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The Lyman Continuum Escape Fraction of Low-Mass Star-Forming Galaxies at z~1

, , , , , , , , , , , , and . (2015)cite arxiv:1511.01998Comment: submitted for second review to ApJ.

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Detection of HI in Emission in the Lyman Alpha Emitting Galaxy Haro 11, , , , and . (2016)cite arxiv:1609.04020Comment: 9 pages, 7 figures, accepted in AJ.On the influence of physical galaxy properties on Lyman-alpha escape in star-forming galaxies, , , , , , , and . (2013)cite arxiv:1308.6577Comment: 17 pages. Accepted for publication.The Lyman alpha Reference Sample: Extended Lyman alpha Halos Produced at Low Dust Content, , , , , , , , , and 7 other author(s). (2013)cite arxiv:1303.0006Comment: Published in ApJ Letters ~~ 6 pages using emulateapj, 4 figures ~~ Higher-resolution, larger, nicer jpeg versions of Figures 1 and 2 can be found here: http://xayes.org/pub/press_lars.html.Exploitation of Quasi-Orthogonal Space Time Block Codes in Virtual Antenna Arrays: Part I - Theoretical Capacity and throughput Gains., , , and . VTC Spring, page 349-352. IEEE, (2008)Detecting large deletions at base pair level by combining split read and paired read data., and . BMC Bioinform., 18 (S-12): 107-113 (2017)A single-carrier quasi-orthogonal transmission scheme for asynchronous cooperative relay networks., , and . EUSIPCO, page 125-129. IEEE, (2009)The Synchrony of Production & Escape: Half the Bright Ly$\alpha$ Emitters at $z\approx2$ have Lyman Continuum Escape Fractions $\approx50\%$, , , , , , , , , and 7 other author(s). (2021)cite arxiv:2110.11961Comment: Submitted to MNRAS. Figure 4 and Table 2 show key results from the stacks. Figure 8 presents a unifying scheme for the LyC duty cycle. Our companion paper (Matthee & Naidu et al. 2021) works out implications of these results for the cosmic UV background at $z\approx2-8$. Comments warmly welcomed and greatly appreciated!.(Re)Solving Reionization with Ly\alpha: How Bright Ly\alpha Emitters account for the $z\approx2-8$ Cosmic Ionizing Background, , , , , , , , , and 5 other author(s). (2021)cite arxiv:2110.11967Comment: Submitted to MNRAS. Figure 2 shows the main result -- the comoving emissivity due to bright LAEs. Our fiducial model is based on results presented in our companion paper -- Naidu & Matthee et al. 2021. Comments welcome.Spectro-polarimetry confirms central powering of a Ly$\alpha$ nebula at z=3.09, , , , and . (2016)cite arxiv:1601.06786Comment: 11 pages, 7 figures, accepted for publication in ApJ.The Lyman Continuum Escape and ISM properties in Tololo 1247-232 - New Insights from HST and VLA, , , , , , , , , and . (2017)cite arxiv:1704.05943.