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Disambiguation of "Belli, Sirio"

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KMOS-3D Reveals Low-Level Star Formation Activity in Massive Quiescent Galaxies at 0.7 < z < 2.7

, , , , , , , , , , , , , , , , , , , , , , , , , and . (2017)cite arxiv:1703.07778Comment: 7 pages, 5 figures, submitted to ApJ Letters.

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Fevzi Belli

Renan Belli

Eduard Belli

Fevzi Belli

Fevzi Belli

 

Other publications of authors with the same name

The evolution of metallicity and metallicity gradients from z=2.7-0.6 with KMOS3D, , , , , , , , , and 21 other author(s). (2016)cite arxiv:1603.01139Comment: submitted to ApJ.Bulge-forming galaxies with an extended rotating disk at z~2, , , , , , , , , and 17 other author(s). (2016)cite arxiv:1608.05412Comment: 10 pages, 5 figures, 2 tables, submitted to ApJ.Lyman-alpha and CIII Emission in z=7-9 Galaxies: Accelerated Reionization Around Luminous Star Forming Systems?, , , , , , , , , and 2 other author(s). (2016)cite arxiv:1606.01304Comment: Submitted to MNRAS, 13 pages, 8 figures.Lyman-alpha Emission from a Luminous z=8.68 Galaxy: Implications for Galaxies as Tracers of Cosmic Reionization, , , , , , , , and . (2015)cite arxiv:1507.02679Comment: ApJL Submitted; 6 pages, 4 figures, 1 table.Testing the Universality of the Fundamental Metallicity Relation at High Redshift Using Low-Mass Gravitationally Lensed Galaxies, , , and . (2013)cite arxiv:1302.3614Comment: Submitted to ApJ, 14 pages, 8 figures.The Evolution and Origin of Ionized Gas Velocity Dispersion from $z\sim2.6$ to $z\sim0.6$ with KMOS$^3D$, , , , , , , , , and 20 other author(s). (2019)cite arxiv:1906.02737Comment: ~30 pages, 16 figures, 9 tables; accepted for publication in ApJ.Schrodinger's Galaxy Candidate: Puzzlingly Luminous at $z\approx17$, or Dusty/Quenched at $z\approx5$?, , , , , , , , , and 15 other author(s). (2022)cite arxiv:2208.02794Comment: Submitted to ApJL. Fig. 1 shows the "superposed" state, Fig. 2 presents the potential z~5 protocluster, Fig. 3 shows some atypical z~5 SEDs, Fig. 4 studies the morphology, Fig. 5 summarizes the extraordinary situation at z~17, and Fig. 6 argues for why such interlopers may not be a major issue for z>10 searches. Comments warmly welcomed.KMOS-3D Reveals Low-Level Star Formation Activity in Massive Quiescent Galaxies at 0.7 < z < 2.7, , , , , , , , , and 16 other author(s). (2017)cite arxiv:1703.07778Comment: 7 pages, 5 figures, submitted to ApJ Letters.MOSFIRE Absorption Line Spectroscopy of z > 2 Quiescent Galaxies: Probing a Period of Rapid Size Growth, , , and . (2014)cite arxiv:1404.4872Comment: 6 pages, 4 figures. Submitted to ApJ Letters.A Pilot Survey for CIII Emission in the Reionization Era: Gravitationally-Lensed z$\sim7-8$ Galaxies in the Frontier Fields Cluster Abell 2744, , , and . (2015)cite arxiv:1504.07686Comment: 7 pages, 4 figures, 1 table; accepted for publication in ApJ Letters.