The Next Generation Deep Extragalactic Exploratory Public (NGDEEP) Survey

被引：38

作者：

Bagley, Micaela B. ^{[1
]}

Pirzkal, Nor ^{[2
,3
]}

Finkelstein, Steven L. ^{[1
]}

Papovich, Casey ^{[4
,5
]}

Berg, Danielle A. ^{[1
]}

Lotz, Jennifer M. ^{[6
]}

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

Ferguson, Henry C. ^{[3
]}

Koekemoer, Anton M. ^{[3
]}

Dickinson, Mark ^{[7
]}

Kartaltepe, Jeyhan S. ^{[8
]}

Kocevski, Dale D. ^{[9
]}

Somerville, Rachel S. ^{[10
]}

Yung, L. Y. Aaron ^{[11
]}

Backhaus, Bren E. ^{[12
]}

Casey, Caitlin M. ^{[1
,13
]}

Castellano, Marco ^{[14
]}

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

Chworowsky, Katherine ^{[1
]}

Cox, Isabella G. ^{[8
]}

Dave, Romeel ^{[15
,16
]}

Davis, Kelcey ^{[12
]}

Estrada-Carpenter, Vicente ^{[17
]}

Fontana, Adriano ^{[14
]}

Fujimoto, Seiji ^{[1
]}

Gardner, Jonathan P. ^{[11
]}

Giavalisco, Mauro ^{[18
]}

Grazian, Andrea ^{[19
]}

Grogin, Norman A. ^{[3
]}

Hathi, Nimish P. ^{[3
]}

Hutchison, Taylor A. ^{[11
]}

Jaskot, Anne E. ^{[20
]}

Jung, Intae ^{[3
]}

Kewley, Lisa J. ^{[21
]}

Kirkpatrick, Allison ^{[22
]}

Larson, Rebecca L. ^{[1
]}

Matharu, Jasleen ^{[13
]}

Natarajan, Priyamvada ^{[23
,24
,25
]}

Pentericci, Laura ^{[14
]}

Perez-Gonzalez, Pablo G. ^{[26
]}

Rothberg, Barry ^{[27
,28
]}

Ravindranath, Swara ^{[3
]}

Ryan, Russell ^{[3
]}

Shen, Lu ^{[4
,5
]}

Simons, Raymond C. ^{[12
]}

Snyder, Gregory F. ^{[3
]}

Trump, Jonathan R. ^{[12
]}

Wilkins, Stephen M. ^{[29
,30
]}

机构：

[1] Univ Texas Austin, Dept Astron, Austin, TX 78712 USA

[2] ESA AURA, Baltimore, MD USA

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

[4] Texas A&M Univ, Dept Phys & Astron, College Stn, TX USA

[5] Texas A&M Univ, George P & Cynthia Woods Mitchell Inst Fundamental, College Stn, TX 77843 USA

[6] NSFs Natl Opt Infrared Astron Res Lab, Gemini Observ, 950 N Cherry Ave, Tucson, AZ 85719 USA

[7] NSFs Natl Opt Infrared Astron Res Lab, 950 N Cherry Ave, Tucson, AZ 85719 USA

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

[9] Colby Coll, Dept Phys & Astron, Waterville, ME 04901 USA

[10] Flatiron Inst, Ctr Computat Astrophys, 162 5th Ave, New York, NY 10010 USA

[11] NASA Goddard Space Flight Ctr, Astrophys Sci Div, 8800 Greenbelt Rd, Greenbelt, MD 20771 USA

[12] Univ Connecticut, Dept Phys, 196 Auditorium Rd,Unit 3046, Storrs, CT USA

[13] Univ Copenhagen, Niels Bohr Inst, Cosm Dawn Ctr, Radmandsgade 62, DK-2200 Copenhagen, Denmark

[14] INAF Osservatorio Astron Roma, Via Frascati 33, I-00078 Monte Porzio Catone, Italy

[15] Univ Edinburgh, Inst Astron, Royal Observ, Edinburgh EH9 3HJ, Scotland

[16] Univ Western Cape, ZA-7535 Cape Town, South Africa

[17] St Marys Univ, Dept Astron & Phys, 923 Robie St, Halifax, NS, Canada

[18] Univ Massachusetts, Dept Astron, Amherst, MA 01003 USA

[19] INAF Osservatorio Astron Padova, Vicolo Osservatorio 5, Padua, Italy

[20] Williams Coll, Dept Astron, Williamstown, MA 01267 USA

[21] Harvard & Smithsonian, Ctr Astrophys, 60 Garden St, Cambridge, MA 02138 USA

[22] Univ Kansas, Dept Phys & Astron, Lawrence, KS 66045 USA

[23] Yale Univ, Yale, CO 06511 USA

[24] Yale Univ, Dept Phys, POB 208121, New Haven, CT USA

[25] Harvard Univ, Black Hole Initiat, 20 Garden St, Cambridge, MA 02138 USA

[26] Ctr Astrobiol CAB, CSIC INTA, Ctra Ajalvir km 4, Madrid, Spain

[27] George Mason Univ, Dept Phys & Astron, 4400 Univ Dr,MSN 3F3, Fairfax, VA USA

[28] US Naval Observ, 3450 Massachusetts Ave NW, Washington, DC USA

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

[30] Univ Malta, Msida 2080, Msd, Malta

来源：

ASTROPHYSICAL JOURNAL LETTERS | 2024年 / 965卷 / 01期

关键词：

UV LUMINOSITY FUNCTIONS; LYMAN-BREAK GALAXIES; MASS-METALLICITY RELATION; STAR-FORMATION HISTORY; SYNTHETIC NEBULAR EMISSION; HIGH-REDSHIFT GALAXIES; NEAR-INFRARED CAMERA; UDF05; FOLLOW-UP; TO; GALAXIES; DATA REDUCTION;

D O I：

10.3847/2041-8213/ad2f31

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We present the Next Generation Deep Extragalactic Exploratory Public (NGDEEP) Survey, a deep slitless spectroscopic and imaging Cycle 1 JWST treasury survey designed to constrain feedback mechanisms in low-mass galaxies across cosmic time. NGDEEP targets the Hubble Ultra Deep Field (HUDF) with NIRISS slitless spectroscopy (f(lim,line,5 sigma )approximate to 1.2 x 10(-18) erg s(-1) cm(-2)) to measure metallicities and star formation rates (SFRs) for low-mass galaxies through the peak of the cosmic SFR density (0.5 < z < 4). In parallel, NGDEEP targets the HUDF-Par2 parallel field with NIRCam (m(lim, 5 sigma )= 30.6-30.9) to discover galaxies to z > 12, constraining the slope of the faint end of the rest-ultraviolet luminosity function. NGDEEP overlaps with the deepest HST Advanced Camera for Surveys optical imaging in the sky, F435W in the HUDF (m(lim,F435W )= 29.6) and F814W in HUDF-Par2 (m(lim,F814W )= 30), making this a premier HST+JWST deep field. As a treasury survey, NGDEEP data are public immediately, and we will rapidly release data products and catalogs in the spirit of previous deep-field initiatives. In this paper we present the NGDEEP survey design, summarize the science goals, and detail plans for the public release of NGDEEP reduced data products.

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