The ALMA Spectroscopic Survey in the HUDF: The Cosmic Dust and Gas Mass Densities in Galaxies up to z similar to 3

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The ALMA Spectroscopic Survey in the HUDF : The Cosmic Dust and Gas Mass Densities in Galaxies up to z similar to 3. / Magnelli, Benjamin; Boogaard, Leindert; Decarli, Roberto; Gonzalez-Lopez, Jorge; Novak, Mladen; Popping, Gergo; Smail, Ian; Walter, Fabian; Aravena, Manuel; Assef, Roberto J.; Bauer, Franz Erik; Bertoldi, Frank; Carilli, Chris; Cortes, Paulo C.; da Cunha, Elisabete; Daddi, Emanuele; Diaz-Santos, Tanio; Inami, Hanae; Ivison, Robert J.; Le Fevre, Olivier; Oesch, Pascal; Riechers, Dominik; Rix, Hans-Walter; Sargent, Mark T.; van der Werf, Paul; Wagg, Jeff; Weiss, Axel.

In: Astrophysical Journal, Vol. 892, No. 1, 66, 20.03.2020.

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

Harvard

Magnelli, B, Boogaard, L, Decarli, R, Gonzalez-Lopez, J, Novak, M, Popping, G, Smail, I, Walter, F, Aravena, M, Assef, RJ, Bauer, FE, Bertoldi, F, Carilli, C, Cortes, PC, da Cunha, E, Daddi, E, Diaz-Santos, T, Inami, H, Ivison, RJ, Le Fevre, O, Oesch, P, Riechers, D, Rix, H-W, Sargent, MT, van der Werf, P, Wagg, J & Weiss, A 2020, 'The ALMA Spectroscopic Survey in the HUDF: The Cosmic Dust and Gas Mass Densities in Galaxies up to z similar to 3', Astrophysical Journal, vol. 892, no. 1, 66. https://doi.org/10.3847/1538-4357/ab7897

APA

Magnelli, B., Boogaard, L., Decarli, R., Gonzalez-Lopez, J., Novak, M., Popping, G., Smail, I., Walter, F., Aravena, M., Assef, R. J., Bauer, F. E., Bertoldi, F., Carilli, C., Cortes, P. C., da Cunha, E., Daddi, E., Diaz-Santos, T., Inami, H., Ivison, R. J., ... Weiss, A. (2020). The ALMA Spectroscopic Survey in the HUDF: The Cosmic Dust and Gas Mass Densities in Galaxies up to z similar to 3. Astrophysical Journal, 892(1), [66]. https://doi.org/10.3847/1538-4357/ab7897

Vancouver

Magnelli B, Boogaard L, Decarli R, Gonzalez-Lopez J, Novak M, Popping G et al. The ALMA Spectroscopic Survey in the HUDF: The Cosmic Dust and Gas Mass Densities in Galaxies up to z similar to 3. Astrophysical Journal. 2020 Mar 20;892(1). 66. https://doi.org/10.3847/1538-4357/ab7897

Author

Magnelli, Benjamin ; Boogaard, Leindert ; Decarli, Roberto ; Gonzalez-Lopez, Jorge ; Novak, Mladen ; Popping, Gergo ; Smail, Ian ; Walter, Fabian ; Aravena, Manuel ; Assef, Roberto J. ; Bauer, Franz Erik ; Bertoldi, Frank ; Carilli, Chris ; Cortes, Paulo C. ; da Cunha, Elisabete ; Daddi, Emanuele ; Diaz-Santos, Tanio ; Inami, Hanae ; Ivison, Robert J. ; Le Fevre, Olivier ; Oesch, Pascal ; Riechers, Dominik ; Rix, Hans-Walter ; Sargent, Mark T. ; van der Werf, Paul ; Wagg, Jeff ; Weiss, Axel. / The ALMA Spectroscopic Survey in the HUDF : The Cosmic Dust and Gas Mass Densities in Galaxies up to z similar to 3. In: Astrophysical Journal. 2020 ; Vol. 892, No. 1.

Bibtex

@article{576b7de10ca54ddfad8c3450bb58f8ed,
title = "The ALMA Spectroscopic Survey in the HUDF: The Cosmic Dust and Gas Mass Densities in Galaxies up to z similar to 3",
abstract = "Using the deepest 1.2 mm continuum map to date in the Hubble Ultra Deep Field, which was obtained as part of the ALMA Spectroscopic Survey (ASPECS) large program, we measure the cosmic density of dust and implied gas (H-2+H i) mass in galaxies as a function of look-back time. We do so by stacking the contribution from all H-band selected galaxies above a given stellar mass in distinct redshift bins, M decreases down to 10(10) M, but this growth slows down toward lower stellar masses. This flattening implies that at our stellar mass-completeness limits (10(8) M and 10(8.9) M at z similar to 0.4 and z similar to 3), both quantities converge toward the total cosmic dust and gas mass densities in galaxies. The cosmic dust and gas mass densities increase at early cosmic time, peak around z similar to 2, and decrease by a factor similar to 4 and 7, when compared to the density of dust and molecular gas in the local universe, respectively. The contribution of quiescent galaxies (i.e., with little on-going star formation) to the cosmic dust and gas mass densities is minor (less than or similar to 10%). The redshift evolution of the cosmic gas mass density resembles that of the SFR density, as previously found by CO-based measurements. This confirms that galaxies have relatively constant star formation efficiencies (within a factor similar to 2) across cosmic time. Our results also imply that by z similar to 0, a large fraction (similar to 90%) of dust formed in galaxies across cosmic time has either been destroyed or ejected to the intergalactic medium.",
keywords = "High-redshift galaxies, Galaxy evolution, Galaxy formation, ULTRA DEEP FIELD, INFRARED-EMISSION, INTERSTELLAR DUST, MOLECULAR GAS, REDSHIFT, MODEL, EVOLUTION, STELLAR, HALOES, Z=0",
author = "Benjamin Magnelli and Leindert Boogaard and Roberto Decarli and Jorge Gonzalez-Lopez and Mladen Novak and Gergo Popping and Ian Smail and Fabian Walter and Manuel Aravena and Assef, {Roberto J.} and Bauer, {Franz Erik} and Frank Bertoldi and Chris Carilli and Cortes, {Paulo C.} and {da Cunha}, Elisabete and Emanuele Daddi and Tanio Diaz-Santos and Hanae Inami and Ivison, {Robert J.} and {Le Fevre}, Olivier and Pascal Oesch and Dominik Riechers and Hans-Walter Rix and Sargent, {Mark T.} and {van der Werf}, Paul and Jeff Wagg and Axel Weiss",
year = "2020",
month = mar,
day = "20",
doi = "10.3847/1538-4357/ab7897",
language = "English",
volume = "892",
journal = "Astrophysical Journal",
issn = "0004-637X",
publisher = "Institute of Physics Publishing, Inc",
number = "1",

