JWST NIRSpec Spectroscopy of the Triply Lensed z=10.17 Galaxy MACS0647-JD

被引：18

作者：

Hsiao, Tiger Yu-Yang ^{[1
,2
,3
]}

Abdurrro'uf, Dan ^{[1
,2
,3
,4
]}

Coe, Dan ^{[1
,2
,3
,4
]}

Larson, Rebecca L. ^{[5
]}

Jung, Intae ^{[3
]}

Mingozzi, Matilde ^{[3
]}

Dayal, Pratika ^{[6
]}

Kumari, Nimisha ^{[3
,4
]}

Kokorev, Vasily ^{[7
]}

Vikaeus, Anton ^{[8
]}

Brammer, Gabriel ^{[9
,10
]}

Furtak, Lukas J. ^{[11
]}

Adamo, Angela ^{[12
]}

Andrade-Santos, Felipe ^{[1
,13
,14
]}

Antwi-Danso, Jacqueline ^{[15
,16
,17
]}

Bradac, Marusa ^{[3
]}

Bradley, Larry D. ^{[3
]}

Broadhurst, Tom ^{[18
,19
,20
]}

Carnall, Adam C. ^{[21
]}

Conselice, Christopher J. ^{[22
]}

Diego, Jose M. ^{[23
]}

Donahue, Megan ^{[24
]}

Eldridge, Jan J. ^{[25
]}

Fujimoto, Seiji ^{[7
]}

Henry, Alaina ^{[2
,3
]}

Hernandez, Svea ^{[3
,4
]}

Hutchison, Taylor A. ^{[26
]}

James, Bethan L. ^{[3
,4
]}

Norman, Colin ^{[2
,3
]}

Park, Hyunbae ^{[27
]}

Pirzkal, Norbert ^{[3
]}

Postman, Marc ^{[3
]}

Ricotti, Massimo ^{[28
]}

Rigby, Jane R. ^{[26
]}

Vanzella, Eros ^{[29
]}

Welch, Brian ^{[26
,28
]}

Wilkins, Stephen M. ^{[30
,31
]}

Windhorst, Rogier A. ^{[32
]}

Xu, Xinfeng ^{[33
,34
]}

Zackrisson, Erik ^{[8
]}

Zitrin, Adi ^{[11
]}

机构：

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

[2] Johns Hopkins Univ, Ctr Astrophys Sci, Dept Phys & Astron, 3400 N Charles St, Baltimore, MD 21218 USA

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

[4] Assoc Univ Res Astron AURA Inc, European Space Agcy ESA, Washington, DC USA

[5] Rochester Inst Technol, Sch Phys & Astron, 84 Lomb Mem Dr, Rochester, NY 14623 USA

[6] Univ Groningen, Kapteyn Astron Inst, POB 800, NL-9700 AV Groningen, Netherlands

[7] Univ Texas Austin, Dept Astron, Austin, TX USA

[8] Uppsala Univ, Dept Phys & Astron, Observat Astrophys, Box 516, SE-75120 Uppsala, Sweden

[9] Cosm Dawn Ctr DAWN, Copenhagen, Denmark

[10] Univ Copenhagen, Niels Bohr Inst, Jagtvej 128, Copenhagen, Denmark

[11] Ben Gurion Univ Negev, Bengur Res Inst Study Israel, POB 653, IL-84105 Beer Sheva, Israel

[12] Stockholm Univ, AlbaNova Univ Ctr, Oskar Klein Ctr, Dept Astron, SE-10691 Stockholm, Sweden

[13] Berklee Coll Mus, Dept Liberal Arts & Sci, 7 Haviland St, Boston, MA 02215 USA

[14] Clay Ctr Observ, 20 Newton St, Brookline, MA 02445 USA

[15] Texas A&M Univ, George P & Cynthia Woods Mitchell Inst Fundamental, College Stn, TX 78743 USA

