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

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 evolu...
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Autor*in:	Tomoko L. Suzuki [verfasserIn] Sophie E. van Mierlo [verfasserIn] Karina I. Caputi [verfasserIn]

Format:	E-Artikel
Sprache:	Englisch

Erschienen:	2023

Schlagwörter:	High-redshift galaxies Submillimeter astronomy Galaxy evolution

Übergeordnetes Werk:	In: The Astrophysical Journal - IOP Publishing, 2022, 959(2023), 2, p 82
Übergeordnetes Werk:	volume:959 ; year:2023 ; number:2, p 82

Links:	Link aufrufen Link aufrufen Link aufrufen Journal toc

DOI / URN:	10.3847/1538-4357/ad023c

Katalog-ID:	DOAJ099996510

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spelling	10.3847/1538-4357/ad023c doi (DE-627)DOAJ099996510 (DE-599)DOAJ1c74944dbfc64678b842d624bb61679d DE-627 ger DE-627 rakwb eng QB460-466 Tomoko L. Suzuki verfasserin aut ALMA Millimeter/Submillimeter Sources among Spitzer SMUVS Galaxies at z < 2 in the COSMOS Field 2023 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier 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 μ 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. High-redshift galaxies Submillimeter astronomy Galaxy evolution Astrophysics Sophie E. van Mierlo verfasserin aut Karina I. Caputi verfasserin aut In The Astrophysical Journal IOP Publishing, 2022 959(2023), 2, p 82 (DE-627)269019219 (DE-600)1473835-1 15384357 nnns volume:959 year:2023 number:2, p 82 https://doi.org/10.3847/1538-4357/ad023c kostenfrei https://doaj.org/article/1c74944dbfc64678b842d624bb61679d kostenfrei https://doi.org/10.3847/1538-4357/ad023c kostenfrei https://doaj.org/toc/1538-4357 Journal toc kostenfrei GBV_USEFLAG_A SYSFLAG_A GBV_DOAJ GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2014 GBV_ILN_2088 GBV_ILN_2522 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 AR 959 2023 2, p 82
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allfieldsGer	10.3847/1538-4357/ad023c doi (DE-627)DOAJ099996510 (DE-599)DOAJ1c74944dbfc64678b842d624bb61679d DE-627 ger DE-627 rakwb eng QB460-466 Tomoko L. Suzuki verfasserin aut ALMA Millimeter/Submillimeter Sources among Spitzer SMUVS Galaxies at z < 2 in the COSMOS Field 2023 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier 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 μ 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. High-redshift galaxies Submillimeter astronomy Galaxy evolution Astrophysics Sophie E. van Mierlo verfasserin aut Karina I. Caputi verfasserin aut In The Astrophysical Journal IOP Publishing, 2022 959(2023), 2, p 82 (DE-627)269019219 (DE-600)1473835-1 15384357 nnns volume:959 year:2023 number:2, p 82 https://doi.org/10.3847/1538-4357/ad023c kostenfrei https://doaj.org/article/1c74944dbfc64678b842d624bb61679d kostenfrei https://doi.org/10.3847/1538-4357/ad023c kostenfrei https://doaj.org/toc/1538-4357 Journal toc kostenfrei GBV_USEFLAG_A SYSFLAG_A GBV_DOAJ GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2014 GBV_ILN_2088 GBV_ILN_2522 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 AR 959 2023 2, p 82
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source	In The Astrophysical Journal 959(2023), 2, p 82 volume:959 year:2023 number:2, p 82
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callnumber-first	Q - Science
author	Tomoko L. Suzuki
spellingShingle	Tomoko L. Suzuki misc QB460-466 misc High-redshift galaxies misc Submillimeter astronomy misc Galaxy evolution misc Astrophysics ALMA Millimeter/Submillimeter Sources among Spitzer SMUVS Galaxies at z < 2 in the COSMOS Field
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topic_title	QB460-466 ALMA Millimeter/Submillimeter Sources among Spitzer SMUVS Galaxies at z < 2 in the COSMOS Field High-redshift galaxies Submillimeter astronomy Galaxy evolution
topic	misc QB460-466 misc High-redshift galaxies misc Submillimeter astronomy misc Galaxy evolution misc Astrophysics
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title	ALMA Millimeter/Submillimeter Sources among Spitzer SMUVS Galaxies at z < 2 in the COSMOS Field
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title_full	ALMA Millimeter/Submillimeter Sources among Spitzer SMUVS Galaxies at z < 2 in the COSMOS Field
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title_sort	alma millimeter/submillimeter sources among spitzer smuvs galaxies at z < 2 in the cosmos field
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title_auth	ALMA Millimeter/Submillimeter Sources among Spitzer SMUVS Galaxies at z < 2 in the COSMOS Field
abstract	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 μ 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.
abstractGer	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 μ 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.
abstract_unstemmed	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 μ 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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title_short	ALMA Millimeter/Submillimeter Sources among Spitzer SMUVS Galaxies at z < 2 in the COSMOS Field
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ALMA Millimeter/Submillimeter Sources among Spitzer SMUVS Galaxies at z < 2 in the COSMOS Field

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