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The Luminosity Function at z~8 from 97 Y-band dropouts: Inferences About Reionization

, , , , , , , , and . (2014)cite arxiv:1402.4129Comment: Re-submitted to ApJ after first positive referee report, 22 pages, 15 figures.

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The Grism lens-amplified survey from space (GLASS). VIII. The influence of the cluster properties on Halpha emitter galaxies at 0.3<z<0.7, , , , , , , , , and 6 other author(s). (2016)cite arxiv:1610.04615Comment: submitted to ApJ (17 pages, 10 figures).The Luminosity Function at z~8 from 97 Y-band dropouts: Inferences About Reionization, , , , , , , , and . (2014)cite arxiv:1402.4129Comment: Re-submitted to ApJ after first positive referee report, 22 pages, 15 figures.Primordial star clusters at extreme magnification, , , , , , and . (2014)cite arxiv:1411.6628Comment: 8 pages, 3 figures. Submitted to MNRAS. Comments are welcome.Connecting Faint End Slopes of the Lyman-$\alpha$ emitter and Lyman-break Galaxy Luminosity Functions, , , and . (2015)cite arxiv:1502.00022Comment: 8 pages, 6 figures, submitted to MNRAS (after revision following referee's report).RELICS-DP7: Spectroscopic Confirmation of a Dichromatic Primeval Galaxy at z ~ 7, , , , , , , , , and 5 other author(s). (2020)cite arxiv:2011.08857Comment: 8 pages, 3 figures, 1 table. Submitted to ApJL.A Physical Model for the Quasar Luminosity Function Evolution between Cosmic Dawn and High Noon, and . (2021)cite arxiv:2110.03853Comment: 13 pages, 4 figures; accepted for publication in ApJ; data products available at https://github.com/renkeven/QuasarEvolutionData.Early results from GLASS-JWST. III: Galaxy candidates at z$\sim$9-15, , , , , , , , , and 19 other author(s). (2022)cite arxiv:2207.09436Comment: Submitted to ApJL, 9 pages, 4 figures.Early Results from GLASS-JWST. I: Confirmation of Lensed $z\geqslant7$ Lyman-Break Galaxies Behind the Abell 2744 Cluster With NIRISS, , , , , , , , , and 22 other author(s). (2022)cite arxiv:2207.11387Comment: Submitted to ApJL. 10 pages, 3 figures, 1 table.Small-scale Intensity Mapping: Extended Ly$\alpha$, H$\alpha$ and Continuum emission as a Probe of Halo Star Formation in High-redshift Galaxies, , , , , and . (2017)cite arxiv:1703.02593Comment: 13 pages, 6 figures, submitted to ApJ.The Impact of Scatter in the Galaxy UV Luminosity to Halo Mass Relation on Ly$\alpha$ Visibility During the Epoch of Reionization, , , , , , , and . (2019)cite arxiv:1911.03499Comment: 12 pages, 7 figures, submitted to MNRAS.