C2A can access and display the Tycho-2 catalogue.
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The K - range spanned by the normal stars is much smaller than the V T - range because we now probe the Rayleigh-Jeans tail of the spectral energy distribution for all stars. The resulting data is of wonderful quality, with small astrometric residuals suitable for last-minute astrometry to improve occultation predictions and for use in computing the orbit of Eros for the NEAR mission.
Abstract Stars of all evolutionary phases have been found to have excess infrared emission due to the presence of circumstellar material. The F-, G- and K-type stars have fewer excess objects. Wicenek of the ESO. To resolve the situation we have looked at the spectral energy distributions of the subsample with IRAS detections. With the arrival of Tycho-2 , the ACT is now obsolete.
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- THE TYCHO-2 CATALOGUE IS AN ASTROMETRIC REFERENCE CATALOGUE CONTAINING POSITIONS, PROPER MOTIONS...
- THE POSITIONS AND MAGNITUDES OF THE STARS IN THE TYCHO-2 CATALOGUE HAVE IN THE TYCHO-2 CATALOGUE...
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Right now, you can get A1. I think the magnitudes may be better than those from A2. Perhaps unsurprisingly, the carbon stars follow a similar band as the M stars. It has only one small defect, relative to B1.