ARCHIVE RATAN-600 Observation Schedule
from January 1 to June 30, 2020


Executive Secretary: request@sao.ru
Russian version

  North Sector South+Flat South Sector West Sector
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Feed-cabin 1

(01-31): Radio variability of the Galactic X-ray binaries with relativistic jets1,
Trushkin S. (SAO RAS).
Responsible Erkenov A.K.

(01-24): Radio properties of the Narrow-Line Seyfert 1 Galaxies,
Lahteenmaki Anne (Metsahovi Radio Observatory, Finland).
Responsible Erkenov A.K.

(01-24): Radio properties of the blazars on the long time scales,
Mufakharov T. (Shanghai Astronomical Observatory, China).
Responsible Erkenov A.K.

(25-31): Radio properties of OH Megamaser (OHM) galaxies,
Zhongzu Wu (Guizhou University, China).
Responsible Erkenov A.K.

Feed-cabin 3

(01-31): The Sun five-azimuth observations 4.
Responsible Milenko V.S.

Feed-cabin 2

(01-31): Radio variability of the Galactic X-ray binaries with relativistic jets1,
Trushkin S. (SAO RAS).
Responsible Erkenov A.K.

(01-31): Radio properties of the blazars on the long time scales,
Mufakharov T. (Shanghai Astronomical Observatory, China).
Responsible Erkenov A.K.

(01-31): Radio properties of the Narrow-Line Seyfert 1 Galaxies,
Lahteenmaki Anne (Metsahovi Radio Observatory, Finland).
Responsible Erkenov A.K.

Feed-cabin 3

(10-31): The Sun multi-azimuth observations 5.
Responsible Milenko V.S.

Feed-cabin 2

(01-31): Radio variability of the Galactic X-ray binaries with relativistic jets1,
Trushkin S. (SAO RAS).
Responsible Erkenov A.K.

Feed-cabin 5

(01-31): Test observations (SAO RAS).
Responsible Trushkin S.A.

F
E
B
R
U
A
R
Y

Feed-cabin 1

(01-04): Reserve time (SAO RAS)

(05-22): Radio variability of the Galactic X-ray binaries with relativistic jets2,
Trushkin S. (SAO RAS).
Responsible Erkenov A.K.

(05-15): Study of the long-term variability of the extragalactic radio sources in the declination range from 11 up to 18 degrees,
Konnikova V.K. (SAI MSU).
Responsible Erkenov A.K.

(16-22): The AGN study with the RATAN-600 and VLBI 3,
Kovalev Yu.A. (ASC).
Responsible Erkenov A.K.

(23-29): Radio variability of the Galactic X-ray binaries with relativistic jets,
Trushkin S. (SAO RAS).
Responsible Erkenov A.K.

(23-29): Radio properties of the Narrow-Line Seyfert 1 Galaxies,
Lahteenmaki Anne (FINCA, Finland; Metsahovi Radio Observatory, Finland).
Responsible Erkenov A.K.

(23-29): Radio properties of the blazars on the long time scales,
Mufakharov T. (Shanghai Astronomical Observatory, China).
Responsible Erkenov A.K.

(23-29): Radio properties of the FR0 galaxies,
Mikhailov A. (SAO RAS).
Responsible Erkenov A.K.

Feed-cabin 3

(01-29): The Sun five-azimuth observations 4.
Responsible Milenko V.S.

Feed-cabin 2

(01-29): Radio variability of the Galactic X-ray binaries with relativistic jets,
Trushkin S. (SAO RAS).
Responsible Erkenov A.K.

(01-29): Radio properties of the blazars on the long time scales,
Mufakharov T. (Shanghai Astronomical Observatory, China).
Responsible Erkenov A.K.

(01-29): Radio properties of the Narrow-Line Seyfert 1 Galaxies,
Lahteenmaki Anne (Metsahovi Radio Observatory, Finland).
Responsible Erkenov A.K.

Feed-cabin 2

(01-29): Radio variability of the Galactic X-ray binaries with relativistic jets,
Trushkin S. (SAO RAS).
Responsible Erkenov A.K.

Feed-cabin 5

(01-29): Test observations (SAO RAS).
Responsible Trushkin S.A.

M
A
R
C
H

Feed-cabin 1

(01): Radio variability of the Galactic X-ray binaries with relativistic jets,
Trushkin S. (SAO RAS).
Responsible Erkenov A.K.

(01): Radio properties of the blazars on the long time scales,
Mufakharov T. (Shanghai Astronomical Observatory, China).
Responsible Erkenov A.K.

