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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Journal ArticleDOI
Forming Super Star Clusters in the Central Starburst of NGC 253
Adam K. Leroy,Alberto D. Bolatto,Eve C. Ostriker,Fabian Walter,Mark Gorski,Adam Ginsburg,Nico Krieger,David S. Meier,Elisabeth A. C. Mills,Juergen Ott,Erik Rosolowsky,Todd A. Thompson,Sylvain Veilleux,Laura K. Zschaechner +13 more
TL;DR: In this article, the authors used ALMA to image the 350 GHz dust continuum and molecular line emission from NGC 253 at 2-3 pc FWHM resolution, showing that gas still constitutes a large fraction of the overall mass in these sources.
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The Enigmatic Radio Afterglow of GRB 991216
Dale A. Frail,Edo Berger,Titus Galama,Shrinivas R. Kulkarni,Gerald H. Moriarty-Schieven,Guy G. Pooley,Re'em Sari,Debra Shepherd,G. B. Taylor,Fabian Walter +9 more
TL;DR: In this article, the authors present wide-band radio observations spanning from 1.4 GHz to 350 GHz of the afterglow of GRB 991216, taken from 1 to 80 days after the burst.
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The first high-redshift quasar from Pan-STARRS
E. Morganson,Gisella De Rosa,Roberto Decarli,Fabian Walter,K. C. Chambers,Ian D. McGreer,Xiaohui Fan,W. S. Burgett,H. Flewelling,Jochen Greiner,Klaus W. Hodapp,Nick Kaiser,Eugene A. Magnier,Paul A. Price,Hans-Walter Rix,Bill Sweeney,Christopher Waters +16 more
TL;DR: The first high-redshift (z > 5.7) quasar from the Panoramic Survey Telescope and Rapid Response System 1 (Pan-STARRS1 or PS1) was discovered in this article.
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Bright [CII] 158$\mu$m emission in a quasar host galaxy at $z=6.54$
TL;DR: In this paper, the authors reported a strong detection of the [CII] line in the host galaxy of the brightest quasar known at $z>6.0498 (hereafter P036+03), using the IRAM NOEMA millimeter interferometer.
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Dynamical Characterization of Galaxies at z~4-6 via Tilted Ring Fitting to ALMA [CII] Observations
G. C. Jones,Chris Carilli,Y. Shao,Ran Wang,Peter Capak,Riccardo Pavesi,Dominik Riechers,Alexander Karim,Marcel Neeleman,Fabian Walter +9 more
TL;DR: In this article, the authors used a procedure centered around GIPSY's ROTCUR task to fit tilted ring models to some of the best available ALMA [CII] data of a small set of galaxies: the MS galaxies HZ9 & HZ10, the Damped Lyman-alpha Absorber (DLA) host galaxy ALMA J0817+1351, the submm galaxies AzTEC/C159 and COSMOS J1000+0234, and the quasar host galaxy ULAS J1319+09