You signed in with another tab or window. Reload to refresh your session.You signed out in another tab or window. Reload to refresh your session.You switched accounts on another tab or window. Reload to refresh your session.Dismiss alert
Does this include Neil's latest updates on scan strategy here?
What happens to subscan information? Do we have the turnarounds? How do you identify the subscans in the TOD?
The text was updated successfully, but these errors were encountered:
No it does not include Neil's latest updates on scan strategy but this is something I can add it (slide 4 is exactly what I need)! Let me know if you need it.
subscan information: For the moment there is none, i.e. a timestream is one unique long vector. However, I have already a routine to define those (tod.TimeOrderedDataPairDiff.get_timestream_masks) if needed.
turnarounds: not implemented yet, but can be done easily given that we have the telescope velocity (just mask TOD when v isn't constant).
How do we identify the subscans in the TOD? That's up to us. The most common way is to define each sweep in azimuth as a subscan.
Let me know whether you want me to implement asap points 2 - 4.
Does this include Neil's latest updates on scan strategy here?
What happens to subscan information? Do we have the turnarounds? How do you identify the subscans in the TOD?
The text was updated successfully, but these errors were encountered: