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| === Planned changes for the next releases === | === 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 |
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| * Ignore the first exposure generated with the illumination template. This exposure is taken to estimate the needed exposure time. | |
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| * '''kmo_std_star''' * Will be modified in several ways, so don't wonder if the products of this recipe will change. |
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| * Additionally a switch will be introduced to map just the collapsed cubes in order to get a fast preview. | |
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| The list of bugs, requests and to-do's can be viewed at [[http://pcerw/mantisbt|SPARK Bug Tracking]]. It is read-only and is maintained by the SPARK developers. |
KMOS SPARK Wiki
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
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. It is read-only and is maintained by the SPARK developers.
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