The ALPINE-ALMA [CII] survey: Obscured star formation rate density and main sequence of star-forming galaxies at z > 4

Y. Khusanova; M. Bethermin; O. Le Fevre; P. Capak; A. L. Faisst; D. Schaerer; J. D. Silverman; P. Cassata; L. Yan; M. Ginolfi; Y. Fudamoto; F. Loiacono; R. Amorin; S. Bardelli; M. Boquien; A. Cimatti; M. Dessauges-Zavadsky; C. Gruppioni; N. P. Hathi; G. C. Jones; A. M. Koekemoer; G. Lagache; R. Maiolino; B. C. Lemaux; P. Oesch; F. Pozzi; D. A. Riechers; M. Romano; M. Talia; S. Toft; D. Vergani; G. Zamorani; E. Zucca

doi:10.1051/0004-6361/202038944

The ALPINE-ALMA [CII] survey: Obscured star formation rate density and main sequence of star-forming galaxies at z > 4

Y. Khusanova^*, M. Bethermin, O. Le Fevre, P. Capak, A. L. Faisst, D. Schaerer, J. D. Silverman, P. Cassata, L. Yan, M. Ginolfi, Y. Fudamoto, F. Loiacono, R. Amorin, S. Bardelli, M. Boquien, A. Cimatti, M. Dessauges-Zavadsky, C. Gruppioni, N. P. Hathi, G. C. JonesA. M. Koekemoer, G. Lagache, R. Maiolino, B. C. Lemaux, P. Oesch, F. Pozzi, D. A. Riechers, M. Romano, M. Talia, S. Toft, D. Vergani, G. Zamorani, E. Zucca

^*Corresponding author af dette arbejde

The Cosmic Dawn Center

Publikation: Bidrag til tidsskrift › Tidsskriftartikel › Forskning › peer review

66 Citationer (Scopus)

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Abstract

Star formation rate (SFR) measurements at z>4 have relied mostly on the rest-frame far-ultraviolet (FUV) observations. The corrections for dust attenuation based on the IRX-beta relation are highly uncertain and are still debated in the literature. Hence, rest-frame far-infrared (FIR) observations are necessary to constrain the dust-obscured component of the SFR. In this paper, we exploit the rest-frame FIR continuum observations collected by the ALMA Large Program to INvestigate [CII] at Early times (ALPINE) to directly constrain the obscured SFR in galaxies at 4.4

Originalsprog	Engelsk
Artikelnummer	A152
Tidsskrift	Astronomy & Astrophysics
Vol/bind	649
Antal sider	18
ISSN	0004-6361
DOI	https://doi.org/10.1051/0004-6361/202038944
Status	Udgivet - 1 jun. 2021

Adgang til dokumentet

10.1051/0004-6361/202038944Licens: CC BY

aa38944-20Forlagets udgivne version, 2,41 MBLicens: CC BY

Citationsformater

Khusanova, Y., Bethermin, M., Le Fevre, O., Capak, P., Faisst, A. L., Schaerer, D., Silverman, J. D., Cassata, P., Yan, L., Ginolfi, M., Fudamoto, Y., Loiacono, F., Amorin, R., Bardelli, S., Boquien, M., Cimatti, A., Dessauges-Zavadsky, M., Gruppioni, C., Hathi, N. P., ... Zucca, E. (2021). The ALPINE-ALMA [CII] survey: Obscured star formation rate density and main sequence of star-forming galaxies at z > 4. Astronomy & Astrophysics, 649, Artikel A152. https://doi.org/10.1051/0004-6361/202038944

Khusanova, Y, Bethermin, M, Le Fevre, O, Capak, P, Faisst, AL, Schaerer, D, Silverman, JD, Cassata, P, Yan, L, Ginolfi, M, Fudamoto, Y, Loiacono, F, Amorin, R, Bardelli, S, Boquien, M, Cimatti, A, Dessauges-Zavadsky, M, Gruppioni, C, Hathi, NP, Jones, GC, Koekemoer, AM, Lagache, G, Maiolino, R, Lemaux, BC, Oesch, P, Pozzi, F, Riechers, DA, Romano, M, Talia, M, Toft, S, Vergani, D, Zamorani, G & Zucca, E 2021, 'The ALPINE-ALMA [CII] survey: Obscured star formation rate density and main sequence of star-forming galaxies at z > 4', Astronomy & Astrophysics, bind 649, A152. https://doi.org/10.1051/0004-6361/202038944

