When presenting the time history, how would you suggest handling the confused
fluxes? I thought for LSST that the deep detection was running
infrequently, not constantly.
As the template improves, the instance of confused Astronomical
Objects will diminish,
but confused flux measurements will still exist. And the confused
Astronomical Objects
will still need to be handled in the first several sky coverages.
Each night we'll be analysing the data for variables, and these variables
will be stuffed into a database (which will be public, as will all LSST
data). There will be cases of pairs of variable objects that need to be
handled as the seeing comes and goes.
However, the deep detection stuff will be run simultaneously on all the
data that we have in hand, and this will assign unique IDs to OBJECTS
not to detections. T
--
---------------------------------------------------------
Deborah Levine, Ph.D. (626)395-8567 (Office)
Operations Scientist (626)590-7500 (Mobile)
(626)568-0673 (FAX)
Spitzer Science Center [EMAIL PROTECTED]
Mail Code 314-6, Pasadena, CA 91125 text messaging : [EMAIL PROTECTED]
"Make everything as simple as possible, but not simpler."
Albert Einstein
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