ALMA twenty-six arcmin(2) survey of GOODS-S at one millimeter (ASAGAO): Millimeter properties of stellar mass selected galaxies

Research output: Contribution to journal › Journal article › Research › peer-review

Standard

ALMA twenty-six arcmin(2) survey of GOODS-S at one millimeter (ASAGAO) : Millimeter properties of stellar mass selected galaxies. / Yamaguchi, Yuki; Kohno, Kotaro; Hatsukade, Bunyo; Wang, Tao; Yoshimura, Yuki; Ao, Yiping; Dunlop, James S.; Egami, Eiichi; Espada, Daniel; Fujimoto, Seiji; Hayatsu, Natsuki H.; Ivison, Rob J.; Kodama, Tadayuki; Kusakabe, Haruka; Nagao, Tohru; Ouchi, Masami; Rujopakarn, Wiphu; Tadaki, Ken-ichi; Tamura, Yoichi; Ueda, Yoshihiro; Umehata, Hideki; Wang, Wei-Hao.

In: Publications of the Astronomical Society of Japan, Vol. 72, No. 4, 69, 08.08.2020.

Research output: Contribution to journal › Journal article › Research › peer-review

Harvard

Yamaguchi, Y, Kohno, K, Hatsukade, B, Wang, T, Yoshimura, Y, Ao, Y, Dunlop, JS, Egami, E, Espada, D, Fujimoto, S, Hayatsu, NH, Ivison, RJ, Kodama, T, Kusakabe, H, Nagao, T, Ouchi, M, Rujopakarn, W, Tadaki, K, Tamura, Y, Ueda, Y, Umehata, H & Wang, W-H 2020, 'ALMA twenty-six arcmin(2) survey of GOODS-S at one millimeter (ASAGAO): Millimeter properties of stellar mass selected galaxies', Publications of the Astronomical Society of Japan, vol. 72, no. 4, 69. https://doi.org/10.1093/pasj/psaa057

APA

Yamaguchi, Y., Kohno, K., Hatsukade, B., Wang, T., Yoshimura, Y., Ao, Y., Dunlop, J. S., Egami, E., Espada, D., Fujimoto, S., Hayatsu, N. H., Ivison, R. J., Kodama, T., Kusakabe, H., Nagao, T., Ouchi, M., Rujopakarn, W., Tadaki, K., Tamura, Y., ... Wang, W-H. (2020). ALMA twenty-six arcmin(2) survey of GOODS-S at one millimeter (ASAGAO): Millimeter properties of stellar mass selected galaxies. Publications of the Astronomical Society of Japan, 72(4), [69]. https://doi.org/10.1093/pasj/psaa057

Vancouver

Yamaguchi Y, Kohno K, Hatsukade B, Wang T, Yoshimura Y, Ao Y et al. ALMA twenty-six arcmin(2) survey of GOODS-S at one millimeter (ASAGAO): Millimeter properties of stellar mass selected galaxies. Publications of the Astronomical Society of Japan. 2020 Aug 8;72(4). 69. https://doi.org/10.1093/pasj/psaa057

Author

Yamaguchi, Yuki ; Kohno, Kotaro ; Hatsukade, Bunyo ; Wang, Tao ; Yoshimura, Yuki ; Ao, Yiping ; Dunlop, James S. ; Egami, Eiichi ; Espada, Daniel ; Fujimoto, Seiji ; Hayatsu, Natsuki H. ; Ivison, Rob J. ; Kodama, Tadayuki ; Kusakabe, Haruka ; Nagao, Tohru ; Ouchi, Masami ; Rujopakarn, Wiphu ; Tadaki, Ken-ichi ; Tamura, Yoichi ; Ueda, Yoshihiro ; Umehata, Hideki ; Wang, Wei-Hao. / ALMA twenty-six arcmin(2) survey of GOODS-S at one millimeter (ASAGAO) : Millimeter properties of stellar mass selected galaxies. In: Publications of the Astronomical Society of Japan. 2020 ; Vol. 72, No. 4.

