The ALPINE-ALMA [CII] survey: The nature, luminosity function, and star formation history of dusty galaxies up to z similar or equal to 6

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

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The ALPINE-ALMA [CII] survey : The nature, luminosity function, and star formation history of dusty galaxies up to z similar or equal to 6. / Gruppioni, C.; Bethermin, M.; Loiacono, F.; Le Fevre, O.; Capak, P.; Cassata, P.; Faisst, A. L.; Schaerer, D.; Silverman, J.; Yan, L.; Bardelli, S.; Boquien, M.; Carraro, R.; Cimatti, A.; Dessauges-Zavadsky, M.; Ginolfi, M.; Fujimoto, S.; Hathi, N. P.; Jones, G. C.; Khusanova, Y.; Koekemoer, A. M.; Lagache, G.; Lemaux, B. C.; Oesch, P. A.; Pozzi, F.; Riechers, D. A.; Rodighiero, G.; Romano, M.; Talia, M.; Vallini, L.; Vergani, D.; Zamorani, G.; Zucca, E.

In: Astronomy & Astrophysics, Vol. 643, A8, 27.10.2020.

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

Harvard

Gruppioni, C, Bethermin, M, Loiacono, F, Le Fevre, O, Capak, P, Cassata, P, Faisst, AL, Schaerer, D, Silverman, J, Yan, L, Bardelli, S, Boquien, M, Carraro, R, Cimatti, A, Dessauges-Zavadsky, M, Ginolfi, M, Fujimoto, S, Hathi, NP, Jones, GC, Khusanova, Y, Koekemoer, AM, Lagache, G, Lemaux, BC, Oesch, PA, Pozzi, F, Riechers, DA, Rodighiero, G, Romano, M, Talia, M, Vallini, L, Vergani, D, Zamorani, G & Zucca, E 2020, 'The ALPINE-ALMA [CII] survey: The nature, luminosity function, and star formation history of dusty galaxies up to z similar or equal to 6', Astronomy & Astrophysics, vol. 643, A8. https://doi.org/10.1051/0004-6361/202038487

APA

Gruppioni, C., Bethermin, M., Loiacono, F., Le Fevre, O., Capak, P., Cassata, P., Faisst, A. L., Schaerer, D., Silverman, J., Yan, L., Bardelli, S., Boquien, M., Carraro, R., Cimatti, A., Dessauges-Zavadsky, M., Ginolfi, M., Fujimoto, S., Hathi, N. P., Jones, G. C., ... Zucca, E. (2020). The ALPINE-ALMA [CII] survey: The nature, luminosity function, and star formation history of dusty galaxies up to z similar or equal to 6. Astronomy & Astrophysics, 643, [A8]. https://doi.org/10.1051/0004-6361/202038487

Vancouver

Gruppioni C, Bethermin M, Loiacono F, Le Fevre O, Capak P, Cassata P et al. The ALPINE-ALMA [CII] survey: The nature, luminosity function, and star formation history of dusty galaxies up to z similar or equal to 6. Astronomy & Astrophysics. 2020 Oct 27;643. A8. https://doi.org/10.1051/0004-6361/202038487

Author

Gruppioni, C. ; Bethermin, M. ; Loiacono, F. ; Le Fevre, O. ; Capak, P. ; Cassata, P. ; Faisst, A. L. ; Schaerer, D. ; Silverman, J. ; Yan, L. ; Bardelli, S. ; Boquien, M. ; Carraro, R. ; Cimatti, A. ; Dessauges-Zavadsky, M. ; Ginolfi, M. ; Fujimoto, S. ; Hathi, N. P. ; Jones, G. C. ; Khusanova, Y. ; Koekemoer, A. M. ; Lagache, G. ; Lemaux, B. C. ; Oesch, P. A. ; Pozzi, F. ; Riechers, D. A. ; Rodighiero, G. ; Romano, M. ; Talia, M. ; Vallini, L. ; Vergani, D. ; Zamorani, G. ; Zucca, E. / The ALPINE-ALMA [CII] survey : The nature, luminosity function, and star formation history of dusty galaxies up to z similar or equal to 6. In: Astronomy & Astrophysics. 2020 ; Vol. 643.

