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Code Block
titleLogin to psana node and set lcls2 environment on pcds
collapsetrue
ssh -Y pslogin.slac.stanford.edu
ssh -Y psana
source /cds/sw/ds/ana/conda1/manage/bin/psconda.sh
Code Block
titleLogin to psana node and set lcls2 environment on s3df
ssh -Y s3dflogin.slac.stanford.edu
ssh -Y psana
source /sdf/group/lcls/ds/ana/sw/conda2conda1/manage/bin/psconda.sh

Code examples

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Code Block
kwa = <dict-of-mask-parameters>
a = o.calib(evt, cmpars=(7,2,100,10), **kwa)
a = o.image(evt, nda=None, **kwa) # reduced shape for available segment only
a = o.image(evt, nda=None, value_for_missing_segments=800, **kwa) # full image including missing segments

Calibration constants

All detector calibration constants (np.array) and associated  metadata (dict) are available through the dictionary det.calibconst with calibration type as a key. For example:

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