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Disambiguation of "Maseda, M."

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The Grism Lens-Amplified Survey from Space (GLASS). III. A census of Ly\alpha\ Emission at $z\gtrsim$7 from HST Spectroscopy

, , , , , , , , , , , , , , , , , and . (2015)cite arxiv:1511.04205Comment: Accepted for publication in ApJ, 23 pages, 11 figures, 6 tables.

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Damian Maseda Caballero

Michael Vincent Maseda

Simon M M Laimer

M. Biswas M. Dam

Bernhard M M Lang

 

Other publications of authors with the same name

The MUSE-Wide Survey: A first catalogue of 831 emission line galaxies, , , , , , , , , and 4 other author(s). (2017)cite arxiv:1705.08215Comment: 24 pages, 14 figures, accepted for publication in A&A, data products are available for download from http://muse-vlt.eu/science/muse-wide-survey/ and later via the CDS.Evidence of very low metallicity and high ionization state in a strongly lensed, star-forming dwarf galaxy at z=3.417, , , , , , , , and . (2014)cite arxiv:1403.6470Comment: 5 pages, 3 figures and 1 table. Accepted for publication in ApJ Letters.The Grism Lens-Amplified Survey from Space (GLASS). III. A census of Ly\alpha\ Emission at $z\gtrsim$7 from HST Spectroscopy, , , , , , , , , and 8 other author(s). (2015)cite arxiv:1511.04205Comment: Accepted for publication in ApJ, 23 pages, 11 figures, 6 tables.The MUSE Hubble Ultra Deep Field Survey: III. Testing photometric redshifts to 30th magnitude, , , , , , , , , and 7 other author(s). (2017)cite arxiv:1710.05062Comment: 24 pages and 25 figures, accepted for A&A.Equivalent widths of Lyman $\alpha$ emitters in MUSE-Wide and MUSE-Deep, , , , , , , , , and 8 other author(s). (2022)cite arxiv:2202.06642Comment: 28 pages, 21 + 1 figures, 7 + 1 tables, accepted for publication in A&A.Very low-luminosity galaxies in the early universe have observed sizes similar to single star cluster complexes, , , , , , and . (2017)cite arxiv:1711.02090Comment: 23 pages, 14 figures, 4 tables, submitted to the Astrophysical Journal, Figures 9 and 10 show comparisons with the sizes and luminosities of local star cluster complexes and evolved objects, respectively, Figure 11 presents our constraints on the z~6 proto-globular cluster LF.The MUSE-Wide survey: Three-dimensional clustering analysis of Lyman-$\alpha$ emitters at $3.3<z<6$, , , , , , , , , and 5 other author(s). (2021)cite arxiv:2107.03723Comment: Accepted for publication in A&A. 22 pages, 20 figures, 4 tables.The VLT LEGA-C Spectroscopic Survey: The Physics of Galaxies at a Lookback Time of 7 Gyr, , , , , , , , , and 10 other author(s). (2016)cite arxiv:1603.05479Comment: Accepted for publication in ApJS - LEGA-C website: http://www.mpia.de/home/legac/index.html.The chemical enrichment in the early Universe as probed by JWST via direct metallicity measurements at z~8, , , , , , , , , and 22 other author(s). (2022)cite arxiv:2207.12375Comment: 13 pages, 7 figures.