Search Results - "Astone, P."

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  1. 1

    Direct Constraints on the Ultralight Boson Mass from Searches of Continuous Gravitational Waves by Palomba, C., D’Antonio, S., Astone, P., Frasca, S., Intini, G., La Rosa, I., Leaci, P., Mastrogiovanni, S., Miller, A. L., Muciaccia, F., Piccinni, O. J., Rei, L., Simula, F.

    Published in Physical review letters (22-10-2019)
    “…Superradiance can trigger the formation of an ultralight boson cloud around a spinning black hole. Once formed, the boson cloud is expected to emit a nearly…”
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    First search for gravitational wave bursts with a network of detectors by Allen, ZA, Astone, P, Baggio, L, Busby, D, Bassan, M, Blair, DG, Bonaldi, M, Bonifazi, P, Carelli, P, Cerdonio, M, Coccia, E, Conti, L, Cosmelli, C, Crivelli Visconti V, D'Antonio, S, Fafone, V, V, Falferi, P, Fortini, P, Frasca, S, Hamilton, WO, Heng, IS, Ivanov, EN, Johnson, WW, Kingham, M, Locke, CR, Marini, A

    Published in Physical review letters (11-12-2000)
    “…We report the initial results from a search for bursts of gravitational radiation by a network of five cryogenic resonant detectors during 1997 and 1998. This…”
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    Increasing the bandwidth of resonant gravitational antennas: the case of explorer by Astone, P, Babusci, D, Bassan, M, Carelli, P, Cavallari, G, Coccia, E, Cosmelli, C, D'Antonio, S, Fafone, V, Fauth, A C, Federici, G, Giordano, G, Marini, A, Minenkov, Y, Modena, I, Modestino, G, Moleti, A, Pallottino, G V, Pizzella, G, Quintieri, L, Rocchi, A, Ronga, F, Terenzi, R, Torrioli, G, Visco, M

    Published in Physical review letters (12-09-2003)
    “…Resonant gravitational wave detectors with an observation bandwidth of tens of hertz are a reality: the antenna Explorer, operated at CERN by the ROG…”
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    The gravitational wave detector NAUTILUS operating at T = 0.1 K by Astone, P, Bassan, M, Bonifazi, P, Carelli, P, Coccia, E, Cosmelli, C, Fafone, V, Frasca, S, Marini, A, Mazzitelli, G, Minenkov, Y, Modena, I, Modestino, G, Moleti, A, Pallottino, G.V, Papa, M.A, Pizzella, G, Rapagnani, P, Ricci, F, Ronga, F, Terenzi, R, Visco, M, Votano, L

    Published in Astroparticle physics (01-08-1997)
    “…We report on the ultralow-temperature resonant-mass gravitational-wave detector NAUTILUS, operating at the Frascati INFN Laboratories. The present aim of this…”
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    On upper limits for gravitational radiation by Astone, P., Pizzella, G.

    Published in Astroparticle physics (01-02-2002)
    “…A procedure with a Bayesan approach for calculating upper limits to gravitational wave bursts from coincidence experiments with multiple detectors is…”
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    Effect of cosmic rays on the resonant gravitational wave detector Nautilus at temperature T=1.5 K by Astone, P, Babusci, D, Bassan, M, Bonifazi, P, Carelli, P, Coccia, E, D'Antonio, S, Fafone, V, Giordano, G, Marini, A, Mazzitelli, G, Minenkov, Y, Modena, I, Modestino, G, Moleti, A, Pallottino, G.V, Pizzella, G, Quintieri, L, Rocchi, A, Ronga, F, Terenzi, R, Visco, M

    Published in Physics letters. B (01-08-2002)
    “…The interaction between cosmic rays and the gravitational wave bar detector Nautilus is experimentally studied with the aluminum bar at temperature of T=1.5 K…”
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    Method for narrow-band search of continuous gravitational wave signals by Astone, P., Colla, A., D’Antonio, S., Frasca, S., Palomba, C., Serafinelli, R.

    “…Targeted searches of continuous waves from spinning neutron stars normally assume that the frequency of the gravitational wave signal is at a given known ratio…”
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    Cosmic rays observed by the resonant gravitational wave detector NAUTILUS by Astone, P, Bassan, M, Bonifazi, P, Carelli, P, Coccia, E, Fafone, V, V, D'Antonio, S, Frasca, S, Marini, A, Mauceli, E, Mazzitelli, G, Minenkov, Y, Modena, I, I, Modestino, G, Moleti, A, Pallottino, GV, Papa, MA, Pizzella, G, Ronga, F, Terenzi, R, Visco, M, Votano, L

    Published in Physical review letters (03-01-2000)
    “…The passage of cosmic rays has been observed to excite mechanical vibrations in the resonant gravitational wave detector NAUTILUS operating at temperature of…”
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    Energetic cosmic rays observed by the resonant gravitational wave detector NAUTILUS by Astone, P., Bassan, M., Bonifazi, P., Carelli, P., Coccia, E., D'Antonio, S., Fafone, V., Federici, G., Marini, A., Mazzitelli, G., Minenkov, Y., Modena, I., Modestino, G., Moleti, A., Pallottino, G.V., Pampaloni, V., Pizzella, G., Quintieri, L., Ronga, F., Terenzi, R., Visco, M., Votano, L.

