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The ALPINE-ALMA [CII] survey : Small Ly alpha-[CII] velocity offsets in main-sequence galaxies at 4.4 <z <6. / Cassata, P.; Morselli, L.; Faisst, A.; Ginolfi, M.; Bethermin, M.; Capak, P.; Le Fevre, O.; Schaerer, D.; Silverman, J.; Yan, L.; Lemaux, B. C.; Romano, M.; Talia, M.; Bardelli, S.; Boquien, M.; Cimatti, A.; Dessauges-Zavadsky, M.; Fudamoto, Y.; Fujimoto, S.; Giavalisco, M.; Hathi, N. P.; Ibar, E.; Jones, G.; Koekemoer, A. M.; Mendez-Hernandez, H.; Mancini, C.; Oesch, P. A.; Pozzi, F.; Riechers, D. A.; Rodighiero, G.; Vergani, D.; Zamorani, G.; Zucca, E.
I:
Astronomy & Astrophysics, Bind 643, A6, 27.10.2020.
Publikation: Bidrag til tidsskrift › Tidsskriftartikel › Forskning › fagfællebedømt
Harvard
Cassata, P, Morselli, L, Faisst, A, Ginolfi, M, Bethermin, M, Capak, P, Le Fevre, O, Schaerer, D, Silverman, J, Yan, L, Lemaux, BC, Romano, M, Talia, M, Bardelli, S, Boquien, M, Cimatti, A, Dessauges-Zavadsky, M, Fudamoto, Y, Fujimoto, S, Giavalisco, M, Hathi, NP, Ibar, E, Jones, G, Koekemoer, AM, Mendez-Hernandez, H, Mancini, C, Oesch, PA, Pozzi, F, Riechers, DA, Rodighiero, G, Vergani, D, Zamorani, G & Zucca, E 2020, '
The ALPINE-ALMA [CII] survey: Small Ly alpha-[CII] velocity offsets in main-sequence galaxies at 4.4 <z <6',
Astronomy & Astrophysics, bind 643, A6.
https://doi.org/10.1051/0004-6361/202037517APA
Cassata, P., Morselli, L., Faisst, A., Ginolfi, M., Bethermin, M., Capak, P., Le Fevre, O., Schaerer, D., Silverman, J., Yan, L., Lemaux, B. C., Romano, M., Talia, M., Bardelli, S., Boquien, M., Cimatti, A., Dessauges-Zavadsky, M., Fudamoto, Y., Fujimoto, S., ... Zucca, E. (2020).
The ALPINE-ALMA [CII] survey: Small Ly alpha-[CII] velocity offsets in main-sequence galaxies at 4.4 <z <6.
Astronomy & Astrophysics,
643, [A6].
https://doi.org/10.1051/0004-6361/202037517Vancouver
Cassata P, Morselli L, Faisst A, Ginolfi M, Bethermin M, Capak P o.a.
The ALPINE-ALMA [CII] survey: Small Ly alpha-[CII] velocity offsets in main-sequence galaxies at 4.4 <z <6.
Astronomy & Astrophysics. 2020 okt. 27;643. A6.
https://doi.org/10.1051/0004-6361/202037517Author
Cassata, P. ; Morselli, L. ; Faisst, A. ; Ginolfi, M. ; Bethermin, M. ; Capak, P. ; Le Fevre, O. ; Schaerer, D. ; Silverman, J. ; Yan, L. ; Lemaux, B. C. ; Romano, M. ; Talia, M. ; Bardelli, S. ; Boquien, M. ; Cimatti, A. ; Dessauges-Zavadsky, M. ; Fudamoto, Y. ; Fujimoto, S. ; Giavalisco, M. ; Hathi, N. P. ; Ibar, E. ; Jones, G. ; Koekemoer, A. M. ; Mendez-Hernandez, H. ; Mancini, C. ; Oesch, P. A. ; Pozzi, F. ; Riechers, D. A. ; Rodighiero, G. ; Vergani, D. ; Zamorani, G. ; Zucca, E. / The ALPINE-ALMA [CII] survey : Small Ly alpha-[CII] velocity offsets in main-sequence galaxies at 4.4 <z <6. I: Astronomy & Astrophysics. 2020 ; Bind 643.
