ARCHIVE |
RATAN-600 Observation Schedule from January 1 to June 30, 2020 Executive Secretary: request@sao.ru |
Russian version |
North Sector | South+Flat | South Sector | West Sector | |
---|---|---|---|---|
J A N U A R Y |
Feed-cabin 1 (01-31): Radio variability of the Galactic X-ray binaries with relativistic jets1, (01-24): Radio properties of the Narrow-Line Seyfert 1 Galaxies, (01-24): Radio properties of the blazars on the long time scales, (25-31): Radio properties of OH Megamaser (OHM) galaxies, |
Feed-cabin 3 (01-31): The Sun five-azimuth observations 4. Feed-cabin 2 (01-31): Radio variability of the Galactic X-ray binaries with relativistic jets1, (01-31): Radio properties of the blazars on the long time scales, (01-31): Radio properties of the Narrow-Line Seyfert 1 Galaxies, Feed-cabin 3 (10-31): The Sun multi-azimuth observations 5. |
Feed-cabin 2 (01-31): Radio variability of the Galactic X-ray binaries with relativistic jets1, |
Feed-cabin 5 (01-31): Test observations (SAO RAS). |
F E B R U A R Y |
Feed-cabin 1 (01-04): Reserve time (SAO RAS) (05-22): Radio variability of the Galactic X-ray binaries with relativistic jets2, (05-15): Study of the long-term variability of the extragalactic radio sources in the declination range from 11 up to 18 degrees, (16-22): The AGN study with the RATAN-600 and VLBI 3, (23-29): Radio variability of the Galactic X-ray binaries with relativistic jets, (23-29): Radio properties of the Narrow-Line Seyfert 1 Galaxies, (23-29): Radio properties of the blazars on the long time scales, (23-29): Radio properties of the FR0 galaxies, |
Feed-cabin 3 (01-29): The Sun five-azimuth observations 4. Feed-cabin 2 (01-29): Radio variability of the Galactic X-ray binaries with relativistic jets, (01-29): Radio properties of the blazars on the long time scales, (01-29): Radio properties of the Narrow-Line Seyfert 1 Galaxies, |
Feed-cabin 2 (01-29): Radio variability of the Galactic X-ray binaries with relativistic jets, |
Feed-cabin 5 (01-29): Test observations (SAO RAS). |
M A R C H |
Feed-cabin 1 (01): Radio variability of the Galactic X-ray binaries with relativistic jets, (01): Radio properties of the blazars on the long time scales, (01): Radio properties of the FR0 galaxies, (02-29): Radio variability of the Galactic X-ray binaries with relativistic jets2, (02-29): The AGN study with the RATAN-600 and VLBI 3, (30-31): Technical support, |
Feed-cabin 3 (01-09): The Sun five-azimuth observations 4. Feed-cabin 2 (01-31): Radio variability of the Galactic X-ray binaries with relativistic jets, (01-31): Radio properties of the blazars on the long time scales, (01-31): Radio properties of the Narrow-Line Seyfert 1 Galaxies, Feed-cabin 3 (10-25): The Sun multi-azimuth observations5. Testing of the antenna system (South+Flat). (26-31): The Sun five-azimuth observations 4. |
Feed-cabin 2 (01-31): Radio variability of the Galactic X-ray binaries with relativistic jets, |
Feed-cabin 5 (01-31): Test observations (SAO RAS). |
A P R I L |
(01-13): Technical support, (14-18): Adjustment, antenna measurements, Feed-cabin 1 (19-24): Test observations, secondary mirror focus search, (25-26): Reserve time (SAO RAS) (27-30): Radio variability of the Galactic X-ray binaries with relativistic jets, (27-30): Study of the long-term variability of the extragalactic radio sources in the declination range from 11 up to 18 degrees, |
Feed-cabin 3 (01-15): The Sun five-azimuth observations 4. Feed-cabin 2 (01-15): Radio variability of the Galactic X-ray binaries with relativistic jets, (01-15): Radio properties of the blazars on the long time scales, (01-15): Radio properties of the Narrow-Line Seyfert 1 Galaxies, (16-30): Technical support, |
