| Space Telescope Science Institute |
| STIS Data Handbook 6.0 May 2011 |
| help@stsci.edu |
G140L and G140M moved from 3" above center to 3" below center
to avoid repeller wire (see the STIS Instrument Handbook, Section 7.5
MAMA Spectral Offsetting) shadow Time-dependent sensitivity correction implemented for MAMA data Time-dependent sensitivity correction implemented for CCD data Charge transfer inefficiency correction implemented for CCD data Echelle data flux calibration significantly improved, trace rotation
implemented for commonly used first order modes