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The ALMA Spectroscopic Survey in the Hubble Ultra Deep Field : Multiband Constraints on Line-luminosity Functions and the Cosmic Density of Molecular Gas. / Decarli, Roberto; Aravena, Manuel; Boogaard, Leindert; Carilli, Chris; Gonzalez-Lopez, Jorge; Walter, Fabian; Cortes, Paulo C.; Cox, Pierre; da Cunha, Elisabete; Daddi, Emanuele; Diaz-Santos, Tanio; Hodge, Jacqueline A.; Inami, Hanae; Neeleman, Marcel; Novak, Mladen; Oesch, Pascal; Popping, Gergoe; Riechers, Dominik; Smail, Ian; Uzgil, Bade; van der Werf, Paul; Wagg, Jeff; Weiss, Axel.
In:
Astrophysical Journal, Vol. 902, No. 2, 110, 19.10.2020.
Research output: Contribution to journal › Journal article › Research › peer-review
Harvard
Decarli, R, Aravena, M, Boogaard, L, Carilli, C, Gonzalez-Lopez, J, Walter, F, Cortes, PC, Cox, P, da Cunha, E, Daddi, E, Diaz-Santos, T, Hodge, JA, Inami, H, Neeleman, M, Novak, M, Oesch, P, Popping, G, Riechers, D, Smail, I, Uzgil, B, van der Werf, P, Wagg, J & Weiss, A 2020, '
The ALMA Spectroscopic Survey in the Hubble Ultra Deep Field: Multiband Constraints on Line-luminosity Functions and the Cosmic Density of Molecular Gas',
Astrophysical Journal, vol. 902, no. 2, 110.
https://doi.org/10.3847/1538-4357/abaa3bAPA
Decarli, R., Aravena, M., Boogaard, L., Carilli, C., Gonzalez-Lopez, J., Walter, F., Cortes, P. C., Cox, P., da Cunha, E., Daddi, E., Diaz-Santos, T., Hodge, J. A., Inami, H., Neeleman, M., Novak, M., Oesch, P., Popping, G., Riechers, D., Smail, I., ... Weiss, A. (2020).
The ALMA Spectroscopic Survey in the Hubble Ultra Deep Field: Multiband Constraints on Line-luminosity Functions and the Cosmic Density of Molecular Gas.
Astrophysical Journal,
902(2), [110].
https://doi.org/10.3847/1538-4357/abaa3bVancouver
Decarli R, Aravena M, Boogaard L, Carilli C, Gonzalez-Lopez J, Walter F et al.
The ALMA Spectroscopic Survey in the Hubble Ultra Deep Field: Multiband Constraints on Line-luminosity Functions and the Cosmic Density of Molecular Gas.
Astrophysical Journal. 2020 Oct 19;902(2). 110.
https://doi.org/10.3847/1538-4357/abaa3bAuthor
Decarli, Roberto ; Aravena, Manuel ; Boogaard, Leindert ; Carilli, Chris ; Gonzalez-Lopez, Jorge ; Walter, Fabian ; Cortes, Paulo C. ; Cox, Pierre ; da Cunha, Elisabete ; Daddi, Emanuele ; Diaz-Santos, Tanio ; Hodge, Jacqueline A. ; Inami, Hanae ; Neeleman, Marcel ; Novak, Mladen ; Oesch, Pascal ; Popping, Gergoe ; Riechers, Dominik ; Smail, Ian ; Uzgil, Bade ; van der Werf, Paul ; Wagg, Jeff ; Weiss, Axel. / The ALMA Spectroscopic Survey in the Hubble Ultra Deep Field : Multiband Constraints on Line-luminosity Functions and the Cosmic Density of Molecular Gas. In: Astrophysical Journal. 2020 ; Vol. 902, No. 2.
