F
Fabian Walter
Researcher at Max Planck Society
Publications - 1053
Citations - 92179
Fabian Walter is an academic researcher from Max Planck Society. The author has contributed to research in topics: Galaxy & Star formation. The author has an hindex of 146, co-authored 999 publications receiving 83016 citations. Previous affiliations of Fabian Walter include California Institute of Technology & University of Bonn.
Papers
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Journal ArticleDOI
Star Formation and ISM Properties in the Host Galaxies of Three Far-infrared Luminous Quasars at z ∼ 6
Yali Shao,Ran Wang,Chris Carilli,Chris Carilli,Jeff Wagg,Fabian Walter,Fabian Walter,Fabian Walter,Jianan Li,Xiaohui Fan,Linhua Jiang,Dominik Riechers,Frank Bertoldi,Michael A. Strauss,Pierre Cox,A. Omont,Karl M. Menten +16 more
TL;DR: In this article, the CO (2-1) line emission of the Atacama Large Millimeter/submillimeter Array (Atacama Array) has been used to estimate the molecular gas masses of the three high-redshift quasars.
Journal ArticleDOI
The Turbulent Gas Structure in the Centers of NGC 253 and the Milky Way
Nico Krieger,Alberto D. Bolatto,Eric W. Koch,Adam K. Leroy,Erik Rosolowsky,Fabian Walter,Axel Weiß,David Eden,Rebecca C. Levy,David S. Meier,Elisabeth A. C. Mills,Toby J. T. Moore,Jürgen Ott,Yang Su,Sylvain Veilleux +14 more
TL;DR: In this paper, the authors compare molecular gas properties in the starbursting center of NGC253 and the Milky Way Galactic Center (GC) on scales of ~1-100 pc using dendograms and resolution-, area and noise-matched datasets in CO (1-0) and CO (3-2).
Journal ArticleDOI
Random Forests as a Viable Method to Select and Discover High-redshift Quasars
Lukas Wenzl,Jan-Torge Schindler,Xiaohui Fan,Irham Taufik Andika,Eduardo Bañados,Roberto Decarli,Knud Jahnke,Chiara Mazzucchelli,Masafusa Onoue,Bram Venemans,Fabian Walter,Jinyi Yang +11 more
TL;DR: In this article, a method of selecting quasars up to redshift approx 6 with random forests is presented. But this method is limited to the region around z = 5.5.
Journal ArticleDOI
A Comparison of the Stellar, CO and Dust-Continuum Emission from Three, Star-Forming HUDF Galaxies at $z\sim 2$
Melanie Kaasinen,Fabian Walter,Mladen Novak,Marcel Neeleman,Ian Smail,Leindert Boogaard,Elisabete da Cunha,Axel Weiss,Daizhong Liu,Roberto Decarli,Gergö Popping,Tanio Díaz-Santos,Paulo C. Cortes,Manuel Aravena,Paul van der Werf,Dominik Riechers,Hanae Inami,Jacqueline Hodge,Hans-Walter Rix,Pierre Cox +19 more
TL;DR: In this article, the authors compare the extent of the dust, molecular gas and stars in three star-forming galaxies, selected from the Hubble Ultra Deep Field based on their bright CO and dust-continuum emission as well as their large rest-frame optical sizes.
Posted Content
Key Science Goals for the Next Generation Very Large Array (ngVLA): Report from the ngVLA Science Advisory Council
Alberto D. Bolatto,Shami Chatterjee,Caitlin M. Casey,Laura Chomiuk,Imke de Pater,Mark Dickinson,James Di Francesco,Gregg Hallinan,Andrea Isella,Kotaro Kohno,Shrinivas R. Kulkarni,Cornelia C. Lang,T. Joseph W. Lazio,Adam K. Leroy,Laurent Loinard,Thomas J. Maccarone,Brenda C. Matthews,Rachel A. Osten,Mark J. Reid,Dominik Riechers,Nami Sakai,Fabian Walter,David J. Wilner +22 more
TL;DR: The Next Generation Very Large Array (ngVLA) as mentioned in this paper is the next generation very large array (NGVLA), which will have roughly 10 times the collecting area of the Jansky VLA, operate at frequencies from 1 GHz to 116 GHz with up to 20 GHz of bandwidth, and possess a compact core for high surface-brightness sensitivity.