The ALPINE-ALMA [CII] survey: Little to no evolution in the [CII]-SFR relation over the last 13 Gyr

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The ALPINE-ALMA [CII] survey : Little to no evolution in the [CII]-SFR relation over the last 13 Gyr. / Schaerer, D.; Ginolfi, M.; Bethermin, M.; Fudamoto, Y.; Oesch, P. A.; Le Fevre, O.; Faisst, A.; Capak, P.; Cassata, P.; Silverman, J. D.; Yan, Lin; Jones, G. C.; Amorin, R.; Bardelli, S.; Boquien, M.; Cimatti, A.; Dessauges-Zavadsky, M.; Giavalisco, M.; Hathi, N. P.; Fujimoto, S.; Ibar, E.; Koekemoer, A.; Lagache, G.; Lemaux, B. C.; Loiacono, F.; Maiolino, R.; Narayanan, D.; Morselli, L.; Mendez-Hernandez, H.; Pozzi, F.; Riechers, D.; Talia, M.; Toft, S.; Vallini, L.; Vergani, D.; Zamorani, G.; Zucca, E.

In: Astronomy & Astrophysics, Vol. 643, A3, 27.10.2020.

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

Harvard

Schaerer, D, Ginolfi, M, Bethermin, M, Fudamoto, Y, Oesch, PA, Le Fevre, O, Faisst, A, Capak, P, Cassata, P, Silverman, JD, Yan, L, Jones, GC, Amorin, R, Bardelli, S, Boquien, M, Cimatti, A, Dessauges-Zavadsky, M, Giavalisco, M, Hathi, NP, Fujimoto, S, Ibar, E, Koekemoer, A, Lagache, G, Lemaux, BC, Loiacono, F, Maiolino, R, Narayanan, D, Morselli, L, Mendez-Hernandez, H, Pozzi, F, Riechers, D, Talia, M, Toft, S, Vallini, L, Vergani, D, Zamorani, G & Zucca, E 2020, 'The ALPINE-ALMA [CII] survey: Little to no evolution in the [CII]-SFR relation over the last 13 Gyr', Astronomy & Astrophysics, vol. 643, A3. https://doi.org/10.1051/0004-6361/202037617

APA

Schaerer, D., Ginolfi, M., Bethermin, M., Fudamoto, Y., Oesch, P. A., Le Fevre, O., Faisst, A., Capak, P., Cassata, P., Silverman, J. D., Yan, L., Jones, G. C., Amorin, R., Bardelli, S., Boquien, M., Cimatti, A., Dessauges-Zavadsky, M., Giavalisco, M., Hathi, N. P., ... Zucca, E. (2020). The ALPINE-ALMA [CII] survey: Little to no evolution in the [CII]-SFR relation over the last 13 Gyr. Astronomy & Astrophysics, 643, [A3]. https://doi.org/10.1051/0004-6361/202037617

Vancouver

Schaerer D, Ginolfi M, Bethermin M, Fudamoto Y, Oesch PA, Le Fevre O et al. The ALPINE-ALMA [CII] survey: Little to no evolution in the [CII]-SFR relation over the last 13 Gyr. Astronomy & Astrophysics. 2020 Oct 27;643. A3. https://doi.org/10.1051/0004-6361/202037617

Author

Schaerer, D. ; Ginolfi, M. ; Bethermin, M. ; Fudamoto, Y. ; Oesch, P. A. ; Le Fevre, O. ; Faisst, A. ; Capak, P. ; Cassata, P. ; Silverman, J. D. ; Yan, Lin ; Jones, G. C. ; Amorin, R. ; Bardelli, S. ; Boquien, M. ; Cimatti, A. ; Dessauges-Zavadsky, M. ; Giavalisco, M. ; Hathi, N. P. ; Fujimoto, S. ; Ibar, E. ; Koekemoer, A. ; Lagache, G. ; Lemaux, B. C. ; Loiacono, F. ; Maiolino, R. ; Narayanan, D. ; Morselli, L. ; Mendez-Hernandez, H. ; Pozzi, F. ; Riechers, D. ; Talia, M. ; Toft, S. ; Vallini, L. ; Vergani, D. ; Zamorani, G. ; Zucca, E. / The ALPINE-ALMA [CII] survey : Little to no evolution in the [CII]-SFR relation over the last 13 Gyr. In: Astronomy & Astrophysics. 2020 ; Vol. 643.