(01): Radio properties of the FR0 galaxies,
Mikhailov A. (SAO RAS).
Responsible Erkenov A.K.

(02-29): Radio variability of the Galactic X-ray binaries with relativistic jets2,
Trushkin S. (SAO RAS).
Responsible Erkenov A.K.

(02-29): The AGN study with the RATAN-600 and VLBI 3,
Kovalev Yu.A. (ASC).
Responsible Erkenov A.K.

(30-31): Technical support,
Yakovenko S.V., Shtondin A.F.

Feed-cabin 3

(01-09): The Sun five-azimuth observations 4.
Responsible Milenko V.S.

Feed-cabin 2

(01-31): Radio variability of the Galactic X-ray binaries with relativistic jets,
Trushkin S. (SAO RAS).
Responsible Erkenov A.K.

(01-31): Radio properties of the blazars on the long time scales,
Mufakharov T. (Shanghai Astronomical Observatory, China).
Responsible Erkenov A.K.

(01-31): Radio properties of the Narrow-Line Seyfert 1 Galaxies,
Lahteenmaki Anne (Metsahovi Radio Observatory, Finland).
Responsible Erkenov A.K.

Feed-cabin 3

(10-25): The Sun multi-azimuth observations5. Testing of the antenna system (South+Flat).
Responsible Milenko V.S.

(26-31): The Sun five-azimuth observations 4.
Responsible Milenko V.S.

Feed-cabin 2

(01-31): Radio variability of the Galactic X-ray binaries with relativistic jets,
Trushkin S. (SAO RAS).
Responsible Erkenov A.K.

Feed-cabin 5

(01-31): Test observations (SAO RAS).
Responsible Trushkin S.A.

A
P
R
I
L

(01-13): Technical support,
Yakovenko S.V., Shtondin A.F.

(14-18): Adjustment, antenna measurements,
Zharov V.I.

Feed-cabin 1

(19-24): Test observations, secondary mirror focus search,
Trushkin S.

(25-26): Reserve time (SAO RAS)

(27-30): Radio variability of the Galactic X-ray binaries with relativistic jets,
Trushkin S. (SAO RAS).
Responsible Erkenov A.K.

(27-30): Study of the long-term variability of the extragalactic radio sources in the declination range from 11 up to 18 degrees,
Erkenov A.K. (SAI MSU)

Feed-cabin 3

(01-15): The Sun five-azimuth observations 4.
Responsible Milenko V.S.

Feed-cabin 2

(01-15): Radio variability of the Galactic X-ray binaries with relativistic jets,
Trushkin S. (SAO RAS).
Responsible Erkenov A.K.

(01-15): Radio properties of the blazars on the long time scales,
Mufakharov T. (Shanghai Astronomical Observatory, China).
Responsible Erkenov A.K.

(01-15): Radio properties of the Narrow-Line Seyfert 1 Galaxies,
Lahteenmaki Anne (Metsahovi Radio Observatory, Finland).
Responsible Erkenov A.K.

(16-30): Technical support,
Yakovenko S.V., Shtondin A.F.

Feed-cabin 2

(01-15): Radio variability of the Galactic X-ray binaries with relativistic jets,
Trushkin S. (SAO RAS).
Responsible Erkenov A.K.

(16-30): Technical support,
Yakovenko S.V., Shtondin A.F.

Feed-cabin 5

(01-30): Test observations (SAO RAS).
Responsible Trushkin S.A.

M
A
Y

Feed-cabin 1

(01-31): Radio variability of the Galactic X-ray binaries with relativistic jets1,
Trushkin S. (SAO RAS).
Responsible Erkenov A.K.

(01-06): Study of the long-term variability of the extragalactic radio sources in the declination range from 11 up to 18 degrees,
Konnikova V.K. (SAI MSU).
Responsible Erkenov A.K.

(07-31): Radio properties of the distant quasars,
Sotnikova Yu.V. (SAO RAS).
Responsible Sotnikova Yu.V.

Feed-cabin 3

(01-31): The Sun five-azimuth observations 4.
Responsible Milenko V.S.

Feed-cabin 2

(01-31): Radio variability of the Galactic X-ray binaries with relativistic jets,
Trushkin S. (SAO RAS).
Responsible Erkenov A.K.

(01-31): Radio properties of the blazars on the long time scales,
Mufakharov T. (Shanghai Astronomical Observatory, China).
Responsible Erkenov A.K.

