G
Gordon P. Garmire
Researcher at Pennsylvania State University
Publications - 493
Citations - 38165
Gordon P. Garmire is an academic researcher from Pennsylvania State University. The author has contributed to research in topics: Galaxy & Luminosity. The author has an hindex of 99, co-authored 485 publications receiving 36277 citations. Previous affiliations of Gordon P. Garmire include Harvard University.
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Discovery of X-Ray Emission Associated with the GUM Nebula
TL;DR: The first detection of X-ray emission associated with the Gum Nebula is reported in this article, which is consistent with a supernova remnant in the shell stage of evolution, which was the product of an energetic supernova explosion which occurred about 2 x 10 exp 6 yr ago.
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Search for soft X-ray emission from SN 1987A with a CCD X-ray imaging spectrometer
TL;DR: In this paper, the results of soft X-ray observations of SN 1987A over the energy band 0.65-2.0 keV are reported and the upper limits on the soft x-ray flux are inconsistent with an extrapolation of the spectrum measured by the Ginga Satellite to the energy bands and require a turnover in the Xray spectrum between 2 and 4 keV.
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The Frequency of Intrinsic X-ray Weakness Among Broad Absorption Line Quasars
TL;DR: In this article, Chandra observations of seven high-ionization broad absorption line (HiBAL) quasars selected from the Large Bright Quasar Survey (LBQS) were combined to detect intrinsically X-ray weak AGNs.
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Evidence for line-of-sight structure in a comparison of X-ray and optical observations of the high-redshift cluster RCS 043938-2904.7
Benjamin Cain,David G. Gilbank,Marshall W. Bautz,Amalia Hicks,H. K. C. Yee,Michael D. Gladders,Erica Ellingson,L. F. Barrientos,Gordon P. Garmire +8 more
TL;DR: In this article, Chandra observations of a high-redshift galaxy cluster discovered in the Red-Sequence Cluster Survey (RCS): RCS 043938-2904.7.
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Parsec-scale X-ray Flows in High-mass Star-forming Regions
Leisa K. Townsley,Eric D. Feigelson,T. Montmerle,Patrick S. Broos,You-Hua Chu,Gordon P. Garmire,Konstantin V. Getman +6 more
TL;DR: The Chandra X-ray Observatory is providing remarkable new views of massive star-forming regions, revealing all stages in the life cycle of high-mass stars and their effects on their surroundings as discussed by the authors.