Results 71 to 80 of about 178,608 (254)
The specifics of pulsar radio emission
Open Astronomy, 2022 A characteristic property of pulsars is pulsed periodic radio emission, which has a high stability of periods. Despite the high stability of the emission periods of pulsars, monitoring the time of arrival of pulses (timing) shows the presence of ...Losovsky Boris Ya.doaj +1 more sourceSelection of radio pulsar candidates using artificial neural networks
, 2010 Radio pulsar surveys are producing many more pulsar candidates than can be
inspected by human experts in a practical length of time. Here we present a
technique to automatically identify credible pulsar candidates from pulsar
surveys using an artificial ...A. G. Lyne, A. Noutsos, B. W. Stappers, Belokurov, Bishop, Cordes, Eatough, Faulkner, Firth, Hewish, Jenet, Keith, Kohonen, Lintott, Lorimer, M. J. Keith, M. Kramer, Manchester, N. Molkenthin, R. P. Eatough, Smits, Smits, Storrie-Lombardi, Van Leeuwen, Zhang +24 morecore +1 more sourceDiscovery of an optical bow-shock around pulsar B0740-28 [PDF]
, 2002 We report the discovery of a faint H-alpha pulsar wind nebula (PWN) powered
by the radio pulsar B0740-28. The characteristic bow-shock morphology of the
PWN implies a direction of motion consistent with the previously measured
velocity vector for the ...Aldcroft, Arzoumanian, B. M. Gaensler, B. W. Stappers, Bailes, Bell, Bland-Hawthorn, Blandford, Bucciantini, Chen, Cordes, D. H. Jones, Dopita, Fomalont, Gaensler, Hester, Koribalski, Kulkarni, McCulloch, Neckel, Stone, Taylor, Wilkin, Wilkin +23 morecore +2 more sourcesThe first pulsar discovered by FAST [PDF]
Science China Physics Mechanics and Astronomy, 2019 To assist with the commissioning (Jiang et al. 2019) of the Five-hundred-meter Aperture Spherical radio Telescope (FAST), we performed a pulsar search, with the primary goal of developing and testing the pulsar data acquisition and processing pipelines ...L. Qian, Z. Pan, Di Li, G. Hobbs, Weiwei Zhu, Pei Wang, Zhijie Liu, Y. Yue, Yan Zhu, Hongfei Liu, Dongjun Yu, Jinghai Sun, P. Jiang, Gaofeng Pan, Hui Li, H. Gan, R. Yao, Xiaoyao Xie, F. Camilo, A. Cameron, Lei Zhang, Shen Wang, Fast collaboration +22 moresemanticscholar +1 more sourcePulsar’s Application in Energy Systems: Review of Current Status, Challenges, and Opportunities
EnergiesTo accelerate progress toward the realization of advanced energy systems, this review explores the potential of pulsar technology to create a more stable, economical, and environmentally friendly energy infrastructure.Yongxin Zhang, Yuru Wu, Yu Liu, Biao Sun, Jiahui Yang, Naga Lakshmi Thotakura, Kazi Ishrak Ahmed, Qian Liu, Chong Shen, Yilu Liu +9 moredoaj +1 more sourceQuark Deconfinement in Rotating Neutron Stars
Universe, 2017 In this paper, we use a three flavor non-local Nambu–Jona-Lasinio (NJL) model, an improved effective model of Quantum Chromodynamics (QCD) at low energies, to investigate the existence of deconfined quarks in the cores of neutron stars.Richard D. Mellinger, Fridolin Weber, William Spinella, Gustavo A. Contrera, Milva G. Orsaria +4 moredoaj +1 more sourceComparing Recent Pulsar Timing Array Results on the Nanohertz Stochastic Gravitational-wave Background
Astrophysical JournalThe Australian, Chinese, European, Indian, and North American pulsar timing array (PTA) collaborations recently reported, at varying levels, evidence for the presence of a nanohertz gravitational-wave background (GWB).G. Agazie, J. Antoniadis, A. Anumarlapudi, A. M. Archibald, P. Arumugam, S. Arumugam, Z. Arzoumanian, J. Askew, S. Babak, M. Bagchi, M. Bailes, A. B. Nielsen, P. Baker, C. Bassa, A. Bathula, B. Bécsy, A. Berthereau, N. Bhat, L. Blecha, M. Bonetti, E. Bortolas, A. Brazier, P. R. Brook, M. Burgay, S. Burke-Spolaor, R. Burnette, R. N. Caballero, A. Cameron, R. Case, A. Chalumeau, D. Champion, S. Chanlaridis, M. Charisi, S. Chatterjee, K. Chatziioannou, B. Cheeseboro, S. Chen, Z.