We present a measurement of the fraction of Lyman $\alpha$ (Ly$\alpha$)
emitters ($X_Ly \alpha$) amongst HST continuum-selected galaxies at
$3<z<6$ with the Multi-Unit Spectroscopic Explorer (MUSE) on the VLT. Making
use of the first 24 MUSE-Wide pointings in GOODS-South, each having an
integration time of 1 hour, we detect 100 Ly$\alpha$ emitters and find
$X_Ly \alpha\gtrsim0.5$ for most of the redshift range covered, with 29%
of the Ly$\alpha$ sample exhibiting rest equivalent widths (rest-EWs) $łeq$
15\AA. Adopting a range of rest-EW cuts (0 - 75\AA), we find no evidence of a
dependence of $X_Ly \alpha$ on either redshift or UV luminosity.
Description
[1709.00991] The MUSE-Wide survey: A measurement of the Ly$\alpha$ emitting fraction among $z>3$ galaxies
%0 Generic
%1 caruana2017musewide
%A Caruana, Joseph
%A Wisotzki, Lutz
%A Herenz, Edmund Christian
%A Kerutt, Josephine
%A Urrutia, Tanya
%A Schmidt, Kasper Borello
%A Bouwens, Rychard
%A Brinchmann, Jarle
%A Cantalupo, Sebastiano
%A Carollo, Marcella
%A Diener, Catrina
%A Drake, Alyssa
%A Garel, Thibault
%A Marino, Raffaella Anna
%A Richard, Johan
%A Saust, Rikke
%A Schaye, Joop
%A Verhamme, Anne
%D 2017
%K Lya MUSE emitting fraction
%T The MUSE-Wide survey: A measurement of the Ly$\alpha$ emitting fraction
among $z>3$ galaxies
%U http://arxiv.org/abs/1709.00991
%X We present a measurement of the fraction of Lyman $\alpha$ (Ly$\alpha$)
emitters ($X_Ly \alpha$) amongst HST continuum-selected galaxies at
$3<z<6$ with the Multi-Unit Spectroscopic Explorer (MUSE) on the VLT. Making
use of the first 24 MUSE-Wide pointings in GOODS-South, each having an
integration time of 1 hour, we detect 100 Ly$\alpha$ emitters and find
$X_Ly \alpha\gtrsim0.5$ for most of the redshift range covered, with 29%
of the Ly$\alpha$ sample exhibiting rest equivalent widths (rest-EWs) $łeq$
15\AA. Adopting a range of rest-EW cuts (0 - 75\AA), we find no evidence of a
dependence of $X_Ly \alpha$ on either redshift or UV luminosity.
@misc{caruana2017musewide,
abstract = {We present a measurement of the fraction of Lyman $\alpha$ (Ly$\alpha$)
emitters ($X_{\rm{Ly} \alpha}$) amongst HST continuum-selected galaxies at
$3<z<6$ with the Multi-Unit Spectroscopic Explorer (MUSE) on the VLT. Making
use of the first 24 MUSE-Wide pointings in GOODS-South, each having an
integration time of 1 hour, we detect 100 Ly$\alpha$ emitters and find
$X_{\rm{Ly} \alpha}\gtrsim0.5$ for most of the redshift range covered, with 29%
of the Ly$\alpha$ sample exhibiting rest equivalent widths (rest-EWs) $\leq$
15\AA. Adopting a range of rest-EW cuts (0 - 75\AA), we find no evidence of a
dependence of $X_{\rm{Ly} \alpha}$ on either redshift or UV luminosity.},
added-at = {2017-09-05T11:38:27.000+0200},
author = {Caruana, Joseph and Wisotzki, Lutz and Herenz, Edmund Christian and Kerutt, Josephine and Urrutia, Tanya and Schmidt, Kasper Borello and Bouwens, Rychard and Brinchmann, Jarle and Cantalupo, Sebastiano and Carollo, Marcella and Diener, Catrina and Drake, Alyssa and Garel, Thibault and Marino, Raffaella Anna and Richard, Johan and Saust, Rikke and Schaye, Joop and Verhamme, Anne},
biburl = {https://www.bibsonomy.org/bibtex/2f082748867e2e9f9a625fc786194ce96/miki},
description = {[1709.00991] The MUSE-Wide survey: A measurement of the Ly$\alpha$ emitting fraction among $z>3$ galaxies},
interhash = {c2041ecdc0fb976b64048cd1bb414111},
intrahash = {f082748867e2e9f9a625fc786194ce96},
keywords = {Lya MUSE emitting fraction},
note = {cite arxiv:1709.00991Comment: 10 pages, 5 figures},
timestamp = {2017-09-05T11:38:27.000+0200},
title = {The MUSE-Wide survey: A measurement of the Ly$\alpha$ emitting fraction
among $z>3$ galaxies},
url = {http://arxiv.org/abs/1709.00991},
year = 2017
}