March 06, 2012
- Features:
- Added ESO P90 configuration
- Corrected AMBER noise parameters: visibility and phase bias set to 5% and 3 deg respectively
- Updated PIONIER instrument configuration: corrected noise parameters and added spectral modes (LARGE-H, SMALL-H and BROAD-H)
- Improved Java Web Start packaging (JNLP) to provide faster downloads
- Added ESO P89 configuration
- Added one preliminary OIFits viewer: only square visiblity (VIS2) vs radius plot is available with error bars
when the noise modeling is able to compute them
- Fixed CHARA delay line configuration: E1 cart moves in range [-1.4 to +44.0] like others (july 2011)
- Updated CHARA VEGA (2T/3T/4T) configuration (beams and station reference per baseline)
- Corrected zenithal restriction to 4 degrees applied to UT and AT telescopes according to "ESO Call for Proposals – P88 (UT)" (VLTI)
- Updated CHARA configuration to have both MIRC_5T and MIRC_6T configurations
- Updated CHARA configuration using the latest official configuration file (telescopes.chara)
- Better File choosers: use the last used directory (per file type and saved in user preferences)
- Filled "OBSERVATION.DESCRIPTION.NAME" in VLTI OBs to help P2PP users better navigate among targets
- Changed OIFits file extension to '.fits'
- Added 'Export targets to Observing blocks' in the File menu to export all targets at once (VLTI)
- Allow zooming on the observability plot (targets and time range)
- Changed color for orphan calibrators in the observability plot
- Added 'Center plot arround night' preference to have the complete night centered on the observability plot
- Added civil and nautical twilight zones and a new preference 'Twilight used as Night limit' to choose which twilight limits are used for night restrictions
- Added a new preference 'Default min Elevation' set to 45 degrees by default
- Changes:
- Changed VOTable message handler (SAMP) to accept PIVOT messages using VOTable for targets
- Added 'Send StarList to PIVOT' action (SAMP)
- Enhanced performance to find best PoPs (CHARA)
- Fixed logging configuration to avoid important performance loss during observability computations (best PoPs)
- Major performance improvements to determine best PoPs (CHARA) in the observability computation
- Added information about best / good PoPs in the warning messages displayed by the status indicator (CHARA)
- Updated Export to Observing blocks (VEGA, VLTI) to use the user minimum elevation instead of 30 deg (required by ESO OB)
- Minor ergonomic change: when the target editor is opened, the 'Targets' tab is displayed by default; when the UV coverage plot is selected,
the 'Models' tab is displayed instead.
- Minor changes related to CHARA VEGA Observing blocks (spectral type format, disk diameter set from SearchCal diameters)
- Fixed export OB for CHARA VEGA to handle properly calibrators in the StarList format
- Automatic Pops set with values defined in CHARA VEGA configuration dedicated to June 2011 run (read-only)
- Added CHARA VEGA configuration dedicated to June 2011 runs and minor changes in CHARA configuration (sorted instrument list)
- Added 'Scroll view' checkbox button to see all targets (or only some of them) on the observability plot
- Enable mouse zooming on the observability plot
- Always show the scrollbar (with margins) on the observability plot
- Bug fixes:
- Corrected effective wavelength in OIFits output (channel center)
- Fixed alternative distribution package (JAR file): missing jMAL embedded libraries
- Fixed out of range exception when mouse zooming on UV Coverage Panel arround borders
- Fixed exception when exporting an Observing block
and the spectral type is undefined for one target (SearchCal calibrator)
- Changed PIONIER OB template to take 100 scans of DARK instead of 50
- Fixed bug related to SearchCal integration:
always use the bright scenario as the faint scenario is not available for all instrumental bands
- Adapt the number of visible targets on the observability plot when the application window is resized
Last updated:
May 19, 2012 01:30 PM
All times are UTC.
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