An All-Russia scientific conference "The Multifaceted Universe: Theory and Observations - 2022" dedicated to the 90th anniversary of Yu.N. Parijskij was held at the Special Astrophysical Observatory of the Russian Academy of Sciences on May 23-27, 2022. Yury Nikolaevich Parijskij, a full member of the Russian Academy of Sciences, was one of the founders of Russian radio astronomy. He is the author of hundreds of scientific papers and two monographs. Under his leadership, the largest radio telescope RATAN-600 was created, with which various studies of cosmic radio sources have been carried out. Yu.N. Parijskij brought up the scientific and engineering staff of the telescope as a professional scientific school consisting of a dozen of doctors of sciences and almost a hundred of PhDs. Yuri Nikolaevich had been creating and developing modern radio astronomy methods. His scientific interests extended to many areas: the Early Universe origin and evolution, multiwavelength study of quasars and radio galaxies, deep sky radio surveys, search for the cosmic microwave background fluctuations, the Milky Way, and the Solar System.
About 140 astronomers from Russia and other countries took part in the conference.
The conference topic is broad - from planets and the Sun to objects of the Early Universe.
Reports on the scientific heritage of Yu.N. Parijskij were welcome. The conference involves review talks, thematic and poster sessions.
| Astronomical instruments and methods |
| A new Method for Verification of Astronomical Spectral Flux Density Calibrators based on SRT Data PoS(MUTO2022)001 pdf attachments |
| Development of the prototype of a large-volume liquid scintillation detector with photosensors based on silicon photomultiplayers PoS(MUTO2022)002 pdf attachments |
| The Methods and a Hardware-Software Complex for Measuring the Stability of Radio Telescope Receiving Systems PoS(MUTO2022)003 pdf attachments |
| On the role of empirical boundary conditions in space weather prediction results PoS(MUTO2022)004 pdf |
| Detection of absorption in the decimeter radio emission of solar corona PoS(MUTO2022)005 pdf |
| Digital methods of RFI mitigation in radio astronomy PoS(MUTO2022)006 pdf |
| Results of a new approach to the analysis of multi-wavelength observations data obtained with RATAN-600 PoS(MUTO2022)007 pdf |
| Computer simulation of a new deployment system for precise solid space reflector PoS(MUTO2022)008 pdf |
| A method for Identifying the Effects of Nonstationarity in the Radio Emission from Nearby Stellar Systems in Spaced Observations PoS(MUTO2022)009 pdf attachments |
| Gaia vs Hipparcos: the Accuracy of Parallax Measurements PoS(MUTO2022)010 pdf |
| The Receiving System for a Compact Antenna of the Mobile VLBI Station PoS(MUTO2022)011 pdf |
| Microwave imaging spectroscopy of the solar corona PoS(MUTO2022)014 pdf |
| Continuum radiometers of the RATAN-600 radio telescope: current state and directions of development PoS(MUTO2022)015 pdf attachments |
| A study of the astroclimate in the Dagestan mountains Agul region and at the Ali Observatory in Tibet as possible locations for the Eurasian SubMM Telescopes (ESMT) PoS(MUTO2022)072 pdf |
| Cosmology and physics of galaxies |
| CII Emission from High-Redshift Quasars As a Signature of Obscured AGNs PoS(MUTO2022)016 pdf |
| Detailed study of galaxies with the stellar counter-rotation phenomenon PoS(MUTO2022)017 pdf |
| Study of a bright sources sample in the RATAN-600 Western sector observations PoS(MUTO2022)018 pdf |
| Comparison of spectral properties of microwave background inhomogeneities on Planck maps with spectral properties of sources of RCR, NVSS and Planck catalogues PoS(MUTO2022)019 pdf |
| The intensities of Balmer lines in low resolution integrated light spectra of globular clusters PoS(MUTO2022)020 pdf |
| Determination of distances to galaxies by the brightest stars PoS(MUTO2022)021 pdf |
| Search for distant radio galaxies. Big Trio Project PoS(MUTO2022)022 pdf |
| Sources of the "Cold Experiment" surveys in different ranges of the electromagnetic spectrum PoS(MUTO2022)023 pdf |
