An Overview of the Performance of the Chandra X-ray Observatory

@article{Weisskopf2003AnOO,
  title={An Overview of the Performance of the Chandra X-ray Observatory},
  author={Martin. C. Weisskopf and Thomas Lytell Aldcroft and Mark W. Bautz and R. A. Cameron and Daniel Dewey and Jeremy J. Drake and Catherine E. Grant and Herman L. Marshall and Stephen S. Murray},
  journal={Experimental Astronomy},
  year={2003},
  volume={16},
  pages={1-68}
}
The Chandra X-ray Observatory is the X-ray component of NASA's Great Observatory Program which includes the recently launched Spitzer Infrared Telescope, the Hubble Space Telescope (HST) for observations in the visible, and the Compton Gamma-Ray Observatory (CGRO) which, after providing years of useful data has reentered the atmosphere. All these facilities provide, or provided, scientific data to the international astronomical community in response to peer-reviewed proposals for their use. The… 
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References

SHOWING 1-10 OF 60 REFERENCES
Chandra X-Ray Spectroscopic Imaging of Sagittarius A* and the Central Parsec of the Galaxy
We report the results of the first-epoch observation with the ACIS-I instrument on the Chandra X-Ray Observatory of Sagittarius A* (Sgr A*), the compact radio source associated with the supermassive
Observed on-orbit background of the ACIS instrument on the Chandra X-ray Observatory
We have analyzed data acquired during the Orbital Activation and Checkout (OAC) and Guest Observer (GO) phases of the Chandra X-ray Observatory mission in order to characterize the background of the
Discovery of X-rays from Mars with Chandra
On 4 July 2001, X-rays from Mars were detected for the first time. The observation was performed with the ACIS-I detector onboard Chandra and yielded data of high spatial and temporal resolution,
First Results from the X-Ray and Optical Survey of the Chandra Deep Field South
We present our first results from 120 ks of X-ray observations obtained with the Advanced CCD Imaging Spectrometer on the Chandra X-Ray Observatory. The field of the two combined exposures is 0.096
Chandra imaging of the complex X-ray core of the Perseus cluster
ABSTRACT We report subarcsec-resolution X-ray imaging of the core ofthe Perseus cluster around thegalaxy NGC1275 with the Chandra X-ray Observatory. The ROSAT-discovered holes asso-ciated with the
Discovery of Spatial and Spectral Structure in the X-Ray Emission from the Crab Nebula.
TLDR
Zeroth-order images with the High-Energy Transmission Grating (HETG) readout by the Advanced CCD Imaging Spectrometer spectroscopy array (ACIS-S) show a striking richness of X-ray structure at a resolution comparable to that of the best ground-based visible-light observations.
The X-Ray Remnant of SN 1987A
We present high-resolution Chandra observations of the remnant of SN 1987A in the Large Magellanic Cloud. The high angular resolution of the Chandra X-Ray Observatory permits us to resolve the X-ray
CHANDRA SPECTRA OF THE SOFT X-RAY DIFFUSE BACKGROUND
We present an exploratory Chandra ACIS-S3 study of the diffuse component of the cosmic X-ray background (CXB) in the 0.3-7 keV band for four directions at high Galactic latitudes, with emphasis on
High-resolution X-ray spectroscopy of Procyon by Chandra and XMM-Newton
We report the analysis of the high-resolution soft X-ray spectrum of the nearby F-type star Procyon in the wavelength range from 5 to 175 A obtained with the Low Energy Transmission Grating
The Chandra Deep Field North Survey. XIV. X-Ray-detected Obscured AGNs and Starburst Galaxies in the Bright Submillimeter Source Population
We provide X-ray constraints and perform the first X-ray spectral analyses for bright SCUBA sources (f850 μm ≥ 5 mJy; signal-to-noise ratio ≥4) in an 8.′4 × 8.′4 area of the 2 Ms Chandra Deep Field
...
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