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Evidence for feedback in action from the molecular gas content in the z~1.6 outflowing QSO XID2028

, , , , , , , , , , , , , , , , , , and . (2015)cite arxiv:1503.01783Comment: 8 pages, 4 figures. Astronomy and Astrophysics, in press.

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The dust mass function from z~0 to z~2, , , , , and . (2019)cite arxiv:1909.11333Comment: MNRAS in press, 12 pages, 6 pages.A low escape fraction of ionizing photons of L&gt;L* Lyman break galaxies at z=3.3, , , , , , , , , and 5 other author(s). (2011)cite arxiv:1104.5237 Comment: 15 pages, 2 figures, 1 table, accepted for publication in ApJ.Evidence for feedback in action from the molecular gas content in the z~1.6 outflowing QSO XID2028, , , , , , , , , and 9 other author(s). (2015)cite arxiv:1503.01783Comment: 8 pages, 4 figures. Astronomy and Astrophysics, in press.The assembly of "normal" galaxies at z=7 probed by ALMA, , , , , , , , , and 5 other author(s). (2015)cite arxiv:1502.06634Comment: 13 pages, 8 figures, 3 tables, submitted to MNRAS.Early Results From GLASS-JWST. XII: The Morphology of Galaxies at the Epoch of ReionizationY, , , , , , , , , and 16 other author(s). (2022)cite arxiv:2207.13527Comment: 15 pages, 4 figures, submitted to ApJL.Early results from GLASS-JWST. V: the first rest-frame optical size-luminosity relation of galaxies at $z>7$, , , , , , , , , and 16 other author(s). (2022)cite arxiv:2207.13101Comment: Submitted to ApJL, 9 pages, 3 figures, 2 tables.Early results from GLASS-JWST. X: Rest-frame UV-optical properties of galaxies at 7 < z < 9, , , , , , , , , and 16 other author(s). (2022)cite arxiv:2207.11135Comment: Submitted to ApJL. 12 pages, 3 Figures.Early results from GLASS-JWST. XI: Stellar masses and mass-to-light ratio of z>7 galaxies, , , , , , , , , and 19 other author(s). (2022)cite arxiv:2207.11379Comment: Submitted to ApJL.Closing in on the sources of cosmic reionization: first results from the GLASS-JWST program, , , , , , , , , and 22 other author(s). (2023)cite arxiv:2301.02816Comment: submitted to A&A, 11 pages, 8 figures.ALMA and Herschel reveal that AGN and main-sequence galaxies have different star formation rate distributions, , , , , , , , , and 8 other author(s). (2015)cite arxiv:1506.05459Comment: 5 pages, 3 figures, 1 table; Submitted to MNRAS.