| The splashback radius of groups and clusters of galaxies at low redshifts PoS(MUTO2022)024 pdf |
| Nearby voids and their galaxies: recent progress and prospects PoS(MUTO2022)026 pdf |
| Active galactic nuclei |
| The keys by Nikolai Kardashev and Yuri Parijskij to the Nature of Active Galactic Nuclei PoS(MUTO2022)027 pdf |
| Spectral and photometric study of the Seyfert Galaxy MRK 1095 (ARK 120) PoS(MUTO2022)028 pdf |
| Study of the radio spectra evolution of Narrow-line Seyfert 1 galaxies with RATAN-600 PoS(MUTO2022)029 pdf |
| New GPS sources candidates at high redshifts PoS(MUTO2022)030 pdf |
| The optical variability of some blazars at different time scales - recent results PoS(MUTO2022)031 pdf |
| Multi-messenger astronomy |
| The Search for Neutrino Events from the Blazar PKS 0735+17 at the Baksan Underground Scintillation Telescope PoS(MUTO2022)033 pdf |
| An approximation of the observed extragalactic neutrino background PoS(MUTO2022)034 pdf |
| Search for neutrino bursts at the Baksan Underground Scintillation Telescope PoS(MUTO2022)035 pdf |
| Stars and interstellar medium |
| The influence of host galaxy morphology on Type Ia Supernovae standardization and cosmological analysis PoS(MUTO2022)037 pdf |
| Deuterated molecules in regions of high-mass star formation PoS(MUTO2022)038 pdf |
| Photometric monitoring of eclipsing cataclysmic variables PoS(MUTO2022)039 pdf |
| A study of unknown X-ray sources PoS(MUTO2022)040 pdf |
| Long-term spectral monitoring of the high-luminosity stars in the Cas OB5 association PoS(MUTO2022)041 pdf |
| Some mathematical and physical aspects of the gravitational collapse of massive stars PoS(MUTO2022)042 pdf |
| Pushchino multibeams pulsar search: First results PoS(MUTO2022)043 pdf |
| Stars like gamma Cassiopeia: close to us and enigmatic PoS(MUTO2022)044 pdf attachments |
| Statistical physical parameter properties of Ap/Bp-stars in the Orion OB1 Association PoS(MUTO2022)045 pdf |
| The Intraday multi-frequency radio observations of the microquasar Cygnus X-3 PoS(MUTO2022)046 pdf |
| Confirmation of the star J004229.87$+$410551.8 in M31 as B[e]-supergiant PoS(MUTO2022)047 pdf |
| The history of long-term studies of Galactic X-ray binaries with jet emissions with RATAN-600 PoS(MUTO2022)048 pdf |
| Wind parameters of the new LBV in NGC1156 PoS(MUTO2022)049 pdf |
| Accretion Induced Collapse of White Dwarfs as an Alternative Symbiotic Channel to Millisecond Pulsars PoS(MUTO2022)050 pdf |
| Magnetic field of chemically peculiar stars in the Orion OB1 Association PoS(MUTO2022)051 pdf |
| Cowling resistivity and Joule dissipation in solar atmosphere PoS(MUTO2022)052 pdf |
| Two new LBV candidates in the galaxy IC342 PoS(MUTO2022)053 pdf |
| The Extremely He-rich Star HD144914 PoS(MUTO2022)055 pdf |
| Relativistic astrophysics |
| Long-term X-ray/UV observations of the ultraluminous X-ray source HolmbergII X-1. PoS(MUTO2022)056 pdf |
| Stellar mass black hole candidates in the birthplaces of radio pulsars PoS(MUTO2022)057 pdf |
| On turbulent viscosity in relativistic jets and accretion disks PoS(MUTO2022)058 pdf attachments |
| Fast transitions between single and double-peaked optical pulse profiles of millisecond pulsar J1023$+$0038 PoS(MUTO2022)059 pdf |
| On a spin-up phase in the evolutionary tracks of AR Scorpii and AE Aquarii PoS(MUTO2022)061 pdf |
| the SUN |
| Analysis of Pulsation Spectra of Chromospheric Radiation from a Solar Flare SOL2015-10-01 PoS(MUTO2022)062 pdf |
| Investigation of the polar coronal hole in the Sun with RATAN-600 in the centimeter radio range PoS(MUTO2022)063 pdf |
| The Form of Sunspots in Cycle 24 PoS(MUTO2022)064 pdf |
| A study of the Relationship Between the Microwave and Meter-Wavelength Emissions from the Solar Flare on June 3, 2021 PoS(MUTO2022)065 pdf |
| Forecasting of Solar Flares According to the Maximum Brightness Temperatures in the Period of 2011--2015 PoS(MUTO2022)066 pdf |
| Planets and planetary systems |
| Lidov-Kozai perturbation in the motion of Jupiter Trojans PoS(MUTO2022)069 pdf |
| Early universe |
| Objects with Ultra Steep Spectra in the Central Section of the RATAN Zenith Field (RZF) Catalog PoS(MUTO2022)071 pdf |