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20062026
most cited3D Lyman-alpha radiation transfer. I. Understanding Lyman-alpha line profile morphologies

492 citations · 8.5k across the 124 of their papers we have counts for

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Showing 2017Show all

13 papers · 1 filter

astro-ph.GA2017★ 53 cited

On the Origin of Diffuse Ionized Gas in the Antennae Galaxy

Peter M. Weilbacher, Ana Monreal-Ibero, Anne Verhamme +14

The "Antennae Galaxy" (NGC 4038/39) is the closest major interacting galaxy system and therefore often taken as merger prototype. We present the first comprehensive integral field…

astro-ph.GA2017★ 246 cited

J1154+2443: a low-redshift compact star-forming galaxy with a 46 per cent leakage of Lyman continuum photons

Y. I. Izotov, D. Schaerer, G. Worseck +5

We report the detection of the Lyman continuum (LyC) radiation of the compact star-forming galaxy (SFG) J1154+2443 observed with the Cosmic Origins Spectrograph (COS) onboard the H…

astro-ph.GA2017★ 80 cited

The MUSE Hubble Ultra Deep Field Survey X. Ly Equivalent Widths at

Takuya Hashimoto, Thibault Garel, Bruno Guiderdoni +17

We present rest-frame Ly equivalent widths (EW) of 417 Ly emitters (LAEs) detected with Multi Unit Spectroscopic Explorer (MUSE) on the Very Large Telescope (VLT) at $2.9 < z…

astro-ph.GA2017★ 45 cited

The MUSE-Wide survey: A measurement of the Ly emitting fraction among galaxies

Joseph Caruana, Lutz Wisotzki, Edmund Christian Herenz +15

We present a measurement of the fraction of Lyman (Ly) emitters () amongst HST continuum-selected galaxies at with the Multi-Unit Spectroscopic Explor…

astro-ph.GA2017★ 72 cited

The MUSE Hubble Ultra Deep Field Survey VIII : Extended Lyman-alpha haloes around high-redshift star-forming galaxies

Floriane Leclercq, Roland Bacon, Lutz Wisotzki +17

We report the detection of extended Lyman-alpha (Lya) haloes around 145 individual star-forming galaxies at redshifts 3<z<6 in the Hubble Ultra Deep Field observed with the Multi-U…

astro-ph.GA2017★ 37 cited

The MUSE Hubble Ultra Deep Field Survey: VII. FeII* Emission in Star-Forming Galaxies

Hayley Finley, Nicolas Bouché, Thierry Contini +15

Non-resonant FeII* 2365, 2396, 2612, 2626 emission can potentially trace galactic winds in emission and provide useful constraints to wind models. From the 3'x3' mosaic of the Hubb…