K
Karl D. Gordon
Researcher at Space Telescope Science Institute
Publications - 619
Citations - 55985
Karl D. Gordon is an academic researcher from Space Telescope Science Institute. The author has contributed to research in topics: Galaxy & Star formation. The author has an hindex of 115, co-authored 599 publications receiving 51952 citations. Previous affiliations of Karl D. Gordon include University of Arizona & Commonwealth Scientific and Industrial Research Organisation.
Papers
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Journal ArticleDOI
Techniques and Review of Absolute Flux Calibration from the Ultraviolet to the Mid-Infrared
TL;DR: In this paper, the spectral energy distributions (SEDs) of redshifted Ia supernovae in the rest frame are compared to the CALSPEC reference standard spectrophotometry.
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Spatially Resolved Ultraviolet, H-alpha, Infrared, and Radio Star Formation in M81
Karl D. Gordon,Pablo G. Pérez-González,Karl Misselt,Eric J. Murphy,George J. Bendo,Fabian Walter,Michele D. Thornley,Robert C. Kennicutt,George H. Rieke,C. W. Engelbracht,Jd Smith,A. Alonso-Herrero,P. N. Appleton,D. Calzetti,Daniel A. Dale,Bruce T. Draine,Dave Frayer,George Helou,Joannah L. Hinz,Dean C. Hines,D. M. Kelly,J. E. Morrison,James Muzerolle,Michael W. Regan,J. A. Stansberry,Susan R. Stolovy,Lisa J. Storrie-Lombardi,Kate Y. L. Su,Erick T. Young +28 more
TL;DR: In this article, multiband imaging photometer for Spitzer (MIPS) observations of M81 at 24, 70, and 160 micron were used to investigate the variation of the ultraviolet (UV), H-alpha, and infrared (IR) luminosities and star formation rate (SFR) indicators across the face of a galaxy.
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The excitation of extended red emission: new constraints on its carrier from hst observations of ngc 7023 1
TL;DR: In this article, the authors used the imaging capabilities of the Hubble Space Telescope to constrain the character of the ERE carrier further by determining the wavelengths of the radiation that initia tes the extended red emission (ERE) in many dusty interstellar environments.
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A detailed study of the radio-FIR correlation in NGC 6946 with Herschel-PACS/SPIRE from KINGFISH
Fatemeh Tabatabaei,Eva Schinnerer,Eric J. Murphy,Rainer Beck,Brent Groves,Sharon E. Meidt,Marita Krause,H. W. Rix,Karin Sandstrom,Alison F. Crocker,Maud Galametz,George Helou,Christine D. Wilson,Robert C. Kennicutt,D. Calzetti,Bruce T. Draine,G. Aniano,Daniel A. Dale,G. Dumas,Charles W. Engelbracht,Charles W. Engelbracht,Karl D. Gordon,J. Hinz,Kathryn Kreckel,E. Montiel,H. Roussel +25 more
TL;DR: In this article, the distribution of the synchrotron spectral index across NGC 6946 and investigate the correlation between the radio continuum (synchoretron) and far-infrared (FIR) emission using the KINGFISH Herschel-PACS and SPIRE data.
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The 24 micron view of embedded star formation in ngc 7129
James Muzerolle,S. T. Megeath,Robert A. Gutermuth,Lori E. Allen,Judith L. Pipher,Lee Hartmann,Karl D. Gordon,Deborah Padgett,Alberto Noriega-Crespo,Philip C. Myers,Giovanni G. Fazio,George H. Rieke,Erick T. Young,Jane E. Morrison,Dean C. Hines,Dean C. Hines,Kate Y. L. Su,Charles W. Engelbracht,Karl Misselt +18 more
TL;DR: In this article, a significant population of sources, likely pre-main-sequence members of the young stellar cluster, are revealed outside the central photoionization region, where they are associated with the densest part of the molecular cloud surrounding the photometric region.