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.
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Science with an ngVLA: Imaging Cold Gas to 1 kpc Scales in High-Redshift Galaxies with the ngVLA
Caitlin M. Casey,Desika Narayanan,Chris Carilli,Jaclyn B. Champagne,Chao-Ling Hung,Romeel Davé,Roberto Decarli,Eric J. Murphy,Gergö Popping,Dominik Riechers,Rachel S. Somerville,Fabian Walter +11 more
TL;DR: In this article, the authors employ a series of high-resolution, cosmological, hydrodynamic zoom simulations from the MUFASA simulation suite and a CASA simulator to generate mock very large array (ngVLA) observations of a gas rich star-forming galaxy.
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Scaling Relations between Gas and Star Formation in Nearby Galaxies
TL;DR: In this paper, high-resolution multi-wavelength maps of a sizeable set of nearby galaxies have made it possible to study how the surface densities of HI, H2 and star formation rate relate on scales of a few hundred parsecs.
Journal Article
APEX CO (3-2) Observations of NGC 6822
S. De Rijcke,Pieter Buyle,John M. Cannon,Fabian Walter,A. Lundgren,D. Michelsen,Herwig Dejonghe +6 more
TL;DR: In this paper, the authors used a simple LTE model to estimate the mass of the Hubble V region and the H$_2/I/I_{/rm CO(3\\rightarrow 2)}$ conversion factor.
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Star Formation in Quasar Host Galaxies at Redshift 6: Millimeter Surveys and New Insights from ALMA
Ran Wang,Ran Wang,Jeff Wagg,Chris Carilli,Fabian Walter,Xiaohui Fan,Frank Bertoldi,Dominik A. Riechers,Alain Omont,Karl M. Menten,Pierre Cox,Michael A. Strauss,Desika Narayanan +12 more
TL;DR: In this article, the authors carried out a systematic survey of the star formation and ISM properties in the host galaxies of z~6 quasars using ALMA observations and available data from the literature.
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High Sensitivity Array Observations of the $z = 4.4$ QSO BRI 1335-0417
TL;DR: In this article, a phase-referenced VLBI image at the high sensitivity array (HSA) was used to detect radio continuum emission from BRI 1335--0417 at 1.4 GHz.