The results of the analysis of 205 brightest sources, which were found in the sky survey at the declination of the pulsar in the Crab Nebula, are presented.
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We present a study of the radio variability of bright, S1.4≥100 mJy, high-redshift quasars at z≥3 on timescales of up to 30–40 yrs. The study involved simultaneous RATAN-600 measurements at the frequencies of 2.3, 4.7, 8.2, 11.2, and 22.3 GHz in 2017–2020.
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We carry out the long-term multi-frequency monitoring of the Galactic microquasars with the RATAN-600 radio telescope almost daily in 2024 at 1.24-30 GHz. We have detected the activity from the microquasar Cygnus X-3 on 27 March after the long period of the very low hard X-ray state at 15-50 keV, named by a hyper-soft state, as according to the Swift/BAT public domain data.
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Based on the collected multiwavelength data, namely in the radio (NVSS, FIRST, RATAN-600), IR (WISE), optical (Pan-STARRS), UV (GALEX), and X-ray (ROSAT, Swift-XRT) ranges, we have performed a cluster analysis for the blazars of the Roma-BZCAT catalog.
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The microquasar Cyg X-3 entered in the hyper-soft X-ray state in mid January 2024 (Swift/BAT monitor). Bright radio flares of different intensity were observed by the Nasu telescope array (ATels #16455, #16520) and with the Allen Telescope Array (ATA; ATel #16466) in February 2024.
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Context : Understanding the mechanisms that launch and shape powerful relativistic jets from supermassive black holes (SMBHs) in high-redshift active galactic nuclei (AGN) is crucial for probing the co-evolution of SMBHs and galaxies over cosmic time.
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We present the results of our observations using the Giant Meterwave Radio Telescope (GMRT) to investigate the radio continuum and OH line emission of 10 OHM candidates from the Arecibo Legacy Fast ALFA (ALFALFA) survey.
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Eurasian patent for an invention has been received: Method for generating a catalog of measurements of radio emission parameters from blazars.
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<div>Study of high-redshift radio galaxies (HzRGs) can shed light on the active galactic nuclei (AGNs) evolution in massive elliptical galaxies. The vast majority of observed high-redshift AGNs are quasars, and there are very few radio galaxies at redshifts z>3.</div> read more →
Aims. The X-ray luminous and radio-loud AGN SRGE J170245.3+130104 discovered at z ∼ 5.5 provides unique chances to probe the SMBH growth and evolution with powerful jets in the early Universe.
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Numerical simulations of a propagating slow magnetoacoustic wave guided by a field-aligned low-β plasma nonuniformity are performed in terms of ideal magnetohydrodynamics, aiming at modeling propagating extreme ultraviolet (EUV) emission disturbances observed in the solar corona.
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This article presents the results of evaluating the possibility of conducting radio astronomy studies in the windows of atmospheric transparency ~100, ~230, and ~350 GHz using the optical Big Telescope Alt-Azimuthal (BTA) of the Special Astrophysical Observatory of the Russian Academy of Sciences (SAO RAS).
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We present the results of our study of cross-correlations between long-term multi-band observations of the radio variability of the blazar 3C 279.
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We have received a new physical characteristics fitting based on actual observational data from the Swift mission's long-duration gamma-ray bursts (LGRBs).
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The development of methods for the radio frequency interference mitigation becomes a fundamental challenge for any radio astronomy research.
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In this paper, the first in a series of four articles, the scientific goals of the Metron project are highlighted, and the characteristics of the cosmic objects available for study within its framework are provided.
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We report on a campaign on the bright black hole X-ray binary Swift J1727.8 − 1613 centered around five observations by the Imaging X-ray Polarimetry Explorer (IXPE).
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The existence of high-energy astrophysical neutrinos has been unambiguously demonstrated, but their sources remain elusive. IceCube reported an association of a 290-TeV neutrino with a gamma-ray flare of TXS 0506+056, an active galactic nucleus with a compact radio jet pointing to us.
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