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In this paper we present a catalog which includes 141 bright candidates($\leq10.27$ mag, V band) showing the infrared (IR) excess at 22 $\mu$m. Ofwhich, 38 stars are known IR excess stars or disk, 23 stars are double ormultiple stars and 4 are Be stars. While the remaining more than 70 stars areidentified as the 22 $\mu$m excess candidates in our work. The criterion ofselecting candidates is $K_s-[22]_{\mu m}$. All these candidates are selectedfrom \emph{WISE} All-sky data cross-correlated with \emph{Hipparcos} MainCatalog and the likelihood-ratio technique is employed. Considering the effectof background, we introduce the \emph{IRAS} 100 $\mu$m level to exclude thehigh background. We also estimated the coincidence probability of thesesources. In addition, we presented the optical to mid-infrared SEDs and opticalimages of all the candidates, and gave the observed optical spectra of 6 starswith NAOC's 2.16-m telescope. To measure for the dust amount around each star,the fractional luminosity is also provided. We also test whether our method ofselecting IR excess stars can be used to search for extra-solar planets, wecross-matched our catalog with known IR-excess stars having planets but none ismatched. Finally, we give the fraction of stars showing IR-excess for differentspectral type of main-sequence stars.

Bright 22 $\mu$m Excess Candidates from WISE All-Sky Catalog and Hipparcos Main Catalog