Bibtex

@article{927548956e1d45199514b5c875d72835,
title = "ALMA twenty-six arcmin(2) survey of GOODS-S at one millimeter (ASAGAO): Millimeter properties of stellar mass selected galaxies",
abstract = "We make use of the ALMA twenty-Six Arcmin(2) survey of GOODS-S At One-millimeter (ASAGAO), deep 1.2 mm continuum observations of a 26-arcmin(2) region in the Great Observatories Origins Deep Survey-South (GOODS-S) obtained with Atacama Large Millimeter/sub-millimeter Array (ALMA), to probe dust-enshrouded star formation in K-band selected (i.e., stellar mass selected) galaxies, which are drawn from the FourStar Galaxy Evolution Survey (ZFOURGE) catalog. Based on the ASAGAO combined map, which was created by combining ASAGAO and ALMA archival data in the GOODS-South field, we find that 24 ZFOURGE sources have 1.2 mm counterparts with a signal-to-noise ratio >4.5 (1 sigma similar or equal to 30-70 mu Jy beam(-1) at 1.2 mm). Their median redshift is estimated to be Z(median) = 2.38 +/- 0.14. They generally follow the tight relationship of the stellar mass versus star formation rate (i.e., the main sequence of star-forming galaxies). ALMA-detected ZFOURGE sources exhibit systematically larger infrared (IR) excess (IRX L-IR/L-UV) compared to ZFOURGE galaxies without ALMA detections even though they have similar redshifts, stellar masses, and star formation rates. This implies the consensus stellar-mass versus IRX relation, which is known to be tight among rest-frame-ultraviolet-selected galaxies, cannot fully predict the ALMA detectability of stellar-mass-selected galaxies. We find that ALMA-detected ZFOURGE sources are the main contributors to the cosmic IR star formation rate density at z = 2-3.",
keywords = "galaxies: evolution, galaxies: high-redshift, galaxies: star formation, submillimeter: galaxies, DEEP-FIELD-SOUTH, COSMIC STAR-FORMATION, PHOTOMETRIC REDSHIFT SURVEY, AZTEC/ASTE 1.1-MM SURVEY, FORMATION RATE DENSITY, LYMAN-BREAK GALAXIES, IRX-BETA RELATION, DUST ATTENUATION, BOLOMETER CAMERA, SOURCE CATALOG",
author = "Yuki Yamaguchi and Kotaro Kohno and Bunyo Hatsukade and Tao Wang and Yuki Yoshimura and Yiping Ao and Dunlop, {James S.} and Eiichi Egami and Daniel Espada and Seiji Fujimoto and Hayatsu, {Natsuki H.} and Ivison, {Rob J.} and Tadayuki Kodama and Haruka Kusakabe and Tohru Nagao and Masami Ouchi and Wiphu Rujopakarn and Ken-ichi Tadaki and Yoichi Tamura and Yoshihiro Ueda and Hideki Umehata and Wei-Hao Wang",
year = "2020",
month = aug,
day = "8",
doi = "10.1093/pasj/psaa057",
language = "English",
volume = "72",
journal = "Publication of the Astronomical Society of Japan",
issn = "0004-6264",
publisher = "Astronomical Society of Japan",
number = "4",

}

RIS

TY - JOUR

T1 - ALMA twenty-six arcmin(2) survey of GOODS-S at one millimeter (ASAGAO)

T2 - Millimeter properties of stellar mass selected galaxies

AU - Yamaguchi, Yuki

AU - Kohno, Kotaro

AU - Hatsukade, Bunyo

AU - Wang, Tao

AU - Yoshimura, Yuki

AU - Ao, Yiping

AU - Dunlop, James S.

AU - Egami, Eiichi

AU - Espada, Daniel

AU - Fujimoto, Seiji

AU - Hayatsu, Natsuki H.

AU - Ivison, Rob J.

