ON POSSIBLE LONG-PERIOD PULSATIONS IN THE HARD X-RAY FLUX OF CYGNUS X - 1FRONTERA F; FULIGNI F.1976; ASTROPHYS. SPACE SCI.; NETHERL.; DA. 1976; VOL. 42; NO 1; PP. 185-188; BIBL. 10 REF.Article

POWER SPECTRAL DENSITY ANALYSIS OF HARD X-RAY EMISSION OF CYG X-1FRONTERA F; FULIGNI F.1981; SPACE SCI. REV.; ISSN 0038-6308; NLD; DA. 1981; VOL. 30; NO 1-4; PP. 379-384; BIBL. 12 REF.Conference Paper

THE EFFECT OF DEAD TIME ON THE POWER SPECTRAL DENSITY ESTIMATES OF DISCRETE TIME SERIESFRONTERA F; FULIGNI F.1978; NUCL. INSTRUM. METHODS; NLD; DA. 1978; VOL. 157; NO 3; PP. 557-561; BIBL. 3 REF.Article

EVIDENCE FOR LONG-PERIOD SPORADIC PULSATIONS IN THE HARD X-RAY FLUX OF CYGNUS X-1.FRONTERA F; FULIGNI F.1975; ASTROPHYS. J.; U.S.A.; DA. 1975; VOL. 198; NO 3 PART. 2; PP. 105-108; BIBL. 5 REF.Article

SEARCH FOR 4.8-HOUR MODULATION OF THE CYG X - 3 INTENSITY IN HARD X-RAYS.FERETTI L; FRONTERA F; FULIGNI F et al.1975; ASTROPHYS. LETTERS; U.S.A.; DA. 1975; VOL. 16; NO 1; PP. 13-15; BIBL. 6 REF.Article

LONG TERM VARIABILITY OF CYG X-1 IN HARD X-RAYS.FRONTERA F; FULIGNI F; CAVANI C et al.1975; ASTROPHYS. SPACE SCI.; NETHERL.; DA. 1975; VOL. 32; NO 1; PP. 197-203; BIBL. 10 REF.Article

ON THE DETECTABILITY OF ADVANCED GRAVITATIONAL RADIATIONFORTINI P; FULIGNI F; GUALDI C et al.1978; LETTERE NUOVO CIMENTO; ITA; DA. 1978; VOL. 23; NO 9; PP. 345-348; BIBL. DISSEM.Article

Parametric detector as a tunable antenna for continuous gravitational radiationBORDONI, F; FULIGNI, F.Physical review. D. Particles and fields. 1983, Vol 28, Num 6, pp 1285-1290, issn 0556-2821Article

CORRELATION OF COSMIC-RAY COUNTS AT BALLOON ALTITUDES ON 100 MS TIME SCALE.CAVANI C; FRONTERA F; FULIGNI F et al.1974; LETTERE NUOVO CIMENTO; ITAL.; DA. 1974; VOL. 11; NO 16; PP. 673-675Article

FLARE FROM THE PERSEUS REGION IN HARD X-RAYS.FULIGNI F; BRINI D; DUSI W et al.1976; ASTROPHYS. J.; U.S.A.; DA. 1976; VOL. 208; NO 3 PART. 2; PP. L111-L113; BIBL. 12 REF.Article

A NEW ROCKET MEASUREMENT OF THE DIFFUSE X-RAY BACKGROUND.HORSTMAN MORETTI E; FULIGNI F; HORSTMAN HM et al.1974; ASTROPHYS. SPACE SCI.; NETHERL.; DA. 1974; VOL. 27; NO 1; PP. 195-201; BIBL. 21 REF.Article

DETECTION OF PSEUDO GAMMA-RAY BURSTS OF LONG DURATIONFRONTERA F; FULIGNI F; MORELLI E et al.1981; ASTROPHYS. SPACE SCI.; ISSN 0004-640X; NLD; DA. 1981; VOL. 75; NO 1; PP. 211-217; BIBL. 15 REF.Conference Paper

HARD X-RAY OBSERVATION OF THE PERSEUS REGION.BRINI D; FRONTERA F; FULIGNI F et al.1976; ASTROPHYS. LETTERS; U.S.A.; DA. 1976; VOL. 18; NO 1; PP. 15-17; BIBL. 11 REF.Article

HARD X-RAY EMISSION FROM NGC 4151 AND MCG 8-11-11 REGIONSFRONTERA F; FULIGNI F; MORELLI E et al.1979; ASTROPHYS. J.; USA; DA. 1979; VOL. 234; NO 2 PART. 1; PP. 477-480; BIBL. 14 REF.Article

Recent developments in gravity gradiometry from the space-shuttle-borne tethered satellite systemLORENZINI, E. C; GULLAHORN, G. E; FULIGNI, F et al.Journal of applied physics. 1988, Vol 63, Num 1, pp 216-223, issn 0021-8979Article

Testing deviations from the inverse square law with a freely falling gravity gradiometer at balloon altitudesCIUFOLINI, I; FULIGNI, F; IAFOLLA, V et al.Nuovo cimento della società italiana di fisica. C. 1992, Vol 15, Num 6, pp 973-982, issn 0390-5551Conference Paper

Application to other fields of techniques used for gravity wave detectionBORDONI, F; FULIGNI, F; IAFOLLA, V et al.Nuovo cimento della società italiana di fisica. C. 1990, Vol 13, Num 1, pp 49-58, issn 0390-5551, 10 p.Conference Paper

INFORMATION ON THE OPERATION OF THE M=389 KG GRAVITATIONAL-WAVE ANTENNA OF THE ROMA GROUP AT AN EFFECTIVE NOISE TEMPERATURE OF T_EFF=0.3 KAMALDI E; MODENA I; PALLOTTINO GV et al.1980; LETTERE NUOVO CIMENTO; ITA; DA. 1980; VOL. 28; NO 10; PP. 362-366; BIBL. 5 REF.Article

Noise attenuators for gravity experiments in spaceNOBILI, A. M; CATASTINI, G; DI VIRGILIO, A et al.Physics letters. A. 1991, Vol 160, Num 1, pp 45-54, issn 0375-9601Article