Small telescopes being effective: MAGIC or not?
The paper describes the MAGIC multi-mode focal reducer (Monitoring of Active Galaxies by Investigation of their Cores), commissioned on the 1-m Zeiss-1000 telescope of the Special Astrophysical Observatory of the Russian Academy of Sciences in September 2020. Three observational modes are currently...
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Main Authors | , , , , , , |
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Format | Journal Article |
Language | English |
Published |
23.09.2023
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Subjects | |
Online Access | Get full text |
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Summary: | The paper describes the MAGIC multi-mode focal reducer (Monitoring of Active
Galaxies by Investigation of their Cores), commissioned on the 1-m Zeiss-1000
telescope of the Special Astrophysical Observatory of the Russian Academy of
Sciences in September 2020. Three observational modes are currently realised:
photometry, polarimetry, and long-slit spectroscopy. Reducing the focal length
makes it possible to obtain a sufficiently large field of view for photometry
and a large slit height for spectroscopy of $\sim$12$'$, as well as a large
field of view for polarimetry with a quadrupole Wollaston prism of
$\sim$6$'$.4. This feature makes the complex study of extended nebulae and
galaxies efficient. The MAGIC capabilities are presented in examples of
observations of various astronomical objects. The spectral mode in the range of
4000-7200 AA provides the spectral resolution $R \sim$ 1000; for a starlike
target up to 14 mag in medium-band filters with a seeing of 1$''$ for 20
minutes of total exposure, the photometry accuracy is better than 0.01 mag and
the polarization accuracy is better than 0.6%. Especially for the new focal
reducer, an offset guide and a position angle rotation system were implemented.
The results of the modernization of the baffle system in the optical scheme of
the telescope for the suppression of scattered light are also described. |
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DOI: | 10.48550/arxiv.2309.13371 |