In archaeoastronomical orientation purposes. employing appropriate software
, the star declination (D) is determined from the geographical coordinates
of the site, the plate bearing of the horizon point (azimuth, Az), and the
altitude of the horizontal point (skyline), with appropriate corrections. E
rrors to the second of a degree in latitude have not any apparent effect on
D, errors in Az and latitude of the skyline, however, transmit significant
respective percentage errors in D. This note discusses the impact of such
error variation on all parameters involved in archaeoastronomical orientati
on, and presents the case of two small sized pyramidals in Greece.