(01-31): Radio properties of the Narrow-Line Seyfert 1 Galaxies,
Lahteenmaki Anne (Metsahovi Radio Observatory, Finland).
Responsible Erkenov A.K.

Feed-cabin 2

(01-31): Radio variability of the Galactic X-ray binaries with relativistic jets,
Trushkin S. (SAO RAS).
Responsible Erkenov A.K.

Feed-cabin 5

(01-31): Test observations (SAO RAS).
Responsible Trushkin S.A.

J
U
N
E

Feed-cabin 1

(01-06): Radio properties of the distant quasars,
Sotnikova Yu.V. (SAO RAS).
Responsible Sotnikova Yu.V.

(01-13): Radio variability of the Galactic X-ray binaries with relativistic jets1,
Trushkin S. (SAO RAS).
Responsible Erkenov A.K.

(07-13): Radio properties of OH Megamaser (OHM) galaxies,
Zhongzu Wu (Guizhou University, China).
Responsible Sotnikova Yu.V.

(07-13): Radio properties of the blazars on the long time scales,
Mufakharov T. (Shanghai Astronomical Observatory, China).
Responsible Erkenov A.K.

(14-20): The AGN study with the RATAN-600 and VLBI 3,
Kovalev Yu.A. (ASC).
Responsible Erkenov A.K.

(14-30): Radio variability of the Galactic X-ray binaries with relativistic jets2,
Trushkin S. (SAO RAS).
Responsible Erkenov A.K.

(21-30): Study of the long-term variability of the extragalactic radio sources in the declination range from 11 up to 18 degrees,
Konnikova V.K. (SAI MSU).
Responsible Erkenov A.K.

Feed-cabin 3

(01-09): The Sun five-azimuth observations 4.
Responsible Milenko V.S.

Feed-cabin 2

(01-30): Radio variability of the Galactic X-ray binaries with relativistic jets,
Trushkin S. (SAO RAS).
Responsible Erkenov A.K.

(01-30): Radio properties of the blazars on the long time scales,
Mufakharov T. (Shanghai Astronomical Observatory, China).
Responsible Erkenov A.K.

(01-30): Radio properties of the Narrow-Line Seyfert 1 Galaxies,
Lahteenmaki Anne (Metsahovi Radio Observatory, Finland).
Responsible Erkenov A.K.

Feed-cabin 3

(10-25): The Sun multi-azimuth observations 4. Testing of the antenna system (South+Flat) in the tracking mode.
Responsible Milenko V.S.

(26-30): The Sun five-azimuth observations 4.
Responsible Milenko V.S.

Feed-cabin 2

(01-30): Radio variability of the Galactic X-ray binaries with relativistic jets,
Trushkin S. (SAO RAS).
Responsible Erkenov A.K.

Feed-cabin 5

(01-30): Test observations (SAO RAS).
Responsible Trushkin S.A.

1 - SAO RAS; ICRANet, Italy; INAF-IAPS Italy; SAO, USA; Finnish Centre for Astronomy with ESO FINCA; Curtin U., Australia.
2 - During a trigger.
3 - NRAO, USA; Shanghai Astronomical Observatory, China; Max-Planck-Insitut für Radioastronomie, Germany; Joint Institute for VLBI in Europe; IRA INAF, Italy; Netherlands Institute for Radio Astronomy, Netherlands.
4 - The study of the active regions magnetosphere in a wide radio waves range (Bogod V., SAO RAS, Russia); Investigation of ultra-weak solar activity at microwaves (Lesovoi S., Institute of Solar-Terrestrial physics, Russia); Study of the solar floccules in the CaIIK line and in the microwave range with GAS GAO and RATAN-600 (Tlatov A., CAO RAS, Russia); Development of the determining physical conditions methods on the Sun flare-active regions (Yasnov L., St. Petersburg State University, Russia); Structure and evolution of solar active regions (Alissandrakis Costas, University of Ioannina, Greece); Correlational analysis between preflare CaII K and radio plages (Elagandula N., Osmania State University, India); Study of the chromosphere and the transition region of sunspots with ALMA interferometer and RATAN-600 (Lukicheva M., New Jersey Institute of Technology, USA); The Sun microflare observations (Nakaryakov V., The University of Warwick, UK).
5 - During simultaneous observations on ALMA.

Feed-cabin 1 - secondary mirror with complex equipment of the continuous spectrum of 1.28-21.7 GHz.
Feed-cabin 2 - secondary mirror with complex equipment of the continuous spectrum of 2.25-21.7 GHz (ERIDAN).
Feed-cabin 3 - secondary mirror with solar spectral-polarization complex.