ARCHIVE RATAN-600 Observation Schedule
from January 1 to June 30, 2022


Executive Secretary: [email protected]
Russian version

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

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

(01-31): IceCube trigger: monthly monitoring of the new high-energy neutrino candidates,
Troitski S.V. (IKI RAS; Institute for Nuclear Research).
Responsible Erkenov A.K.

(01-31): Multifrequency monitoring of blazar variability on long time scales,
Mufakharov T. (Shanghai Astronomical Observatory, China).
Responsible Erkenov A.K.

(01-31): The radio properties of OH Megamaser galaxies,
Zhongzu Wu (Guizhou University, China).
Responsible Erkenov A.K.

(01-31): Monitoring SRGE J170245.3 + 130104 - the most powerful X-ray quasar at z> 5,
Horunzhev G.A. (IKI RAS).
Responsible Erkenov A.K.

Feed-cabin 2

(01-31): Multifrequency monitoring of blazar variability on long time scales,
Mufakharov T. (Shanghai Astronomical Observatory, China).
Responsible Erkenov A.K.

(01-31): Radio spectra and variability of quasars at z>45,
Sotnikova Yu.V. (SAO RAS).
Responsible Erkenov A.K.

(01-31): The radio properties of OH Megamaser galaxies,
Zhongzu Wu (Guizhou University, China).
Responsible Erkenov A.K.

(01-31): Monitoring SRGE J170245.3 + 130104 - the most powerful X-ray quasar at z> 5,
Horunzhev G.A. (IKI RAS).
Responsible Erkenov A.K.

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

Feed-cabin 3

(01-31): The Sun five-azimuth observations 3 (SAO RAS).
Responsible Kazanina T.N.

Feed-cabin 2

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

Feed-cabin 5

(01-31): Search of fast radio bursts at 4.7 GHz,
Trushkin S. (SAO RAS).
Responsible Trushkin S.A.

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Y

Feed-cabin 1

(01-28): Monitoring of the Galactic X-ray binaries with relativistic jets1,
Trushkin S. (SAO RAS).
Responsible Trushkin S.A.

(01-28): IceCube trigger: monthly monitoring of the new high-energy neutrino candidates,
Troitski S.V. (Institute for Nuclear Research).
Responsible Erkenov A.K.

(01-16): Multifrequency monitoring of blazar variability on long time scales,
Mufakharov T. (Shanghai Astronomical Observatory, China).
Responsible Erkenov A.K.

(01-16): The radio properties of OH Megamaser galaxies,
Zhongzu Wu (Guizhou University, China).
Responsible Erkenov A.K.

(01-13): Monitoring SRGE J170245.3 + 130104 - the most powerful X-ray quasar at z> 5,
Horunzhev G.A. (IKI RAS).
Responsible Erkenov A.K.

(14-28): Spectra of FR0 galaxies in the centimeter range,
Mikhailov A. (SAO RAS).
Responsible Erkenov A.K.

(17-28): Radio spectra and variability of quasars at z>45,
Sotnikova Yu.V. (SAO RAS).
Responsible Erkenov A.K.

Feed-cabin 2

(01-28): Multifrequency monitoring of blazar variability on long time scales,
Mufakharov T. (Shanghai Astronomical Observatory, China).
Responsible Erkenov A.K.

(01-28): Radio spectra and variability of quasars at z>45,
Sotnikova Yu.V. (SAO RAS).
Responsible Erkenov A.K.

(01-28): The radio properties of OH Megamaser galaxies,
Zhongzu Wu (Guizhou University, China).
Responsible Erkenov A.K.

(01-28): Monitoring of the Galactic X-ray binaries with relativistic jets1,
Trushkin S. (SAO RAS).
Responsible Trushkin S.A.

(01-16): Monitoring SRGE J170245.3 + 130104 - the most powerful X-ray quasar at z> 5,
Horunzhev G.A. (IKI RAS).
Responsible Erkenov A.K.

Feed-cabin 3

(01-28): The Sun five-azimuth observations 3 (SAO RAS).
Responsible Kazanina T.N.

Feed-cabin 2

(01-28): Monitoring of the Galactic X-ray binaries with relativistic jets1,
Trushkin S. (SAO RAS).
Responsible Trushkin S.A.

Feed-cabin 5

(01-28): Search of fast radio bursts at 4.7 GHz,
Trushkin S. (SAO RAS).
Responsible Trushkin S.A.

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H

Feed-cabin 1

(01-31): Monitoring of the Galactic X-ray binaries with relativistic jets2,
Trushkin S. (SAO RAS).
Responsible Trushkin S.A.

(01-31): IceCube trigger: monthly monitoring of the new high-energy neutrino candidates,
Troitski S.V. (Institute for Nuclear Research).
Responsible Erkenov A.K.

(01-31): RATAN-600 in multichannel astronomy: a complete sample of AGNs with VLBI-compact jet as indicators of high-energy neutrinos,
Kovalev Yu.A. (ASC).
Responsible Erkenov A.K.