Bibtex

@article{25775c95a8f3427c989d40395788d4db,
title = "The ALPINE-ALMA [CII] survey: Little to no evolution in the [CII]-SFR relation over the last 13 Gyr",
abstract = "The [CII] 158 mu m line is one of the strongest IR emission lines, which has been shown to trace the star formation rate (SFR) of galaxies in the nearby Universe, and up to z similar to 2. Whether this is also the case at higher redshift and in the early Universe remains debated. The ALPINE survey, which targeted 118 star-forming galaxies at 4.4 6 [CII] measurements (detections and upper limits) do not behave very differently to the z similar to 4-6 data. We find a weak dependence of L([CII])/SFR on the Ly alpha equivalent width. Finally, we find that the ratio L([CII])/L-IR similar to (1-3) x 10(-3) for the ALPINE sources, comparable to that of {"}normal{"} galaxies at lower redshift. Our analysis, which includes the largest sample (similar to 150 galaxies) of [CII] measurements at z>4 available so far, suggests no or little evolution of the [CII]-SFR relation over the last 13 Gyr of cosmic time.",
keywords = "galaxies: high-redshift, galaxies: star formation, galaxies: formation, C II EMISSION, STAR-FORMATION, INTERSTELLAR-MEDIUM, NORMAL GALAXIES, DUST CONTENT, LINE, GAS, STELLAR",
author = "D. Schaerer and M. Ginolfi and M. Bethermin and Y. Fudamoto and Oesch, {P. A.} and {Le Fevre}, O. and A. Faisst and P. Capak and P. Cassata and Silverman, {J. D.} and Lin Yan and Jones, {G. C.} and R. Amorin and S. Bardelli and M. Boquien and A. Cimatti and M. Dessauges-Zavadsky and M. Giavalisco and Hathi, {N. P.} and S. Fujimoto and E. Ibar and A. Koekemoer and G. Lagache and Lemaux, {B. C.} and F. Loiacono and R. Maiolino and D. Narayanan and L. Morselli and H. Mendez-Hernandez and F. Pozzi and D. Riechers and M. Talia and S. Toft and L. Vallini and D. Vergani and G. Zamorani and E. Zucca",
year = "2020",
month = oct,
day = "27",
doi = "10.1051/0004-6361/202037617",
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 - Little to no evolution in the [CII]-SFR relation over the last 13 Gyr

AU - Schaerer, D.

AU - Ginolfi, M.

AU - Bethermin, M.

AU - Fudamoto, Y.

AU - Oesch, P. A.

AU - Le Fevre, O.

AU - Faisst, A.

AU - Capak, P.

AU - Cassata, P.

AU - Silverman, J. D.

AU - Yan, Lin

AU - Jones, G. C.

AU - Amorin, R.

AU - Bardelli, S.

AU - Boquien, M.

AU - Cimatti, A.

AU - Dessauges-Zavadsky, M.

AU - Giavalisco, M.

AU - Hathi, N. P.

AU - Fujimoto, S.

AU - Ibar, E.

AU - Koekemoer, A.

AU - Lagache, G.

AU - Lemaux, B. C.

AU - Loiacono, F.

AU - Maiolino, R.

AU - Narayanan, D.

AU - Morselli, L.

AU - Mendez-Hernandez, H.

AU - Pozzi, F.

AU - Riechers, D.

AU - Talia, M.

AU - Toft, S.

AU - Vallini, L.

AU - Vergani, D.

AU - Zamorani, G.

AU - Zucca, E.

PY - 2020/10/27

Y1 - 2020/10/27

N2 - The [CII] 158 mu m line is one of the strongest IR emission lines, which has been shown to trace the star formation rate (SFR) of galaxies in the nearby Universe, and up to z similar to 2. Whether this is also the case at higher redshift and in the early Universe remains debated. The ALPINE survey, which targeted 118 star-forming galaxies at 4.4 6 [CII] measurements (detections and upper limits) do not behave very differently to the z similar to 4-6 data. We find a weak dependence of L([CII])/SFR on the Ly alpha equivalent width. Finally, we find that the ratio L([CII])/L-IR similar to (1-3) x 10(-3) for the ALPINE sources, comparable to that of "normal" galaxies at lower redshift. Our analysis, which includes the largest sample (similar to 150 galaxies) of [CII] measurements at z>4 available so far, suggests no or little evolution of the [CII]-SFR relation over the last 13 Gyr of cosmic time.

AB - The [CII] 158 mu m line is one of the strongest IR emission lines, which has been shown to trace the star formation rate (SFR) of galaxies in the nearby Universe, and up to z similar to 2. Whether this is also the case at higher redshift and in the early Universe remains debated. The ALPINE survey, which targeted 118 star-forming galaxies at 4.4 6 [CII] measurements (detections and upper limits) do not behave very differently to the z similar to 4-6 data. We find a weak dependence of L([CII])/SFR on the Ly alpha equivalent width. Finally, we find that the ratio L([CII])/L-IR similar to (1-3) x 10(-3) for the ALPINE sources, comparable to that of "normal" galaxies at lower redshift. Our analysis, which includes the largest sample (similar to 150 galaxies) of [CII] measurements at z>4 available so far, suggests no or little evolution of the [CII]-SFR relation over the last 13 Gyr of cosmic time.

KW - galaxies: high-redshift

KW - galaxies: star formation

KW - galaxies: formation

KW - C II EMISSION

KW - STAR-FORMATION

KW - INTERSTELLAR-MEDIUM

KW - NORMAL GALAXIES

KW - DUST CONTENT

KW - LINE

KW - GAS

KW - STELLAR

U2 - 10.1051/0004-6361/202037617

DO - 10.1051/0004-6361/202037617

M3 - Journal article

VL - 643

JO - Astronomy & Astrophysics

JF - Astronomy & Astrophysics

SN - 0004-6361

M1 - A3

ER -

ID: 252148323