Up: The Hipparcos transit data: how?
Fortran programs interfacing the TD with aperture synthesis software
and with GaussFit are available via the Lund Observatory Internet address
http://www.astro.lu.se/
lennart/TD/.
The program td2uv.f extracts the TD for a given HIP identifier and
converts them into a UV-FITS file that can be used e.g. by Difmap.
The program td2gf.f similarly extracts TD data and generates
a data file suitable as input for GaussFit. Sample data files,
additional information on the TD (including descriptions of the
known errors), and links for retrieving aperture synthesis software
and GaussFit are also given at this site.
Up: The Hipparcos transit data: how?
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