Gordon P. Garmire

TL;DR: The Age JX method as discussed by the authors is sensitive to a wide range of evolutionary stages, from disk-bearing stars embedded in a cloud to widely dispersed older pre-main-sequence (PMS) stars.

TL;DR: In this paper, the authors investigated the physical processes responsible for the variable radio, near-infrared, and X-ray counterpart Sagittarius A* (SgrA*) and found that highly variable and NIR polarized flare emission is non-thermal and that there exists a class of synchronous NIR/X-ray flares.

TL;DR: The Massive Star-forming Regions (MSFRs) Omnibus X-ray Catalog (MOXC) as discussed by the authors is a compendium of point sources from Chandra/ACIS observations of a selection of MSFRs across the Galaxy, plus 30 Doradus in the Large Magellanic Cloud.

TL;DR: In this article, the authors present the results of a Chandra X-ray survey of the 8 most massive galaxy clusters at z>1.2 in the South Pole Telescope 2500 deg^2 survey.

TL;DR: In this article, the 2-8 keV number counts from the 1 Ms Chandra observation of the Chandra Deep Field-North were combined with the number counts obtained from independent analyses of Chandra Deep Fields-South and the Hawaii Survey field SSA13 to determine the number count from 2 × 10-16 to 10-13 ergs cm-2 s-1 deg-2.