Abstract:
Using CCD observations, photometric magnitudes have been obtained in two galactic directions at intermediate latitude. A total of 7 sub-fields in one direction (l = 3°, b = 47°) have been observed leading to photometric magnitudes for 52 stars. In the second direction (l = 278°, b = 47°) a total of 10 sub-fields have been observed yielding photometric magnitudes for 139 stars. The magnitude range covered is 13< V < 19.
