{"push_id":1346238668,"size":9,"distinct_size":2,"ref":"refs/heads/feature_cleanup_cont-int_freidt","head":"25cf937104a008fcf8c5f3807e21e0dc091b74f8","before":"8a3100dc380fb08cef1faa62290f2afbaca4cd3b","commits":[{"sha":"1d3f2a45d4c901dae1eae81304d063bb5193bddd","author":{"name":"Kilian Lohmann","email":"bb373ef8a4e5f03fe000fac636b88c615ef86bc2@phys.uni-goettingen.de"},"message":"added 2D residual histograms and changed axes from mm to um","distinct":false,"url":"https://api.github.com/repos/freidt/eutelescope/commits/1d3f2a45d4c901dae1eae81304d063bb5193bddd"},{"sha":"cf9c2cd6f747ffee8cb85c54c6504fe8feaf6c4e","author":{"name":"Kilian Lohmann","email":"bb373ef8a4e5f03fe000fac636b88c615ef86bc2@phys.uni-goettingen.de"},"message":"increased histogram x-axis limits","distinct":false,"url":"https://api.github.com/repos/freidt/eutelescope/commits/cf9c2cd6f747ffee8cb85c54c6504fe8feaf6c4e"},{"sha":"b5c8cae11c4261e11536304eaaa3eb10eeca0638","author":{"name":"tbisanz","email":"2ef5f328e52f26480c6133cbf68f552f203b60eb@users.noreply.github.com"},"message":"Merge pull request #312 from KilianLohmann/HitAnalysis\n\nHit analysis","distinct":false,"url":"https://api.github.com/repos/freidt/eutelescope/commits/b5c8cae11c4261e11536304eaaa3eb10eeca0638"},{"sha":"b83e2bdade1846a7d7459cb4616b446d9d01ef83","author":{"name":"Felix Reidt","email":"113228c8841ada9d7aa7d525df0c56d24f56b508@cern.ch"},"message":"Bugsandcosmetics #299\n--\nSquashed commits contained in pull request #299\nhttps://github.com/eutelescope/eutelescope/pull/299\n--\nDescription:\n\nPoint and getImpactPoint take care of that. The new function\ngetImpactPoint has two advantages. First, it allows for an easy usage of\na track slope. So far, the track direction is set to be in\nz-direction (i.e. zero slope), but in principle one could add the slope\nof a track here. Secondly, the new function does not require matrix\ninversion, which makes it more efficient.\n\nEUTelGeometryTelscopeGeoDescription.cpp\n2.) In order to make the rotation-order consistent, the\nEUTelGeometryTelscopeGeoDescription.cpp was changed in order to have the\nrotation-order: first around the global X-axis, then around the global\nY-axis and finally around the global Z-axis. Since this also goes into\nthe HitMaker, all rotations in the HitMaker now have the order\nX,Y,Z. After this change, the rotation order of the HitMaker, the\nEUTelGeometryTelscopeGeoDescription, the Alignment (EUTelMille.cc), the\nEUTelProcessorApplyAlignment.cc and the EUTelTestFitter.cc are the\nsame. If this change should be rejected, the rotation order in all\nmentioned files should be checked for consistency. Additionally, the\nrotation order in our next pull request, from the branch analysisupdate,\nalso has to be changed correspondingly. I also suggest to document\nsomewhere, which rotation-order is used. On long-term basis one could\nalso consider making the rotation order a parameter, for example from\nthe config-file.\n\nEUTelMille.cc\n3.) The binsize and the plot ranges of the histograms drawn by\nEUTelMille.cc were increased, since reading the resulting histograms\notherwise was difficult for our data.\n\nsteering-template files\n4.) Some purely cosmetic changes were applied to some steering-template\nfiles.","distinct":false,"url":"https://api.github.com/repos/freidt/eutelescope/commits/b83e2bdade1846a7d7459cb4616b446d9d01ef83"},{"sha":"eecfd0d1c63cae6836d722296e426074c7cc4787","author":{"name":"Felix Reidt","email":"113228c8841ada9d7aa7d525df0c56d24f56b508@cern.ch"},"message":"Analysisupdate #300\n--\nsquashed commits contained in pull request #300\nhttps://github.com/eutelescope/eutelescope/pull/300\n--\nDescription:\n\nThe changes here affect the EUTelProcessorAnalysisPALPIDEfs.cc only. I.e. only changes to code from the ALICE testbeam analysis software were done. These changes are:\n\n1.) The way the RemoveAlign function, which removes the alignment from aligned data, removes the alignment, was made consistent with way the EUTelProcessorApplyAlignment.cc applies the alignment.\n\n2.) The rotation order in the _EulerRotationBack function was made consistent with the X, Y, Z order from the previous pull-request. If this order should have been changed, please also alter this order, such that it is the inverse of the order, in which the rotations are applied. This refers in particular to the order, in which rotations are applied in the EUTelGeometryTelescopeGeoDescription.cpp.\n\n3.) Some code was put into the function _LayerRotationBack, to make the overall code more readable.\n\n4.) Some other, purely cosmetic changes were added.","distinct":false,"url":"https://api.github.com/repos/freidt/eutelescope/commits/eecfd0d1c63cae6836d722296e426074c7cc4787"},{"sha":"abf0aed0ddf82bb91658a820744f48291bf30cf9","author":{"name":"Felix Reidt","email":"113228c8841ada9d7aa7d525df0c56d24f56b508@cern.ch"},"message":"added ALPIDE (pALPIDE-4) with a single sector","distinct":false,"url":"https://api.github.com/repos/freidt/eutelescope/commits/abf0aed0ddf82bb91658a820744f48291bf30cf9"},{"sha":"b831ec5bd575a4a27388bf74578b2a70148317e7","author":{"name":"Felix Reidt","email":"113228c8841ada9d7aa7d525df0c56d24f56b508@cern.ch"},"message":"chipVersion 5: ALPIDE but split into 4 sectors to extract the resolution using a pALPIDE-1 telescope","distinct":false,"url":"https://api.github.com/repos/freidt/eutelescope/commits/b831ec5bd575a4a27388bf74578b2a70148317e7"},{"sha":"c92811522d54b36a358d0508913cc45685d646d7","author":{"name":"Felix Reidt","email":"113228c8841ada9d7aa7d525df0c56d24f56b508@cern.ch"},"message":"added log messages for events in which the DUT does not see the track","distinct":true,"url":"https://api.github.com/repos/freidt/eutelescope/commits/c92811522d54b36a358d0508913cc45685d646d7"},{"sha":"25cf937104a008fcf8c5f3807e21e0dc091b74f8","author":{"name":"Felix Reidt","email":"113228c8841ada9d7aa7d525df0c56d24f56b508@cern.ch"},"message":"cleaning up and commenting","distinct":true,"url":"https://api.github.com/repos/freidt/eutelescope/commits/25cf937104a008fcf8c5f3807e21e0dc091b74f8"}]}
{"actor":{"display_login":"freidt"}}