Abstract
In this paper we report about 100 new M dwarfs, confirmed in the DFBS database. The DFBS is the
digitized version of the First Byurakan Survey (FBS, or Markarian survey). FBS plates have been used to
search and study faint Late-Type Stars (LTS). The confirmations is based on Gaia DR3 BP/RP spectral
database. In previous studies of the DFBS plates, these objects were presented as LTS candidates. TESS
phased light curves for some of them shows flares. In SEDs of these objects the infrared excess is clearly
visible.
Publisher
National Academy of Sciences of the Republic of Armenia
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