( en | de | ru )

 

Disambiguation of "Walter, Fabian"

Author of the publication

copydeleteadd this publication to your clipboard
Dust-to-Gas Ratio in the Extremely Metal Poor Galaxy I ZW 18

, , , , , , , , , and . (2012)cite arxiv:1204.4745Comment: Accepted for publication in ApJ: 8 pages, 4 figures, 1 table.

Please choose a person to relate this publication to

To differ between persons with the same name, the academic degree and the title of an important publication will be displayed. You can also use the button next to the name to display some publications already assigned to the person.

Walter Fabian

Walter Fabian

Fabian Walter

Fabian Walter

Fabian Walter

 

Other publications of authors with the same name

ALMA spectroscopic survey in the Hubble Ultra Deep Field: CO luminosity functions and the evolution of the cosmic density of molecular gas, , , , , , , , , and 30 other author(s). (2016)cite arxiv:1607.06770Comment: Submitted to the Astrophysical Journal, incorporating the first round of referee comments.ALMA Spectroscopic Survey in the Hubble Ultra Deep Field: The Infrared Excess of UV-selected z=2-10 galaxies as a function of UV-continuum Slope and Stellar Mass, , , , , , , , , and 18 other author(s). (2016)cite arxiv:1606.05280Comment: 31 pages, 16 figures, 13 tables, incorporating the first feedback from the referee on our submitted ApJ manuscript, paper VI of the ASPECS (ALMA Spectroscopic Survey in the Hubble Ultra Deep Field) series.Mg II Absorption at 2<z<7 with Magellan/FIRE, III. Full Statistics of Absorption Towards 100 High-Redshift QSOs, , , , , , , , , and 5 other author(s). (2016)cite arxiv:1612.02829Comment: 23 Pages, 17 figures, submitted to ApJ.An ALMA survey of Sub-millimeter Galaxies in the Extended Chandra Deep Field South: Physical properties derived from ultraviolet-to-radio modelling, , , , , , , , , and 8 other author(s). (2015)cite arxiv:1504.04376Comment: 22 pages, 14 figures, 2 tables. Accepted for publication in the Astrophysical Journal. The new MAGPHYS model libraries used in this paper will appear in www.iap.fr/magphys. The SMG SED templates shown in Section 6.1 are available at http://astronomy.swinburne.edu.au/~ecunha/ecunha/SED_Templates.html.Hydrogen reionisation ends by $z=5.3$: Lyman-$\alpha$ optical depth measured by the XQR-30 sample, , , , , , , , , and 15 other author(s). (2021)cite arxiv:2108.03699Comment: Submitted to MNRAS. 22 pages, 17 figures.ALMA 200 pc imaging of a z~7 quasar reveals a compact, disk-like host galaxy, , , , , , , , , and 3 other author(s). (2022)cite arxiv:2201.06396Comment: Accepted for publication in The Astrophysical Journal.Tracing Cold HI Gas in Nearby, Low-Mass Galaxies, , , , , , , , and . (2012)cite arxiv:1208.0983Comment: 44 pages, 13 figures, Accepted for publication in ApJ.Dust continuum emission as a tracer of gas mass in galaxies, , , , , , , , , and 1 other author(s). (2014)cite arxiv:1411.2975Comment: Accepted for publication in ApJ.ALMA resolves turbulent, rotating CII emission in a young starburst galaxy at z=4.8, , , , , , , , , and 2 other author(s). (2014)cite arxiv:1404.2295Comment: Accepted for publication in A&A.The LBT Bootes Field Survey: I. The Rest-frame UV and Luminosity Functions and Clustering of Bright Lyman Break Galaxies at z~3, , , , , , , , , and . (2013)cite arxiv:1307.4835Comment: 23 pages and 17 figures, Accepted by ApJ.