Zobrazeno 1 - 5
of 5
pro vyhledávání: '"D. J. Casperson"'
Autor:
Konstantin N. Borozdin, Katherine E. McGowan, W. T. Vestrand, P. R. Wozniak, Robert White, D. J. Casperson, Jim Wren, D. Starr, M. Galassi, E. E. Fenimore
Publikováno v:
Astronomische Nachrichten. 325:549-552
Laboratory. RAPTOR is a fully autonomous robotic system that is designed to identify and make follow-up observations of optical transients with durations as short as one minute. The RAPTOR design is based on Biomimicry of Human Vision. The sky monito
Autor:
J. Wren, Robert White, David C. Thompson, W. T. Vestrand, R. Shirey, E. Raby, D. J. Casperson, C. Ho
Publikováno v:
AIP Conference Proceedings.
With the coming launch of the Swift satellite, there will be many new opportunities to study the physics of the prompt optical emission from gamma ray bursts with robotic ground‐based telescopes. We discuss a new imaging system under development at
Autor:
Katherine E. McGowan, M. Galassi, D. Starr, S. Davidoff, P. R. Wozniak, W. T. Vestrand, J. Wren, Robert White, H. Davis, D. J. Casperson, E. E. Fenimore, Konstantin N. Borozdin
Publikováno v:
AIP Conference Proceedings.
While it has been known for centuries that the optical sky is variable, monitoring the sky for optical transients with durations as short as a minute is an area of astronomical research that remains largely unexplored. Prompt follow‐up observations
Autor:
K. E. McGowan, Steven P. Brumby, Przemyslaw Wozniak, D. J. Casperson, W. T. Vestrand, D. Starr, Robert White, Konstantin N. Borozdin, Simon Perkins, E. E. Fenimore, Galen Gisler, William C. Priedhorsky, M. Galassi, Jim Wren
Publikováno v:
AIP Conference Proceedings.
A rich, but relatively unexplored, region in optical astronomy is the study of transients with durations of less than a day. We describe a wide‐field optical monitoring system, RAPTOR, which is designed to identify and make follow‐up observations
Autor:
K. Borozdin, D. J. Casperson, E. Fenimore, M. Galassi, K. McGowan, D. Starr, R. R. White, P. Wozniak, J. Wren
Publikováno v:
Astronomische Nachrichten; Oct2004, Vol. 325 Issue 6-8, p549-552, 4p