Wondering what to do with the NondetectionLimit in the LSST alert schema. Before arranging the storage of a few billion of these, I’d like to know what they mean!
There are only 4 attributes in the schema:
- ccdVisitId
- midPointTai (== MJD)
- filterName
- diaNoise
I am guessing that the last of that list is the payload. Does the diaNoise have units of nanoJansky, like the source flux?
For analysis of light curves, we would quote a 5 sigma upper limit, since the a diaSource is created on the condition that psfFlux >=5 sigma. Is diaNoise the 1-sigma noise measurement? Therefore the flux upper limit is 5-sigma = 5*diaNoise?
I am also guessing that the NondetectionLimit packet only appears within an alert, so that a diaObjectId and its sky position can be inferred, is that right?