activity
20002026
most citedThe Chandra High Energy Transmission Grating: Design, Fabrication, Ground Calibration and Five Years in Flight

360 citations · 700 across the 20 of their papers we have counts for

collaborators
Showing astro-phShow all

7 papers · 1 filter

astro-ph2005★ 360 cited

The Chandra High Energy Transmission Grating: Design, Fabrication, Ground Calibration and Five Years in Flight

Claude R. Canizares, John E. Davis, Daniel Dewey +11

Details of the design, fabrication, ground and flight calibration of the High Energy Transmission Grating, HETG, on the Chandra X-ray Observatory are presented after five years of…

astro-ph2003★ 69 cited

Chandra High-Resolution X-Ray Spectrum of Supernova Remnant 1E0102.2-7219

K. A. Flanagan, C. R. Canizares, D. Dewey +5

Chandra High Energy Transmission Grating Spectrometer observations of the supernova remnant 1E0102.2-7219 in the Small Magellanic Cloud reveal a spectrum dominated by X-ray emissio…

astro-ph2001★ 2 cited

High Resolution Spectroscopy of Two Oxygen-Rich SNRs with the Chandra HETG

C. R. Canizares, K. A. Flanagan, D. S. Davis +3

The HETG can be used to obtain spatially resolved spectra of moderately extended sources. We present preliminary results for two well studied, oxygen rich supernova remnants in the…

astro-ph2001

Ionization and Velocity Structure in the Supernova Remnant E0102-72

K. A. Flanagan, C. R. Canizares, D. S. Davis +4

The High Energy Transmission Grating (HETG) Spectrometer aboard the Chandra X-Ray Observatory was used to observe E0102-72, a ~1000 year old, oxygen rich supernova in the Small Mag…

astro-ph2001

Ionization Structure and the Reverse Shock in E0102-72

K. A. Flanagan, C. R. Canizares, D. S. Davis +3

The young oxygen-rich supernova remnant E0102-72 in the Small Magellanic Cloud has been observed with the High Energy Transmission Grating Spectrometer of Chandra. The high resolut…

astro-ph2001

Spectral Line Imaging Observations of 1E0102.2-7219

D. S. Davis, K. A. Flanagan, J. C. Houck +5

E0102-72 is the second brightest X-ray source in the Small Magellanic Cloud and the brightest supernova remnant in the SMC. We observed this SNR for ~140 ksec with the High Energy…