In a UV table, there can be a telescope pair column (code code_uvt_tele, see value in Appendix C). It
describes the pair of telescopes used for the given baseline.
This column is directly linked to the telescope section possibly
available in any GDF file. The pair value is an integer equal to
, where
is a factor
available in the telescope section, and
is the telescope
number from this section (corresponding to antenna
for the
baseline
). This allows to identify each telescope (in
particular its diameter). If there is only one telescope for the given
baseline, only
is saved. Decoding
is then simple and generic:
if (pair.gt.magic) then itele(iant) = pair/magic itele(jant) = pair-itele(iant)*magic else itele(iant) = pair itele(jant) = pair endifThe respective diameter for each antenna is then h%gil%teles(itele(xant))%diam.