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.
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页数:16
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