Gordon P. Garmire

TL;DR: In this article, the jet-linked X-ray emission from highly radio-loud quasars (HRLQs; log R>2.5) at high redshift was investigated, and the typical factor of enhancement was revised to $1.9^{+0.5}_{-0.4}$, which was smaller than but consistent with previous results.

TL;DR: In this paper, the second brightest X-ray supernova remnant (SNR) in the Small Magellanic Cloud (SMC) has been observed with the Chandra X-Ray Observatory.

TL;DR: The results of a Chandra study of 21 broad absorption line (BAL) radio-loud quasars (RLQs) are presented in this article, with observed X-ray luminosities less than those of non-BAL RLQs, having comparable optical/UV luminosity by typical factors of 4.1-8.5.

TL;DR: In this paper, the authors reported the discovery of a point-like source (CXOU J160103.1-513353) at the center of the Galactic supernova remnant (SNR) G330.2+1.0 with Chandra X-Ray Observatory.

TL;DR: In this paper, the authors reported the discovery of eight X-ray sources with periodic variability in 487 ks of observations of the Galactic center with Chandra, with luminosities of (1-5) × 1032 ergs s-1 (2-8 keV at 8 kpc) and their periods range from 300 s to 4.5 hr, with amplitudes between 40% and 70% rms.