13
]}

Vulcani, B. ^{[25
]}

Yang, L. ^{[28
]}

机构：

[1] Univ Calif Los Angeles, Dept Phys & Astron, 430 Portola Plaza, Los Angeles, CA 90095 USA

[2] Univ Ljubljana, Dept Math & Phys, Jadranska Ulica 19, SI-1000 Ljubljana, Slovenia

[3] Univ Calif Davis, Dept Phys & Astron, 1 Shields Ave, Davis, CA 95616 USA

[4] Cosm Dawn Ctr DAWN, Copenhagen, Denmark

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

[6] INAF Osservatorio Astron Roma, Via Frascati 33, I-00078 Rome, Italy

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

[8] Johns Hopkins Univ, Ctr Astrophys Sci, Dept Phys & Astron, Baltimore, MD 21218 USA

[9] CALTECH, Infrared Proc & Anal Ctr, 1200 E Calif Blvd, Pasadena, CA 91125 USA

[10] Univ Milan, Dipartimento Fis, Via Celoria 16, I-20133 Milan, Italy

[11] INAF IASF Milano, Via A Corti 12, I-20133 Milan, Italy

[12] Univ Texas Austin, Dept Astron, RLM 15308, Austin, TX 78712 USA

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

[14] ASI Space Sci Data Ctr, Via Politecn, I-00133 Rome, Italy

[15] Univ Melbourne, Sch Phys, Parkville, Vic 3010, Australia

[16] ARC Ctr Excellence All Sky Astrophys 3 Dimens AST, Canberra, ACT, Australia

[17] Carnegie Observ, Las Campanas Observ, Casilla 601, La Serena, Chile

[18] Max Planck Inst Astrophys, Karl Schwarzschild Str 1, D-85748 Garching, Germany

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

[20] Swinburne Univ Technol, Ctr Astrophys & Supercomp, POB 218, Hawthorn, Vic 3122, Australia

[21] Univ Minnesota, Minnesota Inst Astrophys, 116 Church St SE, Minneapolis, MN 55455 USA

[22] Tufts Univ, Dept Phys & Astron, 574 Boston Ave, Medford, MA 02155 USA

[23] INAF Osservatorio Astron Capodimonte, Via Moiariello 16, I-80131 Naples, Italy

[24] INAF Osservatorio Astron Trieste, Via Tiepolo 11, I-34143 Trieste, Italy

[25] INAF Osservatorio Astron Padova, Vicolo Osservatorio 5, I-35122 Padua, Italy

[26] Univ Ferrara, Dipartimento Fis & Sci Terra, Via Saragat 1, I-44122 Ferrara, Italy

[27] Univ Minnesota, Sch Phys & Astron, Minneapolis, MN 55455 USA

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

来源：

ASTROPHYSICAL JOURNAL | 2022年 / 935卷 / 02期

基金：

欧洲研究理事会; 新加坡国家研究基金会; 澳大利亚研究理事会;

关键词：

STAR-FORMING GALAXIES; LENS-AMPLIFIED SURVEY; MASS-METALLICITY RELATION; SIMILAR-TO; 8; LY-ALPHA; SPATIAL OFFSETS; ANALYTIC MODEL; COSMIC NOON; O III; REIONIZATION;

D O I：

10.3847/1538-4357/ac8158

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The GLASS-JWST Early Release Science (hereafter GLASS-JWST-ERS) Program will obtain and make publicly available the deepest extragalactic data of the ERS campaign. It is primarily designed to address two key science questions, namely, "what sources ionized the universe and when?" and "how do baryons cycle through galaxies?", while also enabling a broad variety of first look scientific investigations. In primary mode, it will obtain NIRISS and NIRSpec spectroscopy of galaxies lensed by the foreground Hubble Frontier Field cluster, Abell 2744. In parallel, it will use NIRCam to observe two fields that are offset from the cluster center, where lensing magnification is negligible, and which can thus be effectively considered blank fields. In order to prepare the community for access to this unprecedented data, we describe the scientific rationale, the survey design (including target selection and observational setups), and present pre-commissioning estimates of the expected sensitivity. In addition, we describe the planned public releases of high-level data products, for use by the wider astronomical community.

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