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- W2079692712 abstract "We present the design parameters, production process, and in-flight performance of the X-ray telescope (XRT) onboard Suzaku. The imaging capability is significantly improved over the ASCA XRT, which had half-power diameters of |${3rlap {.}{}^{mathrm {prime }}6}$|, to |${1rlap {.}{}^{mathrm {prime }}8}$|–|${2rlap {.}{}^{mathrm {prime }}3}$| for all four XRT-I modules. The optical axes are found to be distributed within a radius of |${1rlap {.}{}^{mathrm {prime }}3}$|, which makes the observation efficiency of all the XRTs more than 97% at the XIS-default observing position. The vignetting over the XIS field of view predicted via ray-tracing coincides with that measured for observations of the Crab Nebula to within |$sim 10%$|. Contemporaneous fits of a power law to all of the XIS spectra of the Crab Nebula taken at the two standard observing positions (XIS/HXD-default positions) gives a flux consistent with that obtained by Toor and Seward (1974, AJ, 79, 995) to within |$sim 2%$|. The pre-collimator on the top of each XRT module successfully reduces the intensity of the stray light from the |$20'$| and |$50'$|-off directions down to the level of pre-flight expectations." @default.
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- W2079692712 date "2007-01-30" @default.
- W2079692712 modified "2023-10-17" @default.
- W2079692712 title "The X-Ray Telescope onboard Suzaku" @default.
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- W2079692712 doi "https://doi.org/10.1093/pasj/59.sp1.s9" @default.
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