  NSV 14264 and NSV 14172 are suspected to be variable stars of RR Lyr type
(Brun, 1964). They were observed during three nights in October 2018 with a
25cm diameter telescope. These observations completed by ASAS-SN survey data
bring to the conclusion that these two stars are not RR Lyraes but constant
stars in the limit of the precision of the present photometry. The analysis of
GAIA data allows to say that NSV 14264 is a main sequence dwarf similar to the
Sun but that NSV 14172 is a yellow giant star located in the HR diagram at the
limit between RR Lyraes and CW cepheids; however, it does not pulsate with
significant amplitude.