-C. Chen, I. Cognard, T. Cohen, W. A. Coles, J. Cordes, N. Cornish, F. Crawford, H. Cromartie, K. Crowter, M. Curyło, C. Cutler, S. Dai, S. Dandapat, D. Deb, M. DeCesar, D. DeGan, P. Demorest, H. Deng, S. Desai, G. Desvignes, L. Dey, N. Dhanda-Batra, V. Di Marco, T. Dolch, B. Drachler, C. Dwivedi, J. Ellis, M. Falxa, Y. Feng, R. Ferdman, E. Ferrara, W. Fiore, E. Fonseca, A. Franchini, G. Freedman, J. Gair, N. Garver-Daniels, P. Gentile, K. Gersbach, J. Glaser, D. Good, B. Goncharov, A. Gopakumar, E. Graikou, J. Grießmeier, L. Guillemot, K. Gültekin, Y. J. Guo, Y. Gupta, K. Grunthal, J. Hazboun, S. Hisano, G. Hobbs, S. Hourihane, H. Hu, F. Iraci, K. Islo, D. Izquierdo-Villalba, J. Jang, J. Jawor, G. Janssen, R. Jennings, A. Jessner, A. D. Johnson, M. Jones, B. C. Joshi, A. Kaiser, D. Kaplan, A. Kapur, Fazal Kareem, R. Karuppusamy, E. Keane, M. Keith, L. Kelley, M. Kerr, J. Key, D. Kharbanda, T. Kikunaga, T. C. Klein, N. Kolhe, M. Kramer, M. A. Krishnakumar, A. Kulkarni, N. Laal, K. Lackeos, M. Lam, W. Lamb, B. Larsen, T. Lazio, K. J. Lee, Y. Levin, N. Lewandowska, T. Littenberg, K. Liu, T. Liu, Y. Liu, A. Lommen, D. R. Lorimer, M. Lower, J. Luo, R. Luo, R. Lynch, A. Lyne, C.-P. Ma, Y. Maan, D. Madison, R. Main, R. Manchester, R. Mandow, M. A. Mattson, A. McEwen, J. Mckee, M. McLaughlin, N. McMann, B. W. Meyers, P. Meyers, M. Mickaliger, M. Miles, C. Mingarelli, A. Mitridate, P. Natarajan, R. Nathan, C. Ng, D. Nice, I. C. Niţu, K. Nobleson, S. Ocker, K. Olum, S. Osłowski, A. K. Paladi, A. Parthasarathy, T. Pennucci, B. Perera, D. Perrodin, A. Petiteau, P. Petrov, N. Pol, N. Porayko, A. Possenti, T. Prabu, H. Q. Leclere, H. Radovan, P. Rana, S. Ransom, P. Ray, D. Reardon, A. F. Rogers, J. Romano, C. Russell, A. Samajdar, S. Sanidas, S. Sardesai, A. Schmiedekamp, C. Schmiedekamp, K. Schmitz, L. Schult, A. Sesana, G. Shaifullah, R. Shannon, B. Shapiro-Albert, X. Siemens, J. Simon, J. Singha, M. Siwek, L. Speri, R. Spiewak, A. Srivastava, I. Stairs, B. Stappers, D. Stinebring, K. Stovall, J. P. Sun, M. Surnis, S. Susarla, A. Susobhanan, J. Swiggum, K. Takahashi, P. Tarafdar, J. Taylor, S. Taylor, G. Theureau, E. Thrane, N. Thyagarajan, C. Tiburzi, L. Toomey, J. Turner, C. Unal, M. Vallisneri, E. van der Wateren, R. van Haasteren, A. Vecchio, V. Venkatraman Krishnan, J. Verbiest, S. Vigeland, H. Wahl, S. Wang, Q. Wang, C. Witt, J. Wang, L. Wang, K. Wayt, Z. Wu, O. Young, L. Zhang, S. Zhang, X.-J. Zhu, A. Zic +243 moresemanticscholar +1 more sourceLOFAR Discovery of a 23.5 s Radio Pulsar [PDF]
Astrophysical Journal, 2018 We present the discovery of PSR J0250+5854, a radio pulsar with a spin period of 23.5 s. This is the slowest-spinning radio pulsar known. PSR J0250+5854 was discovered by the LOFAR Tied-Array All-Sky Survey (LOTAAS), an all-northern-sky survey for ...C. Tan, C. Bassa, S. Cooper, T. J. Dijkema, P. Esposito, J. Hessels, V. Kondratiev, M. Kramer, D. Michilli, S. Sanidas, T. Shimwell, B. Stappers, J. V. Leeuwen, I. Cognard, J. Grießmeier, A. Karastergiou, E. Keane, C. Sobey, P. W. J. B. C. F. Astrophysics, S. O. Physics, Astronomy, U. Manchester, Manchester, Uk, Astron, The Netherlands Institute for Radio Astronomy, The Netherlands., A. S. M. F. Astronomy, U. Amsterdam, Amsterdam, I. D. F. Cosmica, Milano, Italy, A. Centre, L. Institute, R. A. O. Sciences, Moscow, Russia., Max Planck Institut fur Radioastronomie, Germany, Laboratoire de Physique et Chimie de l'Environnement et de l'Espace, Universit'e d'Orl'eansCNRS, France, Station de radioastronomie de Nanccay, O. Paris, Cnrsinsu, O. Astrophysics, Denys Wilkinson Building, Keble Road, Oxford, Department of Applied Physics, U. W. Cape, S. Africa, Electronics, Rhodes University, Ska Organisation, Jodrell Bank Observatory, I. C. F. R. A. R. -. C. University, Australia., C. Astronomy, S. Science +60 moresemanticscholar +1 more source