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bug
bug
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documentation
documentation
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duplicate
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O1
O1
Understanding the effects of crowding on LSST astrometry
O2
O2
Using that understanding to create a model of the astrometric uncertainties
O3
O3
Combining model w/ photometric information to provide cross-matches between LSST & other catalogues
question
question
Further information is requested
testing
testing
Intermediate tests of DAC-run cross-matches
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Waiting for