5.
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Locate focal position along optical axis such that image shift in knife-edge test is < 0.1" . 5 positions along x-axis. hsiimage with 4 shutter settings at each focal setting. Unresolved issue: how will we coordinate between the XDACS and the HRC to control the acquisition of data and the control of the shutters? What GSE will be used to make the SIM motions? |
maximize sensitivity for point source detection, for example, knots in jetsc. |
4 energies: Cu K, Al K, TI K, Cu K |
5.1.1 |
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5.2 Focus by Changes in PSF Core |
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Use image acquisition capability of HRC. |
4 energies: Cu K, Al K, TI K, Cu K |
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5.3 Effective Area Confirmation |
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Effective area at one image radius Accuracy to 1%. The HRC must be translated & rotated so the images striking it duplicate the conditions in flight. The SIM rotates and translates to keep the HRC detectors in a rigid body relationship with the HRMA. XGA turned down to 10-4 of max.
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25 energies |
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6 energies: TBD based on an examination of the predicted curve of effective area of combined HRMA and HRC-I vs. energy, to select critical energies at features in the curve. |
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5.4 On-axis HRMA/HRC-I PSF & PSF-Wing Calibration |
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1% of the measured value in 1 x 1 arc sec cells within 2 arcsec of image center, 3% of the measured value in 1 x 1 arc sec cells from 2-20 arcsec. |
Source structure and detection of extended emission around point sources. (strongest source: 0.01 Crab) |
10 energies:B K, C K, Cr L, Cu L, Al K, Ag L, Ti K |
5.4.1 |
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5.5 HRMA/HRC-I Plate Scale and Related Properties |
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Relative image positions to 1 arcsec on scales of 5 arcmin to 1 arcsec (?). |
Identification of sources in deep surveys, source positions. |
5.5.1 |
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5.6 HRMA/HRC-I Count Rate Linearity |
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Identification of sources in deep surveys, source positions. |
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5.7 X-ray ghost images, outer |
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Imaging detector used for quick survey, 0.1 mm resolution, out to 100 mm diameter. |
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5.8 Background Data for Interpreting XRCF Calibrations |
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5.9 Total Integration Time for HRMA/HRC |
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b.Faint source detection & identification, e.g. deep surveys, nearby galaxzies, globular cluster source masses. (HRC proposal).
d.Wilson response to MSFC Project Scientist inquiry, May 24. 1991.
g. ACIS response to MSFC Project Scientist inquiry, Apr 30, 1991.
g. ACIS response to MSFC Project Scientist inquiry, Apr 30, 1991.
h. XRS response to MSFC Project Scientist inquiry, May 22, 1991.