ARCHIVE RATAN-600 Observation Schedule
from January 1 to June 30, 2026

Executive Secretary: request@sao.ru 		Russian version

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

(01-31): IceCube trigger: monthly monitoring of the new high-energy neutrino candidates 1,
Troitski S.V. (Institute for Nuclear Research).
Responsible Erkenov A.K.

(01-31): Monitoring of the Galactic X-ray binaries with relativistic jets 2,
Trushkin S. (SAO RAS).
Responsible Erkenov A.K.

(01-31): MALBRICS collaboration: multi-frequency monitoring of blazars 3,
Mufakharov T. (SAO RAS).
Responsible Erkenov A.K.

(01-26): The radio properties of OH Megamaser galaxies 4,
Zhongzu Wu (Guizhou University, China).
Responsible Semenova T.A.

(01-31): Multi-frequency monitoring of TeV -flaring AGN: probing particle acceleration mechanisms in jets,
An Tao (Shanghai Astronomical Observatory, China).
Responsible Sotnikova Yu.V.

(01-31): Monitoring the most powerful X-ray quasars on z>3,
Khorunzhev G.A. (IKI RAS).
Responsible Mikhailov A.G.

(01-31): Radio variability of the NLS1 galaxies,
Volvach A. E. (CrAO RAS).
Responsible Erkenov A.K.

(01-31): Antenna measurements (3 hours a week),
AMG R-600 (SAO RAS)

(27-31): Study of radio spectra of Peaked Spectrum sources,
Iuzhanina K. (SAO RAS).
Responsible Erkenov A.K.

Feed-cabin 2

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

(01-31): Spectra of FR0 galaxies in the centimeter range,
Mikhailov A. (SAO RAS).
Responsible Mikhailov A.G.

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

(01-31): Radio variability of the NLS1 galaxies,
Volvach A. E. (CrAO RAS).
Responsible Erkenov A.K.

(01-31): MALBRICS collaboration: multi-frequency monitoring of blazars,
Mufakharov T. (SAO RAS).
Responsible Erkenov A.K.

(01-31): Radio spectra and variability of quasars at z>4,
Sotnikova Yu.V. (SAO RAS).
Responsible Sotnikova Yu.V.

(01-31): Monitoring the most powerful X-ray quasars on z>3,
Khorunzhev G.A. (IKI RAS).
Responsible Mikhailov A.G.

(01-31): Multi-frequency monitoring of TeV -flaring AGN: probing particle acceleration mechanisms in jets,
Tao An (Shanghai Astronomical Observatory, China).
Responsible Sotnikova Yu.V.

Feed-cabin 3

(01-31): The Sun 13-azimuth observations 6 (SAO RAS).
Responsible Kratov D. V.

Feed-cabin 2

(01-31): Monitoring of the Galactic X-ray binaries with relativistic jets,
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 Bursov N.N.
F
E
B
R
U
A
R
Y

Feed-cabin 1

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

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

(01-28): Multi-frequency monitoring of TeV -flaring AGN: probing particle acceleration mechanisms in jets,
An Tao (Shanghai Astronomical Observatory, China).
Responsible Sotnikova Yu.V.

(01-28): Monitoring the most powerful X-ray quasars on z>3,
Khorunzhev G.A. (IKI RAS).
Responsible Mikhailov A.G.

(01-16): MALBRICS collaboration: multi-frequency monitoring of blazars,
Mufakharov T. (SAO RAS).
Responsible Erkenov A.K.

(01-05): Study of radio spectra of Peaked Spectrum sources,
Iuzhanina K. (SAO RAS).
Responsible Erkenov A.K.

(01-28): Antenna measurements (3 hours a week),
AMG R-600 (SAO RAS)

(08-28): Spectra of FR0 galaxies in the centimeter range,
Mikhailov A. (SAO RAS).
Responsible Mikhailov A.G.

(18-28): Radio spectra and variability of quasars at z>4 5,
Sotnikova Yu.V. (SAO RAS).
Responsible Sotnikova Yu.V.

Feed-cabin 2

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

(01-28): Spectra of FR0 galaxies in the centimeter range,
Mikhailov A. (SAO RAS).
Responsible Mikhailov A.G.

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

(01-28): Radio variability of the NLS1 galaxies,
Volvach A. E. (CrAO RAS).
Responsible Erkenov A.K.

