ARCHIVE RATAN-600 Observation Schedule
from 1 July to 31 December, 2026

Executive Secretary: request@sao.ru 		Russian version

  North Sector South+Flat South Sector West Sector
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Y

Feed-cabin 1

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

(05-31): IceCube trigger: monthly monitoring of the new high-energy neutrino candidates 1,
Troitski S.V. (Institute for Nuclear Research).
Responsible Erkenov A.K.

(05-31): Monitoring of the Galactic X-ray binaries with relativistic jets 2,
Trushkin S. (SAO RAS).
Responsible Trushkin S.A.

(05-31): Monitoring the most powerful X-ray quasars on z>3 3,
Khorunzhev G.A. (IKI RAS).
Responsible Mikhailov A.G.

(05-31): Multi-frequency monitoring of TeV-flaring AGN: probing particle acceleration mechanisms in jets 4,
Tao An (Shanghai Astronomical Observatory, China).
Responsible Sotnikova Yu.V.

(05-31): MALBRICS collaboration: multi-frequency monitoring of blazars 5,
Mufakharov T. (Xinjiang Astronomical Observatory, China).
Responsible Erkenov A.K.

(05-26): The radio properties of OH Megamaser galaxies 6,
Zhongzu Wu (Guizhou University, China).
Responsible Semenova T.A.

(05-20): Radio variability of the NLS1 galaxies 7,
Volvach A. E. (CrAO RAS).
Responsible Erkenov A.K.

(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. (Xinjiang Astronomical Observatory, China).
Responsible Erkenov A.K.

(01-31): Radio spectra and variability of quasars at z>4,
Mufakharov T. (Xinjiang Astronomical Observatory, China).
Responsible Sotnikova Yu.V.

(01-31): Monitoring the most powerful X-ray quasars on z>3,
Khorunzhev G.A. (CrAO 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 10 (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
U
G
U
S
T

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): 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.

(01-16): MALBRICS collaboration: multi-frequency monitoring of blazars,
Mufakharov T. (Xinjiang Astronomical Observatory, China).
Responsible Erkenov A.K.

(01-16): Study of radio spectra of Peaked Spectrum sources,
Iuzhanina K. (SAO RAS).
Responsible Erkenov A.K.

(13-31): Spectra of FR0 galaxies in the centimeter range,
Mikhailov A. (SAO RAS).
Responsible Mikhailov A.G.

(17-31): Radio spectra and variability of quasars at z>4 8,
Mufakharov T. (Xinjiang Astronomical Observatory, China).
Responsible Sotnikova Yu.V.

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. (Xinjiang Astronomical Observatory, China).
Responsible Erkenov A.K.

(01-31): Radio spectra and variability of quasars at z>4,
Mufakharov T. (Xinjiang 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): 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.
S
E
P
T
E
M
B
E
R

Feed-cabin 1

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

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

(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,
Tao An (Shanghai Astronomical Observatory, China).
Responsible Sotnikova Yu.V.

(01-30): RATAN-600 in multichannel astronomy: a complete sample of AGNs with VLBI-jet as indicators of relativistic protons and high-energy neutrinos 9,
Kovalev Yu.A. (ASC).
Responsible Erkenov A.K.

Feed-cabin 2

(01-30): Multi-frequency monitoring of TeV-flaring AGN: probing particle acceleration mechanisms in jets 3,
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. (Xinjiang Astronomical Observatory, China).
Responsible Erkenov A.K.

(01-30): Radio spectra and variability of quasars at z>4,
Mufakharov T. (Xinjiang Astronomical Observatory, China).
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.

(14-30): Antenna measurements (4 hours a day),
AMG R-600 (SAO RAS).
Responsible Zharov V.I.

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.
O
C
T
O
B
E
R

Feed-cabin 1

(01-09): IceCube trigger: monthly monitoring of the new high-energy neutrino candidates,
Troitski S.V. (Institute for Nuclear Research).
Responsible Erkenov A.K.

(01-09): Monitoring of the Galactic X-ray binaries with relativistic jets,
Trushkin S. (SAO RAS).
Responsible Trushkin S.A.

(01-09): Monitoring the most powerful X-ray quasars on z>3,
Khorunzhev G.A. (IKI RAS).
Responsible Mikhailov A.G.

(01-09): Multi-frequency monitoring of TeV-flaring AGN: probing particle acceleration mechanisms in jets,
Tao An (Shanghai Astronomical Observatory, China).
Responsible Sotnikova Yu.V.

