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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A Chandra X-ray survey of nearby dwarf starburst galaxies - I. Data reduction and results
TL;DR: In this article, Chandra X-ray observations of a sample of eight dwarf starburst galaxies (IZw18, VIIZw403, NGC1569 and NGC3077) were analyzed.
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The Ionized Gas in Nearby Galaxies as Traced by the [NII] 122 and 205 \mu m Transitions
Rodrigo Herrera-Camus,A. D. Bolatto,J. D. T. Smith,Bruce T. Draine,Eric W. Pellegrini,Mark Wolfire,K. V. Croxall,I. De Looze,D. Calzetti,Robert C. Kennicutt,A. Crocker,L. Armus,P. van der Werf,Karin Sandstrom,M. Galametz,Bernhard R. Brandl,Brent Groves,D. Rigopoulou,Fabian Walter,Adam K. Leroy,M. Boquien,Fatemeh Tabatabaei,P. Beirao +22 more
TL;DR: In this paper, the authors derived relations between the [NII] emission and SFR in the low-density limit and in the case of a log-normal distribution of densities.
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Modeling Dust and Starlight in Galaxies Observed by Spitzer and Herschel: The KINGFISH Sample
G. Aniano,G. Aniano,B. T. Draine,Leslie K. Hunt,Karin Sandstrom,Daniela Calzetti,R. C. Kennicutt,R. C. Kennicutt,Daniel A. Dale,Maud Galametz,Karl D. Gordon,Adam K. Leroy,J. D. T. Smith,Helene Roussel,Marc Sauvage,Fabian Walter,Lee Armus,Alberto D. Bolatto,Médéric Boquien,Alison F. Crocker,I. De Looze,I. De Looze,J. Donovan Meyer,George Helou,J. Hinz,Benjamin D. Johnson,Jin Koda,Adam Miller,Adam Miller,E. Montiel,E. Montiel,Eric J. Murphy,M. Relaño,H.-W. Rix,Eva Schinnerer,Ramin A. Skibba,Mark G. Wolfire,Charles W. Engelbracht +37 more
TL;DR: In this paper, the authors used a physical dust model to estimate the surface density, polycyclic aromatic hydrocarbons (PAHs), distribution of starlight intensities heating the dust, and total infrared (IR) luminosity emitted by the dust.
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Interferometric Detections of GOODS 850-5 at 1 mm and 1.4 GHz*
TL;DR: In this article, the authors obtained a position (at subarcsecond accuracy) of the submillimeter bright source GOODS 850-5 (also known as GN 10) in the GOODS-North field using the IRAM Plateau de Bure interferometer at 1.25 mm wavelengths.
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Complete infrared spectral energy distributions of millimeter detected quasars at z > 5
C. Leipski,Klaus Meisenheimer,Fabian Walter,M.-A. Besel,Helmut Dannerbauer,Xiaohui Fan,M. Haas,Ulrich Klaas,Oliver Krause,H. W. Rix +9 more
TL;DR: In this article, the authors performed spectral energy distribution (SED) fits over the wavelength range λrest ~ 0.1-400 μm for those objects with good Herschel detections.