Resolving ambiguities in the inferred star formation histories of intense [O iii] emitters in the reionization Era

被引:22
作者
Laporte, N. [1 ,2 ]
Ellis, R. S. [3 ]
Witten, C. E. C. [4 ]
Roberts-Borsani, G. [5 ]
机构
[1] Univ Cambridge, Kavli Inst Cosmol, Madingley Rd, Cambridge CB3 0HA, England
[2] Univ Cambridge, Cavendish Lab, 19 JJ Thomson Ave, Cambridge CB3 0HE, England
[3] UCL, Dept Phys & Astron, Gower St, London WC1E 6BT, England
[4] Univ Cambridge, Inst Astron, Madingley Rd, Cambridge CB3 0HA, England
[5] Univ Calif Los Angeles, Dept Phys & Astron, Los Angeles, CA 90095 USA
基金
英国科学技术设施理事会; 欧洲研究理事会;
关键词
galaxies: formation; galaxies: high-redshift; (cosmology:) dark ages; reionization; first stars; REMARKABLY LUMINOUS GALAXY; TO; 8; GALAXIES; SPECTROSCOPIC SURVEY; STELLAR POPULATIONS; COSMIC DAWN; CANDIDATES; EMISSION; DENSITY; FIELDS; 3D-HST;
D O I
10.1093/mnras/stad1597
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Early JWST spectroscopic campaigns have confirmed the presence of strong [O III ] line-emitting galaxies in the redshift interval 7 < z < 9. Although deduced earlier from Spitzer photometry as an indicative of young stellar populations, some studies suggested the rele v ant photometric excesses attributed to [O III ] emission could, in part, be due to Balmer breaks arising from older stars. We demonstrate that this is likely the case by exploiting medium-band near-infrared JWST photometry in the Hubble Ultra Deep Field. We locate a sample of six galaxies with redshifts 8.2
引用
收藏
页码:3018 / 3024
页数:7
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