(01-09): Spectra of FR0 galaxies in the centimeter range,
Mikhailov A. (SAO RAS).
Responsible Mikhailov A.G.

(01-09): Radio spectra and variability of quasars at z>4,
Mufakharov T. (Xinjiang Astronomical Observatory, China).
Responsible Sotnikova Yu.V.

(10-25): Technical support,
MS R-600 (SAO RAS)

(26-29): Adjustment, antenna measurements,
AMG R-600 (SAO RAS)

(30-31): Test observations, secondary mirror focus search,
Trushkin S. (SAO RAS)

Feed-cabin 2

(01-23): Monitoring of the Galactic X-ray binaries with relativistic jets,
Trushkin S. (SAO RAS).
Responsible Trushkin S.A.

(01-23): Spectra of FR0 galaxies in the centimeter range,
Mikhailov A. (SAO RAS).
Responsible Mikhailov A.G.

(01-23): The radio properties of OH Megamaser galaxies,
Zhongzu Wu (Guizhou University, China).
Responsible Semenova T.A.

(01-23): Radio variability of the NLS1 galaxies,
Volvach A. E. (CrAO RAS).
Responsible Erkenov A.K.

(01-23): MALBRICS collaboration: multi-frequency monitoring of blazars,
Mufakharov T. (Xinjiang Astronomical Observatory, China).
Responsible Erkenov A.K.

(01-23): Radio spectra and variability of quasars at z>4,
Mufakharov T. (Xinjiang Astronomical Observatory, China).
Responsible Sotnikova Yu.V.

(01-23): Monitoring the most powerful X-ray quasars on z>3,
Khorunzhev G.A. (IKI RAS).
Responsible Mikhailov A.G.

(01-23): 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

(01-23): The Sun 13-azimuth observations (SAO RAS).
Responsible Kratov D. V.

(01-14): Antenna measurements (4 hours a day),
AMG R-600 (SAO RAS)

(24-31): Technical support,
MS R-600 (SAO RAS)

Feed-cabin 2

(01-23): Monitoring of the Galactic X-ray binaries with relativistic jets,
Trushkin S. (SAO RAS).
Responsible Trushkin S.A.

(24-31): Technical support,
MS R-600 (SAO RAS)

Feed-cabin 5

(01-31): Search of fast radio bursts at 4.7 GHz,
Trushkin S. (SAO RAS).
Responsible Bursov N.N.
N
O
V
E
M
B
E
R

(01-02): Test observations, secondary mirror focus search,
Trushkin S. (SAO RAS)

(03-08): Reserve time,
SAO RAS (SAO RAS)

Feed-cabin 1

(09-30): IceCube trigger: monthly monitoring of the new high-energy neutrino candidates,
Troitski S.V. (Institute for Nuclear Research).
Responsible Erkenov A.K.

(09-30): Monitoring of the Galactic X-ray binaries with relativistic jets,
Trushkin S. (SAO RAS).
Responsible Trushkin S.A.

(09-30): Monitoring the most powerful X-ray quasars on z>3,
Khorunzhev G.A. (IKI RAS).
Responsible Mikhailov A.G.

(09-30): Multi-frequency monitoring of TeV-flaring AGN: probing particle acceleration mechanisms in jets,
Tao An (Shanghai Astronomical Observatory, China).
Responsible Sotnikova Yu.V.

(09-30): Spectra of FR0 galaxies in the centimeter range,
Mikhailov A. (SAO RAS).
Responsible Mikhailov A.G.

(09-26): Radio spectra and variability of quasars at z>4,
Mufakharov T. (Xinjiang Astronomical Observatory, China).
Responsible Sotnikova Yu.V.

(09-30): Radio variability of the NLS1 galaxies,
Volvach A. E. (CrAO RAS).
Responsible Erkenov A.K.

(01-06): Technical support,
MS R-600 (SAO RAS)

(07-11): Adjustment, antenna measurements,
AMG R-600 (SAO RAS)

(12-15): Test observations, secondary mirror focus search,
Trushkin S. (SAO RAS).
Responsible Trushkin S.A.

(16-21): Reserve time (SAO RAS)

Feed-cabin 2

(22-30): Monitoring of the Galactic X-ray binaries with relativistic jets,
Trushkin S. (SAO RAS).
Responsible Trushkin S.A.