Feed-cabin 2 (01-15): Radio variability of the Galactic X-ray binaries with relativistic jets, (16-30): Technical support, |
Feed-cabin 5 (01-30): Test observations (SAO RAS). |
M A Y |
Feed-cabin 1 (01-31): Radio variability of the Galactic X-ray binaries with relativistic jets1, (01-06): Study of the long-term variability of the extragalactic radio sources in the declination range from 11 up to 18 degrees, (07-31): Radio properties of the distant quasars, |
Feed-cabin 3 (01-31): The Sun five-azimuth observations 4. Feed-cabin 2 (01-31): Radio variability of the Galactic X-ray binaries with relativistic jets, (01-31): Radio properties of the blazars on the long time scales, (01-31): Radio properties of the Narrow-Line Seyfert 1 Galaxies, |
Feed-cabin 2 (01-31): Radio variability of the Galactic X-ray binaries with relativistic jets, |
Feed-cabin 5 (01-31): Test observations (SAO RAS). |
J U N E |
Feed-cabin 1 (01-06): Radio properties of the distant quasars, (01-13): Radio variability of the Galactic X-ray binaries with relativistic jets1, (07-13): Radio properties of OH Megamaser (OHM) galaxies, (07-13): Radio properties of the blazars on the long time scales, (14-20): The AGN study with the RATAN-600 and VLBI 3, (14-30): Radio variability of the Galactic X-ray binaries with relativistic jets2, (21-30): Study of the long-term variability of the extragalactic radio sources in the declination range from 11 up to 18 degrees, |
Feed-cabin 3 (01-09): The Sun five-azimuth observations 4. Feed-cabin 2 (01-30): Radio variability of the Galactic X-ray binaries with relativistic jets, (01-30): Radio properties of the blazars on the long time scales, (01-30): Radio properties of the Narrow-Line Seyfert 1 Galaxies, Feed-cabin 3 (10-25): The Sun multi-azimuth observations 4. Testing of the antenna system (South+Flat) in the tracking mode. (26-30): The Sun five-azimuth observations 4. |
Feed-cabin 2 (01-30): Radio variability of the Galactic X-ray binaries with relativistic jets, |
Feed-cabin 5 (01-30): Test observations (SAO RAS). |
1 - SAO RAS; ICRANet, Italy; INAF-IAPS Italy; SAO, USA; Finnish Centre for Astronomy with ESO FINCA; Curtin U., Australia.
2 - During a trigger.
3 - NRAO, USA; Shanghai Astronomical Observatory, China; Max-Planck-Insitut für Radioastronomie, Germany; Joint Institute for VLBI in Europe; IRA INAF, Italy; Netherlands Institute for Radio Astronomy, Netherlands.
4 - The study of the active regions magnetosphere in a wide radio waves range (Bogod V., SAO RAS, Russia); Investigation of ultra-weak solar activity at microwaves (Lesovoi S., Institute of Solar-Terrestrial physics, Russia); Study of the solar floccules in the CaIIK line and in the microwave range with GAS GAO and RATAN-600 (Tlatov A., CAO RAS, Russia); Development of the determining physical conditions methods on the Sun flare-active regions (Yasnov L., St. Petersburg State University, Russia); Structure and evolution of solar active regions (Alissandrakis Costas, University of Ioannina, Greece); Correlational analysis between preflare CaII K and radio plages (Elagandula N., Osmania State University, India); Study of the chromosphere and the transition region of sunspots with ALMA interferometer and RATAN-600 (Lukicheva M., New Jersey Institute of Technology, USA); The Sun microflare observations (Nakaryakov V., The University of Warwick, UK).
5 - During simultaneous observations on ALMA.
Feed-cabin 1 - secondary mirror with complex equipment
of the continuous spectrum of 1.28-21.7 GHz.
Feed-cabin 2 - secondary mirror with complex equipment
of the continuous spectrum of 2.25-21.7 GHz (ERIDAN).
Feed-cabin 3 - secondary mirror with solar
spectral-polarization complex.