Alpha Per faint stars photometry (Barrado y Navascues+, 2002)
We obtained deep optical imaging of the Alpha Per open cluster using the KPNO 4-m CCD mosaic camera, MOSA, on November 19-22 1998. All of the images were obtained with the facility R and I filters. In addition to the KPNO/MOSA observations, we undertook several infrared observing campaigns at the Hispano-German Calar Alto Observatory in order to
Barrado Y Navascues, D. et al.
Fecha de publicación:
1
2003