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| === Planned changes for the next releases === * '''kmo_illumination''' * Ignore the first exposure generated with the illumination template. This exposure is taken to estimate the needed exposure time. * Cross-correlate sky exposures with the masterflat. This will reduce artifacts in the processed science frames due to instrument flexure. * '''kmo_std_star''' * Will be modified in several ways, so don't wonder if the products of this recipe will change. * '''kmo_sci_red''' * speed up mapping mode (for mapping24-template approx. 3h) * Additionally a switch will be introduced to map just the collapsed cubes in order to get a fast preview. * 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''' |
=== Some planned changes for the next releases to come === * '''kmo_sky_tweak''' * Advanced recipe for OH-line subtraction * '''kmo_multi_reconstruct''' * same functionality as kmo_sci_red |
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The list of bugs, requests and to-do's can be viewed at [[http://pcerw/mantisbt|SPARK Bug Tracking]] (only from within MPE). It is read-only and is maintained by the SPARK developers. |
KMOS SPARK Wiki
Some planned changes for the next releases to come
kmo_sky_tweak
- Advanced recipe for OH-line subtraction
kmo_multi_reconstruct
- same functionality as kmo_sci_red
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 SPARK Bug Tracking (only from within MPE). It is read-only and is maintained by the SPARK developers.
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