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The user pipeline
The pipeline products for each experiment, along with a wealth of other
information, can be accessed online via the
EVN Data Archive: Select the EVN experiment
form the pull-down list. Clicking on ``Show experiment <XXnnn>'' will open the
archive page for the selected experiment with links to all archived data
products.
The calibration tables are stored as a FITS file and can be found among the
pipeline calibration products. This file was written out
from AIPS using TASAV and can be copied to the multi-source
file in AIPS using TACOP. The tables that are contained in
the TASAV FITS file are:
- CL - calibration tables. There should be three of these
attached to your data.
- CL1 - virgin calibration table.
- CL2 - amplitude calibration. If any corrections have been
made for telescope positions or axis offsets post-correlation
(due to more precise measurements since) then they will be included
here. The parallactic angle correction will also be found here.
- CL3 - delay, rate and phase calibration (fringe-fit).
- BP - bandpass calibration.
- AN - antenna table. If corrections to telescope positions or
axis offsets have been made then the AN table will have been updated.
- FG - flag table. This will include flags based on slew times
calculated by the Sched scheduling tool or directly from the
antenna control information for experiments observed since session 3
(November) 2002 (for those antennas that have this implemented). There
will also be flags that remove the edge (noisy) channels in the bandpass.
- TY - antenna system temperatures.
- GC - antenna gain curves.
Next: 2 Obtaining your data
Up: 1 Introduction
Previous: Example: N02L1
Contents
Stefanie Muehle
2008-01-28