Results 11 to 20 of about 800,901 (220)
The LOFAR pilot surveys for pulsars and fast radio transients [PDF]
, 2014 We have conducted two pilot surveys for radio pulsars and fasttransients with the Low-Frequency Array (LOFAR) around 140 MHz and herereport on the first low-frequency fast-radio burst limit and thediscovery of two new pulsars. The first survey, the LOFAR Röttgering, H., Wucknitz, O, Weltevrede, Patrick, McFadden, R., M. Brüggen, Wijnholds, S., van Amesfoort, A. S., Hassall, T., Brüggen, M, Kuniyoshi, M, Orru, E, Karastergiou, A., Corstanje, A., Garrett, M., Hessels, Jason W T, McKay-Bukowski, D., Thoudam, S, Tasse, C, Hassall, T E, Sluman, J, Zensus, A, Kramer, M, van Weeren, R., C. Sobey, Zagkouris, K, Broderick, J, Kuper, G, Brüggen, M., Bilous, A, Rowlinson, A, Pilia, M., Sobey, Charlotte, van der Horst, A., T. E. Hassall, Fender, R, Hessels, Jason W. T., Ciardi, B., Noutsos, A, Falcke, H, Jason W. T. Hessels, Vladislav I. Kondratiev, M. J. Bentum, Röttgering, H, Anderson, J., Gajjar, V., M. E. Bell, Noutsos, A., Schwarz, D, S. Cooper, Stappers, B.W., Griessmeier, J-M., Paas, H., Butcher, H., E. Juette, Sobey, C., van Weeren, R. J., Karastergiou, A, Verbiest, J, A. van der Horst, Bell, M. E., Hoeft, M., R. P. Breton, Verbiest, J., Mann, G., Keane, E., Renting, A., J. Broderick, Hamaker, J., Kuper, G., H. Röttgering, G. Mann, Hassall, T.E., Hassall, T. E., K. Zagkouris, Garrett, Michael; id_orcid, Toribio, C, Grießmeier, J., Tagger, M., Thoudam, S., Grießmeier, J.-M., Cooper, S., Osłowski, S., I. M. Avruch, W. Reich, Polatidis, A G, Eislöffel, J., R. McFadden, Juette, E., Munk, H, Griessmeier, J.M., A. Bilous, C. Schrijvers, Kondratiev, Vladislav I., A. M. M. Scaife, Veen, S., Garrett, M. A., Amesfoort, A., Schrijvers, C., Thijs Coenen, Bell, M E, Deller, A., Fallows, R A, R. Fender, Zarka, P., Schwarz, Dominik ; https://orcid.org/, Bonafede, A, Kondratiev, V., Pilia, M, Sobey, C, Heald, G., Tagger, Michel, Garrett, M.A., P. Zarka, Smirnov, O., Keane, E. F., van Weeren, R J, Bell, M., Breton, Rene P; id_orcid, Oslowski, S., J. Anderson, C. Ferrari, et al., C. Law, J.-M. Grießmeier, Alexov, A, Scaife, A M M; id_orcid, Serylak, M, E. Orru, McKean, J P, Thoudam, Satyendra,, O. Smirnov, Breitling, F., Hamaker, J P, M. Hoeft, Coenen, Thijs, Butcher, H. R., Avruch, I., G. Bernardi, A. Corstanje, Hessels, J., Kramer, M., R. J. van Weeren, Scaife, A., S. Duscha, Gunst, A. W., Best, P, Corstanje, A, van Amesfoort, A S, Zagkouris, K., Bernardi, G., S. Osłowski, Broderick, J., de Geus, E., McKean, J., McKean, J. P., C. Tasse, Swinbank, J., et al, Vocks, C., A. W. Gunst, Vocks, C, Oslowski, Stefan, Schwarz, D., Bernardi, G, A. Karastergiou, Breitling, F, Breton, R.P., D. McKay-Bukowski, Gasperin, F., Tasse, C., Stappers, Benjamin W; id_orcid, A. G. Polatidis, Cooper, S, ter Veen, S, Gunst, A., F. Breitling, et al., [Unknown], A. Noutsos, Deller, A, Sluman, J., Joeri van Leeuwen, Brueggen, M., Veen, S. ter, V. Gajjar, M. Serylak, Gajjar, V, R. Vermeulen, Kuniyoshi, M., E. F. Keane, M. Kramer, M. Pilia, Gunst, A W, van der Horst, A, Y. Tang, Asgekar, A., Fallows, R., Bilous, A., Scaife, A. M. M., Juette, E, Stappers, Ben W., Bentum, M J, Hoeft, M, Ferrari, C., J. P. Hamaker, Ben W. Stappers, Keane, E F, Geus, E., Toribio, C., Coenen, T., Kondratiev, Vladislav