@article{11bd9b41384842708bea893cf78d611d,

title = "The ALPINE-ALMA [CII] survey: Obscured star formation rate density and main sequence of star-forming galaxies at z > 4",

abstract = "Star formation rate (SFR) measurements at z>4 have relied mostly on the rest-frame far-ultraviolet (FUV) observations. The corrections for dust attenuation based on the IRX-beta relation are highly uncertain and are still debated in the literature. Hence, rest-frame far-infrared (FIR) observations are necessary to constrain the dust-obscured component of the SFR. In this paper, we exploit the rest-frame FIR continuum observations collected by the ALMA Large Program to INvestigate [CII] at Early times (ALPINE) to directly constrain the obscured SFR in galaxies at 4.4",

keywords = "galaxies: high-redshift, galaxies: evolution, galaxies: star formation, submillimeter: galaxies, LYMAN-BREAK GALAXIES, ULTRA DEEP FIELD, UV LUMINOSITY FUNCTIONS, STELLAR MASS FUNCTION, SPECTROSCOPIC SURVEY, PHOTOMETRIC REDSHIFTS, DUST ATTENUATION, EMISSION-LINES, NUMBER COUNTS, BILLION YEARS",

author = "Y. Khusanova and M. Bethermin and {Le Fevre}, O. and P. Capak and Faisst, {A. L.} and D. Schaerer and Silverman, {J. D.} and P. Cassata and L. Yan and M. Ginolfi and Y. Fudamoto and F. Loiacono and R. Amorin and S. Bardelli and M. Boquien and A. Cimatti and M. Dessauges-Zavadsky and C. Gruppioni and Hathi, {N. P.} and Jones, {G. C.} and Koekemoer, {A. M.} and G. Lagache and R. Maiolino and Lemaux, {B. C.} and P. Oesch and F. Pozzi and Riechers, {D. A.} and M. Romano and M. Talia and S. Toft and D. Vergani and G. Zamorani and E. Zucca",

year = "2021",

month = jun,

day = "1",

doi = "10.1051/0004-6361/202038944",

language = "English",

volume = "649",

journal = "Astronomy & Astrophysics",

issn = "0004-6361",

publisher = "E D P Sciences",

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TY - JOUR

T1 - The ALPINE-ALMA [CII] survey

T2 - Obscured star formation rate density and main sequence of star-forming galaxies at z > 4

AU - Khusanova, Y.

AU - Bethermin, M.

AU - Le Fevre, O.

AU - Capak, P.

AU - Faisst, A. L.

AU - Schaerer, D.

AU - Silverman, J. D.

AU - Cassata, P.

AU - Yan, L.

AU - Ginolfi, M.

AU - Fudamoto, Y.

AU - Loiacono, F.

AU - Amorin, R.

AU - Bardelli, S.

AU - Boquien, M.

AU - Cimatti, A.

AU - Dessauges-Zavadsky, M.

AU - Gruppioni, C.

AU - Hathi, N. P.

AU - Jones, G. C.

AU - Koekemoer, A. M.

AU - Lagache, G.

AU - Maiolino, R.

AU - Lemaux, B. C.

AU - Oesch, P.

AU - Pozzi, F.

AU - Riechers, D. A.

AU - Romano, M.

AU - Talia, M.

AU - Toft, S.

AU - Vergani, D.

AU - Zamorani, G.

AU - Zucca, E.

PY - 2021/6/1

Y1 - 2021/6/1

N2 - Star formation rate (SFR) measurements at z>4 have relied mostly on the rest-frame far-ultraviolet (FUV) observations. The corrections for dust attenuation based on the IRX-beta relation are highly uncertain and are still debated in the literature. Hence, rest-frame far-infrared (FIR) observations are necessary to constrain the dust-obscured component of the SFR. In this paper, we exploit the rest-frame FIR continuum observations collected by the ALMA Large Program to INvestigate [CII] at Early times (ALPINE) to directly constrain the obscured SFR in galaxies at 4.4

AB - Star formation rate (SFR) measurements at z>4 have relied mostly on the rest-frame far-ultraviolet (FUV) observations. The corrections for dust attenuation based on the IRX-beta relation are highly uncertain and are still debated in the literature. Hence, rest-frame far-infrared (FIR) observations are necessary to constrain the dust-obscured component of the SFR. In this paper, we exploit the rest-frame FIR continuum observations collected by the ALMA Large Program to INvestigate [CII] at Early times (ALPINE) to directly constrain the obscured SFR in galaxies at 4.4

KW - galaxies: high-redshift

KW - galaxies: evolution

KW - galaxies: star formation

KW - submillimeter: galaxies

KW - LYMAN-BREAK GALAXIES

KW - ULTRA DEEP FIELD

KW - UV LUMINOSITY FUNCTIONS

KW - STELLAR MASS FUNCTION

KW - SPECTROSCOPIC SURVEY

KW - PHOTOMETRIC REDSHIFTS

KW - DUST ATTENUATION

KW - EMISSION-LINES

KW - NUMBER COUNTS

KW - BILLION YEARS

U2 - 10.1051/0004-6361/202038944

DO - 10.1051/0004-6361/202038944

M3 - Journal article

SN - 0004-6361

VL - 649

JO - Astronomy & Astrophysics

JF - Astronomy & Astrophysics

M1 - A152

ER -