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dc.contributor.authorMarchi, F
dc.contributor.authorPentericci, L
dc.contributor.authorGuaita, L
dc.contributor.authorRibeiro, B
dc.contributor.authorCastellano, M
dc.contributor.authorSchaerer, D
dc.contributor.authorHathi, NP
dc.contributor.authorLemaux, BC
dc.contributor.authorGrazian, A
dc.contributor.authorLe Fèvre, O
dc.contributor.authorGarilli, B
dc.contributor.authorMaccagni, D
dc.contributor.authorAmorin, R
dc.contributor.authorBardelli, S
dc.contributor.authorCassata, P
dc.contributor.authorFontana, A
dc.contributor.authorKoekemoer, AM
dc.contributor.authorLe Brun, V
dc.contributor.authorTasca, LAM
dc.contributor.authorThomas, R
dc.contributor.authorVanzella, E
dc.contributor.authorZamorani, G
dc.contributor.authorZucca, E
dc.date.accessioned2017-04-05T11:04:40Z
dc.date.available2017-04-05T11:04:40Z
dc.date.issued2017
dc.identifier.issn0004-6361
dc.identifier.urihttps://www.repository.cam.ac.uk/handle/1810/263473
dc.description.abstractDetermining the average fraction of Lyman continuum (LyC) photons escaping high redshift galaxies is essential for understanding how reionization proceeded in the z>6 Universe. We want to measure the LyC signal from a sample of sources in the Chandra Deep Field South (CDFS) and COSMOS fields for which ultra-deep VIMOS spectroscopy as well as multi-wavelength Hubble Space Telescope (HST) imaging are available. We select a sample of 46 galaxies at $z\sim 4$ from the VIMOS Ultra Deep Survey (VUDS) database, such that the VUDS spectra contain the LyC part of the spectra, that is, the rest-frame range $880-910\AA$. Taking advantage of the HST imaging, we apply a careful cleaning procedure and reject all the sources showing nearby clumps with different colours, that could potentially be lower-redshift interlopers. After this procedure, the sample is reduced to 33 galaxies. We measure the ratio between ionizing flux (LyC at $895\AA$) and non-ionizing emission (at $\sim 1500 \AA$) for all individual sources. We also produce a normalized stacked spectrum of all sources. Assuming an intrinsic average $L_{\nu}(1470)/L_{\nu}(895)$ of 3, we estimate the individual and average relative escape fraction. We do not detect ionizing radiation from any individual source, although we identify a possible LyC emitter with very high Ly$\alpha$ equivalent width (EW). From the stacked spectrum and assuming a mean transmissivity for the sample, we measure a relative escape fraction $f_{esc}^{rel}=0.09\pm0.04$. We also look for correlations between the limits in the LyC flux and source properties and find a tentative correlation between LyC flux and the EW of the Ly$\alpha$ emission line. Our results imply that the LyC flux emitted by $V=25-26$ star-forming galaxies at z$\sim$4 is at most very modest, in agreement with previous upper limits from studies based on broad and narrow band imaging.
dc.description.sponsorshipThis work is supported by funding from the European Research Council Advanced Grant ERC–2010–AdG–268107–EARLY and by INAF Grants PRIN 2010, PRIN 2012 and PICS 2013. AC, OC, MT and VS acknowledge the grant MIUR PRIN 2010– 2011. This work is based on data products made available at the CESAM data center, Laboratoire d’Astrophysique de Marseille. R.A. acknowledges support from the ERC Advanced Grant 695671 'QUENCH'.
dc.languageEnglish
dc.language.isoen
dc.publisherEDP Sciences
dc.titleNew constraints on the average escape fraction of Lyman continuum radiation in z ∼ 4 galaxies from the VIMOS Ultra Deep Survey (VUDS)
dc.typeArticle
prism.publicationDate2017
prism.publicationNameAstronomy and Astrophysics
prism.volume601
dc.identifier.doi10.17863/CAM.8817
dcterms.dateAccepted2016-12-23
rioxxterms.versionofrecord10.1051/0004-6361/201630054
rioxxterms.versionVoR
rioxxterms.licenseref.urihttp://www.rioxx.net/licenses/all-rights-reserved
rioxxterms.licenseref.startdate2017-05-01
dc.contributor.orcidAmorin Barbieri, Ricardo [0000-0001-5758-1000]
dc.identifier.eissn1432-0746
rioxxterms.typeJournal Article/Review
pubs.funder-project-idEuropean Research Council (695671)
cam.issuedOnline2017-05-04


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