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UV Dataset

A MIRIAD uv dataset is composed of a collection of items and `$u-v$ variables'. The variables are parameters that are known at the time of the observation, and include measured data, and the description of the observation set up (e.g. correlator set up and observing centers).

Table D.1 gives a list of the items that are used to build up a MIRIAD uv dataset.


Table D.1: MIRIAD items in a uv visibility dataset
Item name Type Description
obstype ascii value: `cross', `auto' or `mixed'
history text history text file (in principle editable)
vartable text lookup table for all uv variables (never edit!)
visdata mixed data stream of uv variables
flags integer optional flags for narrowband data
wflags integer optional flags for wideband data
gains mixed antenna gain table; delhd (or rm) this item to disable gain table
bandpass complex bandpass function gains; delhd (or rm) this item to disable passband corrections
freqs mixed frequency set up description table for `bandpass'
nspect0 integer number of windows in the bandpass function
nchan0 integer total number of channels in the bandpass function
nfeeds integer number of feeds on each antenna
ntau integer Number of delay/spectral index terms per antenna in `gains'
nsols integer number of records in `gains'
ngains integer number of antenna gains in each record of `gains'
interval double gain interpolation time tolerance (days)
freq0 double reference frequency for delay terms
leakage complex polarization leakage parameters
cgains complex baseline based channel gains
ncgains integer  
ncbase integer  
wgains complex baseline based wideband gains
nwgains integer  
nwbase integer  

SADLY, the latex2html converter does not deal with this table very well, please consult the online PDF version for this table


next up previous contents index
Next: Telescope specific notes Up: UV Variables Previous: UV Variables
Peter
2009-10-05