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Disambiguierung von "Franx, Marijn"

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Is the evidence for a variable initial mass function from ATLAS3D robust?

, , und . (2014)cite arxiv:1406.0854Comment: 12 pages, 10 figures.

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Marijn Huijbregts

Marijn Van Putten

Eefke Marijn van der Lee

 

Weitere Publikationen von Autoren mit dem selben Namen

Elevated ionizing photon production efficiency in faint high-equivalent-width Lyman-alpha emitters, , , , , , , , , und 9 andere Autor(en). (2020)cite arxiv:2002.11117Comment: 12 Pages, 6 Figures; Accepted for publication in MNRAS.Quiescent Galaxies in the 3D-HST Survey: Spectroscopic Confirmation of a Large Number of Galaxies with Relatively Old Stellar Populations at z~2, , , , , , , , , und 3 andere Autor(en). (2013)cite arxiv:1305.1943Comment: 6 pages, 4 figures, resubmitted to the Astrophysical Journal Letters after minor revisions.Direct measurement of dust attenuation in z~1.5 star-forming galaxies from 3D-HST: Implications for dust geometry and star formation rates, , , , , , , , , und 5 andere Autor(en). (2013)cite arxiv:1310.4177Comment: Submitted for publication in the Astrophysical Journal.Confirmation of Small Dynamical and Stellar Masses for Extreme Emission Line Galaxies at z~2, , , , , , , , , und 14 andere Autor(en). (2013)cite arxiv:1310.6358Comment: Accepted for publication in ApJL, 5 pages, 1 table, 4 figures.A 10 deg$^2$ Lyman-$\alpha$ survey at z=8.8 with spectroscopic follow-up: strong constraints on the LF and implications for other surveys, , , , , , , , und . (2014)cite arxiv:1402.6697Comment: 15 pages, 9 figures, accepted for publication in MNRAS.Where stars form: inside-out growth and coherent star formation from HST Halpha maps of 2676 galaxies across the main sequence at z~1, , , , , , , , , und 10 andere Autor(en). (2015)cite arxiv:1507.03999Comment: Submitted to ApJ. Main results: Fig. 6 shows the scale lengths of ionized gas vs. stellar disks. Fig. 9 shows where Halpha in galaxies is enhanced above and suppressed below the star-forming main sequence. Data points for Halpha profiles are available upon request.Simulating and interpreting deep JWST/NIRSpec observations in the Hubble Ultra Deep Field, , , , , , , , , und 9 andere Autor(en). (2017)cite arxiv:1711.07481Comment: 20 pages, 14 figures, submitted to MNRAS.Spatially-resolved dust maps from Balmer decrements in galaxies at z~1.4, , , , , , , , und . (2015)cite arxiv:1511.04443Comment: Submitted to ApJ Letters. Fig. 2. shows measured radial Balmer decrement profiles. Fig. 3 shows inferred dust gradients. Fig. 4 shows dust-corrected radial profiles of star formation and the likely growth of bulges in high mass galaxies through in-situ star formation.Halpha and 4000 Angstrom Break Measurements for ~3500 K-selected Galaxies at 0.5<z<2.0, , , , , und . (2011)cite arxiv:1103.0279 Comment: Submitted to ApJ, high-resolution version can be downloaded at https://www.cfa.harvard.edu/~mkriek/papers/.The Star-formation Mass Sequence out to z=2.5, , , und . (2012)cite arxiv:1205.0547Comment: Submitted to the Astrophysical Journal Letters, 6 pages, 5 figures. NMBS IR+UV SFRs are now available at http://www.astro.yale.edu/nmbs/Data_Products.html.