A young star-forming galaxy at z = 3.5 with an extended Ly\,$α$ halo seen with MUSE

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

Standard

A young star-forming galaxy at z = 3.5 with an extended Ly\,$α$ halo seen with MUSE. / Patrício, Vera; Richard, Johan; Verhamme, Anne; Wisotzki, Lutz; Brinchmann, Jarle; Turner, Monica L.; Christensen, Lise Bech; Weilbacher, Peter M.; Blaizot, Jérémy; Bacon, Roland; Contini, Thierry; Lagattuta, David; Cantalupo, Sebastiano; Clément, Benjamin; Soucail, Geneviève.

In: Monthly Notices of the Royal Astronomical Society, Vol. 456, No. 4, 14.01.2016, p. 4191-4208.

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

Harvard

Patrício, V, Richard, J, Verhamme, A, Wisotzki, L, Brinchmann, J, Turner, ML, Christensen, LB, Weilbacher, PM, Blaizot, J, Bacon, R, Contini, T, Lagattuta, D, Cantalupo, S, Clément, B & Soucail, G 2016, 'A young star-forming galaxy at z = 3.5 with an extended Ly\,$α$ halo seen with MUSE', Monthly Notices of the Royal Astronomical Society, vol. 456, no. 4, pp. 4191-4208. https://doi.org/10.1093/mnras/stv2859

APA

Patrício, V., Richard, J., Verhamme, A., Wisotzki, L., Brinchmann, J., Turner, M. L., Christensen, L. B., Weilbacher, P. M., Blaizot, J., Bacon, R., Contini, T., Lagattuta, D., Cantalupo, S., Clément, B., & Soucail, G. (2016). A young star-forming galaxy at z = 3.5 with an extended Ly\,$α$ halo seen with MUSE. Monthly Notices of the Royal Astronomical Society, 456(4), 4191-4208. https://doi.org/10.1093/mnras/stv2859

Vancouver

Patrício V, Richard J, Verhamme A, Wisotzki L, Brinchmann J, Turner ML et al. A young star-forming galaxy at z = 3.5 with an extended Ly\,$α$ halo seen with MUSE. Monthly Notices of the Royal Astronomical Society. 2016 Jan 14;456(4):4191-4208. https://doi.org/10.1093/mnras/stv2859

Author

Patrício, Vera ; Richard, Johan ; Verhamme, Anne ; Wisotzki, Lutz ; Brinchmann, Jarle ; Turner, Monica L. ; Christensen, Lise Bech ; Weilbacher, Peter M. ; Blaizot, Jérémy ; Bacon, Roland ; Contini, Thierry ; Lagattuta, David ; Cantalupo, Sebastiano ; Clément, Benjamin ; Soucail, Geneviève. / A young star-forming galaxy at z = 3.5 with an extended Ly\,$α$ halo seen with MUSE. In: Monthly Notices of the Royal Astronomical Society. 2016 ; Vol. 456, No. 4. pp. 4191-4208.

Bibtex

@article{b7cf8605749243bab30078a5a8486076,
title = "A young star-forming galaxy at z = 3.5 with an extended Ly\,$α$ halo seen with MUSE",
abstract = "Spatially resolved studies of high redshift galaxies, an essential insight into galaxy formation processes, have been mostly limited to stacking or unusually bright objects. We present here the study of a typical (L$^{*}$, M$_\star$ = 6 $\times 10^9$ $M_\odot$) young lensed galaxy at $z=3.5$, observed with MUSE, for which we obtain 2D resolved spatial information of Ly$\alpha$ and, for the first time, of CIII] emission. The exceptional signal-to-noise of the data reveals UV emission and absorption lines rarely seen at these redshifts, allowing us to derive important physical properties (T$_e\sim$15600 K, n$_e\sim$300 cm$^{-3}$, covering fraction f$_c\sim0.4$) using multiple diagnostics. Inferred stellar and gas-phase metallicities point towards a low metallicity object (Z$_{\mathrm{stellar}}$ = $\sim$ 0.07 Z$_\odot$ and Z$_{\mathrm{ISM}}$ $",
keywords = "astro-ph.GA",
author = "Vera Patr{\'i}cio and Johan Richard and Anne Verhamme and Lutz Wisotzki and Jarle Brinchmann and Turner, {Monica L.} and Christensen, {Lise Bech} and Weilbacher, {Peter M.} and J{\'e}r{\'e}my Blaizot and Roland Bacon and Thierry Contini and David Lagattuta and Sebastiano Cantalupo and Benjamin Cl{\'e}ment and Genevi{\`e}ve Soucail",
note = "19 pages, 15 figures, accepted in MNRAS",
year = "2016",
month = jan,
day = "14",
doi = "10.1093/mnras/stv2859",
language = "English",
volume = "456",
pages = "4191--4208",
journal = "Royal Astronomical Society. Monthly Notices",
issn = "0035-8711",
publisher = "Oxford University Press",
number = "4",