(01-28): MALBRICS collaboration: multi-frequency monitoring of blazars,
Mufakharov T. (SAO RAS).
Responsible Erkenov A.K.

(01-28): Radio spectra and variability of quasars at z>4,
Sotnikova Yu.V. (SAO RAS).
Responsible Sotnikova Yu.V.

(01-28): Monitoring the most powerful X-ray quasars on z>3,
Khorunzhev G.A. (IKI RAS).
Responsible Mikhailov A.G.

(01-28): Multi-frequency monitoring of TeV -flaring AGN: probing particle acceleration mechanisms in jets,
An Tao (Shanghai Astronomical Observatory, China).
Responsible Sotnikova Yu.V.

Feed-cabin 3

(01-28): The Sun 13-azimuth observations (SAO RAS).
Responsible Kratov D. V.

Feed-cabin 2

(01-28): Monitoring of the Galactic X-ray binaries with relativistic jets,
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 Bursov N.N.
M
A
R
C
H

Feed-cabin 1

(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): Monitoring of the Galactic X-ray binaries with relativistic jets 7,
Trushkin S. (SAO RAS).
Responsible Trushkin S.A.

(01-31): Multi-frequency monitoring of TeV -flaring AGN: probing particle acceleration mechanisms in jets,
An Tao (Shanghai Astronomical Observatory, China).
Responsible Sotnikova Yu.V.

(01-31): Monitoring the most powerful X-ray quasars on z>3,
Khorunzhev G.A. (IKI RAS).
Responsible Mikhailov A.G.

(01): Spectra of FR0 galaxies in the centimeter range,
Mikhailov A. (SAO RAS).
Responsible Mikhailov A.G.

(01): Radio spectra and variability of quasars at z>4,
Sotnikova Yu.V. (SAO RAS).
Responsible Sotnikova Yu.V.

(01-31): Antenna measurements (3 hours a week),
AMG R-600 (SAO RAS)

(02-05): Reserve time (SAO RAS)

(06-31): RATAN-600 in multichannel astronomy: a complete sample of AGNs with VLBI-jet as indicators of relativistic protons and high-energy neutrinos,
Kovalev Yu.A. (ASC; MIPT).
Responsible Erkenov A.K.

Feed-cabin 2

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

(01-31): Spectra of FR0 galaxies in the centimeter range,
Mikhailov A. (SAO RAS).
Responsible Mikhailov A.G.

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

(01-31): Radio variability of the NLS1 galaxies,
Volvach A. E. (CrAO RAS).
Responsible Erkenov A.K.

(01-31): MALBRICS collaboration: multi-frequency monitoring of blazars,
Mufakharov T. (SAO RAS).
Responsible Erkenov A.K.

(01-31): Radio spectra and variability of quasars at z>4,
Sotnikova Yu.V. (SAO RAS).
Responsible Sotnikova Yu.V.

(01-31): Monitoring the most powerful X-ray quasars on z>3,
Khorunzhev G.A. (IKI RAS).
Responsible Mikhailov A.G.

(01-31): Multi-frequency monitoring of TeV -flaring AGN: probing particle acceleration mechanisms in jets,
An Tao (Shanghai Astronomical Observatory, China).
Responsible Sotnikova Yu.V.

Feed-cabin 3

(01-31): The Sun 13-azimuth observations (SAO RAS).
Responsible Kratov D. V.

Feed-cabin 2

(01-31): Monitoring of the Galactic X-ray binaries with relativistic jets,
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 Bursov N.N.
A
P
R
I
L

Feed-cabin 1

(01-03): IceCube trigger: monthly monitoring of the new high-energy neutrino candidates,
Troitski S.V. (Institute for Nuclear Research).
Responsible Erkenov A.K.

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

(01-03): Multi-frequency monitoring of TeV -flaring AGN: probing particle acceleration mechanisms in jets,
An Tao (Shanghai Astronomical Observatory, China).
Responsible Sotnikova Yu.V.

(01-03): Monitoring the most powerful X-ray quasars on z>3,
Khorunzhev G.A. (IKI RAS).
Responsible Mikhailov A.G.

(01-03): RATAN-600 in multichannel astronomy: a complete sample of AGNs with VLBI-jet as indicators of relativistic protons and high-energy neutrinos,
Kovalev Yu.A. (ASC; MIPT).
Responsible Erkenov A.K.

