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Disambiguation of "Calura, F."

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Paving the way for the JWST: witnessing globular cluster formation at z>3

, , , , , , , , , , , , , , , , , , , and . (2016)cite arxiv:1612.01526Comment: 19 pages, 9 figures, 2 tables. Submitted to MNRAS. Comments welcome.

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-F Garcia

F Arndt

F Röpke

F Schmidt

F Himmel

 

Other publications of authors with the same name

Exploring the Thermal State of the Low-Density Intergalactic Medium at z=3 with an Ultra-High Signal-to-Noise QSO Spectrum, , , , , , , , , and 4 other author(s). (2016)cite arxiv:1611.03805Comment: Accepted for publication on MNRAS.Ionising the Intergalactic Medium by Star Clusters ? The first empirical evidence, , , , , , , , , and 7 other author(s). (2019)cite arxiv:1904.07941Comment: 9 pages, 6 figures and 1 table, submitted to MNRAS. Comments welcome.Paving the way for the JWST: witnessing globular cluster formation at z>3, , , , , , , , , and 10 other author(s). (2016)cite arxiv:1612.01526Comment: 19 pages, 9 figures, 2 tables. Submitted to MNRAS. Comments welcome.Chemical evolution models: GRB host identification and cosmic dust predictions, , , , , and . (2014)cite arxiv:1407.6905Comment: 15 pages, 10 figures, accepted for publication in MNRAS.Direct Lyman continuum and Lyman-alpha escape observed at redshift 4, , , , , , , , , and 9 other author(s). (2017)cite arxiv:1712.07661Comment: 5 pages, 4 figures, 1 table, Submitted to MNRAS, Comments Welcome.Metals in the z~3 intergalactic medium: results from an ultra-high signal-to-noise ratio UVES quasar spectrum, , , , , , , , , and 6 other author(s). (2016)cite arxiv:1608.06116Comment: 23 pages, 28 figures. Submitted to MNRAS (revised version after first referee report).A fast and accurate method to compute the mass return from multiple stellar populations, , and . (2013)cite arxiv:1312.1090Comment: 8 pages, 4 figures, submitted, comments welcome.High-resolution spectroscopy at the faintest limits: an "ELT-like" spectrum of a young optically-thin L=0.02L* star-forming galaxy at z=3.12, , , , , , , , , and 22 other author(s). (2016)cite arxiv:1603.01616Comment: 7 pages, 4 figures and 1 table; ApJL submitted.Candidate Population III stellar complex at z=6.629 in the MUSE Deep Lensed Field, , , , , , , , , and 13 other author(s). (2020)cite arxiv:2001.03619Comment: 4 pages, 3 figures and 1 table. Submitted. Comments welcome.The dust mass function from z~0 to z~2, , , , , and . (2019)cite arxiv:1909.11333Comment: MNRAS in press, 12 pages, 6 pages.