(22-30): Spectra of FR0 galaxies in the centimeter range,
Mikhailov A. (SAO RAS).
Responsible Mikhailov A.G.

(22-30): The radio properties of OH Megamaser galaxies,
Zhongzu Wu (Guizhou University, China).
Responsible Semenova T.A.

(22-30): Radio variability of the NLS1 galaxies,
Volvach A. E. (CrAO RAS).
Responsible Erkenov A.K.

(22-30): MALBRICS collaboration: multi-frequency monitoring of blazars,
Mufakharov T. (Xinjiang Astronomical Observatory, China).
Responsible Erkenov A.K.

(22-30): Radio spectra and variability of quasars at z>4,
Mufakharov T. (Xinjiang Astronomical Observatory, China).
Responsible Sotnikova Yu.V.

(22-30): Monitoring the most powerful X-ray quasars on z>3,
Khorunzhev G.A. (IKI RAS).
Responsible Mikhailov A.G.

(22-30): 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

(22-30): The Sun 13-azimuth observations (SAO RAS).
Responsible Kratov D. V.

Feed-cabin 2

(01-06): Technical support,
MS R-600 (SAO RAS)

(07-11): Adjustment, antenna measurements,
AMG R-600 (SAO RAS)

(12-15): Test observations, secondary mirror focus search,
SAO RAS.
Responsible Trushkin S.A.

(16-21): Reserve time (SAO RAS)

(22-30): 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.
D
E
C
E
M
B
E
R

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): 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.

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

(03-31): 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).
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. (Xinjiang Astronomical Observatory, China).
Responsible Erkenov A.K.

(01-31): Radio spectra and variability of quasars at z>4,
Mufakharov T. (Xinjiang 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): 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.

1 - Harvard University, USA; ASC, Russia; MPIfRA, Germany
2 - INAF, Italy; Tuorla observatory, Finland; Harvard, USA
3 - Xinjiang Astronomical Observatory, China; SAO RAS, Russia
4 - Xinjiang Astronomical Observatory, China; SAO RAS, Russia
5 - University of Cambridge, UK; Sun Yat-sen University, China; Raman Research Institute, India; Saha Institute of Nuclear Physics, India
6 - SAO RAS, Russia; Guangzhou University, China; SHAO CAS, China; University of Cambridge, UK; Xinjiang Astronomical Observatory, China
7 - SAO RAS, Russia
8 - SAO RAS, Russia; SHAO CAS, China
9 - SAO RAS, Russia; MIPT, Russia
10 - Determination of physical conditions in active regions on the Sun using multi-frequency radio observations (Stupishin A., SAO RAS, Russia).
Radio spectroscopy of cold formations in the solar corona (Ovchinnikova N., SAO RAS, Russia)
Quasiperiodic pulsations as a metronome of solar flares (Nakaryakov V., SAO RAS, Russia; The Central Astronomical Observatory of the RAS, Russia).
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; SAO RAS, Russia).
Forecasting flares in active regions of the Sun (Space weather) (Kurochkin E., SAO RAS, Russia; Kislovodsk Mountain Astronomical Station The Central Astronomical Observatory of the RAS, Russia; SAO RAS, Russia).
Time series of active formations of the 25th cycle (Knyazeva I., CAO RAS; SAO RAS, Russia)
Energy release processes in weak solar flares (Kashapova L.K., ISTP SB RAS, Russia).
Search for spectral-spatialfluctuations of cosmic microwave background radiation on the RATAN-600 radio telescope (Dubrovich V., SAO RAS, Russia; Research Institute of Physics at St. Petersburg State University, Russia; St. Petersburg Electrotechnical University, Russia).
Study of the solar corona in a wide spectral frequency range using the SRG (ISTP) and RATAN-600 (SAO RAS) instruments (Bogod V., SAO RAS, Russia; ISTP SB RAS, Russia).
Search for solar cyclotron lines on RATAN-600 with high frequency resolution (Bogod V., SAO RAS, Russia).

Feed-cabin 1 - secondary mirror with complex equipment of the continuous spectrum of 1.4-22.3 GHz.
Feed-cabin 2 - secondary mirror with complex equipment of the continuous spectrum of 4.7-22.3 GHz (ERIDAN).
Feed-cabin 3 - secondary mirror with solar spectral-polarization complex 1-3 GHz and 3-18 GHz.