pith. sign in

arxiv: 1411.2552 · v2 · pith:SMEIML2Anew · submitted 2014-11-10 · 🌌 astro-ph.IM

The first light of Mini-MegaTORTORA wide-field monitoring system

classification 🌌 astro-ph.IM
keywords systemlightdegreeseitherfirstmini-megatortoramonitoringoptical
0
0 comments X
read the original abstract

Here we describe the first light of the novel 9-channel wide-field optical monitoring system with sub-second temporal resolution, Mini-MegaTORTORA, which is being tested now at Special Astrophysical Observatory on Russian Caucasus. The system is able to observe the sky simultaneously in either wide (~900 square degrees) or narrow (~100 square degrees) fields of view, either in clear light or with any combination of color (Johnson B, V or R) polarimetric filters installed, with exposure times ranging from 100 ms to 100 s. The primary goal of the system is the detection of rapid -- with sub-second characteristic time-scales -- optical transients, but it may be also used for studying the variability of the sky objects on longer time scales.

This paper has not been read by Pith yet.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.