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) |