}

RIS

TY - JOUR

T1 - The ALMA Spectroscopic Survey in the HUDF

T2 - The Cosmic Dust and Gas Mass Densities in Galaxies up to z similar to 3

AU - Magnelli, Benjamin

AU - Boogaard, Leindert

AU - Decarli, Roberto

AU - Gonzalez-Lopez, Jorge

AU - Novak, Mladen

AU - Popping, Gergo

AU - Smail, Ian

AU - Walter, Fabian

AU - Aravena, Manuel

AU - Assef, Roberto J.

AU - Bauer, Franz Erik

AU - Bertoldi, Frank

AU - Carilli, Chris

AU - Cortes, Paulo C.

AU - da Cunha, Elisabete

AU - Daddi, Emanuele

AU - Diaz-Santos, Tanio

AU - Inami, Hanae

AU - Ivison, Robert J.

AU - Le Fevre, Olivier

AU - Oesch, Pascal

AU - Riechers, Dominik

AU - Rix, Hans-Walter

AU - Sargent, Mark T.

AU - van der Werf, Paul

AU - Wagg, Jeff

AU - Weiss, Axel

PY - 2020/3/20

Y1 - 2020/3/20

N2 - Using the deepest 1.2 mm continuum map to date in the Hubble Ultra Deep Field, which was obtained as part of the ALMA Spectroscopic Survey (ASPECS) large program, we measure the cosmic density of dust and implied gas (H-2+H i) mass in galaxies as a function of look-back time. We do so by stacking the contribution from all H-band selected galaxies above a given stellar mass in distinct redshift bins, M decreases down to 10(10) M, but this growth slows down toward lower stellar masses. This flattening implies that at our stellar mass-completeness limits (10(8) M and 10(8.9) M at z similar to 0.4 and z similar to 3), both quantities converge toward the total cosmic dust and gas mass densities in galaxies. The cosmic dust and gas mass densities increase at early cosmic time, peak around z similar to 2, and decrease by a factor similar to 4 and 7, when compared to the density of dust and molecular gas in the local universe, respectively. The contribution of quiescent galaxies (i.e., with little on-going star formation) to the cosmic dust and gas mass densities is minor (less than or similar to 10%). The redshift evolution of the cosmic gas mass density resembles that of the SFR density, as previously found by CO-based measurements. This confirms that galaxies have relatively constant star formation efficiencies (within a factor similar to 2) across cosmic time. Our results also imply that by z similar to 0, a large fraction (similar to 90%) of dust formed in galaxies across cosmic time has either been destroyed or ejected to the intergalactic medium.

AB - Using the deepest 1.2 mm continuum map to date in the Hubble Ultra Deep Field, which was obtained as part of the ALMA Spectroscopic Survey (ASPECS) large program, we measure the cosmic density of dust and implied gas (H-2+H i) mass in galaxies as a function of look-back time. We do so by stacking the contribution from all H-band selected galaxies above a given stellar mass in distinct redshift bins, M decreases down to 10(10) M, but this growth slows down toward lower stellar masses. This flattening implies that at our stellar mass-completeness limits (10(8) M and 10(8.9) M at z similar to 0.4 and z similar to 3), both quantities converge toward the total cosmic dust and gas mass densities in galaxies. The cosmic dust and gas mass densities increase at early cosmic time, peak around z similar to 2, and decrease by a factor similar to 4 and 7, when compared to the density of dust and molecular gas in the local universe, respectively. The contribution of quiescent galaxies (i.e., with little on-going star formation) to the cosmic dust and gas mass densities is minor (less than or similar to 10%). The redshift evolution of the cosmic gas mass density resembles that of the SFR density, as previously found by CO-based measurements. This confirms that galaxies have relatively constant star formation efficiencies (within a factor similar to 2) across cosmic time. Our results also imply that by z similar to 0, a large fraction (similar to 90%) of dust formed in galaxies across cosmic time has either been destroyed or ejected to the intergalactic medium.

KW - High-redshift galaxies

KW - Galaxy evolution

KW - Galaxy formation

KW - ULTRA DEEP FIELD

KW - INFRARED-EMISSION

KW - INTERSTELLAR DUST

KW - MOLECULAR GAS

KW - REDSHIFT

KW - MODEL

KW - EVOLUTION

KW - STELLAR

KW - HALOES

KW - Z=0

U2 - 10.3847/1538-4357/ab7897

DO - 10.3847/1538-4357/ab7897

M3 - Journal article

VL - 892

JO - Astrophysical Journal

JF - Astrophysical Journal

SN - 0004-637X

IS - 1

M1 - 66

ER -

ID: 258028947