ARCHIVE RATAN-600 Observation Schedule
from January 1 to June 30, 2024

Executive Secretary: [email protected] 		Russian version

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

(02-25): IceCube trigger1: monthly monitoring of the new high-energy neutrino candidates,
Troitski S.V. (Institute for Nuclear Research).
Responsible Erkenov A.K.

(02-25): Monitoring of the Galactic X-ray binaries with relativistic jets2,
Trushkin S. (SAO RAS).
Responsible Trushkin S.A.

(02-25): 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.

(26-29): Reserve time,
SAO RAS

(30-31): Monitoring SRGE J170245.3 + 130104 - the most powerful X-ray quasar at z> 5,
Khorunzhev G.A. (IKI RAS).
Responsible Mikhailov A.G.

(30-31): MALBRICS collaboration3: multi-frequency monitoring of blazars,
Mufakharov T. (SAO RAS).
Responsible Erkenov A.K.

(30-31): The radio properties of OH Megamaser galaxies,
Zhongzu Wu (Guizhou University, China).
Responsible Semenova T.A.

(30-31): Investigation of the radio properties of galaxies at z>3,
Khabibullina M. (SAO RAS).
Responsible Mikhailov A.G.

Feed-cabin 2

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

(02-31): The radio properties of OH Megamaser galaxies,
Zhongzu Wu (Guizhou University, China).
Responsible Semenova T.A.

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

(02-31): Radio variability of the NLS1 galaxies,
Volvach A. E. (CrAO RAS).
Responsible Erkenov A.K.

(02-31): MALBRICS collaboration3: multi-frequency monitoring of blazars,
Mufakharov T. (SAO RAS).
Responsible Erkenov A.K.

(02-31): Radio spectra and variability of quasars at z>44,
Sotnikova Yu.V. (SAO RAS).
Responsible Sotnikova Yu.V.

(02-31): MALBRICS collaboration3: radio properties of transient events,
Yang Lili (Sun Yat-sen University, China).
Responsible Sotnikova Yu.V.

(02-31): Monitoring SRGE J170245.3 + 130104 - the most powerful X-ray quasar at z> 5,
Khorunzhev G.A. (IKI RAS).
Responsible Mikhailov A.G.

Feed-cabin 3

(02-31): The Sun five-azimuth observations 5 (SAO RAS).
Responsible Kazanina T.N.

Feed-cabin 2

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

Feed-cabin 5

(02-31): Search of fast radio bursts at 4.7 GHz,
Trushkin S. (SAO RAS).
Responsible Bursov N.N.
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Feed-cabin 1

(01-24): MALBRICS collaboration3: multi-frequency monitoring of blazars,
Mufakharov T. (SAO RAS).
Responsible Erkenov A.K.

(01-24): Investigation of the radio properties of galaxies at z>3,
Khabibullina M. (SAO RAS).
Responsible Mikhailov A.G.

(01-24): The radio properties of OH Megamaser galaxies,
Zhongzu Wu (Guizhou University, China).
Responsible Semenova T.A.

(01-29): IceCube trigger1: monthly monitoring of the new high-energy neutrino candidates,
Troitski S.V. (Institute for Nuclear Research).
Responsible Erkenov A.K.

(01-24): MALBRICS collaboration3: radio properties of transient events,
Yang Lili (Sun Yat-sen University, China).
Responsible Sotnikova Yu.V.

(01-29): Monitoring of the Galactic X-ray binaries with relativistic jets6,
Trushkin S. (SAO RAS).
Responsible Trushkin S.A.

(01-24): Radio variability of the NLS1 galaxies,
Volvach A. E. (CrAO RAS).
Responsible Erkenov A.K.

(01-24): Monitoring SRGE J170245.3 + 130104 - the most powerful X-ray quasar at z> 5,
Khorunzhev G.A. (IKI RAS).
Responsible Mikhailov A.G.

(18-24): Spectra of FR0 galaxies in the centimeter range,
Mikhailov A. (SAO RAS).
Responsible Mikhailov A.G.

(25-29): 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

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

(01-29): The radio properties of OH Megamaser galaxies,
Zhongzu Wu (Guizhou University, China).
Responsible Semenova T.A.

(01-29): Spectra of FR0 galaxies in the centimeter range,
Mikhailov A. (SAO RAS).
Responsible Mikhailov A.G.

(01-29): Radio variability of the NLS1 galaxies,
Volvach A. E. (CrAO RAS).
Responsible Erkenov A.K.

(01-29): MALBRICS collaboration3: multi-frequency monitoring of blazars,
Mufakharov T. (SAO RAS).
Responsible Erkenov A.K.

(01-29): Radio spectra and variability of quasars at z>44,
Sotnikova Yu.V. (SAO RAS).
Responsible Sotnikova Yu.V.

(01-29): MALBRICS collaboration3: radio properties of transient events,
Yang Lili (Sun Yat-sen University, China).
Responsible Sotnikova Yu.V.

