Zobrazeno 1 - 10
of 22
pro vyhledávání: '"Cieślar, Marek"'
Autor:
Koley, Soumen, Harms, Jan, Allocca, Annalisa, Calloni, Enrico, De Rosa, Rosario, Errico, Luciano, Esposito, Marina, Badaracco, Francesca, Rei, Luca, Bertolini, Alessandro, Bulik, Tomasz, Cieslar, Marek, Pietrzak, Mateusz, Suchenek, Mariusz, Fiori, Irene, Paoli, Andrea, Tringali, Maria Concetta, Ruggi, Paolo, Hild, Stefan, Singha, Ayatri, Idzkowski, Bartosz, Suchinski, Maciej, Masserot, Alain, Rolland, Loic, Mours, Benoit, Paoletti, Federico
A system was recently implemented in the Virgo detector to cancel noise in its data produced by seismic waves directly coupling with the suspended test masses through gravitational interaction. The data from seismometers are being filtered to produce
Externí odkaz:
http://arxiv.org/abs/2404.13170
Autor:
Koley, Soumen, Harms, Jan, Allocca, Annalisa, Calloni, Enrico, De Rosa, Rosario, Errico, Luciano, Esposito, Marina, Badaracco, Francesca, Rei, Luca, Bertolini, Alessandro, Bulik, Tomasz, Cieslar, Marek, Pietrzak, Mateusz, Suchenek, Mariusz, Fiori, Irene, Paoli, Andrea, Tringali, Maria Concetta, Ruggi, Paolo, Hild, Stefan, Singha, Ayatri, Idzkowski, Bartosz, Suchinski, Maciej, Masserot, Alain, Rolland, Loic, Mours, Benoit, Paoletti, Federico
Terrestrial gravity perturbations caused by seismic fields produce the so-called Newtonian noise in gravitational-wave detectors, which is predicted to limit their sensitivity in the upcoming observing runs. In the past, this noise was seen as an inf
Externí odkaz:
http://arxiv.org/abs/2310.17781
Publikováno v:
A&A 681, A56 (2024)
The Einstein Telescope (ET) is a proposed third-generation, wide-band gravitational wave (GW) detector. Given its improved detection sensitivity in comparison to the second-generation detectors, it will be capable of exploring the Universe with GWs u
Externí odkaz:
http://arxiv.org/abs/2304.01341
Autor:
Cieślar, Marek, Bulik, Tomasz, Curyło, Małgorzata, Sieniawska, Magdalena, Singh, Neha, Bejger, Michał
Publikováno v:
A&A 649, A92 (2021)
Aims. We estimate the number of pulsars, detectable as continuous gravitational wave sources with the current and future gravitational-wave detectors, assuming a simple phenomenological model of evolving non-axisymmetry of the rotating neutron star.
Externí odkaz:
http://arxiv.org/abs/2102.08854
Autor:
Ebr, Jan, Mandát, Dušan, Pech, Miroslav, Chytka, Ladislav, Juryšek, Jakub, Prouza, Michael, Janeček, Petr, Trávníček, Petr, Blažek, Jiří, Bulik, Tomasz, Cieslar, Marek, Suchenek, Mariusz, Rizi, Vincenzo, Pietropaolo, Ermanno, Iarlori, Marco, Aramo, Carla, Valore, Laura, Di Pierro, Federico, Vallania, Piero, Depaoli, Davide, Will, Martin, Gaug, Markus, Font, Lluís, Mašek, Martin, Eliášek, Jiří, Jelínek, Martin, Karpov, Sergey
Advanced knowledge of the detailed atmospheric properties of both the future sites of the Cherenkov Telescope Array is essential in preparation of the arrival of the first scientific data. Meteorological variables are studied using a dedicated charac
Externí odkaz:
http://arxiv.org/abs/1909.08088
We present a model of evolution of solitary neutron stars, including spin parameters, magnetic field decay, motion in the Galactic potential and birth inside spiral arms. We use two parametrizations of the radio-luminosity law and model the radio sel
Externí odkaz:
http://arxiv.org/abs/1803.02397
Autor:
Tovmassian, Gagik, Hernandez, Mercedes-Stephania, Ochoa, Jose Luis, Ernenwein, Jean-Pierre, Mandat, Dusan, Pech, Miroslav, Frayn, Ilse Plauchu, Colorado, Enrique, Murillo, Jose Manuel, Cesena, Urania, Garcia, Benjamin, Lee, William H., Bulik, Tomasz, Garczarczyk, Markus, Fruck, Christian, Costantini, Heide, Cieslar, Marek, Aune, Taylor, Vincent, Stephane, Carr, John, Serre, Natalia, Janecek, Petr, Haefner, Dennis
We conducted an 18 month long study of the weather conditions of the Vallecitos, a proposed site in Mexico to harbor the northern array of the Cherenkov Telescope Array (CTA). It is located in Sierra de San Pedro Martir (SPM) a few kilometers away fr
Externí odkaz:
http://arxiv.org/abs/1601.02383
Autor:
Fruck, Christian, Gaug, Markus, Ernenwein, Jean-Pierre, Mandát, Dušan, Schweizer, Thomas, Häfner, Dennis, Bulik, Tomasz, Cieslar, Marek, Costantini, Heide, Dominik, Michal, Ebr, Jan, Garczarczyk, Markus, Lorentz, Eckart, Pareschi, Giovanni, Pech, Miroslav, Puerto-Giménez, Irene, Teshima, Masahiro
Many atmospheric and climatic criteria have to be taken into account for the selection of a suitable site for the next generation of imaging air-shower Cherenkov telescopes, the "Cherenkov Telescope Array" CTA. Such data are not available with suffic
Externí odkaz:
http://arxiv.org/abs/1501.02156
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Akademický článek
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