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Run 2.1 preflight checklist #188
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I accidentally left out issue #178 -Determining the list of headers to add to the primary HDU. Now it is in the list. |
Of the items listed above, I think only a few are strictly needed to proceed with Run2.1i:
The first one listed here entails a release tag of GalSim at v2.1 and a corresponding lsst_sims release. The third one would be implemented in |
Scott has confirmed that the sky brightness fix is in 2_11 (oops crossed with Jim above) |
Well, I agree the first three in the list are the ones that are absolutely necessary to be able to run the program, but I think in particular skipping:
would be very problematic. Those both include things that we have to or should add at run time that we need later to use the files for testing, processing and analysis. I agree the e-image fix is not necessary but I think would be useful for early running based on our experiences so far trying to process things through DM. I put the performance issue in since, in the discussion, I thought there were a few things that Mike still wanted to check and I wanted it there as a reminder to make sure we either have signed off on it being done for now, or knew there would be more changes down the line. |
I moved the performance check into a separate sub-list following Jim's suggestion. |
In that new category I also added partially implementing binary instance catalog format as a possibility as Jim suggested at the last imSim video meeting. There are more details in #71. |
I agree these would be nice to have, but I don't see how they are strictly necessary. We already know that the current headers allow the data to be processed through the coadd and forced photometry of the drp processing, and we won't even have centroid files for real data. #178 is also a moving target--so we can add what's requested now (even though we know those items aren't needed for processing), but until we have a complete list, that issue won't be closed before (assuming it ever is) we would want to have Run2.1i data in hand. |
Re: discussion of #185 and #178:
|
@cwwalter - my impression had been that the SED simplification would only be used for galaxies faint enough that they aren't part of a canonical WL/LSS sample, and so we wouldn't care about their photo-z (only what they do to the photo-z of others nearby, which should be minimally affected by the SED simplification). If somebody can remind me what flux criterion we're using in each band, I can confirm this given a typical magnitude or SNR cut and typical galaxy colors. |
It's <100 photons for single epoch, which I believe converts to m > 26. (Assuming zeropoint = 31) |
But also, I agree with Chris that this would be vv good to have this information in the output truth catalog regardless of whether we are using these objects for WL or PZ. |
Removing partially implementing binary instance format for this list now due to time constraints. We will work on this next year. |
#130 is now closed but lsst/obs_lsst#41 should be merged into the new obs_lsst package. |
lsst/obs_lsst#41 has now been merged. |
Here is a master list of issues to address before we can start 2.1i:
Please check these off when we know we have stopped performance optimization for the 2.1 run time scale.
Test for correctness (these tests might be tracked elsewhere; no issues yet)
Note: to see a good overview the issues which are grouped in columns, look at this project:
https://github.com/LSSTDESC/imSim/projects/1
Keep up-to-date and note changes in comments below.
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