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The ALPINE-ALMA [CII] survey : Obscured star formation rate density and main sequence of star-forming galaxies at z > 4. / 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.; Jones, G. C.; Koekemoer, A. M.; Lagache, G.; Maiolino, R.; Lemaux, B. C.; Oesch, P.; Pozzi, F.; Riechers, D. A.; Romano, M.; Talia, M.; Toft, S.; Vergani, D.; Zamorani, G.; Zucca, E.
In:
Astronomy & Astrophysics, Vol. 649, A152, 01.06.2021.
Research output: Contribution to journal › Journal article › Research › peer-review
Harvard
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, vol. 649, A152.
https://doi.org/10.1051/0004-6361/202038944APA
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, [A152].
https://doi.org/10.1051/0004-6361/202038944Vancouver
Khusanova Y, Bethermin M, Le Fevre O, Capak P, Faisst AL, Schaerer D et al.
The ALPINE-ALMA [CII] survey: Obscured star formation rate density and main sequence of star-forming galaxies at z > 4.
Astronomy & Astrophysics. 2021 Jun 1;649. A152.
https://doi.org/10.1051/0004-6361/202038944Author
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. ; Jones, G. C. ; Koekemoer, A. M. ; Lagache, G. ; Maiolino, R. ; Lemaux, B. C. ; Oesch, P. ; Pozzi, F. ; Riechers, D. A. ; Romano, M. ; Talia, M. ; Toft, S. ; Vergani, D. ; Zamorani, G. ; Zucca, E. / The ALPINE-ALMA [CII] survey : Obscured star formation rate density and main sequence of star-forming galaxies at z > 4. In: Astronomy & Astrophysics. 2021 ; Vol. 649.
Bibtex
@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",
}
RIS
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
VL - 649
JO - Astronomy & Astrophysics
JF - Astronomy & Astrophysics
SN - 0004-6361
M1 - A152
ER -