(04-19): Technical support,
MS R-600 (SAO RAS)

(20-23): Adjustment, antenna measurements,
AMG R-600 (SAO RAS)

(24-27): Test observations, secondary mirror focus search,
Trushkin S. (SAO RAS).
Responsible Trushkin S.A.

(28-30): Reserve time (SAO RAS)

Feed-cabin 2

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

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

(01-17): The radio properties of OH Megamaser galaxies,
Zhongzu Wu (Shanghai Astronomical Observatory, China).
Responsible Semenova T.A.

(01-17): Radio variability of the NLS1 galaxies,
Volvach A. E. (CrAO RAS).
Responsible Erkenov A.K.

(01-17): MALBRICS collaboration: multi-frequency monitoring of blazars,
Mufakharov T. (SAO RAS).
Responsible Erkenov A.K.

(01-17): Radio spectra and variability of quasars at z>4,
Sotnikova Yu.V. (SAO RAS).
Responsible Sotnikova Yu.V.

(01-17): Monitoring the most powerful X-ray quasars on z>3,
Khorunzhev G.A. (IKI RAS).
Responsible Mikhailov A.G.

(01-17): Multi-frequency monitoring of TeV -flaring AGN: probing particle acceleration mechanisms in jets,
An Tao (Shanghai Astronomical Observatory, China).
Responsible Sotnikova Yu.V.

Feed-cabin 3

(01-17): The Sun 13-azimuth observations (SAO RAS).
Responsible Kratov D. V.

Feed-cabin 2

(06-17): Antenna measurements (4 hours a day),
AMG R-600 (SAO RAS)

Feed-cabin 2, 3

(18-30): Technical support,
MS R-600 (SAO RAS)

Feed-cabin 2

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

(18-30): Technical support,
MS R-600 (SAO RAS)

Feed-cabin 5

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

Feed-cabin 1

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

(02-31): IceCube trigger: monthly monitoring of the new high-energy neutrino candidates,
Troitski S.V. (Institute for Nuclear Research).
Responsible Erkenov A.K.

(02-31): Monitoring of the Galactic X-ray binaries with relativistic jets,
Trushkin S. (SAO RAS).
Responsible Trushkin S.A.

(02-31): Multi-frequency monitoring of TeV -flaring AGN: probing particle acceleration mechanisms in jets,
An Tao (Shanghai Astronomical Observatory, China).
Responsible Sotnikova Yu.V.

(02-31): Monitoring the most powerful X-ray quasars on z>3,
Khorunzhev G.A. (IKI RAS).
Responsible Mikhailov A.G.

(02-12): Study of radio spectra of Peaked Spectrum sources,
Iuzhanina K. (SAO RAS).
Responsible Erkenov A.K.

(02-31): Spectra of FR0 galaxies in the centimeter range,
Mikhailov A. (SAO RAS).
Responsible Mikhailov A.G.

(02-31): Radio spectra and variability of quasars at z>4,
Sotnikova Yu.V. (SAO RAS).
Responsible Sotnikova Yu.V.

(02-12): Radio variability of the NLS1 galaxies,
Volvach A. E. (CrAO RAS).
Responsible Erkenov A.K.

(02-31): Antenna measurements (3 hours a week),
AMG R-600 (SAO RAS)

Feed-cabin 2

(01-01): Technical support,
MS R-600 (SAO RAS)

(02-06): Adjustment, antenna measurements,
AMG R-600 (SAO RAS)

(07-10): Test observations, secondary mirror focus search,
Trushkin S. (SAO RAS).
Responsible Trushkin S.A.

(11-16): Reserve time (SAO RAS)

(17-31): Spectra of FR0 galaxies in the centimeter range,
Mikhailov A. (SAO RAS).
Responsible Mikhailov A.G.

(17-31): The radio properties of OH Megamaser galaxies,
Zhongzu Wu (Guizhou University, China).
Responsible Semenova T.A.

(17-31): Radio variability of the NLS1 galaxies,
Volvach A. E. (CrAO RAS).
Responsible Erkenov A.K.

(17-31): MALBRICS collaboration: multi-frequency monitoring of blazars,
Mufakharov T. (SAO RAS).
Responsible Erkenov A.K.

