+-----------------------------------------------------+ | HST Spectroscopy STIS/GHRS/FOS | | STScI Analysis Newsletter No. 11, Feb. 99 | | | +-----------------------------------------------------+ New HST Spectroscopy STAN Format & Content We are continuing a transition to a new format for the HST Spectroscopy STAN. At the top, an index of topics is listed with the web address where you can go to get all of the details. Below this, short summaries are provided for each topic. And as always, the STAN will be posted on the STIS web site, where all of these topics will be hypertext links directing you to the full writeup. All items appearing here and more are posted on the STIS web site, but we will only highlight items of particular interest or importance in the STAN. New STIS Reference Files Discontinuities in Rectified Spectra Offset between CCD and MAMA Coordinate Systems Aperture Offset Angles +-STIS------------------------------------------------+ New STIS Reference Files Many updated reference files have been installed in the calibration pipeline. Among them are, the aperture throughputs for all apertures (and corresponding photometric throughputs), photometric correction table for new supported apertures, as well as slitless spectroscopy, and improved cosmic ray rejection parameters. Discontinuities in Rectified Spectra An error in the interpolation method used in the rectification of spectral images has caused jumps in flux level in the rectified spectra. This error will be corrected in release 2.1 of CALSTIS. Offset between CCD and MAMA Coordinate Systems Observations of a target taken back-to-back with the MAMAs and the CCD, and with no telescope movement between the individual observations should have the same world coordinates in either detector. It was recently discovered that the postobservation correction for the MSM deflection is currently not applied. Therefore targets will not be centered in the field of view, even if the target and guide star coordinates had no errors. Aperture Offset Angles Each STIS aperture has a specific U3 offset angle which is close to, but not equal to 45-degrees. Precise offset angles for all available spectroscopic slits are available. +-Spectrographs---------------------------------------+ List of Recent Preprints Now on Line The list of preprints based on HST spectrographs data that usually occupies this space is now available at the STIS web site for easy browsing. +-----------------------------------------------------+ | Need help? | | http://www.stsci.edu/cgi-bin/stis?cmd=help | +-----------------------------------------------------+ | To unsubscribe from this mailing list send email to | | majordomo@stsci.edu with the message: | | unsubscribe stis_news | +-----------------------------------------------------+ | The Space Telescope Science Institute is operated | | by the Association of Universities for Research in | | Astronomy, Inc., under NASA contract NAS5-26555. | +-----------------------------------------------------+