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
ALMA Spectroscopic Survey in the Hubble Ultra Deep Field: Survey Description
Fabian Walter,Fabian Walter,Fabian Walter,Roberto Decarli,Manuel Aravena,Chris Carilli,Chris Carilli,Rychard Bouwens,Elisabete da Cunha,Elisabete da Cunha,Emanuele Daddi,Rob Ivison,Rob Ivison,Dominik Riechers,Ian Smail,Mark Swinbank,Axel Weiss,Timo Anguita,Timo Anguita,Roberto J. Assef,Roland Bacon,Franz E. Bauer,Franz E. Bauer,Franz E. Bauer,Eric F. Bell,Frank Bertoldi,Scott Chapman,Luis Colina,Paulo C. Cortes,Pierre Cox,Mark Dickinson,David Elbaz,Jorge González-López,Edo Ibar,Hanae Inami,Leopoldo Infante,Jacqueline Hodge,Alex Karim,Olivier Le Fevre,Benjamin Magnelli,Roberto Neri,Pascal Oesch,Kazuaki Ota,Gergö Popping,Hans-Walter Rix,Mark Sargent,Kartik Sheth,Arjen van der Wel,Paul van der Werf,Jeff Wagg +49 more
TL;DR: In this paper, the authors present the rationale for and the observational description of ASPECS: The ALMA SPECtroscopic Survey in the Hubble Ultra-Deep Field (UDF), the cosmological deep field that has the deepest multi-wavelength data available.
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Young Stars in the Outer HI Disc of NGC 6822
W. J. G. de Blok,Fabian Walter +1 more
TL;DR: In this paper, a wide-field optical imaging covering the entire neutral hydrogen disc of the Local Group dwarf galaxy NGC 6822 is presented, revealing the presence of numerous blue, young stars at large galactocentric radii well beyond R_25.
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Empirical predictions for (SUB-)millimeter line and continuum deep fields
Elisabete da Cunha,Fabian Walter,Roberto Decarli,Frank Bertoldi,Chris Carilli,Emanuele Daddi,David Elbaz,Rob Ivison,Rob Ivison,Roberto Maiolino,Dominik A. Riechers,Dominik A. Riechers,Hans-Walter Rix,Mark Sargent,Ian Smail,Axel Weiss +15 more
TL;DR: In this paper, a physically motivated spectral energy distribution model is used to fit the observed optical/near-infrared emission of 13,099 galaxies with redshifts up to z = 5, and obtain median-likelihood estimates of their stellar mass, star formation rate, dust attenuation, and dust luminosity.
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The Kinematics of z ~ 6 Quasar Host Galaxies
Marcel Neeleman,Mladen Novak,Bram Venemans,Fabian Walter,Fabian Walter,Roberto Decarli,Melanie Kaasinen,Jan-Torge Schindler,Eduardo Bañados,Chris Carilli,Alyssa B. Drake,Xiaohui Fan,Hans-Walter Rix +12 more
TL;DR: In this paper, the kinematics of 27 z~6 quasar host galaxies observed in [CII]-158 micron emission with the Atacama Large Millimeter/sub-millimeter Array at a resolution of ~025'' were explored.
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Clumping and the Interpretation of kpc-Scale Maps of the Interstellar Medium: Smooth HI and Clumpy, Variable H2 Surface Density
Adam K. Leroy,Cheoljong Lee,Andreas Schruba,Alberto D. Bolatto,Annie Hughes,Jérôme Pety,Karin Sandstrom,Eva Schinnerer,Fabian Walter +8 more
TL;DR: In this paper, high spatial resolution (sub-kpc) maps of CO and HI emission from nearby galaxies were used to measure the clumping factor of both atomic and molecular gas.