Bibtex
@article{47b75c78e540433696109cfde9ee5037,
title = "The ALPINE-ALMA [CII] survey: Small Ly alpha-[CII] velocity offsets in main-sequence galaxies at 4.4 <z <6",
abstract = "Context. The Lyman-alpha line in the ultraviolet (UV) and the [CII] line in the far-infrared (FIR) are widely used tools to identify galaxies in the early Universe and to obtain insights into interstellar medium (ISM) properties in high-redshift galaxies. By combining data obtained with ALMA in band 7 at similar to 320 GHz as part of the ALMA Large Program to INvestigate [CII] at Early Times (ALPINE) with spectroscopic data from DEIMOS at the Keck Observatory, VIMOS and FORS2 at the Very Large Telescope, we assembled a unique sample of 53 main-sequence star-forming galaxies at 4.4",
keywords = "galaxies: ISM, galaxies: high-redshift, submillimeter: galaxies, LYMAN BREAK GALAXIES, LY-ALPHA RADIATION, STAR-FORMING GALAXIES, C II, ULTRAVIOLET-SPECTRA, PHYSICAL-PROPERTIES, REDSHIFT EVOLUTION, ESCAPE FRACTION, COSMOS FIELD, DUST CONTENT",
author = "P. Cassata and L. Morselli and A. Faisst and M. Ginolfi and M. Bethermin and P. Capak and {Le Fevre}, O. and D. Schaerer and J. Silverman and L. Yan and Lemaux, {B. C.} and M. Romano and M. Talia and S. Bardelli and M. Boquien and A. Cimatti and M. Dessauges-Zavadsky and Y. Fudamoto and S. Fujimoto and M. Giavalisco and Hathi, {N. P.} and E. Ibar and G. Jones and Koekemoer, {A. M.} and H. Mendez-Hernandez and C. Mancini and Oesch, {P. A.} and F. Pozzi and Riechers, {D. A.} and G. Rodighiero and D. Vergani and G. Zamorani and E. Zucca",
year = "2020",
month = oct,
day = "27",
doi = "10.1051/0004-6361/202037517",
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 - Small Ly alpha-[CII] velocity offsets in main-sequence galaxies at 4.4 <z <6
AU - Cassata, P.
AU - Morselli, L.
AU - Faisst, A.
AU - Ginolfi, M.
AU - Bethermin, M.
AU - Capak, P.
AU - Le Fevre, O.
AU - Schaerer, D.
AU - Silverman, J.
AU - Yan, L.
AU - Lemaux, B. C.
AU - Romano, M.
AU - Talia, M.
AU - Bardelli, S.
AU - Boquien, M.
AU - Cimatti, A.
AU - Dessauges-Zavadsky, M.
AU - Fudamoto, Y.
AU - Fujimoto, S.
AU - Giavalisco, M.
AU - Hathi, N. P.
AU - Ibar, E.
AU - Jones, G.
AU - Koekemoer, A. M.
AU - Mendez-Hernandez, H.
AU - Mancini, C.
AU - Oesch, P. A.
AU - Pozzi, F.
AU - Riechers, D. A.
AU - Rodighiero, G.
AU - Vergani, D.
AU - Zamorani, G.
AU - Zucca, E.
PY - 2020/10/27
Y1 - 2020/10/27
N2 - Context. The Lyman-alpha line in the ultraviolet (UV) and the [CII] line in the far-infrared (FIR) are widely used tools to identify galaxies in the early Universe and to obtain insights into interstellar medium (ISM) properties in high-redshift galaxies. By combining data obtained with ALMA in band 7 at similar to 320 GHz as part of the ALMA Large Program to INvestigate [CII] at Early Times (ALPINE) with spectroscopic data from DEIMOS at the Keck Observatory, VIMOS and FORS2 at the Very Large Telescope, we assembled a unique sample of 53 main-sequence star-forming galaxies at 4.4
AB - Context. The Lyman-alpha line in the ultraviolet (UV) and the [CII] line in the far-infrared (FIR) are widely used tools to identify galaxies in the early Universe and to obtain insights into interstellar medium (ISM) properties in high-redshift galaxies. By combining data obtained with ALMA in band 7 at similar to 320 GHz as part of the ALMA Large Program to INvestigate [CII] at Early Times (ALPINE) with spectroscopic data from DEIMOS at the Keck Observatory, VIMOS and FORS2 at the Very Large Telescope, we assembled a unique sample of 53 main-sequence star-forming galaxies at 4.4
KW - galaxies: ISM
KW - galaxies: high-redshift
KW - submillimeter: galaxies
KW - LYMAN BREAK GALAXIES
KW - LY-ALPHA RADIATION
KW - STAR-FORMING GALAXIES
KW - C II
KW - ULTRAVIOLET-SPECTRA
KW - PHYSICAL-PROPERTIES
KW - REDSHIFT EVOLUTION
KW - ESCAPE FRACTION
KW - COSMOS FIELD
KW - DUST CONTENT
U2 - 10.1051/0004-6361/202037517
DO - 10.1051/0004-6361/202037517
M3 - Journal article
VL - 643
JO - Astronomy & Astrophysics
JF - Astronomy & Astrophysics
SN - 0004-6361
M1 - A6
ER -