[16] Texas A&M Univ, College Stn, TX 78743 USA

[17] Univ Toronto, Dept Astron & Astrophys, Toronto, ON M5S 3H4, Canada

[18] Univ Basque Country, Dept Theoret Phys, UPV EHU, E-48040 Bilbao, Spain

[19] Donostia Int Phys Ctr DIPC, Donostia San Sebastian, Basque Country, Spain

[20] Basque Fdn Sci, IKERBASQUE, Alameda Urquijo 36-5, E-48008 Bilbao, Spain

[21] Univ Edinburgh, Edinburgh EH9 3HJ, Scotland

[22] Univ Manchester, Jodrell Bank Ctr Astrophys, Oxford Rd, Manchester M13 9PL, England

[23] Inst Fis Cantabria CSIC UC, Avda Los Castros S-N, Santander 39005, Spain

[24] Michigan State Univ, Phys & Astron Dept, E Lansing, MI USA

[25] Univ Auckland, Dept Phys, Private Bag 92019, Auckland, New Zealand

[26] NASA Goddard Space Flight Ctr, Observat Cosmol Lab, Greenbelt, MD 20771 USA

[27] Lawrence Berkeley Natl Lab, Berkeley, CA USA

[28] Univ Maryland, Dept Astron, College Pk, MD 20742 USA

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

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

[31] Univ Malta, Inst Space Sci & Astron, MSD-2080 Msida, Malta

[32] Arizona State Univ, Pocatello, ID 85287 USA

[33] USA, Blountstown, FL 60208 USA

[34] Northwestern Univ, Ctr Interdisciplinary Explorat & Res Astrophys CIE, Evanston, IL 60201 USA

来源：

ASTROPHYSICAL JOURNAL | 2024年 / 973卷 / 01期

基金：

瑞典研究理事会; 美国国家科学基金会; 新加坡国家研究基金会;

关键词：

STAR-FORMING GALAXIES; LY-ALPHA EMITTERS; PHOTON PRODUCTION EFFICIENCY; O III EMITTERS; INTERGALACTIC MEDIUM; H-ALPHA; PHYSICAL-PROPERTIES; LUMINOUS GALAXY; FORMATION HISTORIES; CHEMICAL EVOLUTION;

D O I：

10.3847/1538-4357/ad5da8

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We present JWST/NIRSpec prism spectroscopy of MACS0647-JD, a triply lensed z similar to 11 candidate discovered in Hubble Space Telescope imaging and spatially resolved by JWST imaging into two components, A and B. Spectroscopy of component A yields a spectroscopic redshift z = 10.17 based on seven detected emission lines: C iii] lambda lambda 1907, 1909, [O ii] lambda 3727, [Ne iii] lambda 3869, [Ne iii] lambda 3968, H delta lambda 4101, H gamma lambda 4340, and [O iii] lambda 4363. These are the second-most distant detections of these emission lines to date, in a galaxy observed just 460 million years after the Big Bang. Based on observed and extrapolated line flux ratios we derive a gas-phase metallicity 12 + log(O/H) similar to 7.5-8.0, or Z similar to (0.06-0.2) Z( circle dot), ionization parameter log(U) = -1.9 +/- 0.2, and an ionizing photon production efficiency log(xi(ion))=25.2 +/- 0.2 erg(-1) Hz. The spectrum has a softened Ly alpha break, evidence for a strong Ly alpha damping wing. The Ly alpha damping wing also suppresses the F150W photometry, explaining the slightly overestimated photometric redshift z = 10.6 +/- 0.3. MACS0647-JD has a stellar mass log(M/M (circle dot)) = 8.1 +/- 0.3, including similar to 6 x 10(7 )M (circle dot) in component A, most of which formed recently (within similar to 20 Myr) with a star formation rate similar to 2 +/- 1 M (circle dot )yr(-1), all within an effective radius 70 +/- 24 pc. Spectroscopy of a fainter companion galaxy C separated by a distance of similar to 3 kpc reveals a Lyman break consistent with z similar to 10.17. MACS0647-JD is likely the most distant galaxy merger known.

引用

页数：16

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