Physics
Scientific paper
Jul 1990
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990hst..prop.1504b&link_type=abstract
HST Proposal ID #1504
Physics
Hst Proposal Id #1504
Scientific paper
Using a standard star (V 8.2 mag.) in the CVZ near the open cluster NGC188, the instantaneous locations of the centers of the acquisition aperture and various small science apertures will be determined with respect to the V2V3 reference system. The ultimate goal of this third part of the Mission Support Calibration (MSC) procedure is to locate the aperture centers relative to the V2V3 reference frame with an uncertainty not exceeding 0.05 arcsec. It is preceded by Phase I (Deflection Coordinate Calibration) and Phase II (Coarse Alignment). This test is unique to OV. A different test has been submitted for SV purposes. Note: This is RPSS file 1504. Revision history: Richards 4/13/88, Slovak 5/20/88, Richards 6/29/88. Translated by XX into V2 instructions by XX, fall 1988. Corrected errors, Richards, 2/10/89 RPSS V6.2 Added fine lock requirement 3/10/89 Richards. Made to look like SV's 1524 6/20/89 Laurent-Muehleisen. Revised 10/25/89 to match meeting with proposers and implementation plan. Revised 11/9/89......changed target position to NGC188- #998 as per meeting
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