ARCHIVE RATAN-600 Observation Schedule
from 1 July to 31 December, 2021

Executive Secretary: request@sao.ru 		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.

(01-18): 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): IceCube trigger: monthly monitoring of the new high-energy neutrino candidates,
Troitski S.V. (Institute for Nuclear Research).
Responsible Erkenov A.K.

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

(01-31): The Sun observations3 (SAO RAS).
Responsible Kazanina T.N.

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

(01-31): Technical support,
Yakovenko S.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): Radio spectra and variability of quasars at z>45,
Sotnikova Yu.V. (Shanghai Astronomical Observatory, China; SAO RAS; SAO RAS).
Responsible Sotnikova Yu.V.

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

(01-31): Radio properties of the Narrow-Line Seyfert 1 Galaxies,
Lahteenmaki Anne (Metsahovi Radio Observatory, Finland).
Responsible Erkenov A.K.

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

Feed-cabin 5

(01-31): Search of fast radio bursts at 4.7 GHz.
Responsible Trushkin S.A.
A
U
G
U
S
T

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.

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

(01-31): The Sun observations3 (SAO RAS).
Responsible Kazanina T.N.

(01-07): Multifrequency monitoring of blazar variability on long time scales,
Mufakharov T. (Shanghai Astronomical Observatory, China).
Responsible Erkenov A.K.

(08-31): 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.

(01-31): Technical support,
Yakovenko S.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): Radio spectra and variability of quasars at z>45,
Sotnikova Yu.V. (SAO RAS).
Responsible Sotnikova Yu.V.

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

(01-31): Radio properties of the Narrow-Line Seyfert 1 Galaxies,
Lahteenmaki Anne (Metsahovi Radio Observatory, Finland).
Responsible Erkenov A.K.

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

Feed-cabin 5

(01-31): Search of fast radio bursts at 4.7 GHz.
Responsible Trushkin S.A.
S
E
P
T
E
M
B
E
R

Feed-cabin 1

(01-25): Monitoring of the Galactic X-ray binaries with relativistic jets1,
Trushkin S. (SAO RAS).
Responsible Trushkin S.A.

(01-25): IceCube trigger: monthly monitoring of the new high-energy neutrino candidates,
Troitski S.V. (Institute for Nuclear Research).
Responsible Erkenov A.K.

(01-25): Spectra of FR0 galaxies in the centimeter range,
Mikhailov A. (SAO RAS).
Responsible Erkenov A.K.

(01-25): Radio spectra and variability of quasars at z>45,
Sotnikova Yu.V. (SAO RAS).
Responsible Sotnikova Yu.V.

(01-18): Monitoring SRGE J170245.3 + 130104 - the most powerful X-ray quasar at z> 5,
Horunzhev G.A. (IKI RAS).
Responsible Erkenov A.K.

(01-25): The Sun observations3 (SAO RAS).
Responsible Kazanina T.N.

(26-30): Reserve time (SAO RAS)

(01-30): Technical support,
Yakovenko S.V., Shtondin A.F. (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): Radio spectra and variability of quasars at z>45,
Sotnikova Yu.V. (SAO RAS).
Responsible Sotnikova Yu.V.

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

(01-30): Radio properties of the Narrow-Line Seyfert 1 Galaxies,
Lahteenmaki Anne (Metsahovi Radio Observatory, Finland).
Responsible Erkenov A.K.

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

Feed-cabin 5

(01-30): Search of fast radio bursts at 4.7 GHz.
Responsible Trushkin S.A.
O
C
T
O
B
E
R

Feed-cabin 1

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

(02-15): Technical support,
Yakovenko S.V., Shtondin A.F. (SAO RAS)

(16-21): Adjustment, antenna measurements,
Zharov V.I. (SAO RAS)

(22-25): Test observations, secondary mirror focus search,
Trushkin S. (SAO RAS)

(26-31): Spectra of FR0 galaxies in the centimeter range,
Mikhailov A. (SAO RAS).
Responsible Erkenov A.K.

(26-31): Radio spectra and variability of quasars at z>45,
Sotnikova Yu.V. (SAO RAS).
Responsible Erkenov A.K.

(26-31): Monitoring of the Galactic X-ray binaries with relativistic jets1,
Trushkin S. (SAO RAS).
Responsible Trushkin S.A.

(26-31): IceCube trigger: monthly monitoring of the new high-energy neutrino candidates,
Troitski S.V. (Institute for Nuclear Research).
Responsible Erkenov A.K.

(26-31): The Sun observations3 (SAO RAS).
Responsible Kazanina T.N.

(01-31): Adjustment, antenna measurements,
Zharov V.I. (SAO RAS)

Feed-cabin 2

(01-10): Monitoring of the Galactic X-ray binaries with relativistic jets,
Trushkin S. (SAO RAS).
Responsible Trushkin S.A.

