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124por Clark, Colin J., Pletsch, Holger J., Wu, Jason, Guillemot, Lucas, Kerr, Matthew, Johnson, Tyrel J., Camilo, Fernando, Salvetti, David, Allen, Bruce, Anderson, David, Aulbert, Carsten, Beer, Christian, Bock, Oliver, Cuéllar, Andres, Eggenstein, Heinz-Bernd, Fehrmann, Henning, Kramer, Michael, Kwang, Shawn A., Machenschalk, Bernd, Nieder, Lars, Ackermann, Markus, Ajello, Marco, Baldini, Luca, Ballet, Jean, Barbiellini, Guido, Bastieri, Denis, Bellazzini, Ronaldo, Bissaldi, Elisabetta, Blandford, Roger D., Bloom, Elliott D., Bonino, Raffaella, Bottacini, Eugenio, Brandt, Terri J., Bregeon, Johan, Bruel, Philippe, Buehler, Rolf, Burnett, Toby H., Buson, Sara, Cameron, Rob A., Caputo, Regina, Caraveo, Patrizia A., Cavazzuti, Elisabetta, Cecchi, Claudia, Charles, Eric, Chekhtman, Alexandre, Ciprini, Stefano, Cominsky, Lynn R., Costantin, Denise, Cutini, Sara, D’Ammando, Filippo, De Luca, Andrea, Desiante, Rachele, Di Venere, Leonardo, Di Mauro, Mattia, Di Lalla, Niccolò, Digel, Seth W., Favuzzi, Cecilia, Ferrara, Elizabeth C., Franckowiak, Anna, Fukazawa, Yasushi, Funk, Stefan, Fusco, Piergiorgio, Gargano, Fabio, Gasparrini, Dario, Giglietto, Nico, Giordano, Francesco, Giroletti, Marcello, Gomez-Vargas, Germán A., Green, David, Grenier, Isabelle A., Guiriec, Sylvain, Harding, Alice K., Hewitt, John W., Horan, Deirdre, Jóhannesson, Guðlaugur, Kensei, Shiki, Kuss, Michael, La Mura, Giovanni, Larsson, Stefan, Latronico, Luca, Li, Jian, Longo, Francesco, Loparco, Francesco, Lovellette, Michael N., Lubrano, Pasquale, Magill, Jeffrey D., Maldera, Simone, Manfreda, Alberto, Mazziotta, Mario N., McEnery, Julie E., Michelson, Peter F., Mirabal, Nestor, Mitthumsiri, Warit, Mizuno, Tsunefumi, Monzani, Maria Elena, Morselli, Aldo, Moskalenko, Igor V., Nuss, Eric, Ohsugi, Takashi, Omodei, Nicola, Orienti, Monica, Orlando, Elena, Palatiello, Michele, Paliya, Vaidehi S., de Palma, Francesco, Paneque, David, Perkins, Jeremy S., Persic, Massimo, Pesce-Rollins, Melissa, Porter, Troy A., Principe, Giacomo, Rainò, Silvia, Rando, Riccardo, Ray, Paul S., Razzano, Massimiliano, Reimer, Anita, Reimer, Olaf, Romani, Roger W., Saz Parkinson, Pablo M., Sgrò, Carmelo, Siskind, Eric J., Smith, David A., Spada, Francesca, Spandre, Gloria, Spinelli, Paolo, Thayer, Jana B., Thompson, David J., Torres, Diego F., Troja, Eleonora, Vianello, Giacomo, Wood, Kent, Wood, Matthew“…Millisecond pulsars (MSPs) are old neutron stars that spin hundreds of times per second and appear to pulsate as their emission beams cross our line of sight. …”
Publicado 2018
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125“…Against the background of a pulsar-based positioning approach, a geometric trick is applied to determine the position of satellites. …”
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130“…This review is focused on tests of Einstein’s theory of general relativity with gravitational waves that are detectable by ground-based interferometers and pulsar-timing experiments. Einstein’s theory has been greatly constrained in the quasi-linear, quasi-stationary regime, where gravity is weak and velocities are small. …”
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131por Middleton, Hannah, Chen, Siyuan, Del Pozzo, Walter, Sesana, Alberto, Vecchio, Alberto“…Pulsar timing arrays are presently the only means to search for the gravitational wave stochastic background from super massive black hole binary populations, considered to be within the grasp of current or near-future observations. …”
Publicado 2018
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132por Xue, Mengfan, Shi, Yifang, Guo, Yunfei, Huang, Na, Peng, Dongliang, Luo, Ji’an, Shentu, Han, Chen, Zhikun“…The accuracy of X-ray pulsar-based navigation is greatly affected by the Doppler effect caused by the spacecraft orbital motion and the systematic biases introduced by the pulsar directional error, spacecraft-borne clock error, etc. …”
Publicado 2019
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134“…A custom full mesh enabled ATCA board called the Pulsar II has been designed with the goal of creating a scalable architecture abundant in flexible, non-blocking, high bandwidth board- to-board communication channels while keeping the design as simple as possible.…”
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135“…The NANOGrav, Parkes, European, and International Pulsar Timing Array (PTA) Collaborations have reported evidence for a common-spectrum process that can potentially correspond to a stochastic gravitational wave background (SGWB) in the 1–100 nHz frequency range. …”
