Abstract

Since the release of LAMOST (the Large Sky Area Multi-Object Fiber Spectroscopic Telescope) catalog, we have the opportunity to use the LAMOST DR2 stellar catalog and \emph{WISE All-sky catalog} to search for 22 μμm excess candidates. In this paper, we present 10 FGK candidates which show an excess in the infrared (IR) at 22 μμm. The ten sources are all the newly identified 22 μμm excess candidates. Of these 10 stars, 5 stars are F type and 5 stars are G type. The criterion for selecting candidates is Ks−[22]μm≥0.387K_s-[22]_{μm}\geq0.387. In addition, we present the spectral energy distributions (SEDs) covering wavelength from optical to mid-infrared band. Most of them show an obvious excess from 12 μμm band and three candidates even show excess from 3.4 μμm. To characterize the amount of dust, we also estimate the fractional luminosity of ten 22 μμm excess candidates.

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