Bibtex
@article{c7ade1cadf134001a79f74bc7f516e4d,
title = "The ALMA Spectroscopic Survey in the Hubble Ultra Deep Field: Multiband Constraints on Line-luminosity Functions and the Cosmic Density of Molecular Gas",
abstract = "We present a CO and atomic fine-structure line-luminosity function analysis using the ALMA Spectroscopic Survey (ASPECS) in the Hubble Ultra Deep Field. ASPECS consists of two spatially overlapping mosaics that cover the entire ALMA 3 mm and 1.2 mm bands. We combine the results of a line-candidate search of the 1.2 mm data cube with those previously obtained from the 3 mm cube. Our analysis shows that similar to 80% of the line flux observed at 3 mm arises from CO(2-1) or CO(3-2) emitters atz = 1-3 ({"}cosmic noon{"}). At 1.2 mm, more than half of the line flux arises from intermediate-JCO transitions (J(up) = 3-6); similar to 12% from neutral carbon lines; and",
keywords = "Molecular gas, Galaxy evolution, Luminosity function, STAR-FORMING GALAXIES, ATOMIC CARBON, CO, EVOLUTION, RESERVOIRS, FRACTIONS, EMISSION, TIME",
author = "Roberto Decarli and Manuel Aravena and Leindert Boogaard and Chris Carilli and Jorge Gonzalez-Lopez and Fabian Walter and Cortes, {Paulo C.} and Pierre Cox and {da Cunha}, Elisabete and Emanuele Daddi and Tanio Diaz-Santos and Hodge, {Jacqueline A.} and Hanae Inami and Marcel Neeleman and Mladen Novak and Pascal Oesch and Gergoe Popping and Dominik Riechers and Ian Smail and Bade Uzgil and {van der Werf}, Paul and Jeff Wagg and Axel Weiss",
year = "2020",
month = oct,
day = "19",
doi = "10.3847/1538-4357/abaa3b",
language = "English",
volume = "902",
journal = "Astrophysical Journal",
issn = "0004-637X",
publisher = "Institute of Physics Publishing, Inc",
number = "2",
}
RIS
TY - JOUR
T1 - The ALMA Spectroscopic Survey in the Hubble Ultra Deep Field
T2 - Multiband Constraints on Line-luminosity Functions and the Cosmic Density of Molecular Gas
AU - Decarli, Roberto
AU - Aravena, Manuel
AU - Boogaard, Leindert
AU - Carilli, Chris
AU - Gonzalez-Lopez, Jorge
AU - Walter, Fabian
AU - Cortes, Paulo C.
AU - Cox, Pierre
AU - da Cunha, Elisabete
AU - Daddi, Emanuele
AU - Diaz-Santos, Tanio
AU - Hodge, Jacqueline A.
AU - Inami, Hanae
AU - Neeleman, Marcel
AU - Novak, Mladen
AU - Oesch, Pascal
AU - Popping, Gergoe
AU - Riechers, Dominik
AU - Smail, Ian
AU - Uzgil, Bade
AU - van der Werf, Paul
AU - Wagg, Jeff
AU - Weiss, Axel
PY - 2020/10/19
Y1 - 2020/10/19
N2 - We present a CO and atomic fine-structure line-luminosity function analysis using the ALMA Spectroscopic Survey (ASPECS) in the Hubble Ultra Deep Field. ASPECS consists of two spatially overlapping mosaics that cover the entire ALMA 3 mm and 1.2 mm bands. We combine the results of a line-candidate search of the 1.2 mm data cube with those previously obtained from the 3 mm cube. Our analysis shows that similar to 80% of the line flux observed at 3 mm arises from CO(2-1) or CO(3-2) emitters atz = 1-3 ("cosmic noon"). At 1.2 mm, more than half of the line flux arises from intermediate-JCO transitions (J(up) = 3-6); similar to 12% from neutral carbon lines; and
AB - We present a CO and atomic fine-structure line-luminosity function analysis using the ALMA Spectroscopic Survey (ASPECS) in the Hubble Ultra Deep Field. ASPECS consists of two spatially overlapping mosaics that cover the entire ALMA 3 mm and 1.2 mm bands. We combine the results of a line-candidate search of the 1.2 mm data cube with those previously obtained from the 3 mm cube. Our analysis shows that similar to 80% of the line flux observed at 3 mm arises from CO(2-1) or CO(3-2) emitters atz = 1-3 ("cosmic noon"). At 1.2 mm, more than half of the line flux arises from intermediate-JCO transitions (J(up) = 3-6); similar to 12% from neutral carbon lines; and
KW - Molecular gas
KW - Galaxy evolution
KW - Luminosity function
KW - STAR-FORMING GALAXIES
KW - ATOMIC CARBON
KW - CO
KW - EVOLUTION
KW - RESERVOIRS
KW - FRACTIONS
KW - EMISSION
KW - TIME
U2 - 10.3847/1538-4357/abaa3b
DO - 10.3847/1538-4357/abaa3b
M3 - Journal article
VL - 902
JO - Astrophysical Journal
JF - Astrophysical Journal
SN - 0004-637X
IS - 2
M1 - 110
ER -
