Open javierggt opened 2 years ago
Looking at the new page at https://cxc.cfa.harvard.edu/mta/ASPECT/jgonzalez/celmon/mta/ , it has been so long since I've looked at it that I've forgotten how to interpret it.
Previously we'd look at celmon pages with the question of "is it still basically OK or do we need to update CALALIGN". How does one answer that question now?
Previously we'd look at celmon pages with the question of "is it still basically OK or do we need to update CALALIGN". How does one answer that question now?
In what way is this different from before?
A "proper" way to answer this could be to look at whether a fixed number N of points deviate by more than x-sigma, with N and x still to determine. This page does not answer that, and neither did the old one.
This one at least gives a band to give you an idea, because just a scatter plot does not convey that.
Does the band tell me what corrections we've already put in CALALIGN or does it show me the offsets we should put in the next one?
it tells you the offset in the latest processing of the OBSID. In this case it is a mixed state, because if we were to reprocess the data for OBSIDs before the CalDB was updated, then we would see no offset. OBSIDs from after the CalDB update should (in principle) show no offset.
It is a valid question, whether we should reprocess everything with the latest CalDB, but that is not what astromon does currently.
There are two versions of celmon pages. Both have been modified in the latest astromon release, and are updated on a weekly basis. The change should be approved before going online.
These pages are saved in
$SKA/data/astromon/web
. For them to replace the older versions, the only thing we need to do is to create symbolic links (on$SKA
):