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136por Antoniadis, J., Arzoumanian, Z., Babak, S., Bailes, M., Nielsen, A.-S. Bak, Baker, P.T., Bassa, C.G., Becsy, B., Berthereau, A., Bonetti, M., Brazier, A., Brook, P.R., Burgay, M., Burke-Spolaor, S., Caballero, R.N., Casey-Clyde, J.A., Chalumeau, A., Champion, D.J., Charisi, M., Chatterjee, S., Chen, S., Cognard, I., Cordes, J.M., Cornish, N.J., Crawford, F., Cromartie, H.T., Crowter, K., Dai, S., DeCesar, M.E., Demorest, P.B., Desvignes, G., Dolch, T., Drachler, B., Falxa, M., Ferrara, E.C., Fiore, W., Fonseca, E., Gair, J.R., Garver-Daniels, N., Goncharov, B., Good, D.C., Graikou, E., Guillemot, L., Guo, Y.J., Hazboun, J.S., Hobbs, G., Hu, H., Islo, K., Janssen, G.H., Jennings, R.J., Johnson, A.D., Jones, M.L., Kaiser, A.R., Kaplan, D.L., Karuppusamy, R., Keith, M.J., Kelley, L.Z., Kerr, M., Key, J.S., Kramer, M., Lam, M.T., Lamb, W.G., Lazio, T.J.W., Lee, K.J., Lentati, L., Liu, K., Luo, J., Lynch, R.S., Lyne, A.G., Madison, D.R., Main, R.A., Manchester, R.N., McEwen, A., McKee, J.W., McLaughlin, M.A., Mickaliger, M.B., Mingarelli, C.M.F., Ng, C., Nice, D.J., Oslowski, S., Parthasarathy, A., Pennucci, T.T., Perera, B.B.P., Perrodin, D., Petiteau, A., Pol, N.S., Porayko, N.K., Possenti, A., Ransom, S.M., Ray, P.S., Reardon, D.J., Russell, C.J., Samajdar, A., Sampson, L.M., Sanidas, S., Sarkissian, J.M., Schmitz, K., Schult, L., Sesana, A., Shaifullah, G., Shannon, R.M., Shapiro-Albert, B.J., Siemens, X., Simon, J., Smith, T.L., Speri, L., Spiewak, R., Stairs, I.H., Stappers, B.W., Stinebring, D.R., Swiggum, J.K., Taylor, S.R., Theureau, G., Tiburzi, C., Vallisneri, M., van der Wateren, E., Vecchio, A., Verbiest, J.P.W., Vigeland, S.J., Wahl, H., Wang, J.B., Wang, J., Wang, L., Witt, C.A., Zhang, S., Zhu, X.J.“…We searched for an isotropic stochastic gravitational wave background in the second data release of the International Pulsar Timing Array, a global collaboration synthesizing decadal-length pulsar-timing campaigns in North America, Europe, and Australia. …”
Publicado 2022
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137“…Recent measurements of the spin-down rates of soft gamma ray repeaters (SGRs) and anomalous X-ray pulsars (AXPs) have been interpreted as evidence that these objects are ``magnetars'': neutron stars spinning down by magnetic dipole radiation, but with a magnetic field two orders of magnitude larger than that of ordinary neutron stars. …”
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138por Ajuha, S, Cascadan, Andre, Costa de Paiva, Thiago, Das, Souvik, Eusebi, Ricardo, Finotti Ferreira, Vitor, Hahn, Kristian, Hu, Zhen, Jindariani, Sergo, Konigsberg, Jacobo, Liu, Tiehui Ted, Low, Jia Fu, Okumura, Yasuyuki, Olsen, Jamieson, Arruda Ramalho, Lucas, Rossin, Roberto, Ristori, Luciano, Akira Shinoda, Ailton, Tran, Nhan, Trovato, Marco, Ulmer, Keith, Vaz, Mario, Wen, Xianshan, Wu, Jin-Yuan, Xu, Zijun, Yin, Han, Zorzetti, Silvia“…The Pulsar II is a custom ATCA full mesh enabled FPGA-based processor board which has been designed with the goal of creating a scalable architecture abundant in flexible, non-blocking, high bandwidth interconnections. …”
Publicado 2017
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139por Clark, C. J., Kerr, M., Barr, E. D., Bhattacharyya, B., Breton, R. P., Bruel, P., Camilo, F., Chen, W., Cognard, I., Cromartie, H. T., Deneva, J., Dhillon, V. S., Guillemot, L., Kennedy, M. R., Kramer, M., Lyne, A. G., Sánchez, D. Mata, Nieder, L., Phillips, C., Ransom, S. M., Ray, P. S., Roberts, M. S. E., Roy, J., Smith, D. A., Spiewak, R., Stappers, B. W., Tabassum, S., Theureau, G., Voisin, G.“…Black widows and redbacks are compact binaries consisting of millisecond pulsars and semi-degenerate companion stars. Spectroscopy of the optically bright companions can determine their radial velocities, providing inclination-dependent pulsar mass estimates. …”
Publicado 2023
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140por Lichtenberg, Michael, Hailer, Birgit, Kaeunicke, Matthias, Stahlhoff, Wilhelm-Friedrich, Boese, Dirk, Breuckmann, Frank“…PURPOSE: To evaluate the patency and the freedom of target lesion revascularization of the 4-French Pulsar-18 self-expandable (SE) nitinol stent for the treatment of long femoropopliteal occlusive disease in a two-center, prospective, all-comers registry with a follow-up period of 12 months. …”
Publicado 2015
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