Monitoring FGS2r2 S-curves after SMOV4

Details Monitoring FGS2r2 S-curves after SMOV4 Monitoring FGS2r2 S-curves after SMOV4

Jul 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008hst..prop11874n&link_type=abstract

HST Proposal ID #11874. Cycle 17

Physics

Scientific paper

This proposal satisfies the near-term requirement associated with SMOV4 activity OTA/FGS-10, as well as the long term Cycle 17 requirement to monitor the post-SM4 evolution of the FGS2r2 S-curves stability during its first year on orbit. The S-curves will be obtained from Trans mode observations of stars {point sources} at several locations in the FGS2r2 FOV in order to monitor both global and differential {i.e., field-dependent} changes. At each location, both F583W and PUPIL S-curves will be obtained. Stars in the M35 cluster will be used for this proposal since the field lies very near the ecliptic and can therefore be observed by HST at two Orients from August to May.;

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