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M. Born, Emil Wolf, Eugene Hecht (1999)
Principles of optics : electromagnetic theory of propagation, interference and diffraction of lightPhysics Today, 53
V. Debur, T. Arkhipova, G. Beskin, V. Plokhotnichenko, M. Pakhomov, M. Smirnova, A. Solin (2003)
Position-sensitive detector for the 6-meter optical telescope
M. Born, E. Wolf (2019)
Principles of Optics
V. Plokhotnichenko, A. Solin, A. Tikhonov (2009)
The “Quantochron 4-48” facility for registration of random fluxes of multidimensional signalsAstrophysical Bulletin, 64
E. Oliva (1997)
Wedged double Wollaston, a device for single shot polarimetric measurementsAstronomy & Astrophysics Supplement Series, 123
V. Plokhotnichenko, G. Beskin, V. Debur, A. Panferov, A. Panferova (2003)
The multicolor panoramic photometer-polarimeter with high time resolution based on the PSDNuclear Instruments & Methods in Physics Research Section A-accelerators Spectrometers Detectors and Associated Equipment, 513
G. Beskin, V. Komarova, S. Neizvestny, V. Plokhotnichenko, M. Popova, A. Zhuravkov (1997)
The Investigation of Optical Variability on Time Scales of 10-7-102S: Hardware, Software, ResultsExperimental Astronomy, 7
M. Born, E. Wolf (1999)
Principles of optics : electromagnetic theory of propagation, interference and diffraction of light
G. Beskin, V. Debur, V. Plokhotnichenko, Sergey Karpov, A. Biryukov, L. Chmyreva, A. Pozanenko, K. Hurley (2007)
Search for fast optical activity of SGR 1806-20 at the SAO RAS 6-m telescopeAstrophysics and Space Science, 308
Sergey Karpov, G. Beskin, A. Biryukov, V. Debur, V. Plokhotnichenko, Michael Redfern, A. Shearer (2006)
Short time scale pulse stability of the Crab pulsar in the optical bandAstrophysics and Space Science, 308
A hardware and software complex of the MANIA experiment designed to search for and study the photometric variability of astrophysical objects with a temporal resolution of 10−6 s is described. The panoramic photospectropolarimeter uses interchangeable optical units, which allow the observations to be performed in four modes—spectroscopic, spectropolarimetric, photometric, and polarimetric. A coordinate—sensitive detector equipped with a set of microchannel plates is capable of recording flux fluctuations from objects and comparison stars simultaneously in different photometric bands and in different polarization planes. The Quantochron 4–48 data acquisition facility operating on line with a computer acquires observational data with a temporal resolution of 1microsecond. The methods of analysis of panoramic data with high temporal resolution are discussed.
Astrophysical Bulletin – Springer Journals
Published: Aug 21, 2009
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