GHRS Echelle and G140M Long-Term - 5

Details GHRS Echelle and G140M Long-Term - 5 GHRS Echelle and G140M Long-Term - 5

Jul 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995hst..prop.6170s&link_type=abstract

HST Proposal ID #6170

Physics

Hst Proposal Id #6170 Calibration

Scientific paper

This proposal defines a series of observations that will continue the long-term monitor of Ech-A, G140M, and Ech-B. The program should be run once in Cycle5, preferrably in the middle of the cycle. Ech-A and G140M will be made both through the LSA and the SSA. Ech-B observations are through the LSA only. mu Col is used for all observations. For the Echelles, OSCAN observations will measure the sensitivity near the the blaze peak. The setups for Ech-B are chosen to be the same as those used in SV, to maintain traceability to the original calibrations. WSCAN observations will scan across m=20 in ECH-B. Ech-A is used with an OSCAN at the blaze peak (MLAMBDA=56100), plus 1 WSCAN. G140M is used at 1100, 1200, 1300, 1400, 1500, and 1600 A.

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