Autor der Publikation

Massive quenched galaxies at z~0.7 retain large molecular gas reservoirs

, , , , , , , und . (2017)cite arxiv:1708.03337Comment: Accepted for publication in ApJ Letters (6 pages, 5 figures).

Bitte wählen Sie eine Person um die Publikation zuzuordnen

Um zwischen Personen mit demselben Namen zu unterscheiden, wird der akademische Grad und der Titel einer wichtigen Publikation angezeigt. Zudem lassen sich über den Button neben dem Namen einige der Person bereits zugeordnete Publikationen anzeigen.

 

Weitere Publikationen von Autoren mit dem selben Namen

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.The MOSDEF Survey: The strong agreement between H-alpha and UV-to-FIR star formation rates for z~2 star-forming galaxies, , , , , , , , , und 5 andere Autor(en). (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, , , , , , , , , und 6 andere Autor(en). (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/.The MOSDEF Survey: Dissecting the star-formation rate vs. stellar mass relation using H$\alpha$ and H$\beta$ emission lines at z ~ 2, , , , , , , , , und 2 andere Autor(en). (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, , , , , , , , , und 5 andere Autor(en). (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, , , , , , , , , 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.The MOSDEF Survey: Detection of OIII$łambda$4363 and the direct-method oxygen abundance of a star-forming galaxy at z=3.08, , , , , , , , , und 1 andere Autor(en). (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, , , , , und . (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, , , , , , , und . (2017)cite arxiv:1708.03337Comment: Accepted for publication in ApJ Letters (6 pages, 5 figures).The JWST UNCOVER Treasury survey: Ultradeep NIRSpec and NIRCam ObserVations before the Epoch of Reionization, , , , , , , , , und 24 andere Autor(en). (2022)cite arxiv:2212.04026Comment: 17 pages, 8 figures, 4 tables, submitted to ApJ, comments welcome.