Bibtex

@article{a8dddf637aaa40449efb83a3d1ad365e,
title = "The ALPINE-ALMA [CII] survey: The nature, luminosity function, and star formation history of dusty galaxies up to z similar or equal to 6",
abstract = "Aims. We present the detailed characterisation of a sample of 56 sources serendipitously detected in ALMA band 7 as part of the ALMA Large Program to INvestigate CII at Early Times (ALPINE). These sources, detected in COSMOS and ECDFS, have been used to derive the total infrared luminosity function (LF) and to estimate the cosmic star formation rate density (SFRD) up to z similar or equal to 6.Methods. We looked for counterparts of the ALMA sources in all the available multi-wavelength (from HST to VLA) and photometric redshift catalogues. We also made use of deeper UltraVISTA and Spitzer source lists and maps to identify optically dark sources with no matches in the public catalogues. We used the sources with estimated redshifts to derive the 250 mu m rest-frame and total infrared (8-1000 mu m) LFs from z similar or equal to 0.5 to 6.Results. Our ALMA blind survey (860 mu m flux density range: similar to 0.3-12.5 mJy) allows us to further push the study of the nature and evolution of dusty galaxies at high-z, identifying luminous and massive sources to redshifts and faint luminosities never probed before by any far-infrared surveys. The ALPINE data are the first ones to sample the faint end of the infrared LF, showing little evolution from z similar or equal to 2.5 to z similar or equal to 6, and a {"}flat{"} slope up to the highest redshifts (i.e. 4.5 3.",
keywords = "galaxies: evolution, galaxies: high-redshift, galaxies: luminosity function, mass function, cosmology: observations, submillimeter: galaxies, DEEP FIELD-SOUTH, FORMATION RATE DENSITY, FORMING GALAXIES, SPECTROSCOPIC SURVEY, QUIESCENT GALAXY, MASSIVE GALAXIES, FORMATION RATES, REDSHIFT SURVEY, MOLECULAR GAS, MU-M",
author = "C. Gruppioni and M. Bethermin and F. Loiacono and {Le Fevre}, O. and P. Capak and P. Cassata and Faisst, {A. L.} and D. Schaerer and J. Silverman and L. Yan and S. Bardelli and M. Boquien and R. Carraro and A. Cimatti and M. Dessauges-Zavadsky and M. Ginolfi and S. Fujimoto and Hathi, {N. P.} and Jones, {G. C.} and Y. Khusanova and Koekemoer, {A. M.} and G. Lagache and Lemaux, {B. C.} and Oesch, {P. A.} and F. Pozzi and Riechers, {D. A.} and G. Rodighiero and M. Romano and M. Talia and L. Vallini and D. Vergani and G. Zamorani and E. Zucca",
year = "2020",
month = oct,
day = "27",
doi = "10.1051/0004-6361/202038487",
language = "English",
volume = "643",
journal = "Astronomy & Astrophysics",
issn = "0004-6361",
publisher = "E D P Sciences",

}

RIS

TY - JOUR

T1 - The ALPINE-ALMA [CII] survey

T2 - The nature, luminosity function, and star formation history of dusty galaxies up to z similar or equal to 6

AU - Gruppioni, C.

AU - Bethermin, M.

AU - Loiacono, F.

AU - Le Fevre, O.

AU - Capak, P.

AU - Cassata, P.

AU - Faisst, A. L.

AU - Schaerer, D.

AU - Silverman, J.

AU - Yan, L.

AU - Bardelli, S.

AU - Boquien, M.

AU - Carraro, R.

AU - Cimatti, A.

AU - Dessauges-Zavadsky, M.

AU - Ginolfi, M.

AU - Fujimoto, S.

