The ALMA Spectroscopic Survey in the Hubble Ultra Deep Field: The Nature of the Faintest Dusty Star-forming Galaxies

We present a characterization of the physical properties of a sample of 35 securely detected, dusty galaxies in the deep ALMA 1.2 mm image obtained as part of the ALMA Spectroscopic Survey in the Hubble Ultra Deep Field (ASPECS) Large Program. This sample is complemented by 26 additional sources ide...

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Published in:The Astrophysical journal Vol. 901; no. 1; pp. 79 - 103
Main Authors: Aravena, Manuel, Boogaard, Leindert, Gónzalez-López, Jorge, Decarli, Roberto, Walter, Fabian, Carilli, Chris L., Smail, Ian, Weiss, Axel, Assef, Roberto J., Bauer, Franz Erik, Bouwens, Rychard J., Cortes, Paulo C., Cox, Pierre, da Cunha, Elisabete, Daddi, Emanuele, Díaz-Santos, Tanio, Inami, Hanae, Ivison, Rob, Novak, Mladen, Popping, Gergö, Riechers, Dominik, van der Werf, Paul, Wagg, Jeff
Format: Journal Article
Language:English
Published: Philadelphia The American Astronomical Society 01.09.2020
IOP Publishing
American Astronomical Society
Subjects:
Astrophysics
Depletion
Galaxies
Galaxy evolution
Galaxy quenching
High-redshift galaxies
Hubble deep field
Mass ratios
Molecular gases
Physical properties
Physics
Polls & surveys
Red shift
Spectroscopy
Star & galaxy formation
Star formation
Stars & galaxies
Submillimeter astronomy
ISSN:0004-637X, 1538-4357
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Abstract We present a characterization of the physical properties of a sample of 35 securely detected, dusty galaxies in the deep ALMA 1.2 mm image obtained as part of the ALMA Spectroscopic Survey in the Hubble Ultra Deep Field (ASPECS) Large Program. This sample is complemented by 26 additional sources identified via an optical/infrared source positional prior. Using their well-characterized spectral energy distributions, we derive median stellar masses and star formation rates (SFR) of and 30 M☉ yr−1, respectively, and interquartile ranges of (2.4-11.7) × 1010 M☉ and 20-50 M☉ yr−1. We derive a median spectroscopic redshift of 1.8 with an interquartile range 1.1-2.6, significantly lower than submillimeter galaxies detected in shallower, wide-field surveys. We find that 59% 13%, 6% 4%, and 34% 9% of our sources are within, above, and below 0.4 dex from the SFR-stellar-mass relation or main sequence (MS), respectively. The ASPECS galaxies closely follow the SFR-molecular gas mass relation and other previously established scaling relations, confirming a factor of five increase of the gas-to-stellar-mass ratio from z = 0.5 to 2.5 and a mild evolution of the gas depletion timescales with a typical value of 0.7 Gyr at z = 1-3. ASPECS galaxies located significantly below the MS, a poorly exploited parameter space, have low gas-to-stellar-mass ratios of ∼0.1-0.2 and long depletion timescales >1 Gyr. Galaxies along the MS dominate the cosmic density of molecular gas at all redshifts. Systems above the MS have an increasing contribution to the total gas reservoirs from z < 1 to z = 2.5, while the opposite is found for galaxies below the MS.
AbstractList We present a characterization of the physical properties of a sample of 35 securely detected, dusty galaxies in the deep ALMA 1.2 mm image obtained as part of the ALMA Spectroscopic Survey in the Hubble Ultra Deep Field (ASPECS) Large Program. This sample is complemented by 26 additional sources identified via an optical/infrared source positional prior. Using their well-characterized spectral energy distributions, we derive median stellar masses and star formation rates (SFR) of and 30 M☉ yr−1, respectively, and interquartile ranges of (2.4-11.7) × 1010 M☉ and 20-50 M☉ yr−1. We derive a median spectroscopic redshift of 1.8 with an interquartile range 1.1-2.6, significantly lower than submillimeter galaxies detected in shallower, wide-field surveys. We find that 59% 13%, 6% 4%, and 34% 9% of our sources are within, above, and below 0.4 dex from the SFR-stellar-mass relation or main sequence (MS), respectively. The ASPECS galaxies closely follow the SFR-molecular gas mass relation and other previously established scaling relations, confirming a factor of five increase of the gas-to-stellar-mass ratio from z = 0.5 to 2.5 and a mild evolution of the gas depletion timescales with a typical value of 0.7 Gyr at z = 1-3. ASPECS galaxies located significantly below the MS, a poorly exploited parameter space, have low gas-to-stellar-mass ratios of ∼0.1-0.2 and long depletion timescales >1 Gyr. Galaxies along the MS dominate the cosmic density of molecular gas at all redshifts. Systems above the MS have an increasing contribution to the total gas reservoirs from z < 1 to z = 2.5, while the opposite is found for galaxies below the MS.
