  This study aims to assess the properties and classification of 62 variable
stars in Cygnus, little studied since their discovery and originally reported
in the Information Bulletin on Variable Stars (IBVS) 1302. Using data from
previous studies and several astronomical databases, we performed our analysis
mainly utilizing a period analysis software and comparing the photometric
characteristics of the variables in a Colour-Absolute Magnitude Diagram. For
all stars, the variability is confirmed. We discovered new significant results
for the period and/or type of 17 variables and highlighted incorrect
cross-reference names on astronomical databases for 23 stars. For 3 stars,
whose original type was unknown, we propose a new type. We calculated an epoch
of a minimum or a maximum for 24 stars; for 3 of them, the epoch has been
defined for the first time. This assessment also identifies some cases for
which results from the ASAS-SN Catalog of Variable Stars are not consistent
with results from Gaia DR2 and/or our analysis.
