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ItemWhoPre-Meeting NotesNotes and  Action Items
Project/Science updates

No PST meeting last week. Next PST meeting 2022-10-19

  • SR interested in algorithms for CR removal. 
  • JB: Assumption that DI will remove all CRs 
  • EB: AP did a big push on this a few months ago - existing stack algorithm performs well. Slides from the cosmic ray analysis earlier this year
  • GPDF: Presumption of the same answer for every band? No
  • SR: 1x30 per u band and 2x15 in the other band. Operational complexity will remain if no decision to abandon the complexity of 2x15
  • JB: Could stop a lot of work if we make this decision to abandon 2x15.  
Calibration end-to-end flowPresentation of the new calibration end-to-end flow following the CalibPalooza workshop. 
  • Flow chart presented is the order of operations agreed at CalibPalooza and will form the outline for the construction paper for calibration. 
  • Red - work that is not done yet, Black - something is in place.
  • Earlier we can combine snaps, the less expensive it is. 
  • JB: Most steps before BF are fast - as long as we do snap combine < BF we are fine. BF is not fast
  • XT correction is per detector - no evidence for inter-detector XT
  • SR: make clear after each step what the units are 
  • ER: Yes, some are still under debate. Will be electron-like of ADU-like Awaiting a writeup from Pierre
  • GPDF: Figure out what processing is needed in the RT system - rapid analysis producing a post-ISR output. 
  • ER: Will be rewriting ISR task  - for QL rapid analysis various steps can be turned off  - expect most to be fast except BF. e.g. variance plane doubles the size of every image 
  • CTS: Is the purpose of diving by gain primarily to get normalization btw amps or to get electrons
  • ER: 100% primary purpose is normalization btw amps - this cannot be captured by a FF  its a model that depends on 2 temperatures.  And - it would be nice to normalize the gains at the same point and bring them all to 1.
  • ER: Critical issue learnt from AT is that if calibration products re run in a diff. sequence to what there are used there are problems.  
  • LPG: What is the con of normalization at the same time as gain normalization? 
  • ER: Does not understand RHL's concern. 

Post ISR - Now new plans for FFing. The dream of doing FFing better

  • Need to be careful with flats to no t introduce unintended effects. 
  • Subtract fringes was not discussed at CP - ER's thinks it goes aft Subtract BKG. 
  • Do we need a bespoke sly SED when processing or is a reference SED OK? TBD - complicated.
  • fCBP encompasses a lot of work
  • KB: How do we know in a data driven way, which are lateral e-field effects or quantum efficiency effects 
  • ER: Most ate lateral e-field  effects. The 3 listed things we have physical models - develop a template for each and remove it. Not using astrometric residuals. 
  • SR: QE dominated by variations in the anti reflective coating - agree to make evaluation of residual leftovers data driven. 
  • KB: I hope that we will have quasi-independent methods for verification and validation based on on-sky data. This will take some thought.
  • SR: mentioning techniques to be used to assess residuals. Can use on-sky data to evaluate or verify residuals
  • ER: No box for amp-to-am matching - hope that GN does it correctly and no bogus aa-to-a matching is needed. If this is messed up it affects background measurement
  • YAS: amp-to-amp matching could be done in  PCA box. Cannot assume that GN will be done perfectly. 
  • LPG: Withouth RFF without CBP version we are still beyond state of the art due to the different use of MDF
  • DF may fail  -most likely place for dust to change is on the filters - filter change operation will probably move the dust around so once at the beginnign of the night will not work. 
  • RSN: Is there an existing one that is sufficient?? No - what are we missing without this?
  • ER: If Gaia SP gets to the point of being better than our internal - GDR3 is worse than internal. But if in a few years and are down to 17th mag and ave synth ugrizy to mmag level then we can use it and get better calibration.
  • KB: ETA of cell based coadds? 
  • YAS: next summer
  • ER: Cell size is 250x250 incl. boundary 
  • CTS: 
  • LPG: Important to have a CBP/non-CBP route + prioritization scheme
  • ER: CP follow up to discuss prioritiation

#refcats channel to help out on the monster

AOB

Our fortnightly scheduled has shifted. New schedule until end of year TBD

No meeting next week due to LSST@Europe.

Next meeting is: (also the week of ADASS). 



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