Calstis4, calstis11, calstis12: Wavecal Processing in the STIS Calibration Pipeline

Details Calstis4, calstis11, calstis12: Wavecal Processing in the STIS Calibration Pipeline Calstis4, calstis11, calstis12: Wavecal Processing in the STIS Calibration Pipeline

Apr 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998stis.rept...12h&link_type=abstract

Instrument Science Report STIS 98-12, 12 pages

Physics

Hubble Space Telescope, Hst, Space Telescope Science Institute, Stis, Space Telescope Imaging Spectrograph

Scientific paper

Due to uncertainties in positioning by the mode select mechanism (MSM) and thermal drifts internal to STIS, an image may be shifted on the detector by several pixels from its nominal location. The purpose of wavecal processing is to determine the shift of the image on the detector in each axis. This is only used for spectroscopic data. It requires one or more wavecal (line lamp) observations, taken without moving the MSM from the setting used for the science data. This document updates and supersedes STIS ISR 96-19, and it describes the functionality that was implemented for calstis V1.7.

Affiliated with

Also associated with

No associations

Rating

Calstis4, calstis11, calstis12: Wavecal Processing in the STIS Calibration Pipeline does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Calstis4, calstis11, calstis12: Wavecal Processing in the STIS Calibration Pipeline, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Calstis4, calstis11, calstis12: Wavecal Processing in the STIS Calibration Pipeline will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1745475