(01-29): Monitoring SRGE J170245.3 + 130104 - the most powerful X-ray quasar at z> 5,
Khorunzhev G.A. (IKI RAS).
Responsible Mikhailov A.G.

Feed-cabin 3

(01-29): The Sun five-azimuth observations 5 (SAO RAS).
Responsible Kazanina T.N.

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

Feed-cabin 5

(01-29): Search of fast radio bursts at 4.7 GHz,
Trushkin S. (SAO RAS).
Responsible Bursov N.N.
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Feed-cabin 1

(01-24): IceCube trigger1: monthly monitoring of the new high-energy neutrino candidates,
Troitski S.V..
Responsible Erkenov A.K.

(01-24): 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.

(01-24): Monitoring of the Galactic X-ray binaries with relativistic jets6,
Trushkin S. (SAO RAS).
Responsible Trushkin S.A.

(01-24): Monitoring SRGE J170245.3 + 130104 - the most powerful X-ray quasar at z> 5,
Khorunzhev G.A. (IKI RAS).
Responsible Mikhailov A.G.

(25-31): Technical support,
Shtondin V., Shtondin A.F. (SAO RAS)

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

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

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

(01-31): MALBRICS collaboration3: multi-frequency monitoring of blazars,
Mufakharov T. (SAO RAS).
Responsible Erkenov A.K.

(01-31): Radio spectra and variability of quasars at z>44,
Sotnikova Yu.V. (SAO RAS).
Responsible Sotnikova Yu.V.

(01-31): MALBRICS collaboration3: radio properties of transient events,
Yang Lili (Sun Yat-sen University, China).
Responsible Sotnikova Yu.V.

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

Feed-cabin 3

(01-10): The Sun five-azimuth observations 5 (SAO RAS).
Responsible Kazanina T.N.

(11-31): The Sun multi-azimuth observations 5 (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.
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Feed-cabin 1

(01-05): Technical support,
Shtondin V., Shtondin A.F. (SAO RAS)

(04-08): Adjustment, antenna measurements,
Zharov V.I. (SAO RAS)

(09-12): Test observations, secondary mirror focus search

(13-15): Reserve time (SAO RAS)

(16-30): IceCube trigger1: monthly monitoring of the new high-energy neutrino candidates,
Troitski S.V. (Institute for Nuclear Research).
Responsible Erkenov A.K.

(16-30): Monitoring of the Galactic X-ray binaries with relativistic jets,
Trushkin S. (SAO RAS).
Responsible Trushkin S.A.

(16-30): MALBRICS collaboration3: multi-frequency monitoring of blazars,
Mufakharov T. (SAO RAS).
Responsible Erkenov A.K.

(16-30): Monitoring SRGE J170245.3 + 130104 - the most powerful X-ray quasar at z> 5,
Khorunzhev G.A. (IKI RAS).
Responsible Mikhailov A.G.

(16-30): MALBRICS collaboration3: radio properties of transient events,
Yang Lili (Sun Yat-sen University, China).
Responsible Sotnikova Yu.V.

(16-30): Spectra of FR0 galaxies in the centimeter range,
Mikhailov A. (SAO RAS).
Responsible Mikhailov A.G.

(16-26): Radio spectra and variability of quasars at z>44,
Sotnikova Yu.V. (SAO RAS).
Responsible Sotnikova Yu.V.

Feed-cabin 2

(01-07): Monitoring of the Galactic X-ray binaries with relativistic jets,
Trushkin S. (SAO RAS).
Responsible Trushkin S.A.

(01-07): The radio properties of OH Megamaser galaxies,
Zhongzu Wu (Guizhou University, China).
Responsible Semenova T.A.

(01-07): Spectra of FR0 galaxies in the centimeter range,
Mikhailov A. (SAO RAS).
Responsible Mikhailov A.G.

(01-07): Radio variability of the NLS1 galaxies,
Volvach A. E. (CrAO RAS).
Responsible Erkenov A.K.

(01-07): MALBRICS collaboration3: multi-frequency monitoring of blazars,
Mufakharov T. (SAO RAS).
Responsible Erkenov A.K.

(01-07): Radio spectra and variability of quasars at z>44,
Sotnikova Yu.V. (SAO RAS).
Responsible Sotnikova Yu.V.

(01-07): MALBRICS collaboration3: radio properties of transient events,
Yang Lili (Sun Yat-sen University, China).
Responsible Sotnikova Yu.V.

(01-07): Monitoring SRGE J170245.3 + 130104 - the most powerful X-ray quasar at z> 5,
Khorunzhev G.A. (IKI RAS).
Responsible Mikhailov A.G.

Feed-cabin 3

(01-07): The Sun five-azimuth observations 5 (SAO RAS).
Responsible Kazanina T.N.