AU - Kodama, Tadayuki

AU - Kusakabe, Haruka

AU - Nagao, Tohru

AU - Ouchi, Masami

AU - Rujopakarn, Wiphu

AU - Tadaki, Ken-ichi

AU - Tamura, Yoichi

AU - Ueda, Yoshihiro

AU - Umehata, Hideki

AU - Wang, Wei-Hao

PY - 2020/8/8

Y1 - 2020/8/8

N2 - We make use of the ALMA twenty-Six Arcmin(2) survey of GOODS-S At One-millimeter (ASAGAO), deep 1.2 mm continuum observations of a 26-arcmin(2) region in the Great Observatories Origins Deep Survey-South (GOODS-S) obtained with Atacama Large Millimeter/sub-millimeter Array (ALMA), to probe dust-enshrouded star formation in K-band selected (i.e., stellar mass selected) galaxies, which are drawn from the FourStar Galaxy Evolution Survey (ZFOURGE) catalog. Based on the ASAGAO combined map, which was created by combining ASAGAO and ALMA archival data in the GOODS-South field, we find that 24 ZFOURGE sources have 1.2 mm counterparts with a signal-to-noise ratio >4.5 (1 sigma similar or equal to 30-70 mu Jy beam(-1) at 1.2 mm). Their median redshift is estimated to be Z(median) = 2.38 +/- 0.14. They generally follow the tight relationship of the stellar mass versus star formation rate (i.e., the main sequence of star-forming galaxies). ALMA-detected ZFOURGE sources exhibit systematically larger infrared (IR) excess (IRX L-IR/L-UV) compared to ZFOURGE galaxies without ALMA detections even though they have similar redshifts, stellar masses, and star formation rates. This implies the consensus stellar-mass versus IRX relation, which is known to be tight among rest-frame-ultraviolet-selected galaxies, cannot fully predict the ALMA detectability of stellar-mass-selected galaxies. We find that ALMA-detected ZFOURGE sources are the main contributors to the cosmic IR star formation rate density at z = 2-3.

AB - We make use of the ALMA twenty-Six Arcmin(2) survey of GOODS-S At One-millimeter (ASAGAO), deep 1.2 mm continuum observations of a 26-arcmin(2) region in the Great Observatories Origins Deep Survey-South (GOODS-S) obtained with Atacama Large Millimeter/sub-millimeter Array (ALMA), to probe dust-enshrouded star formation in K-band selected (i.e., stellar mass selected) galaxies, which are drawn from the FourStar Galaxy Evolution Survey (ZFOURGE) catalog. Based on the ASAGAO combined map, which was created by combining ASAGAO and ALMA archival data in the GOODS-South field, we find that 24 ZFOURGE sources have 1.2 mm counterparts with a signal-to-noise ratio >4.5 (1 sigma similar or equal to 30-70 mu Jy beam(-1) at 1.2 mm). Their median redshift is estimated to be Z(median) = 2.38 +/- 0.14. They generally follow the tight relationship of the stellar mass versus star formation rate (i.e., the main sequence of star-forming galaxies). ALMA-detected ZFOURGE sources exhibit systematically larger infrared (IR) excess (IRX L-IR/L-UV) compared to ZFOURGE galaxies without ALMA detections even though they have similar redshifts, stellar masses, and star formation rates. This implies the consensus stellar-mass versus IRX relation, which is known to be tight among rest-frame-ultraviolet-selected galaxies, cannot fully predict the ALMA detectability of stellar-mass-selected galaxies. We find that ALMA-detected ZFOURGE sources are the main contributors to the cosmic IR star formation rate density at z = 2-3.

KW - galaxies: evolution

KW - galaxies: high-redshift

KW - galaxies: star formation

KW - submillimeter: galaxies

KW - DEEP-FIELD-SOUTH

KW - COSMIC STAR-FORMATION

KW - PHOTOMETRIC REDSHIFT SURVEY

KW - AZTEC/ASTE 1.1-MM SURVEY

KW - FORMATION RATE DENSITY

KW - LYMAN-BREAK GALAXIES

KW - IRX-BETA RELATION

KW - DUST ATTENUATION

KW - BOLOMETER CAMERA

KW - SOURCE CATALOG

U2 - 10.1093/pasj/psaa057

DO - 10.1093/pasj/psaa057

M3 - Journal article

VL - 72

JO - Publication of the Astronomical Society of Japan

JF - Publication of the Astronomical Society of Japan

SN - 0004-6264

IS - 4

M1 - 69

ER -

ID: 253649401