• release for support of period 79. Large changes have been entered both in the script and in the the program aspro working behind the scenes:
  • new scheme for telescope selection: now by configuration. Uses a simpler choice: MIDI or AMBER, that's all.
  • updated checks for object magnitude vs. sensitivity of telescope+instrumental setup
  • images in plots are now embedded in the svg file sent to the client: faster, surer.
  • uv model (background image in uv plots) is now plotted by aspro_the_program, not by aspro_the_script: for internal reasons, improves speed.
  • help on instruments is provided as a web link to the original CallForPorposals.
• PTI, BURE and GI2T have been removed from the list of known interferometers.
• ASPRO now produces OI_FITS files (task uvttooifits and "MISC.">"Export UV Table as OI_FITS" menu).

• new oipt version correcting SPRs 9, 10 and 11. Additionally, a bug was found where partial derivatives of the binary model were computed, and the help on models is more acurate.

-- Older Changelog is found here