}

RIS

TY - JOUR

T1 - A young star-forming galaxy at z = 3.5 with an extended Ly\,$α$ halo seen with MUSE

AU - Patrício, Vera

AU - Richard, Johan

AU - Verhamme, Anne

AU - Wisotzki, Lutz

AU - Brinchmann, Jarle

AU - Turner, Monica L.

AU - Christensen, Lise Bech

AU - Weilbacher, Peter M.

AU - Blaizot, Jérémy

AU - Bacon, Roland

AU - Contini, Thierry

AU - Lagattuta, David

AU - Cantalupo, Sebastiano

AU - Clément, Benjamin

AU - Soucail, Geneviève

N1 - 19 pages, 15 figures, accepted in MNRAS

PY - 2016/1/14

Y1 - 2016/1/14

N2 - Spatially resolved studies of high redshift galaxies, an essential insight into galaxy formation processes, have been mostly limited to stacking or unusually bright objects. We present here the study of a typical (L$^{*}$, M$_\star$ = 6 $\times 10^9$ $M_\odot$) young lensed galaxy at $z=3.5$, observed with MUSE, for which we obtain 2D resolved spatial information of Ly$\alpha$ and, for the first time, of CIII] emission. The exceptional signal-to-noise of the data reveals UV emission and absorption lines rarely seen at these redshifts, allowing us to derive important physical properties (T$_e\sim$15600 K, n$_e\sim$300 cm$^{-3}$, covering fraction f$_c\sim0.4$) using multiple diagnostics. Inferred stellar and gas-phase metallicities point towards a low metallicity object (Z$_{\mathrm{stellar}}$ = $\sim$ 0.07 Z$_\odot$ and Z$_{\mathrm{ISM}}$ $

AB - Spatially resolved studies of high redshift galaxies, an essential insight into galaxy formation processes, have been mostly limited to stacking or unusually bright objects. We present here the study of a typical (L$^{*}$, M$_\star$ = 6 $\times 10^9$ $M_\odot$) young lensed galaxy at $z=3.5$, observed with MUSE, for which we obtain 2D resolved spatial information of Ly$\alpha$ and, for the first time, of CIII] emission. The exceptional signal-to-noise of the data reveals UV emission and absorption lines rarely seen at these redshifts, allowing us to derive important physical properties (T$_e\sim$15600 K, n$_e\sim$300 cm$^{-3}$, covering fraction f$_c\sim0.4$) using multiple diagnostics. Inferred stellar and gas-phase metallicities point towards a low metallicity object (Z$_{\mathrm{stellar}}$ = $\sim$ 0.07 Z$_\odot$ and Z$_{\mathrm{ISM}}$ $

KW - astro-ph.GA

U2 - 10.1093/mnras/stv2859

DO - 10.1093/mnras/stv2859

M3 - Journal article

VL - 456

SP - 4191

EP - 4208

JO - Royal Astronomical Society. Monthly Notices

JF - Royal Astronomical Society. Monthly Notices

SN - 0035-8711

IS - 4

ER -

ID: 166599894