Hidden Giants in JWST's PEARLS: An Ultramassive z=4.26 Submillimeter Galaxy that Is Invisible to HST

被引：31

作者：

Smail, Ian ^{[1
]}

Dudzeviciute, Ugne ^{[2
]}

Gurwell, Mark ^{[3
]}

Fazio, Giovanni G. ^{[3
]}

Willner, S. P. ^{[3
]}

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

Arumugam, Vinodiran ^{[4
]}

Summers, Jake ^{[5
]}

Cohen, Seth H. ^{[5
]}

Jansen, Rolf A. ^{[5
]}

Windhorst, Rogier A. ^{[5
]}

Meena, Ashish ^{[6
]}

Zitrin, Adi ^{[6
]}

Keel, William C. ^{[7
]}

Coe, Dan ^{[8
]}

Conselice, Christopher J. ^{[9
]}

D'Silva, Jordan C. J. ^{[10
,11
]}

Driver, Simon P. ^{[10
,11
]}

Frye, Brenda ^{[12
]}

Grogin, Norman A. ^{[8
]}

Koekemoer, Anton M. ^{[8
]}

Marshall, Madeline A. ^{[13
]}

Nonino, Mario ^{[14
]}

Pirzkal, Nor ^{[8
]}

Robotham, Aaron ^{[10
,11
]}

Rutkowski, Michael J. ^{[15
]}

Ryan Jr, Russell E. ^{[8
]}

Tompkins, Scott ^{[5
]}

Willmer, Christopher N. A. ^{[12
]}

Yan, Haojing ^{[16
]}

Broadhurst, Thomas J. ^{[17
]}

Cheng, Cheng ^{[18
]}

Diego, Jose M. ^{[19
]}

Kamieneski, Patrick ^{[5
]}

Yun, Min ^{[20
]}

机构：

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

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

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

[4] Domaine Univ, Inst Radioastron Millimetr, 300 Rue Piscine, F-38406 St Martin Dheres, France

[5] Arizona State Univ, Sch Earth & Space Explorat, Tempe, AZ 85287 USA

[6] Ben Gurion Univ Negev, Phys Dept, POB 653, IL-8410501 Beer Sheva, Israel

[7] Univ Alabama, Dept Phys & Astron, Box 870324, Tuscaloosa, AL 35404 USA

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

[9] Univ Manchester, Jodrell Bank Ctr Astrophys, Alan Turing Bldg,Oxford Rd, Manchester M13 9PL, England

[10] Univ Western Australia, Int Ctr Radio Astron Res, M468,35 Stirling Highway, Crawley, WA 6009, Australia

[11] Univ Western Australia, Int Space Ctr, M468,35 Stirling Highway, Crawley, WA 6009, Australia

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

[13] Natl Res Council Canada, Herzberg Astron & Astrophys Res Ctr, 5071 West Saanich Rd, Victoria, BC V9E 2E7, Canada

[14] INAF Osservatorio Astron Trieste, Via Bazzoni 2, I-34124 Trieste, Italy

[15] Minnesota State Univ Mankato, Telescope Sci Inst, TN141, Mankato, MN 56001 USA

[16] Univ Missouri, Dept Phys & Astron, Columbia, MO 65211 USA

[17] Univ Basque Country UPV, Dept Theoret Phys, EHU, E-48080 Bilbao, Spain

[18] Chinese Acad Sci, Natl Astron Observ, CAS South Amer Ctr Astron, Beijing, Peoples R China

[19] Univ Cantabria, Inst Fis Cantabria, Avda Los Castros, Santander 39005, Spain

[20] Univ Massachusetts, Dept Astron, 710 North Pleasant St, Amherst, MA USA

来源：

ASTROPHYSICAL JOURNAL | 2023年 / 958卷 / 01期

基金：

澳大利亚研究理事会; 中国国家自然科学基金; 英国科学技术设施理事会; 美国国家科学基金会; 欧洲研究理事会;

关键词：

SPECTRAL ENERGY-DISTRIBUTION; DEEP FIELD SOUTH; NEAR-INFRARED SPECTROSCOPY; STAR-FORMATION HISTORIES; AZTEC/ASTE 1.1-MM SURVEY; SIMILAR-TO; MASSIVE GALAXIES; ALMA SURVEY; STELLAR MASS; PHYSICAL-PROPERTIES;

D O I：

10.3847/1538-4357/acf931

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We present a multiwavelength analysis using the Submillimeter Array (SMA), James Clerk Maxwell Telescope, NOEMA, JWST, the Hubble Space Telescope (HST), and the Spitzer Space Telescope of two dusty strongly star-forming galaxies, 850.1 and 850.2, seen through the massive cluster lens A 1489. These SMA-located sources both lie at z = 4.26 and have bright dust continuum emission, but 850.2 is a UV-detected Lyman-break galaxy, while 850.1 is undetected at less than or similar to 2 mu m, even with deep JWST/NIRCam observations. We investigate their stellar, interstellar medium, and dynamical properties, including a pixel-level spectral energy distribution analysis to derive subkiloparsec-resolution stellar-mass and A(V) maps. We find that 850.1 is one of the most massive and highly obscured, A(V) similar to 5, galaxies known at z > 4 with M-* similar to 10(11.8)M(circle dot) (likely forming at z > 6), and 850.2 is one of the least massive and least obscured, A(V) similar to 1, members of the z > 4 dusty star-forming population. The diversity of these two dust-mass-selected galaxies illustrates the incompleteness of galaxy surveys at z greater than or similar to 3-4 based on imaging at less than or similar to 2 mu m, the longest wavelengths feasible from HST or the ground. The resolved mass map of 850.1 shows a compact stellar-mass distribution, R-e(mass) similar to 1 kpc, but its expected evolution means that it matches both the properties of massive, quiescent galaxies at z similar to 1.5 and ultramassive early-type galaxies at z similar to 0. We suggest that 850.1 is the central galaxy of a group in which 850.2 is a satellite that will likely merge in the near future. The stellar morphology of 850.1 shows arms and a linear bar feature that we link to the active dynamical environment it resides within.

引用

页数：24

共 11 条

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