We present a characterization of the physical properties of a sample of 35 securely detected, dusty galaxies in the deep ALMA 1.2 mm image obtained as part of the ALMA Spectroscopic Survey in the Hubble Ultra Deep Field (ASPECS) Large Program. This sample is complemented by 26 additional sources identified via an optical/infrared source positional prior. Using their well-characterized spectral energy distributions, we derive median stellar masses and star formation rates (SFR) of \(4.8\times {10}^{10}\,{M}_{\odot }\) and 30 M ☉ yr−1, respectively, and interquartile ranges of (2.4–11.7) נ1010 M ☉ and 20–50 M ☉ yr−1. We derive a median spectroscopic redshift of 1.8 with an interquartile range 1.1–2.6, significantly lower than submillimeter galaxies detected in shallower, wide-field surveys. We find that 59% ± 13%, 6% ± 4%, and 34% ± 9% of our sources are within, above, and below±0.4 dex from the SFR–stellar-mass relation or main sequence (MS), respectively. The ASPECS galaxies closely follow the SFR–molecular gas mass relation and other previously established scaling relations, confirming a factor of five increase of the gas-to-stellar-mass ratio from z = 0.5 to 2.5 and a mild evolution of the gas depletion timescales with a typical value of 0.7 Gyr at z = 1–3. ASPECS galaxies located significantly below the MS, a poorly exploited parameter space, have low gas-to-stellar-mass ratios of ∼0.1–0.2 and long depletion timescales >1 Gyr. Galaxies along the MS dominate the cosmic density of molecular gas at all redshifts. Systems above the MS have an increasing contribution to the total gas reservoirs from z < 1 to z = 2.5, while the opposite is found for galaxies below the MS.
We present a characterization of the physical properties of a sample of 35 securely detected, dusty galaxies in the deep ALMA 1.2 mm image obtained as part of the ALMA Spectroscopic Survey in the Hubble Ultra Deep Field (ASPECS) Large Program. This sample is complemented by 26 additional sources identified via an optical/infrared source positional prior. Using their well-characterized spectral energy distributions, we derive median stellar masses and star formation rates (SFR) of and 30 M ☉ yr −1 , respectively, and interquartile ranges of (2.4–11.7) × 10 10   M ☉ and 20–50  M ☉ yr −1 . We derive a median spectroscopic redshift of 1.8 with an interquartile range 1.1–2.6, significantly lower than submillimeter galaxies detected in shallower, wide-field surveys. We find that 59% ± 13%, 6% ± 4%, and 34% ± 9% of our sources are within, above, and below±0.4 dex from the SFR–stellar-mass relation or main sequence (MS), respectively. The ASPECS galaxies closely follow the SFR–molecular gas mass relation and other previously established scaling relations, confirming a factor of five increase of the gas-to-stellar-mass ratio from z  = 0.5 to 2.5 and a mild evolution of the gas depletion timescales with a typical value of 0.7 Gyr at z  = 1–3. ASPECS galaxies located significantly below the MS, a poorly exploited parameter space, have low gas-to-stellar-mass ratios of ∼0.1–0.2 and long depletion timescales >1 Gyr. Galaxies along the MS dominate the cosmic density of molecular gas at all redshifts. Systems above the MS have an increasing contribution to the total gas reservoirs from z  < 1 to z  = 2.5, while the opposite is found for galaxies below the MS.