Feed-cabin 2

(01-01): Multifrequency monitoring of blazar variability on long time scales,
Mufakharov T. (Shanghai Astronomical Observatory, China).
Responsible Erkenov A.K.

(01-01): Radio spectra and variability of quasars at z>45,
Sotnikova Yu.V. (SAO RAS).
Responsible Erkenov A.K.

(01-01): The radio properties of OH Megamaser galaxies,
Zhongzu Wu (Guizhou University, China).
Responsible Erkenov A.K.

(01-01): Monitoring of the Galactic X-ray binaries with relativistic jets1,
Trushkin S. (SAO RAS).
Responsible Trushkin S.A.

Feed-cabin 3

(01-01): The Sun five-azimuth observations 3 (SAO RAS).
Responsible Kazanina T.N.

(02-09): Reserve time (SAO RAS)

(10-31): The Sun multi-azimuth observations 5 (SAO RAS).
Responsible Kazanina T.N.

Feed-cabin 2

(10-31): Multifrequency monitoring of blazar variability on long time scales,
Mufakharov T. (Shanghai Astronomical Observatory, China).
Responsible Erkenov A.K.

(10-31): Radio spectra and variability of quasars at z>45,
Sotnikova Yu.V. (SAO RAS).
Responsible Erkenov A.K.

(10-31): The radio properties of OH Megamaser galaxies,
Zhongzu Wu (Guizhou University, China).
Responsible Erkenov A.K.

(10-31): Monitoring of the Galactic X-ray binaries with relativistic jets1,
Trushkin S. (SAO RAS).
Responsible Trushkin S.A.

Feed-cabin 2

(01-01): Monitoring of the Galactic X-ray binaries with relativistic jets1,
Trushkin S. (SAO RAS).
Responsible Trushkin S.A.

(02-09): Reserve time (SAO RAS)

(10-31): Monitoring of the Galactic X-ray binaries with relativistic jets1,
Trushkin S. (SAO RAS).
Responsible Trushkin S.A.

Feed-cabin 5

(01-31): Search of fast radio bursts at 4.7 GHz,
Trushkin S. (SAO RAS).
Responsible Trushkin S.A.

A
P
R
I
L

Feed-cabin 1

(01-17): IceCube trigger: monthly monitoring of the new high-energy neutrino candidates,
Troitski S.V. (Institute for Nuclear Research).
Responsible Erkenov A.K.

(01-17): Monitoring of the Galactic X-ray binaries with relativistic jets1,
Trushkin S. (SAO RAS).
Responsible Trushkin S.A.

(01-17): Spectra of FR0 galaxies in the centimeter range,
Mikhailov A. (SAO RAS).
Responsible Erkenov A.K.

(01-17): Radio spectra and variability of quasars at z>45,
Sotnikova Yu.V. (SAO RAS).
Responsible Erkenov A.K.

(18-29): Technical support,
Yakovenko S.V., Shtondin A.F. (SAO RAS)

(30): Adjustment, antenna measurements,
Zharov V.I. (SAO RAS)

Feed-cabin 2

(01-03): Multifrequency monitoring of blazar variability on long time scales,
Mufakharov T. (Shanghai Astronomical Observatory, China).
Responsible Erkenov A.K.

(01-03): Radio spectra and variability of quasars at z>45,
Sotnikova Yu.V. (SAO RAS).
Responsible Erkenov A.K.

(01-03): The radio properties of OH Megamaser galaxies,
Zhongzu Wu (Guizhou University, China).
Responsible Erkenov A.K.

(01-03): Monitoring of the Galactic X-ray binaries with relativistic jets1,
Trushkin S. (SAO RAS).
Responsible Trushkin S.A.

Feed-cabin 3

(01-03): The Sun five-azimuth observations 3 (SAO RAS).
Responsible Erkenov A.K.

(04-15): Technical support,
Yakovenko S.V., Shtondin A.F. (SAO RAS)

(16-19): Adjustment, antenna measurements,
Zharov V.I. (SAO RAS)

(20-23): Test observations, secondary mirror focus search,
Trushkin S. (SAO RAS)

Feed-cabin 2

(24-30): Multifrequency monitoring of blazar variability on long time scales,
Mufakharov T. (Shanghai Astronomical Observatory, China).
Responsible Erkenov A.K.

(24-30): Radio spectra and variability of quasars at z>45,
Sotnikova Yu.V. (SAO RAS).
Responsible Erkenov A.K.

(24-30): The radio properties of OH Megamaser galaxies,
Zhongzu Wu (Guizhou University, China).
Responsible Erkenov A.K.

(24-30): Monitoring of the Galactic X-ray binaries with relativistic jets1,
Trushkin S. (SAO RAS).
Responsible Trushkin S.A.

Feed-cabin 3

(24-30): The Sun five-azimuth observations 3 (SAO RAS).
Responsible Kazanina T.N.

Feed-cabin 2

(01-30): Monitoring of the Galactic X-ray binaries with relativistic jets1,
Trushkin S. (SAO RAS).
Responsible Trushkin S.A.

Feed-cabin 5

(01-30): Search of fast radio bursts at 4.7 GHz,
Trushkin S. (SAO RAS).
Responsible Trushkin S.A.

