ALMA Millimeter/Submillimeter Sources among Spitzer SMUVS Galaxies at z > 2 in the COSMOS Field

被引：0
|
作者：
Suzuki, Tomoko [1 ,2 ]
van Mierlo, Sophie [2 ]
Caputi, Karina [2 ]
机构：
[1] Univ Tokyo, Inst Adv Study, Kavli Inst Phys & Math Universe WPI, Kashiwa, Chiba 2778583, Japan
[2] Univ Groningen, Kapteyn Astron Inst, POB 800, NL-9700 AV Groningen, Netherlands
来源：
ASTROPHYSICAL JOURNAL | 2023年 / 959卷 / 02期
基金：
欧洲研究理事会;
关键词：
STAR-FORMING GALAXIES; STARBURST/MAIN-SEQUENCE BIMODALITY; DEBLENDED DUST EMISSION; EVOLUTION SURVEY COSMOS; DEEP STRIPES SMUVS; SUBMILLIMETER GALAXIES; LEGACY SURVEY; STELLAR MASS; SPECTROSCOPIC SURVEY; PHYSICAL-PROPERTIES;
D O I：
10.3847/1538-4357/ad023c
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
Submillimeter observations reveal the star formation activity obscured by dust in the young Universe. It still remains unclear how galaxies detected at submillimeter wavelengths are related to ultraviolet/optical-selected galaxies in terms of their observed quantities, physical properties, and evolutionary stages. Deep near- and mid-infrared observational data are crucial to characterize the stellar properties of galaxies detected with submillimeter emission. In this study, we make use of a galaxy catalog from the Spitzer Matching survey of the UltraVISTA ultra-deep Stripes. By crossmatching with a submillimeter source catalog constructed with archival data of the Atacama Large Millimeter/submillimeter Array (ALMA), we search for galaxies at z > 2 with a submillimeter detection in our galaxy catalog. We find that the ALMA-detected galaxies at z > 2 are systematically massive and have redder K-s -[4.5] colors than the nondetected galaxies. The redder colors are consistent with the larger dust reddening values of the ALMA-detected galaxies obtained from spectral energy distribution (SED) fitting. We also find that the ALMA-detected galaxies tend to have brighter 4.5 mu m magnitudes. This may suggest that they tend to have smaller mass-to-light ratios and thus to be younger than star-forming galaxies fainter at submillimeter wavelengths with similar stellar masses. We identify starburst galaxies with high specific star formation rates among both ALMA-detected and nondetected SMUVS sources. Irrespective of their brightness at submillimeter wavelengths, these populations have similar dust reddening values, which may suggest a variety of dust SED shapes among the starburst galaxies at z > 2.
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页数：10
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