We present a characterization of the physical properties of a sample of 35 securely-detected, dusty galaxies in the deep ALMA 1.2-mm image obtained as part of the ALMA Spectroscopic Survey in the {\it Hubble} Ultra Deep Field (ASPECS) Large Program. This sample is complemented by 26 additional sources identified via an optical/infrared source positional prior. Using their well-characterized spectral energy distributions, we derive median stellar masses and star formation rates (SFR) of $4.8\times10^{10}~M_\odot$ and 30 $M_\odot$ yr$^{-1}$, and interquartile ranges of $(2.4-11.7)\times10^{10}~M_\odot$ and $20-50~M_\odot$ yr$^{-1}$, respectively. We derive a median spectroscopic redshift of 1.8 with an interquartile range $1.1-2.6$, significantly lower than submillimeter galaxies detected in shallower, wide-field surveys. We find that 59\%$\pm$13\%, 6\%$\pm$4\%, and 34\%$\pm$9\% of our sources are within, above and below $\pm0.4$ dex from the SFR-stellar mass relation or main-sequence (MS), respectively. The ASPECS galaxies closely follow the SFR-molecular gas mass relation and other previously established scaling relations, confirming a factor of five increase of the gas-to-stellar mass ratio from $z=0.5$ to $z=2.5$ and a mild evolution of the gas depletion timescales with a typical value of 0.7 Gyr at $z=1-3$. ASPECS galaxies located significantly below the MS, a poorly exploited parameter space, have low gas-to-stellar-mass ratios of $\sim0.1-0.2$ and long depletion timescales $>1$ Gyr. Galaxies along the MS dominate the cosmic density of molecular gas at all redshifts. Systems above the main sequence have an increasing contribution to the total gas reservoirs from $z<1$ to $z=2.5$, while the opposite is found for galaxies below the MS.
Author Bouwens, Rychard J.
Wagg, Jeff
Gónzalez-López, Jorge
Smail, Ian
Weiss, Axel
da Cunha, Elisabete
Carilli, Chris L.
Cox, Pierre
Popping, Gergö
Riechers, Dominik
Assef, Roberto J.
Díaz-Santos, Tanio
Aravena, Manuel
Cortes, Paulo C.
Bauer, Franz Erik
Ivison, Rob
Novak, Mladen
van der Werf, Paul
Boogaard, Leindert
Walter, Fabian
Daddi, Emanuele
Inami, Hanae
Decarli, Roberto
Author_xml – sequence: 1
  givenname: Manuel
  orcidid: 0000-0002-6290-3198
  surname: Aravena
  fullname: Aravena, Manuel
  email: manuel.aravenaa@mail.udp.cl
  organization: Núcleo de Astronomía, Facultad de Ingeniería y Ciencias, Universidad Diego Portales, Av. Ejército 441, Santiago, Chile
– sequence: 2
  givenname: Leindert
  orcidid: 0000-0002-3952-8588
  surname: Boogaard
  fullname: Boogaard, Leindert
  organization: Leiden University Leiden Observatory, P.O. Box 9513, NL2300 RA Leiden, The Netherlands
– sequence: 3
  givenname: Jorge
  orcidid: 0000-0003-3926-1411
  surname: Gónzalez-López
  fullname: Gónzalez-López, Jorge
  organization: Núcleo de Astronomía, Facultad de Ingeniería y Ciencias, Universidad Diego Portales, Av. Ejército 441, Santiago, Chile
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  surname: Decarli
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  organization: INAF Osservatorio di Astrofisica e Scienza dello Spazio, via Gobetti 93/3, I-40129, Bologna, Italy
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  givenname: Fabian
  orcidid: 0000-0003-4793-7880
  surname: Walter
  fullname: Walter, Fabian
  organization: National Radio Astronomy Observatory, Pete V. Domenici Array Science Center, P.O. Box O, Socorro, NM 87801, USA
– sequence: 6
  givenname: Chris L.
  orcidid: 0000-0001-6647-3861
  surname: Carilli
  fullname: Carilli, Chris L.
  organization: National Radio Astronomy Observatory, Pete V. Domenici Array Science Center, P.O. Box O, Socorro, NM 87801, USA
– sequence: 7
  givenname: Ian
  orcidid: 0000-0003-3037-257X
  surname: Smail
  fullname: Smail, Ian
  organization: Durham University Centre for Extragalactic Astronomy, Department of Physics, South Road, Durham, DH1 3LE, UK
– sequence: 8
  givenname: Axel
  orcidid: 0000-0003-4678-3939
  surname: Weiss
  fullname: Weiss, Axel
  organization: Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, D-53121 Bonn, Germany
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  givenname: Roberto J.
