ARCHIVE RATAN-600 Observation Schedule
from 1 July to 31 December, 2025

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 trigger1: 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 2,
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.

(01-31): MALBRICS collaboration: radio properties of transient events 3,
Yang Lili (Sun Yat-sen University, China).
Responsible Sotnikova Yu.V.

(01-31): MALBRICS collaboration: multi-frequency monitoring of blazars 4,
Mufakharov T. (SAO RAS).
Responsible Erkenov A.K.

(01-26): The radio properties of OH Megamaser galaxies 5,
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): Antenna measurements (3 hours a week),
AMG R-600 (SAO RAS)

(27-31): Spectra of FR0 galaxies in the centimeter range,
Mikhailov A. (SAO RAS).
Responsible Mikhailov A.G.

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.

(01-31): MALBRICS collaboration: radio properties of transient events,
Yang Lili (Sun Yat-sen University, China).
Responsible Sotnikova Yu.V.

Feed-cabin 3

(01-31): The Sun 13-azimuth observations 7 (SAO RAS).
Responsible Kazanina T.N.

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 jets10,
An Tao (Shanghai Astronomical Observatory, China).
Responsible Sotnikova Yu.V.

(01-11): Radio variability of the NLS1 galaxies,
Volvach A. E. (CrAO RAS).
Responsible Erkenov A.K.

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

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

(01-27): Radio spectra and variability of quasars at z>4 6,
Sotnikova Yu.V. (SAO RAS).
Responsible Sotnikova Yu.V.

(01-01): MALBRICS collaboration: radio properties of transient events,
Yang Lili (Sun Yat-sen University, China).
Responsible Sotnikova Yu.V.

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

Feed-cabin 2

(01-31): IceCube trigger: monthly monitoring of the new high-energy neutrino candidates,
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.

(01-31): MALBRICS collaboration: radio properties of transient events,
Yang Lili (Sun Yat-sen University, China).
Responsible Sotnikova Yu.V.

Feed-cabin 3

(01-31): The Sun 13-azimuth observations (SAO RAS).
Responsible Kazanina T.N.

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

(01-28): 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 11,
Trushkin S. (SAO RAS).
Responsible Trushkin S.A.

(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.

(01-28): 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.

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

(29-30): 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.

(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.

(01-30): MALBRICS collaboration: radio properties of transient events,
Yang Lili (Sun Yat-sen University, China).
Responsible Sotnikova Yu.V.

Feed-cabin 3

(01-09): The Sun 13-azimuth observations (SAO RAS).
Responsible Kazanina T.N.

(10-30): The Sun multi-azimuth observations 7 (SAO RAS).
Responsible Kazanina T.N.

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

(01-10): Technical support,
MS R-600 (SAO RAS)

(10-13): Adjustment, antenna measurements,
AMG R-600 (SAO RAS)

(14-17): Test observations, secondary mirror focus search (SAO RAS).
Responsible Trushkin S.A.

(18-24): Reserve time (SAO RAS)

(25-31): Antenna measurements (3 hours a week),
AMG R-600 (SAO RAS)

(25-31): IceCube trigger: monthly monitoring of the new high-energy neutrino candidates,
Troitski S.V. (Institute for Nuclear Research).
Responsible Erkenov A.K.

(25-31): Monitoring of the Galactic X-ray binaries with relativistic jets,
Trushkin S. (SAO RAS).
Responsible Trushkin S.A.

(25-31): Monitoring the most powerful X-ray quasars on z>3,
Khorunzhev G.A. (IKI RAS).
Responsible Mikhailov A.G.

(25-31): Multi-frequency monitoring of TeV-flaring AGN: probing particle acceleration mechanisms in jets,
An Tao (Shanghai Astronomical Observatory, China).
Responsible Sotnikova Yu.V.

(31-31): 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

(01-12): Monitoring of the Galactic X-ray binaries with relativistic jets,
Trushkin S. (SAO RAS).
Responsible Trushkin S.A.

(01-12): Spectra of FR0 galaxies in the centimeter range,
Mikhailov A. (SAO RAS).
Responsible Mikhailov A.G.

(01-12): The radio properties of OH Megamaser galaxies,
Zhongzu Wu (Guizhou University, China).
Responsible Semenova T.A.

(01-12): Radio variability of the NLS1 galaxies,
Volvach A. E. (CrAO RAS).
Responsible Erkenov A.K.

(01-12): MALBRICS collaboration: multi-frequency monitoring of blazars,
Mufakharov T. (SAO RAS).
Responsible Erkenov A.K.

(01-12): Radio spectra and variability of quasars at z>4,
Sotnikova Yu.V. (SAO RAS).
Responsible Sotnikova Yu.V.

(01-12): Monitoring the most powerful X-ray quasars on z>3,
Khorunzhev G.A. (IKI RAS).
Responsible Mikhailov A.G.

(01-12): Multi-frequency monitoring of TeV-flaring AGN: probing particle acceleration mechanisms in jets,
An Tao (Shanghai Astronomical Observatory, China).
Responsible Sotnikova Yu.V.

