MICADO-WISE merge requestshttps://gitlab.astro-wise.org/micado/micadowise/-/merge_requests2020-07-13T14:04:59Zhttps://gitlab.astro-wise.org/micado/micadowise/-/merge_requests/98Resolve "Should be possible to simulate raw science data"2020-07-13T14:04:59ZHugo Buddelmeijerhugo@buddelmeijer.nlResolve "Should be possible to simulate raw science data"Closes #33Closes #33https://gitlab.astro-wise.org/micado/micadowise/-/merge_requests/99Resolve "Create TSF files from Python"2020-07-03T14:45:19ZHugo Buddelmeijerhugo@buddelmeijer.nlResolve "Create TSF files from Python"Closes #69
This creates TSF files from Python classes, in order to make it easier to collaborate with the ICS team.
Note that only the dark template makes sense in this MR, because the values for the other templates are set in !95,...Closes #69
This creates TSF files from Python classes, in order to make it easier to collaborate with the ICS team.
Note that only the dark template makes sense in this MR, because the values for the other templates are set in !95, which is not yet merged.
@verdoes could you see whether the generated TSF files are sensible, in particular https://gitlab.astro-wise.org/micado/micadowise/-/blob/69-create-tsf-files-from-python/src/micado/templates/MCD_img_cal_dark.tsf
Standard Imaging: internal delivery documentationGijs Verdoes Kleijng.a.verdoes.kleijn@rug.nlGijs Verdoes Kleijng.a.verdoes.kleijn@rug.nlhttps://gitlab.astro-wise.org/micado/micadowise/-/merge_requests/95Add OCA rules creation, mock backward chaining, and DM changes2020-07-03T13:26:05ZHugo Buddelmeijerhugo@buddelmeijer.nlAdd OCA rules creation, mock backward chaining, and DM changesThis is initial code to create OCA rules automatically from the data lineage. This supersedes !92.
The goal is not so much to create the OCA rules, but to use the creation of OCA rules as a way to ensure we have designed the pipeline ...This is initial code to create OCA rules automatically from the data lineage. This supersedes !92.
The goal is not so much to create the OCA rules, but to use the creation of OCA rules as a way to ensure we have designed the pipeline properly.
It contains some data model changes:
* All templates now have INS.MODE, DPR.CATG, DPR.TECH and DPR.TYPE defined.
* Persistence now has its own recipe. This is still preliminary, but is a good use-case for the OCA rules.
* There are several 'Unpersisted' classes to remove persistence from the raw data.
* There is now a distinction between Raw data and Sky. Sky inherits from Raw and is on-sky data.
* The reduced images and catalog classes have been refactored, so they are easier to use in OCA rules.
* The photometric and astrometric calibration is now done on fully reduced frames (that is, background subtraction and illumination correction is applied).
* The backward chaining is now ad-hoc defined in `augment_backward_chaining.py`. At some point this should be added to the Data Model properly.
@verdoes can you look at the data model changes in particular? That is, micado.vodsl and associationmatrix.ditaa / .png.
Standard Imaging: internal delivery documentationGijs Verdoes Kleijng.a.verdoes.kleijn@rug.nlGijs Verdoes Kleijng.a.verdoes.kleijn@rug.nlhttps://gitlab.astro-wise.org/micado/micadowise/-/merge_requests/105Resolve "Should be possible to simulate raw science data"2020-07-13T14:22:13ZHugo Buddelmeijerhugo@buddelmeijer.nlResolve "Should be possible to simulate raw science data"Closes #33Closes #33https://gitlab.astro-wise.org/micado/micadowise/-/merge_requests/47Update README.rst (section build instructions) to make them foolproof even fo...2020-03-03T18:23:32ZGijs Verdoes Kleijng.a.verdoes.kleijn@rug.nlUpdate README.rst (section build instructions) to make them foolproof even for non-developers.Closes #40 Closes #40 Hugo Buddelmeijerhugo@buddelmeijer.nlHugo Buddelmeijerhugo@buddelmeijer.nl