  orcidid: 0000-0002-9508-3667
  surname: Assef
  fullname: Assef, Roberto J.
  organization: Núcleo de Astronomía, Facultad de Ingeniería, Universidad Diego Portales, Av. Ejército 441, Santiago, Chile
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  givenname: Franz Erik
  orcidid: 0000-0002-8686-8737
  surname: Bauer
  fullname: Bauer, Franz Erik
  organization: Millennium Institute of Astrophysics (MAS), Nuncio Monseñor Sótero Sanz 100, Providencia, Santiago, Chile
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  givenname: Rychard J.
  orcidid: 0000-0002-4989-2471
  surname: Bouwens
  fullname: Bouwens, Rychard J.
  organization: Leiden University Leiden Observatory, P.O. Box 9513, NL2300 RA Leiden, The Netherlands
– sequence: 12
  givenname: Paulo C.
  orcidid: 0000-0002-3583-780X
  surname: Cortes
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  organization: National Radio Astronomy Observatory, 520 Edgemont Road, Charlottesville, VA 22903, USA
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  givenname: Pierre
  surname: Cox
  fullname: Cox, Pierre
  organization: Sorbonne Université, UPMC Université Paris 6 and CNRS, UMR 7095, Institut d'Astrophysique de Paris, 98bis boulevard Arago, F-75015 Paris, France
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  givenname: Elisabete
  orcidid: 0000-0001-9759-4797
  surname: da Cunha
  fullname: da Cunha, Elisabete
  organization: ARC Centre of Excellence for All Sky Astrophysics in 3 Dimensions (ASTRO 3D), Australia
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  givenname: Emanuele
  orcidid: 0000-0002-3331-9590
  surname: Daddi
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  organization: Laboratoire AIM, CEA/DSM-CNRS-Universite Paris Diderot, Irfu/Service d'Astrophysique, CEA Saclay, Orme des Merisiers, F-91191 Gif-sur-Yvette cedex, France
– sequence: 16
  givenname: Tanio
  orcidid: 0000-0003-0699-6083
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– sequence: 17
  givenname: Hanae
  orcidid: 0000-0003-4268-0393
  surname: Inami
  fullname: Inami, Hanae
  organization: Hiroshima University Hiroshima Astrophysical Science Center, 1-3-1 Kagamiyama, Higashi-Hiroshima, Hiroshima 739-8526, Japan
– sequence: 18
  givenname: Rob
  orcidid: 0000-0001-5118-1313
  surname: Ivison
  fullname: Ivison, Rob
  organization: European Southern Observatory, Karl-Schwarzschild-Strasse 2, D-85748, Garching, Germany
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  surname: Novak
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  organization: Max Planck Institute für Astronomie, Königstuhl 17, D-69117 Heidelberg, Germany
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  givenname: Gergö
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  organization: Leiden University Leiden Observatory, P.O. Box 9513, NL2300 RA Leiden, The Netherlands
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  givenname: Jeff
  surname: Wagg
  fullname: Wagg, Jeff
  organization: SKA Organization, Lower Withington Macclesfield, Cheshire SK11 9DL, UK
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Snippet We present a characterization of the physical properties of a sample of 35 securely detected, dusty galaxies in the deep ALMA 1.2 mm image obtained as part of...
We present a characterization of the physical properties of a sample of 35 securely-detected, dusty galaxies in the deep ALMA 1.2-mm image obtained as part of...
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StartPage 79
SubjectTerms Astrophysics
Depletion
Galaxies
Galaxy evolution
Galaxy quenching
High-redshift galaxies
Hubble deep field
Mass ratios
Molecular gases
Physical properties
Physics
Polls & surveys
Red shift
Spectroscopy
Star & galaxy formation
Star formation
Stars & galaxies
Submillimeter astronomy
Title The ALMA Spectroscopic Survey in the Hubble Ultra Deep Field: The Nature of the Faintest Dusty Star-forming Galaxies
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