(01-10): Radio spectra and variability of quasars at z>45,
Sotnikova Yu.V. (SAO RAS).
Responsible Sotnikova Yu.V.

(01-10): Multifrequency monitoring of blazar variability on long time scales,
Mufakharov T. (SAO RAS).
Responsible Erkenov A.K.

(01-10): Radio properties of the Narrow-Line Seyfert 1 Galaxies,
Lahteenmaki Anne (Metsahovi Radio Observatory, Finland).
Responsible Erkenov A.K.

(01-10): The radio properties of OH Megamaser galaxies,
Zhongzu Wu (Guizhou University, China).
Responsible Erkenov A.K.

(11-15): Reserve time (SAO RAS)

(16-29): Technical support,
Yakovenko S.V., Shtondin A.F. (SAO RAS)

(30-31): Adjustment, antenna measurements,
Zharov V.I. (SAO RAS)

Feed-cabin 5

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

Feed-cabin 1

(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. (Institute for Nuclear Research).
Responsible Erkenov A.K.

(01-03): Spectra of FR0 galaxies in the centimeter range,
Mikhailov A. (SAO RAS).
Responsible Erkenov A.K.

(01-05): Radio spectra and variability of quasars at z>45,
Sotnikova Yu.V. (SAO RAS).
Responsible Sotnikova Yu.V.

(01-05): Multifrequency monitoring of blazar variability on long time scales,
Mufakharov T. (Shanghai Astronomical Observatory, China).
Responsible Erkenov A.K.

(01-13): The Sun observations3 (SAO RAS).
Responsible Kazanina T.N.

(06-28): 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.

(29-30): Multifrequency monitoring of blazar variability on long time scales,
Mufakharov T. (Shanghai Astronomical Observatory, China).
Responsible Erkenov A.K.

(01-09): Adjustment, antenna measurements,
Zharov V.I. (SAO RAS)

Feed-cabin 2

(10-13): Test observations, secondary mirror focus search,
Trushkin S. (SAO RAS).
Responsible Trushkin S.A.

(14-30): Monitoring of the Galactic X-ray binaries with relativistic jets1,
Trushkin S. (SAO RAS).
Responsible Trushkin S.A.

(14-30): Radio spectra and variability of quasars at z>45,
Sotnikova Yu.V. (SAO RAS).
Responsible Sotnikova Yu.V.

(14-30): Multifrequency monitoring of blazar variability on long time scales,
Mufakharov T. (SAO RAS; Shanghai Astronomical Observatory, China).
Responsible Erkenov A.K.

(14-30): Radio properties of the Narrow-Line Seyfert 1 Galaxies,
Lahteenmaki Anne (Metsahovi Radio Observatory, Finland).
Responsible Erkenov A.K.

(14-30): The radio properties of OH Megamaser galaxies,
Zhongzu Wu (SAO RAS; Guizhou University, China).
Responsible Erkenov A.K.

(14-30): The Sun five-azimuth observations 3 (SAO RAS).
Responsible Kazanina T.N.

(01-09): Adjustment, antenna measurements,
Zharov V.I. (SAO RAS)

Feed-cabin 2

(10-13): Test observations, secondary mirror focus search,
Trushkin S. (SAO RAS).
Responsible Trushkin S.A.

(14-30): 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.
Responsible Trushkin S.A.
D
E
C
E
M
B
E
R

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. (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.

(01-25): Radio properties of the Narrow-Line Seyfert 1 Galaxies,
Lahteenmaki Anne (Metsahovi Radio Observatory, Finland).
Responsible Erkenov A.K.

Feed-cabin 2

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

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

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

(01-31): Radio properties of the Narrow-Line Seyfert 1 Galaxies,
Lahteenmaki Anne (Metsahovi Radio Observatory, Finland).
Responsible Erkenov A.K.

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

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

(10-30): The Sun multi-azimuth observations 3 (SAO RAS).
Responsible Kazanina T.N.

(31-31): 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.
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, Russia); Correlational analysis between preflare CaII K and radio plages (Elagandula N., SAO RAS; Tlatov A., Kislovodsk Mountain Astronomical Station of the Pulkovo observatory; Mikhalyaev B., Kalmyk State University); Development of the determining physical conditions methods on the Sun flare-active regions (Yasnov L., St. Petersburg State University); Study of the chromosphere and the transition region of sunspots with ALMA interferometer and RATAN-600 (Lukicheva M., New Jersey Institute of Technology, USA); Supplementing the Coronal-like jet events extended cataloguewith RATAN-600 observational data (Kaltman T.I., SAO RAS, Russiaš).
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.