Feed-cabin 2

(08-19): Technical support,
Shtondin V., Shtondin A.F. (SAO RAS)

(10-30): Adjustment, antenna measurements,
Zharov V.I. (SAO RAS)

Feed-cabin 2

(01-07): Monitoring of the Galactic X-ray binaries with relativistic jets,
Trushkin S. (SAO RAS).
Responsible Trushkin S.A.

(08-19): Technical support,
Shtondin V., Shtondin A.F. (SAO RAS)

(10-30): Adjustment, antenna measurements,
Zharov V.I. (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

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

(01-31): Radio spectra and variability of quasars at z>44,
Sotnikova Yu.V. (SAO RAS).
Responsible Sotnikova Yu.V.

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

(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,
Trushkin S. (SAO RAS).
Responsible Trushkin S.A.

(01-31): MALBRICS collaboration3: radio properties of transient events,
Yang Lili (Sun Yat-sen University, China).
Responsible Sotnikova Yu.V.

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

(01-06): MALBRICS collaboration3: multi-frequency monitoring of blazars,
Mufakharov T. (SAO RAS).
Responsible Erkenov A.K.

Feed-cabin 2

(01-02): Adjustment, antenna measurements,
Zharov V.I. (SAO RAS)

(03-05): Test observations, secondary mirror focus search,
Trushkin S. (SAO RAS)

(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.

(11-31): The radio properties of OH Megamaser galaxies,
Zhongzu Wu (Guizhou University, China).
Responsible Semenova T.A.

(11-31): Spectra of FR0 galaxies in the centimeter range,
Mikhailov A. (SAO RAS).
Responsible Mikhailov A.G.

(11-31): Radio variability of the NLS1 galaxies,
Volvach A. E. (CrAO RAS).
Responsible Erkenov A.K.

(11-31): MALBRICS collaboration3: multi-frequency monitoring of blazars,
Mufakharov T. (SAO RAS).
Responsible Erkenov A.K.

(11-31): Radio spectra and variability of quasars at z>44,
Sotnikova Yu.V. (SAO RAS).
Responsible Sotnikova Yu.V.

(11-31): MALBRICS collaboration3: radio properties of transient events,
Yang Lili (Sun Yat-sen University, China).
Responsible Sotnikova Yu.V.

(11-31): Monitoring SRGE J170245.3 + 130104 - the most powerful X-ray quasar at z> 5,
Khorunzhev G.A. (IKI RAS).
Responsible Mikhailov A.G.

Feed-cabin 3

(11-31): The Sun five-azimuth observations 5 (SAO RAS).
Responsible Kazanina T.N.

Feed-cabin 2

(01-02): Adjustment, antenna measurements,
Zharov V.I. (SAO RAS)

(03-05): Test observations, secondary mirror focus search,
Trushkin S. (SAO RAS)

(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

(01-31): Search of fast radio bursts at 4.7 GHz,
Trushkin S. (SAO RAS).
Responsible Bursov N.N.
J
U
N
E

Feed-cabin 1

(01-30): IceCube trigger1: 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 jets6,
Trushkin S. (SAO RAS).
Responsible Trushkin S.A.

(01-30): Monitoring SRGE J170245.3 + 130104 - the most powerful X-ray quasar at z> 5,
Khorunzhev G.A. (IKI RAS).
Responsible Mikhailov A.G.

(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.

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

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

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

(01-30): MALBRICS collaboration3: multi-frequency monitoring of blazars,
Mufakharov T. (SAO RAS).
Responsible Erkenov A.K.

(01-30): Radio spectra and variability of quasars at z>44,
Sotnikova Yu.V. (SAO RAS).
Responsible Sotnikova Yu.V.

(01-30): MALBRICS collaboration3: radio properties of transient events,
Yang Lili (Sun Yat-sen University, China).
Responsible Sotnikova Yu.V.

(01-30): Monitoring SRGE J170245.3 + 130104 - the most powerful X-ray quasar at z> 5,
Khorunzhev G.A. (IKI RAS).
Responsible Mikhailov A.G.

Feed-cabin 3

(01-09): The Sun five-azimuth observations 5 (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 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 - Astrospace center, 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; ShAO CAS, China (under the contract № 075-15-2022-1227).
4 - INFIP, Argentina; ShAO CAS, China.
5 - Study of flare plasma structures in the decimeter range with new technical capabilities of RATAN-600 (Bogod V., SAO RAS); Data acquisition in the radio spectrum of the quasiperiodic pulsations (QPPs) for the subsequent statistical and theoretical analyses (Elagandula N., SAO RAS, Kalmyk state university, Kalmykia, University of Warwick, UK); Measurement of magnetic fields in the solar corona (Lesovoi S., ISTP SB RAS); Joint studies of the chromosphere and the transitional region of sunspots with the RATAN and ALMA interferometer (Lukicheva M., New Jersey Institute of Technology); Development of methods for determining physical conditions in active regions on the Sun (Stupishin A., SPbU).
6 - 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.