AU - Hathi, N. P.

AU - Jones, G. C.

AU - Khusanova, Y.

AU - Koekemoer, A. M.

AU - Lagache, G.

AU - Lemaux, B. C.

AU - Oesch, P. A.

AU - Pozzi, F.

AU - Riechers, D. A.

AU - Rodighiero, G.

AU - Romano, M.

AU - Talia, M.

AU - Vallini, L.

AU - Vergani, D.

AU - Zamorani, G.

AU - Zucca, E.

PY - 2020/10/27

Y1 - 2020/10/27

N2 - Aims. We present the detailed characterisation of a sample of 56 sources serendipitously detected in ALMA band 7 as part of the ALMA Large Program to INvestigate CII at Early Times (ALPINE). These sources, detected in COSMOS and ECDFS, have been used to derive the total infrared luminosity function (LF) and to estimate the cosmic star formation rate density (SFRD) up to z similar or equal to 6.Methods. We looked for counterparts of the ALMA sources in all the available multi-wavelength (from HST to VLA) and photometric redshift catalogues. We also made use of deeper UltraVISTA and Spitzer source lists and maps to identify optically dark sources with no matches in the public catalogues. We used the sources with estimated redshifts to derive the 250 mu m rest-frame and total infrared (8-1000 mu m) LFs from z similar or equal to 0.5 to 6.Results. Our ALMA blind survey (860 mu m flux density range: similar to 0.3-12.5 mJy) allows us to further push the study of the nature and evolution of dusty galaxies at high-z, identifying luminous and massive sources to redshifts and faint luminosities never probed before by any far-infrared surveys. The ALPINE data are the first ones to sample the faint end of the infrared LF, showing little evolution from z similar or equal to 2.5 to z similar or equal to 6, and a "flat" slope up to the highest redshifts (i.e. 4.5 3.

AB - Aims. We present the detailed characterisation of a sample of 56 sources serendipitously detected in ALMA band 7 as part of the ALMA Large Program to INvestigate CII at Early Times (ALPINE). These sources, detected in COSMOS and ECDFS, have been used to derive the total infrared luminosity function (LF) and to estimate the cosmic star formation rate density (SFRD) up to z similar or equal to 6.Methods. We looked for counterparts of the ALMA sources in all the available multi-wavelength (from HST to VLA) and photometric redshift catalogues. We also made use of deeper UltraVISTA and Spitzer source lists and maps to identify optically dark sources with no matches in the public catalogues. We used the sources with estimated redshifts to derive the 250 mu m rest-frame and total infrared (8-1000 mu m) LFs from z similar or equal to 0.5 to 6.Results. Our ALMA blind survey (860 mu m flux density range: similar to 0.3-12.5 mJy) allows us to further push the study of the nature and evolution of dusty galaxies at high-z, identifying luminous and massive sources to redshifts and faint luminosities never probed before by any far-infrared surveys. The ALPINE data are the first ones to sample the faint end of the infrared LF, showing little evolution from z similar or equal to 2.5 to z similar or equal to 6, and a "flat" slope up to the highest redshifts (i.e. 4.5 3.

KW - galaxies: evolution

KW - galaxies: high-redshift

KW - galaxies: luminosity function

KW - mass function

KW - cosmology: observations

KW - submillimeter: galaxies

KW - DEEP FIELD-SOUTH

KW - FORMATION RATE DENSITY

KW - FORMING GALAXIES

KW - SPECTROSCOPIC SURVEY

KW - QUIESCENT GALAXY

KW - MASSIVE GALAXIES

KW - FORMATION RATES

KW - REDSHIFT SURVEY

KW - MOLECULAR GAS

KW - MU-M

U2 - 10.1051/0004-6361/202038487

DO - 10.1051/0004-6361/202038487

M3 - Journal article

VL - 643

JO - Astronomy & Astrophysics

JF - Astronomy & Astrophysics

SN - 0004-6361

M1 - A8

ER -

ID: 252147978