  We cross-correlate \hip\ main-sequence star catalog with \fis\ catalog, and
identify 136 stars (at $>90$% reliability) with far-infrared detections at
least in one band. After rejecting 51 stars classified as young stellar
objects, Be stars, other type stars with known dust disks or with potential
contaminations and 2 stars without infrared excess emission, we obtain a sample
of 83 candidate stars with debris disks. Stars in our sample cover spectral
types from B to K-types with most being early types. This represents an unique
sample of luminous debris disks that derived uniformly from all sky survey with
a spatial resolution a factor of two better than the previous such survey by
\iras. Moreover, by collecting the infrared photometric data from other public
archives, 85% of them have infrared excesses in more than one bands, allowing
the estimate of the dust temperatures. We fit the blackbody model to the broad
band spectral energy distribution of these stars to derive the statistical
distribution of the disk parameters. 7 stars require an additional warm
component of temperature around 200 K. While a substantial fraction of our
sample(58 stars) have weak 12 \micron\ excess indicating that a warm dust
component maybe common among these bright debris disk systems.