    Published in Physics letters. B (01-02-2001)
    “…Cosmic-ray showers interacting with the resonant mass gravitational wave antenna NAUTILUS have been detected. The experimental results show large signals at a…”
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    Search for subsolar-mass black hole binaries in the second part of Advanced LIGO’s and Advanced Virgo’s third observing run by Abbott, R, Abe, H, Acernese, F, Ackley, K, Adhicary, S, Adhikari, N, Adhikari, R.X, Adkins, V.K, Adya, V.B, Affeldt, C, Agarwal, D, Agathos, M, Aguiar, O.D, Aiello, L, Ain, A, Ajith, P, Akutsu, T, Albanesi, S, Alfaidi, R.A, Alléné, C, Allocca, A, Altin, P.A, Amato, A, Anand, S, Ananyeva, A, Anderson, S.B, Anderson, W.G, Ando, M, Andrade, T, Andres, N, Andrés-Carcasona, M, Andrić, T, Ansoldi, S, Antelis, J.M, Antier, S, Apostolatos, T, Appavuravther, E.Z, Appert, S, Apple, S.K, Arai, K, Araya, A, Araya, M.C, Areeda, J.S, Arène, M, Aritomi, N, Arnaud, N, Arogeti, M, Aronson, S.M, Arun, K.G, Asada, H, Ashton, G, Aso, Y, Assiduo, M, de Souza Melo, S. Assis, Aston, S.M, Astone, P, Aubin, F, Aultoneal, K, Babak, S, Badaracco, F, Badger, C, Bae, S, Bae, Y, Bagnasco, S, Bai, Y, Baier, J.G, Baird, J, Bajpai, R, Baka, T, Ball, M, Ballardin, G, Ballmer, S.W, Baltus, G, Banagiri, S, Banerjee, B, Bankar, D, Barayoga, J.C, Barish, B.C, Barker, D, Barneo, P, Barone, F, Barr, B, Barsotti, L, Barsuglia, M, Barta, D, Bartlett, J, Barton, M.A, Bartos, I, Basak, S, Bassiri, R, Basti, A, Bawaj, M, Bayley, J.C, Bazzan, M, Bécsy, B, Bedakihale, V.M, Beirnaert, F, Bejger, M, Belahcene, I, Bell, A.S

    “…ABSTRACT We describe a search for gravitational waves from compact binaries with at least one component with mass $0.2$–$1.0 \, \mathrm{M}_\odot$ and mass…”
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    Frequency-Dependent Squeezed Vacuum Source for the Advanced Virgo Gravitational-Wave Detector by Acernese, F., Agathos, M., Ain, A., Albanesi, S., Alléné, C., Allocca, A., Amato, A., Amra, C., Andia, M., Andrade, T., Andres, N., Andrés-Carcasona, M., Andrić, T., Ansoldi, S., Antier, S., Apostolatos, T., Appavuravther, E. Z., Arène, M., Arnaud, N., Assiduo, M., Melo, S. Assis de Souza, Astone, P., Aubin, F., Babak, S., Badaracco, F., Bagnasco, S., Baird, J., Baka, T., Ballardin, G., Baltus, G., Banerjee, B., Barneo, P., Barone, F., Barsuglia, M., Barta, D., Basti, A., Bawaj, M., Bazzan, M., Beirnaert, F., Bejger, M., Benedetto, V., Berbel, M., Bernuzzi, S., Bersanetti, D., Bertolini, A., Bhardwaj, U., Bianchi, A., Bilicki, M., Bini, S., Bischi, M., Bitossi, M., Bizouard, M.-A., Bobba, F., Boër, M., Bogaert, G., Boileau, G., Boldrini, M., Bonavena, L. D., Bondarescu, R., Bondu, F., Bonnand, R., Boschi, V., Boudart, V., Bouffanais, Y., Bozzi, A., Bradaschia, C., Braglia, M., Branchesi, M., Breschi, M., Briant, T., Brillet, A., Brooks, J., Bruno, G., Bucci, F., Bulashenko, O., Bulik, T., Bulten, H. J., Buscicchio, R., Buskulic, D., Buy, C., Cabras, G., Cabrita, R., Cagnoli, G., Calloni, E., Canepa, M., Santoro, G. Caneva, Cannavacciuolo, M., Capocasa, E., Carapella, G., Carbognani, F., Carpinelli, M., Carullo, G., Diaz, J. Casanueva, Casentini, C., Caudill, S., Cavalieri, R., Cella, G., Cerdá-Durán, P., Cesarini, E., Chaibi, W.

    Published in Physical review letters (01-07-2023)
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    Upper limit for a gravitational-wave stochastic background with the EXPLORER and NAUTILUS resonant detectors by Astone, P, Bassan, M, Bonifazi, P, Carelli, P, Coccia, E, Cosmelli, C, Fafone, V, Frasca, S, Marini, A, Mazzitelli, G, Modena, I, Modestino, G, Moleti, A, Pallottino, G.V, Papa, M.A, Pizzella, G, Rapagnani, P, Ricci, F, Ronga, F, Terenzi, R, Visco, M, Votano, L

    Published in Physics letters. B (26-09-1996)
    “…We discuss the sensitivity of resonant-mass gravitational-wave detectors to a cosmic stochastic background of gravitational waves. We report the experimental…”
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    Analysis of 3 years of data from the gravitational wave detectors EXPLORER and NAUTILUS by Astone, P., Bassan, M., Coccia, E., D’Antonio, S., Fafone, V., Giordano, G., Marini, A., Minenkov, Y., Modena, I., Moleti, A., Pallottino, G. V., Pizzella, G., Rocchi, A., Ronga, F., Terenzi, R., Visco, M.

    “…We performed a search for short gravitational wave bursts using about 3 years of data of the resonant bar detectors Nautilus and Explorer. Two types of…”
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