The VIMOS Ultra-Deep Survey: the Ly$\alpha$ emission line morphology at $2 < z < 6$

B. Ribeiro; O. Le Fèvre; A. Paulino-Afonso; P. Cassata; V. Le Brun; B. C. Lemaux; D. Maccagni; L. Pentericci; R. Thomas; G. Zamorani; E. Zucca; R. Amorín; S. Bardelli; L. P. Cassarà; L. Guaita; N. P. Hathi; A. Koekemoer; D. Schaerer; M. Talia; J. Pforr; L. Tresse; S. Fotopoulou; D. Vergani

The VIMOS Ultra-Deep Survey: the Ly$\alpha$ emission line morphology at $2 < z < 6$

B. Ribeiro, O. Le Fèvre, A. Paulino-Afonso, P. Cassata, V. Le Brun, B. C. Lemaux, D. Maccagni, L. Pentericci, R. Thomas, G. Zamorani, E. Zucca, R. Amorín, S. Bardelli, L. P. Cassarà, L. Guaita, N. P. Hathi, A. Koekemoer, D. Schaerer, M. Talia, J. PforrL. Tresse, S. Fotopoulou, D. Vergani

School of Physics

Research output: Working paper

Abstract

The Lyman-$\alpha$ (Ly$\alpha$) emission line has been ubiquitously used to confirm and study high redshift galaxies. We report on the line morphology as seen in the 2D spectra from the VIMOS Ultra Deep Survey in a sample of 914 Ly$\alpha$ emitters from a parent sample of 4192 star-forming galaxies at $2

Original language	Undefined/Unknown
Publication status	Published - Jul 2020

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Ribeiro, B., Le Fèvre, O., Paulino-Afonso, A., Cassata, P., Le Brun, V., Lemaux, B. C., Maccagni, D., Pentericci, L., Thomas, R., Zamorani, G., Zucca, E., Amorín, R., Bardelli, S., Cassarà, L. P., Guaita, L., Hathi, N. P., Koekemoer, A., Schaerer, D., Talia, M., ... Vergani, D. (2020). The VIMOS Ultra-Deep Survey: the Ly$\alpha$ emission line morphology at $2 < z < 6$.

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title = "The VIMOS Ultra-Deep Survey: the Ly$\alpha$ emission line morphology at $2 < z < 6$",

abstract = "The Lyman-$\alpha$ (Ly$\alpha$) emission line has been ubiquitously used to confirm and study high redshift galaxies. We report on the line morphology as seen in the 2D spectra from the VIMOS Ultra Deep Survey in a sample of 914 Ly$\alpha$ emitters from a parent sample of 4192 star-forming galaxies at $2",

author = "B. Ribeiro and {Le F{\`e}vre}, O. and A. Paulino-Afonso and P. Cassata and {Le Brun}, V. and Lemaux, {B. C.} and D. Maccagni and L. Pentericci and R. Thomas and G. Zamorani and E. Zucca and R. Amor{\'i}n and S. Bardelli and Cassar{\`a}, {L. P.} and L. Guaita and Hathi, {N. P.} and A. Koekemoer and D. Schaerer and M. Talia and J. Pforr and L. Tresse and S. Fotopoulou and D. Vergani",

year = "2020",

month = jul,

language = "Undefined/Unknown",

type = "WorkingPaper",

}

Ribeiro, B, Le Fèvre, O, Paulino-Afonso, A, Cassata, P, Le Brun, V, Lemaux, BC, Maccagni, D, Pentericci, L, Thomas, R, Zamorani, G, Zucca, E, Amorín, R, Bardelli, S, Cassarà, LP, Guaita, L, Hathi, NP, Koekemoer, A, Schaerer, D, Talia, M, Pforr, J, Tresse, L, Fotopoulou, S & Vergani, D 2020 'The VIMOS Ultra-Deep Survey: the Ly$\alpha$ emission line morphology at $2 < z < 6$'.

TY - UNPB

T1 - The VIMOS Ultra-Deep Survey: the Ly$\alpha$ emission line morphology at $2 < z < 6$

AU - Ribeiro, B.

AU - Le Fèvre, O.

AU - Paulino-Afonso, A.

AU - Cassata, P.

AU - Le Brun, V.

AU - Lemaux, B. C.

AU - Maccagni, D.

AU - Pentericci, L.

AU - Thomas, R.

AU - Zamorani, G.

AU - Zucca, E.

AU - Amorín, R.

AU - Bardelli, S.

AU - Cassarà, L. P.

AU - Guaita, L.

AU - Hathi, N. P.

AU - Koekemoer, A.

AU - Schaerer, D.

AU - Talia, M.

AU - Pforr, J.

AU - Tresse, L.

AU - Fotopoulou, S.

AU - Vergani, D.

PY - 2020/7

Y1 - 2020/7

N2 - The Lyman-$\alpha$ (Ly$\alpha$) emission line has been ubiquitously used to confirm and study high redshift galaxies. We report on the line morphology as seen in the 2D spectra from the VIMOS Ultra Deep Survey in a sample of 914 Ly$\alpha$ emitters from a parent sample of 4192 star-forming galaxies at $2

AB - The Lyman-$\alpha$ (Ly$\alpha$) emission line has been ubiquitously used to confirm and study high redshift galaxies. We report on the line morphology as seen in the 2D spectra from the VIMOS Ultra Deep Survey in a sample of 914 Ly$\alpha$ emitters from a parent sample of 4192 star-forming galaxies at $2

M3 - Working paper

BT - The VIMOS Ultra-Deep Survey: the Ly$\alpha$ emission line morphology at $2 < z < 6$

ER -