(17-31): Radio spectra and variability of quasars at z>4,
Sotnikova Yu.V. (SAO RAS).
Responsible Sotnikova Yu.V.

(17-31): Monitoring the most powerful X-ray quasars on z>3,
Khorunzhev G.A. (IKI RAS).
Responsible Mikhailov A.G.

(17-31): Multi-frequency monitoring of TeV -flaring AGN: probing particle acceleration mechanisms in jets,
An Tao (Shanghai Astronomical Observatory, China).
Responsible Sotnikova Yu.V.

(17-31): Monitoring of the Galactic X-ray binaries with relativistic jets,
Trushkin S. (SAO RAS).
Responsible Trushkin S.A.

Feed-cabin 3

(17-31): The Sun 13-azimuth observations (SAO RAS).
Responsible Kratov D. V.

Feed-cabin 2

(01-01): Technical support,
MS R-600 (SAO RAS)

(02-06): Adjustment, antenna measurements,
AMG R-600 (SAO RAS)

(07-10): Test observations, secondary mirror focus search,
Trushkin S. (SAO RAS).
Responsible Trushkin S.A.

(11-16): Reserve time (SAO RAS)

(17-31): Monitoring of the Galactic X-ray binaries with relativistic jets,
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 Bursov N.N.
J
U
N
E

Feed-cabin 1

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

(01-31): Multi-frequency monitoring of TeV -flaring AGN: probing particle acceleration mechanisms in jets,
An Tao (Shanghai Astronomical Observatory, China).
Responsible Sotnikova Yu.V.

(01-31): Monitoring the most powerful X-ray quasars on z>3,
Khorunzhev G.A. (IKI RAS).
Responsible Mikhailov A.G.

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

(01-31): Antenna measurements (3 hours a week),
AMG R-600 (SAO RAS)

Feed-cabin 2

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

(01-30): Spectra of FR0 galaxies in the centimeter range,
Mikhailov A. (SAO RAS).
Responsible Mikhailov A.G.

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

(01-30): Radio variability of the NLS1 galaxies,
Volvach A. E. (CrAO RAS).
Responsible Erkenov A.K.

(01-30): MALBRICS collaboration: multi-frequency monitoring of blazars,
Mufakharov T. (SAO RAS).
Responsible Erkenov A.K.

(01-30): Radio spectra and variability of quasars at z>4,
Sotnikova Yu.V. (SAO RAS).
Responsible Sotnikova Yu.V.

(01-30): Monitoring the most powerful X-ray quasars on z>3,
Khorunzhev G.A. (IKI RAS).
Responsible Mikhailov A.G.

(01-30): Multi-frequency monitoring of TeV -flaring AGN: probing particle acceleration mechanisms in jets,
An Tao (Shanghai Astronomical Observatory, China).
Responsible Sotnikova Yu.V.

Feed-cabin 3

(01-30): The Sun 13-azimuth observations (SAO RAS).
Responsible Kratov D. V.

Feed-cabin 2

(01-30): Monitoring of the Galactic X-ray binaries with relativistic jets,
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 Bursov N.N.

1 – Harvard University (USA); ASC (Russia); MPIfRA (Germany).
2 - INAF, SRT (Italy); Curtin University (Australia); Tuorla observatory (Finland).
3 - University of Cambridge (UK); Sun Yat-sen University (China); Raman Research Institute, Bangalore (India); Saha Institute of Nuclear Physics, Kolkata (India).
4 - Guangzhou University (China); SHAO CAS (China), University of Cambridge (UK).
5 - INFIP (Argentina); SHAO CAS (China).
6 - Wide-range spectral studies of the Sun on RATAN-600 in the range 1-30 GHz (Bogod V., SPbB SAO RAS; ISTP); Forecasting flares in active regions of the Sun, Space weather (Kurochkin E.A. SPbB SAO RAS, Kislovodsk Mountain Astronomical station of the Pulkovo observatory); Joint studies of the chromosphere and transition region of sunspots using the ALMA interferometer and RATAN-600 (Lukicheva M., New Jersey Institute of Technology, USA); Determination of physical conditions in active regions on the Sun using multi-frequency radio observations (Stupishin A., SAO RAS, SPbB SAO RAS).
7 - The sources of competing programs are observed every other day.

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.