M
A
Y

Feed-cabin 1

(01-03): Adjustment, antenna measurements,
Zharov V.I. (SAO RAS)

(04-07): Test observations, secondary mirror focus search,
Trushkin S. (SAO RAS)

(08-13): Reserve time (SAO RAS)

(14-31): Spectra of FR0 galaxies in the centimeter range,
Mikhailov A. (SAO RAS).
Responsible Erkenov A.K.

(14-28): Radio spectra and variability of quasars at z>45,
Sotnikova Yu.V. (SAO RAS).
Responsible Erkenov A.K.

(14-31): IceCube trigger: monthly monitoring of the new high-energy neutrino candidates,
Troitski S.V. (Institute for Nuclear Research).
Responsible Erkenov A.K.

(14-31): Monitoring of the Galactic X-ray binaries with relativistic jets1,
Trushkin S. (SAO RAS).
Responsible Trushkin S.A.

Feed-cabin 2

(01-31): Multifrequency monitoring of blazar variability on long time scales,
Mufakharov T. (Shanghai Astronomical Observatory, China).
Responsible Erkenov A.K.

(01-31): Radio spectra and variability of quasars at z>45,
Sotnikova Yu.V. (SAO RAS).
Responsible Erkenov A.K.

(01-31): The radio properties of OH Megamaser galaxies,
Zhongzu Wu (Guizhou University, China).
Responsible Erkenov A.K.

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

Feed-cabin 3

(01-31): The Sun five-azimuth observations 3 (SAO RAS).
Responsible Kazanina T.N.

Feed-cabin 2

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

Feed-cabin 5

(01-31): Search of fast radio bursts at 4.7 GHz,
Trushkin S. (SAO RAS).
Responsible Trushkin S.A.

J
U
N
E

Feed-cabin 1

(01-02): Spectra of FR0 galaxies in the centimeter range,
Mikhailov A. (SAO RAS).
Responsible Erkenov A.K.

(01-30): Monitoring of the Galactic X-ray binaries with relativistic jets2,
Trushkin S. (SAO RAS).
Responsible Trushkin S.A.

(01-30): IceCube trigger: monthly monitoring of the new high-energy neutrino candidates,
Troitski S.V. (SAO RAS).
Responsible Erkenov A.K.

(03-30): RATAN-600 in multichannel astronomy: a complete sample of AGNs with VLBI-compact jet as indicators of high-energy neutrinos,
Kovalev Yu.A. (ASC).
Responsible Erkenov A.K.

Feed-cabin 2

(01-30): Multifrequency monitoring of blazar variability on long time scales,
Mufakharov T. (SAO RAS; Shanghai Astronomical Observatory, China).
Responsible Erkenov A.K.

(01-30): Radio spectra and variability of quasars at z>45,
Sotnikova Yu.V. (SAO RAS).
Responsible Erkenov A.K.

(01-30): The radio properties of OH Megamaser galaxies,
Zhongzu Wu (Guizhou University, China).
Responsible Erkenov A.K.

(01-30): Monitoring of the Galactic X-ray binaries with relativistic jets1,
Trushkin S. (SAO RAS).
Responsible Trushkin S.A.

Feed-cabin 3

(01-09): The Sun five-azimuth observations 3 (SAO RAS).
Responsible Kazanina T.N.

(10-30): The Sun multi-azimuth observations 5 (SAO RAS).
Responsible Kazanina T.N.

Feed-cabin 2

(01-30): Monitoring of the Galactic X-ray binaries with relativistic jets1,
Trushkin S. (SAO RAS).
Responsible Trushkin S.A.

Feed-cabin 5

(01-30): Search of fast radio bursts at 4.7 GHz,
Trushkin S. (SAO RAS).
Responsible Trushkin S.A.

1 - SAO RAS; ICRANet, Italy; INAF-IAPS, Italy; SAO, USA; Finnish Centre for Astronomy with ESO FINCA; INAF, Sardinia, Italy; Curtin University, Australia.
2 - During a trigger.
3 - Study of flare plasma structures in the decimeter range with new technical capabilities of RATAN-600 (Bogod V., SAO RAS); Supplementing the Coronal-like jet events extended catalogue with RATAN-600 observational data (Kaltman T.I., SAO RAS); Investigation of superweak solar activity on microwaves (Lesovoy S., ISTP SB RAS); Study of the chromosphere and the transition region of sunspots with ALMA interferometer and RATAN-600 (Lukicheva M., New Jersey Institute of Technology, USA); Development of methods for determining physical conditions in active areas in the sun (Stupishin A., SPbU).
4 - During simultaneous observations with ALMA.
5 - National Institute for Plasma Physics (INFIP), Argentina.

Feed-cabin 1 - secondary mirror with complex equipment of the continuous spectrum of 1.35-22.3 GHz.
Feed-cabin 2 - secondary mirror with complex equipment of the continuous spectrum of 1.35-22.3 GHz (ERIDAN).
Feed-cabin 3 - secondary mirror with solar spectral-polarization complex.