Early Results from GLASS-JWST. VI. Extreme Rest-optical Equivalent Widths Detected in NIRISS Wide Field Slitless Spectroscopy

被引：23

作者：

Boyett, K. ^{[1
,2
]}

Mascia, S. ^{[3
]}

Pentericci, L. ^{[3
]}

Leethochawalit, N. ^{[1
,2
,4
]}

Trenti, M. ^{[1
,2
]}

Brammer, G. ^{[5
,6
]}

Roberts-Borsani, G.

Strait, V. ^{[5
,6
]}

Treu, T. ^{[7
]}

Bradac, M. ^{[8
,9
]}

Glazebrook, K. ^{[10
]}

Acebron, A. ^{[11
,12
]}

Bergamini, P. ^{[11
,13
]}

Calabro, A. ^{[3
]}

Castellano, M. ^{[3
]}

Fontana, A. ^{[3
]}

Grillo, C. ^{[11
,12
]}

Henry, A. ^{[14
,15
]}

Jones, T. ^{[9
]}

Marchesini, D. ^{[16
]}

Mason, C. ^{[5
,6
]}

Mercurio, A. ^{[17
]}

Morishita, T. ^{[18
]}

Nanayakkara, T. ^{[10
]}

Rosati, P. ^{[19
]}

Scarlata, C. ^{[20
]}

Vanzella, E. ^{[13
]}

Vulcani, B. ^{[21
]}

Wang, X.

Willott, C. ^{[22
]}

机构：

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

[2] ARC Ctr Excellence All Sky Astrophys 3 Dimens AST, Stromlo, Australia

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

[4] Natl Astron Res Inst Thailand NARIT, Chiang Mai 50180, Thailand

[5] Cosm Dawn Ctr DAWN, Copenhagen, Denmark

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

[22] NRC Herzberg, 5071 West Saanich Rd, Victoria, BC V9E 2E7, Canada

来源：

ASTROPHYSICAL JOURNAL LETTERS | 2022年 / 940卷 / 02期

基金：

澳大利亚研究理事会; 新加坡国家研究基金会;

关键词：

O III EMITTERS; EMISSION-LINE; SURVEY DESIGN; GALAXIES; I; EVOLUTION; SAMPLE;

D O I：

10.3847/2041-8213/ac9f17

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Wide Field Slitless Spectroscopy (WFSS) provides a powerful tool for detecting strong line emission in star-forming galaxies (SFGs) without the need for target preselection. As part of the GLASS-JWST Early Release Science (ERS) program, we leverage the near-infrared wavelength capabilities of NIRISS (1-2.2 mu m) to observe rest-optical emission lines out to z similar to 3.4, to a depth and with a spatial resolution higher than ever before (H alpha to z < 2.4; [O iii]+H beta to z < 3.4). In this Letter we constrain the rest-frame [O III]lambda 5007 equivalent width (EW) distribution for a sample of 76 1 < z < 3.4 SFGs in the A2744 Hubble Frontier Field and determine an abundance fraction of extreme emission line galaxies with EW > 750 angstrom in our sample to be 12%. We determine a strong correlation between the measured H beta and [O III]lambda 5007 EWs, supporting that the high [O III]lambda 5007 EW objects require massive stars in young stellar populations to generate the high-energy photons needed to doubly ionize oxygen. We extracted spectra for objects up to 2 mag fainter in the near-infrared than previous WFSS studies with the Hubble Space Telescope. Thus, this work clearly highlights the potential of JWST/NIRISS to provide high-quality WFSS data sets in crowded cluster environments.

引用

页数：8

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