I, M. A. Garrett, Eisloeffel, J., McKay-Bukowski, D, Kondratiev, V.I., Wijnholds, S, Stappers, B., G. Heald, Horst, A., Asgekar, A, P. Best, H. Munk, Mann, G, Coenen, T.J., B. Ciardi, Bentum, M. J., J. P. McKean, Zensus, A., S. Thoudam, Ciardi, B, Hessels, J. W. T., Anderson, J, Bentum, Marinus Jan, Verbiest, Joris ; https://orcid.org/, A. Rowlinson, ter Veen, S., M. Pandey-Pommier, Paas, H, Kondratiev, V. I., Polatidis, A. G., Hessels, J.W.T., G. Kuper, Eislöffel, J, Falcke, H., Leeuwen, J., Bentum, M., Rowlinson, A., S. Wijnholds, Pandey-Pommier, M, Polatidis, A., Tagger, M, Orru, E., Serylak, M., Smirnov, O, A. Zensus, Röttgering, H.J.A., Stappers, B. W., H. Falcke, W. Frieswijk, A. Renting, Hamaker, J. P., C. Vocks, Heald, G, A. Deller, M. Tagger, Bonafede, A., Schrijvers, C, J. Swinbank, Fender, R., S. ter Veen, D. Schwarz, E. de Geus, Law, C, R. A. Fallows, O. Wucknitz, A. Alexov, de Geus, E, F. de Gasperin, J. Eislöffel, A. Asgekar, Law, C., Renting, A, Fallows, R. A., Best, P., Frieswijk, W., Van Amesfoort, A., Ferrari, C, Wucknitz, O., Osłowski, S, J. Verbiest, de Gasperin, F, H. R. Butcher, Frieswijk, W, Tang, Y, Breton, R., Swinbank, J, P. Weltevrede, H. Paas, Vermeulen, R., Butcher, H R, de Gasperin, F., Os\lowski, S., van Leeuwen, Joeri, Weltevrede, P., Alexov, A., Zarka, P, Grießmeier, J. -M., Breton, R. P., Reich, W., Grießmeier, J. -M, McFadden, R, J. Sluman, Avruch, I. M., Reich, W, A. S. van Amesfoort, Avruch, I M, Pandey-Pommier, M., Fallows, R.A., Duscha, S., C. Toribio, M. Kuniyoshi, Tang, Y., Duscha, S, A. Bonafede, Munk, H., Vermeulen, R, Grießmeier, J-M, Griessmeier, Jean-Mathias, Van Leeuwen, J. +327 morecore +3 more sourcesInvestigation of Emission States of PSR J1722–3207
The Astrophysical Journal, 2023 We have conducted a detailed study of single-pulse emission from PSR J1722−3207, which was observed at 1369 MHz using the Parkes 64 m radio telescope. PSR J1722−3207 has an asymmetric two-component mean pulse profile.D. Zhao, W. M. Yan, N. Wang, J. P. Yuandoaj +1 more sourceGravitoastronomy with neutron stars [PDF]
, 2004 Recent advances in gravitational wave detectors mean that we can start to make astrophysically important
statements about the physics of neutron stars based on observed upper limits to their gravitational luminosity.Woan, G., Graham Woancore +1 more sourceThe origin of single radio pulsars [PDF]
, 1999 By comparing relative rates of supernovae versus formation rates of single radio pulsars, recycled pulsars, binary pulsars and X-ray binaries we put strong limits on the progenitors of radio pulsars and on the requirement of an asymmetry in the supernova.Edward P.J. Van den Heuvel, Simon F. Portegies Zwart, Portegies Zwart, S.F., Van den Heuvel, E.P.J. +3 morecore +1 more sourceRecycled Pulsars [PDF]
, 2005 We present the results of a large-area survey for millisecond pulsars (MSPs) at moderately high galactic latitudes with the 64 m Parkes radio telescope, along with follow-up timing and optical studies of the newly-discovered pulsars and several others ...Jacoby, Bryan Anthonycore +1 more sourceThe 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 sourceA relativistic navigation system for space [PDF]
, 2011 We present here a method for the relativistic positioning in spacetime based on the reception of pulses from sources of electromagnetic signals whose worldline is known.Capolongo, Emiliano, Tartaglia, Angelo, Moraud, E. M., Chicca, Elisabetta, Ruggiero, Matteo Luca, Chicca, Elisabetta ; https://orcid.org/, Moraud, Eduardo M +6 morecore +1 more source
