Physics
Scientific paper
Jul 1990
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990hst..prop.2949b&link_type=abstract
HST Proposal ID #2949
Physics
Hst Proposal Id #2949
Scientific paper
Using a standard star (V8.2 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 SV. A different test has been submitted for OV purposes. Note: This is RPSS file 1524 and is based on 1504 Revision History (1524): 1504 modified to create SV test - Richards 2/8/89 RPSS V7.2; Added fine lock rqmt 3/10/89 - Richards 3/10/89; Scrubbed for SV - 4/24/89 Laurent; Modified, changed target - Nelson 4/29/89; Minor fixes - Richards 5/1/89; Errors corrected - Laurent 5/1/89; Changed per P. Reppert's comments of 6/6/89 - SALM 8/10/89; Changed to SCP & required ONBRD ACQ - SALM 10/2/89; Scan changes - SALm 10/4/89 3/21/90-PStanley-Split each detector into separate prop - VIS=2950,UV2=2948,POL=2951,UV1=2949. Revised 8/16/90 by C. Taylor (STScI) per IDT redlines; Small changes to punctuation--BJW 9/9/90;
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