M
Michael W. Werner
Researcher at California Institute of Technology
Publications - 394
Citations - 25116
Michael W. Werner is an academic researcher from California Institute of Technology. The author has contributed to research in topics: Galaxy & Spitzer Space Telescope. The author has an hindex of 76, co-authored 392 publications receiving 23814 citations. Previous affiliations of Michael W. Werner include Ames Research Center & W.M. Keck Observatory.
Papers
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Journal ArticleDOI
10 Micron Imaging of Seyfert Galaxies from the 12 Micron Sample
TL;DR: In this paper, small-aperature photometry and new high-resolution images at 10 mu (N band) for 87 Seyfert galaxies from the Extended 12 mu Sample drawn from the IRASX database were presented.
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Herschel-resolved outer belts of two-belt debris disks around a-type stars: hd 70313, hd 71722, hd 159492, and f-type: hd 104860*
TL;DR: In this article, a dual-band Herschel/Photodetector Array Camera and Spectrometer imaging for four stars whose spectral energy distributions suggest two-ring disk architectures that mirror that of the asteroid-Kuiper Belt geometry of our own solar system was presented.
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Simultaneous far-infrared, near-infrared, and radio observations of OH/IR stars
TL;DR: In this paper, a comparison of the far-infrared and maser emission from these sources, which strongly supports the hypothesis that the maser emissions are pumped by 35 micron photons, was made.
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The Compact Nucleus of the Deep Silicate Absorption Galaxy NGC 4418
Aaron S. Evans,Eric E. Becklin,N. Z. Scoville,G. Neugebauer,B. T. Soifer,Keith Matthews,Michael E. Ressler,Michael W. Werner,Marcia J. Rieke +8 more
TL;DR: In this paper, high-resolution Hubble Space Telescope (HST) and Keck mid-infrared images of the heavily extinguished infrared-luminous galaxy NGC 4418 are presented.
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The far-infrared/submillimeter properties of galaxies located behind the Bullet cluster
Marie Rex,T. D. Rawle,Eiichi Egami,Pablo G. Pérez-González,Pablo G. Pérez-González,Michael Zemcov,Michael Zemcov,Itziar Aretxaga,Sun Mi Chung,Dario Fadda,Anthony H. Gonzalez,David H. Hughes,Cathy Horellou,Daniel Johansson,Jean-Paul Kneib,Johan Richard,Bruno Altieri,A. K. Fiedler,M. J. Pereira,George H. Rieke,Ian Smail,Ivan Valtchanov,Andrew Blain,James J. Bock,James J. Bock,Frédéric Boone,Carrie Bridge,Benjamin Clément,Francoise Combes,C. D. Dowell,C. D. Dowell,Miroslava Dessauges-Zavadsky,Olivier Ilbert,Rob Ivison,Rob Ivison,Mathilde Jauzac,Dieter Lutz,Alain Omont,R. Pello,Giulia Rodighiero,Daniel Schaerer,Daniel Schaerer,Graham P. Smith,Gregory Walth,P. van der Werf,Michael W. Werner,Jason E. Austermann,Hajime Ezawa,Ryohei Kawabe,Kotaro Kohno,Thushara Perera,Kimberly S. Scott,Grant W. Wilson,M. S. Yun +53 more
TL;DR: In this article, the spectral energy distributions of 19 MIPS 24 μm-selected galaxies which are located behind the Bullet cluster (1E0657-56) were obtained from the Herschel Lensing Survey (HLS).