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=== Some planned changes for the next releases to come === The next release v1.0.9 will be the one used for COMM3 beginning on March 22nd * '''kmo_illumination''' * Cross-correlate sky exposures with the masterflat. This will reduce artifacts in the processed science frames due to instrument flexure. * '''kmo_sci_red''' * speed up mapping mode (for mapping24-template approx. 3h) * implement enhanced background matching for mapping mode * '''add test in all reconstruction recipes in order to check if XCAL, YCAL, LCAL match together.''' * If for example XCAL and YCAL originate from one set of calibration exposures and LCAL from another, the badpixel mask probably isn't the same. In the future a warning will be emitted in this case. The recipes work anyway, but the results should be questionned anyway... * '''update KMOS Manual with changes since COMM2''' |
=== Bug reports and change requests === {{#!wiki red/solid The KMOS pipeline is in the transition phase to be handed over to ESO. Please send any bug reports or change requests already now to usd-help@eso.org or psd_kmos@eso.org }}} |
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=== Bug reports and change requests === If you encounter a bug or have a change request, please send it to: kmos-spark@mpe.mpg.de The list of bugs, requests and to-do's can be viewed at [[http://pcerw/mantisbt|SPARK Bug Tracking]]. |
The list of bugs, requests and to-do's can be viewed at [[http://macir26/mantisbt|SPARK Bug Tracking]] (only from within MPE). |
KMOS SPARK Wiki
Bug reports and change requests
{{#!wiki red/solid The KMOS pipeline is in the transition phase to be handed over to ESO. Please send any bug reports or change requests already now to usd-help@eso.org or psd_kmos@eso.org }}}
The list of bugs, requests and to-do's can be viewed at SPARK Bug Tracking (only from within MPE). It is read-only and is maintained by the SPARK developers.
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