(01-12): MALBRICS collaboration: radio properties of transient events,
Yang Lili (Sun Yat-sen University, China).
Responsible Sotnikova Yu.V.

Feed-cabin 3

(01-12): The Sun 13-azimuth observations (SAO RAS).
Responsible Kazanina T.N.

(13-26): Technical support,
MS R-600 (SAO RAS)

(27-31): Adjustment, antenna measurements,
AMG R-600 (SAO RAS)

Feed-cabin 2

(01-12): Monitoring of the Galactic X-ray binaries with relativistic jets,
Trushkin S. (SAO RAS).
Responsible Trushkin S.A.

(13-26): Technical support,
MS R-600 (SAO RAS)

(27-31): Adjustment, antenna measurements,
AMG 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

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,
An Tao (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,
Kovalev Yu.A. (ASC).
Responsible Erkenov A.K.

(01-30): Antenna measurements (3 hours a week),
AMG R-600 (SAO RAS)

(01-05): Test observations, secondary mirror focus search (SAO RAS).
Responsible Trushkin S.A.

(06-10): Reserve time (SAO RAS)

Feed-cabin 2

(11-30): Monitoring of the Galactic X-ray binaries with relativistic jets,
Trushkin S. (SAO RAS).
Responsible Trushkin S.A.

(11-30): Spectra of FR0 galaxies in the centimeter range,
Mikhailov A. (SAO RAS).
Responsible Mikhailov A.G.

(11-30): Radio variability of the NLS1 galaxies,
Volvach A. E. (CrAO RAS).
Responsible Erkenov A.K.

(11-30): MALBRICS collaboration: multi-frequency monitoring of blazars,
Mufakharov T. (SAO RAS).
Responsible Erkenov A.K.

(11-30): Radio spectra and variability of quasars at z>4,
Sotnikova Yu.V. (SAO RAS).
Responsible Sotnikova Yu.V.

(11-30): Monitoring the most powerful X-ray quasars on z>3,
Khorunzhev G.A. (IKI RAS).
Responsible Mikhailov A.G.

(11-30): Multi-frequency monitoring of TeV-flaring AGN: probing particle acceleration mechanisms in jets,
An Tao (Shanghai Astronomical Observatory, China).
Responsible Sotnikova Yu.V.

(11-30): MALBRICS collaboration: radio properties of transient events,
Yang Lili (Sun Yat-sen University, China).
Responsible Sotnikova Yu.V.

(11-30): The radio properties of OH Megamaser galaxies,
Zhongzu Wu (Guizhou University, China).
Responsible Semenova T.A.

Feed-cabin 3

(11-30): The Sun 13-azimuth observations (SAO RAS).
Responsible Kazanina T.N.

Feed-cabin 2

(01-05): Test observations, secondary mirror focus search (SAO RAS).
Responsible Trushkin S.A.

(06-10): Reserve time (SAO RAS)

(11-31): 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,
An Tao (Shanghai Astronomical Observatory, China).
Responsible Sotnikova Yu.V.

(01-31): MALBRICS collaboration: radio properties of transient events,
Yang Lili (Sun Yat-sen University, China).
Responsible Sotnikova Yu.V.

(01-16): Spectra of FR0 galaxies in the centimeter range,
Mikhailov A. (SAO RAS).
Responsible Mikhailov A.G.

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

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

(01-31): MALBRICS collaboration: radio properties of transient events,
Yang Lili (Sun Yat-sen University, China).
Responsible Sotnikova Yu.V.

Feed-cabin 3

(01-10): The Sun 13-azimuth observations (SAO RAS).
Responsible Kazanina T.N.

(11-31): The Sun multi-azimuth observations (SAO RAS).
Responsible Kazanina T.N.

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, SRT, Italy; Curtin University, Australia; Tuorla observatory, Finland.
3 - Sun Yat-sen University, China; University of Johannesburg, South Africa; Raman Research Institute, Indian Institute of Science, India; Shanghai Observatory, China.
4 - University of Cambridge, UK; Sun Yat-sen University, China; Raman Research Institute, Bangalore, India; Saha Institute of Nuclear Physics, Kolkata, India.
5 - Guangzhou University, China; Shanghai Observatory, China.
6 - INFIP, Argentina; Shanghai Observatory, China.
7 - Wide-range spectral studies of the Sun on RATAN-600 in the range 1-30 GHz (Bogod V., SAO RAS, SPbSU); Forecasting flares in active regions of the Sun (Space weather) (Kurochkin E.A. SAO RAS; Kislovodsk Mountain Astronomical station RAS); 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; AFRL, USA); Measurement of magnetic fields in the solar corona (Lesovoy S., ISTP SB RAS, Russia); Time series of active formations of the 25th cycle (Knyazeva I., GAO RAS, Russia); Quasiperiodic processes in solar flare active regions (Kupriyanova E., GAO RAS, Russia, SPbSU).
8 - In case of conflict, 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.