Interferometry among telescope arrays has become a standard technique in astronomy. We discuss using quantum repeaters to increase the baseline length, and therefore resolving power, of telescope arrays at optical observing frequencies.

© 2011 Optical Society of America

PDF Article


You do not have subscription access to this journal. Citation lists with outbound citation links are available to subscribers only. You may subscribe either as an OSA member, or as an authorized user of your institution.

Contact your librarian or system administrator
Login to access OSA Member Subscription