G
G. Neugebauer
Researcher at University of Arizona
Publications - 387
Citations - 24341
G. Neugebauer is an academic researcher from University of Arizona. The author has contributed to research in topics: Galaxy & Quasar. The author has an hindex of 73, co-authored 387 publications receiving 23703 citations. Previous affiliations of G. Neugebauer include Jet Propulsion Laboratory & University of Hawaii.
Papers
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Journal ArticleDOI
High Spatial Resolution Imaging of NGC 1068 in the Mid-Infrared
James J. Bock,James J. Bock,G. Neugebauer,Keith Matthews,B. T. Soifer,E. E. Becklin,Michael E. Ressler,K. A. Marsh,Michael W. Werner,E. Egami,Roger Blandford +10 more
TL;DR: In this paper, mid-infrared observations of the central source of NGC 1068 have been obtained with a spatial resolution in the deconvolved image of 0.1 pc.
Journal ArticleDOI
Absolute Calibration and Characterization of the Multiband Imaging Photometer for Spitzer. III. An Asteroid‐based Calibration of MIPS at 160 μm
John Stansberry,Karl D. Gordon,Bidushi Bhattacharya,Charles W. Engelbracht,George H. Rieke,Francine R. Marleau,Dario Fadda,Dave Frayer,Alberto Noriega-Crespo,Stefanie Wachter,Erick T. Young,Thomas G. Müller,D. M. Kelly,Myra Blaylock,David A. Henderson,G. Neugebauer,Jeffrey W. Beeman,Eugene E. Haller,Eugene E. Haller +18 more
TL;DR: In this paper, the authors describe the absolute calibration of the MIPS 160 μm channel and derive a calibration factor of 41.7 MJy sr^(−1) MIPS160 + 1 (MIPS160 being the instrumental units).
Journal ArticleDOI
High Spatial Resolution Imaging of NGC 1068 in the Mid Infrared
J. J. Bock,G. Neugebauer,Keith Matthews,B. T. Soifer,E.E. Becklin M. Ressler,K. A. Marsh,Michael Werner,Eiichi Egami,Roger Blandford +8 more
TL;DR: In this paper, mid-infrared observations of the central source of NGC 1068 have been obtained with a spatial resolution in the deconvolved image of 0.1" (~ 7pc).
Journal ArticleDOI
Iras observations of the diffuse infrared background
M. G. Hauser,F. C. Gillett,F. J. Low,T. N. Gautier,Ca Beichman,G. Neugebauer,H. H. Aumann,B. Baud,N. W. Boggess,J. P. Emerson,[No Value] Houck,B. T. Soifer,R. L. Walker +12 more
TL;DR: In this article, the IRAS data reveal bright emission from interplanetary dust which dominates the celestial background at 12, 25, and 60 microns except near the galactic plane.