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Disambiguation of "Kriek, Mariska"

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Halpha Equivalent Widths from the 3D-HST survey: evolution with redshift and dependence on stellar mass

, , , , , , , , , , , , , , and . (2012)cite arxiv:1206.2645Comment: Submitted to The Astrophysical Journal Letters.

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Mariska Schönrock

Charilaos Kriekoukis

Frans Martinus Krieken

Mariska Kappmeier

Mariska Ott

 

Other publications of authors with the same name

The MOSDEF Survey: The strong agreement between H-alpha and UV-to-FIR star formation rates for z~2 star-forming galaxies, , , , , , , , , and 5 other author(s). (2016)cite arxiv:1603.02284Comment: 7 pages, 5 figures, to be published in ApJ Letters.The Formation of Massive, Compact Galaxies at z=2 in the Illustris Simulation, , , , , , , , , and 6 other author(s). (2014)cite arxiv:1411.0667Comment: 11 pages, 9 figures. Submitted to MNRAS, comments welcome. The official Illustris website can be found at http://www.illustris-project.org/.Quiescent Galaxies in the 3D-HST Survey: Spectroscopic Confirmation of a Large Number of Galaxies with Relatively Old Stellar Populations at z~2, , , , , , , , , and 3 other author(s). (2013)cite arxiv:1305.1943Comment: 6 pages, 4 figures, resubmitted to the Astrophysical Journal Letters after minor revisions.The MOSDEF Survey: Dissecting the star-formation rate vs. stellar mass relation using H$\alpha$ and H$\beta$ emission lines at z ~ 2, , , , , , , , , and 2 other author(s). (2015)cite arxiv:1507.03017Comment: 12 pages, 8 figures, 2 tables, submitted to ApJ.Direct measurement of dust attenuation in z~1.5 star-forming galaxies from 3D-HST: Implications for dust geometry and star formation rates, , , , , , , , , and 5 other author(s). (2013)cite arxiv:1310.4177Comment: Submitted for publication in the Astrophysical Journal.Where stars form: inside-out growth and coherent star formation from HST Halpha maps of 2676 galaxies across the main sequence at z~1, , , , , , , , , and 10 other author(s). (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.The MOSDEF Survey: Detection of OIII$łambda$4363 and the direct-method oxygen abundance of a star-forming galaxy at z=3.08, , , , , , , , , and 1 other author(s). (2016)cite arxiv:1606.04107Comment: 7 pages, 3 figures, 1 table, submitted to ApJ Letters.Halpha and 4000 Angstrom Break Measurements for ~3500 K-selected Galaxies at 0.5<z<2.0, , , , , and . (2011)cite arxiv:1103.0279 Comment: Submitted to ApJ, high-resolution version can be downloaded at https://www.cfa.harvard.edu/~mkriek/papers/.Massive quenched galaxies at z~0.7 retain large molecular gas reservoirs, , , , , , , and . (2017)cite arxiv:1708.03337Comment: Accepted for publication in ApJ Letters (6 pages, 5 figures).The number density and mass density of star-forming and quiescent galaxies at 0.4 < z < 2.2, , , , , , , , , and 2 other author(s). (2011)cite arxiv:1104.2595 Comment: Submitted to the Astrophysical Journal. The release of EAZY v2.0 will accompany the publication of the manuscript in the journal.