All Tables

• Table 1: Magnitude ranges and means in the I filter, and relative to absolute corrections in milliarcseconds as found from the Mendez & van Altena galaxy model.
• Table 2: Parallaxes and proper motions for the six white dwarf candidates in the Torino Program. See text for explanation of columns.
• Table 3: Parallaxes of two binary systems.
• Table 4: Observations from the Fourth Yale Parallax Catalogue for the determination of the parallax of 1716+020.
• Table 5: Absolute magnitudes calculated from TOPP parallaxes and apparent magnitudes along with those derived in MCC99 from spectrophotometry, the code indicates the method used: 2 = multichannel spectrophotometric colors, 3 = uvby colors.