12meter data is often taken with the 25Hz
winking cal to help correct for electronic gain variations.
This includes
A set or idl routines checks for any spectral line scans with
the winking cal data (the pulsar data is not
currently processed). The routines will:
To compute tsys the following routines are
used:
At then end of each month all the data from the previous
month is included in a set of plots..
The data is processed from a cron job that
phil runs every morning around 3:30 am. It always takes the
previous day as the basis for the plots (so you'll have to
wait for the next day to see what happens on a particular
experiment.)
Each set of plots contains:
date (yymm) 
plots 
notes 
2303 
nodata 

2302 

no data 
2301 
(.ps) (.pdf) 

2212 
(.ps) (.pdf) 
has a few tsys measurements, end of dec 
2211 
(.ps) (.pdf) 

2210 
no data 

2209 
(.ps) (.pdf) 

2208 
(.ps) (.pdf) 

2207 
(.ps) (.pdf) 

2206 
(.ps) (.pdf) 
220627: measured cals with sky,absorber 
2205 
(.ps) (.pdf) 