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Amaldi E, Pfetsch ME, Trotter LE. (2003) On the maximum feasible subsystem problem, IISs and IIS-hypergraphs Mathematical Programming, Series B. 95: 533-554
Aglietta M, Castellina A, Fulgione W, et al. (1991) Coincidences among the data recorded by the baksan, kamioka and mont blanc underground neutrino detectors, and by the Maryland and Rome gravitational-wave detectors during Supernova 1987 A Il Nuovo Cimento C. 14: 171-193
Aglietta M, Castellina A, Fulgione W, et al. (1991) Coincidences among the data recorded by the baksan, kamioka and mont blanc underground neutrino detectors, and by the Maryland and Rome gravitational-wave detectors during Supernova 1987 A Il Nuovo Cimento C. 14: 171-193
Amaldi E, Astone P, Bassan M, et al. (1990) Sensitivity of the rome gravitational wave experiment with the explorer cryogenic resonant antenna operating at 2 k Epl. 12: 5-11
Aglietta M, Badino G, Bologna G, et al. (1989) Analysis of the data recorded by the Mont Blanc neutrino detector and by the Maryland and Rome gravitational-wave detectors during SN1987A Il Nuovo Cimento C. 12: 75-103
Amaldi E, Pallottino GV, Pizzella G. (1989) New ways with gravitational waves [10] Nature. 338: 122
Amaldi E, Bonifazi P, Castellano MG, et al. (1987) Data recordered by the rome room temperature gravitational wave antenna, during the supernova sn 1987a in the large magellanic cloud Epl. 3: 1325-1330
Amaldi E, Cosmelli C, Pallottino GV, et al. (1986) Preliminary results on the operation of a 2270 kg cryogenic gravitational-wave antenna with a resonant capacitive transducer and a d.c. SQUID amplifier Il Nuovo Cimento C. 9: 829-845
Amaldi E, Pizzella G. (1986) Estimate of the background of a gravitational-wave detector due to cosmic rays Il Nuovo Cimento C. 9: 612-620
Amaldi E, Pizzella G, Rapagnani P, et al. (1986) Data analysis for a gravitational wave antenna with resonant capacitive transducer Il Nuovo Cimento C. 9: 51-73
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