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ABSOLUTE MEASUREMENTS OF THE FLUX OF CASSIOPEIA-A AND TAURUS A AT 1.87 CENTIMETERSWRIXON GT; GOTT JR III; PENZIAS AA et al.1972; ASTROPHYS. J.; U.S.A.; DA. 1972; VOL. 174; NO 2, PART 1; PP. 399-400; BIBL. 4REF.Serial Issue

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Variability of the Radio Flux Density of the Blazar S5 0716+714 on Time Scales Less Than a MonthGORSHKOV, A. G; IPATOV, A. V; KONNIKOVA, V. K et al.Astronomy reports. 2011, Vol 55, Num 2, pp 97-107, issn 1063-7729, 11 p.Article

Rapid Variability of the Radio Flux Density of the Blazar J0721+7120 (S5 0716+714) in 2010GORSHKOV, A. G; IPATOV, A. V; RUDNITSKII, G et al.Astronomy reports. 2011, Vol 55, Num 12, pp 1096-1104, issn 1063-7729, 9 p.Article

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THE 1975.9 JOVIAN DECIMETRIC SPECTRUMSHAWHAN SD; HODGES MW; SPANGLER SR et al.1977; J. GEOPHYS. RES.; USA; DA. 1977; VOL. 82; NO 13; PP. 1901-1905; BIBL. 18 REF.Article

A FLUX-DENSITY SCALE FOR MICROWAVE FREQUENCIESDENT WA.1972; ASTROPHYS. J.; U.S.A.; DA. 1972; VOL. 177; NO 1, PART 1; PP. 93-99; BIBL. 18REF.Serial Issue

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ON QUASI-PERIODIC COMPONENTS WITH PERIODS FROM 30 TO 60 MIN OF AMPLITUDE FLUCTUATIONS OF X-BAND SOLAR RADIO EMISSIONKOBRIN MM; KORSHUNOV AI.1972; SOLAR PHYS.; NETHERL.; DA. 1972; VOL. 25; NO 2; PP. 339-342; BIBL. 12 REF.Serial Issue

DIRECT OBSERVATIONS OF LOW-ENERGY SOLAR ELECTRONS ASSOCIATED WITH A TYPE III SOLAR RADIO BURSTFRANK LA; GURNETT DA.1972; SOLAR PHYS.; NETHERL.; DA. 1972; VOL. 27; NO 2; PP. 446-465; BIBL. 28 REF.Serial Issue

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AN UPPER LIMIT FOR THE 34.3-MHZ SYNCHROTRON FLUX FROM URANUSSHAWHAN SD; CRONYN WM.1977; J. GEOPHYS. RES.; USA; DA. 1977; VOL. 82; NO 13; PP. 1947-1950; BIBL. 14 REF.Article

THE FLARE-RELATED DEPRESSION OF THE NOISE STORM ON MAY 5, 1978BOEHME A; KRUEGER A.1982; SOL. PHYS.; ISSN 0038-0938; NLD; DA. 1982; VOL. 76; NO 1; PP. 63-75; BIBL. 9 REF.Article

OBSERVATIONS OF TRAVELLING IONOSPHERIC DISTURBANCES AT LONDON, CANADALTVA J.1972; A.G.A.R.D. CONF. PROC.; FR.; DA. 1972; NO 115; PP. 22P.; ABS. FR.; BIBL. 17 REF.Serial Issue

UPPER LIMIT TO ANY 59.35-S PERIODIC RADIO EMISSION AT 18 CM FROM CG195.5+4.5OZEL ME; DICKEL JR; WEBBER JC et al.1980; NATURE; GBR; DA. 1980; VOL. 285; NO 5767; PP. 645-647; BIBL. 19 REF.Article

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Can annihilating dark matter be lighter than a few GeVs?BOEHM, C; ENSSLIN, T. A; SILKY, J et al.Journal of physics. G. Nuclear and particle physics (Print). 2004, Vol 30, Num 3, pp 279-285, issn 0954-3899, 7 p.Article

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The unusual binary pulsar psr j1744-3922 : Radio flux variability, near-infrared observation, and evolutionBRETON, R. P; ROBERTS, M. S. E; RANSOM, S. M et al.The Astrophysical journal. 2007, Vol 661, Num 2, pp 1073-1083, issn 0004-637X, 11 p., 1Article

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Comments on the absolute flux density scale at low radio frequenciesREES, N.Monthly Notices of the Royal Astronomical Society. 1990, Vol 243, Num 4, pp 637-639, issn 0035-8711Article

On secular decrease of flux density of Cassiopeia A at the frequency 38 MHzVINYAJKIN, E. N; VOLODIN, A. G; KOVAL'CHUK, O. M et al.Pis′ma v Astronomičeskij žurnal. 1992, Vol 18, Num 9, pp 755-759, issn 0320-0108Article

BETA PERSEI: RADIO STAR AND PROBABLE X-RAY STARHJELLMING RM.1972; NATURE PHYS. SCI.; G.B.; DA. 1972; VOL. 238; NO 82; PP. 52-55; BIBL. 19 REF.Serial Issue

STATISTICAL STUDY OF THE TIME SEQUENCE OF CALL FLOCCULAE AND SERIES OF RADIO FLUXES DURING SOLAR ACTIVITY CYCLE 20KARLICKY M.1977; BULL. ASTR. INST. CZECHOSL.; CSK; DA. 1977; VOL. 28; NO 4; PP. 200-217; ABS. RUS; BIBL. 21 REF.Article