Gordon P. Garmire

TL;DR: In this article, the authors present a catalog of 14,000 X-ray sources observed by the ACIS instrument on the Chandra Xray Observatory within a 1.42 square degree survey of the Great Nebula in Carina, known as the Chandra Carina Complex Project (CCCP).

TL;DR: In this article, the pulsar wind nebula (PWN) was observed with the Chandra X-ray Observatory and it was shown that the nebular morphology can be explained in terms of a torus of emission in pulsar's equatorial plane and a jet directed along the pulsars spin axis, as is seen in the Xray nebulae powered by other young pulsars.

TL;DR: The Extended Chandra Deep Field-South (E-CDF-S) survey as mentioned in this paper detected 762 distinct X-ray point sources within the 1.5-2.0 keV exposure; 589 of these sources are new (i.e., not previously detected in the ~1 Ms CDF-S).

TL;DR: In this article, the properties of powerful X-ray flares from 161 pre-main sequence (PMS) stars observed with the Chandra Xray Observatory in the Orion Nebula region were studied.

TL;DR: In this article, the authors use Chandra observations of the Hubble Deep Field North region, A370, and the Hawaii Survey Fields SSA13 and SSA22, together with the ROSAT Ultra Deep Survey soft sample and the ASCA Large Sky Survey hard sample, to construct rest-frame 2-8 keV luminosity functions versus redshift for all the X-ray sources, regardless of their optical AGN characteristics.