Zobrazeno 1 - 8
of 8
pro vyhledávání: '"Sobey, Charlotte"'
Autor:
Lower, Marcus E., Johnston, Simon, Dunn, Liam, Shannon, Ryan M., Bailes, Matthew, Dai, Shi, Kerr, Matthew, Manchester, Richard N., Melatos, Andrew, Oswald, Lucy S., Parthasarathy, Aditya, Sobey, Charlotte, Weltevrede, Patrick
We report on a timing programme of 74 young pulsars that have been observed by the Parkes 64-m radio telescope over the past decade. Using modern Bayesian timing techniques, we have measured the properties of 124 glitches in 52 of these pulsars, of w
Externí odkaz:
http://arxiv.org/abs/2109.07612
Autor:
Chernyakova, Maria, Malyshev, Denys, van Soelen, Brian, O'Sullivan, Shane, Sobey, Charlotte, Tsygankov, S., Keague, Samuel Mc., Green, Jacob, Kirwan, Matthew, Santangelo, Andrea, Pühlhofer, Gerd, Monageng, Itumeleng M.
PSR B1259-63 is a gamma-ray binary system hosting a radio pulsar orbiting around a O9.5Ve star, LS 2883, with a period of ~3.4 years. The interaction of the pulsar wind with the LS 2883 outflow leads to unpulsed broadband emission in the radio, X-ray
Externí odkaz:
http://arxiv.org/abs/2106.03759
Autor:
Hutschenreuter, Sebastian, Anderson, Craig S., Betti, Sarah, Bower, Geoffrey C., Brown, Jo-Anne, Brüggen, Marcus, Carretti, Ettore, Clarke, Tracy, Clegg, Andrew, Costa, Allison, Croft, Steve, Van Eck, Cameron, Gaensler, B. M., de Gasperin, Francesco, Haverkorn, Marijke, Heald, George, Hull, Charles L. H., Inoue, Makoto, Johnston-Hollitt, Melanie, Kaczmarek, Jane, Law, Casey, Ma, Yik Ki, MacMahon, David, Mao, Sui Ann, Riseley, Christopher, Roy, Subhashis, Shanahan, Russell, Shimwell, Timothy, Stil, Jeroen, Sobey, Charlotte, O'Sullivan, Shane, Tasse, Cyril, Vacca, Valentina, Vernstrom, Tessa, Williams, Peter K. G., Wright, Melvyn, Enßlin, Torsten A.
Publikováno v:
A&A 657, A43 (2022)
This work gives an update to existing reconstructions of the Galactic Faraday rotation sky by processing almost all Faraday rotation data sets available at the end of the year 2020. Observations of extra-Galactic sources in recent years have, among o
Externí odkaz:
http://arxiv.org/abs/2102.01709
Autor:
Heald, George, Mao, Sui Ann, Vacca, Valentina, Akahori, Takuya, Damas-Segovia, Ancor, Gaensler, B. M., Hoeft, Matthias, Agudo, Ivan, Basu, Aritra, Beck, Rainer, Birkinshaw, Mark, Bonafede, Annalisa, Bourke, Tyler L., Bracco, Andrea, Carretti, Ettore, Feretti, Luigina, Girart, J. M., Govoni, Federica, Green, James A., Han, JinLin, Haverkorn, Marijke, Horellou, Cathy, Johnston-Hollitt, Melanie, Kothes, Roland, Landecker, Tom, Nikiel-Wroczynski, Blazej, O'Sullivan, Shane P., Padovani, Marco, Poidevin, Frederick, Pratley, Luke, Regis, Marco, Riseley, Christopher John, Robishaw, Tim, Rudnick, Lawrence, Sobey, Charlotte, Stil, Jeroen M., Sun, Xiaohui, Sur, Sharanya, Taylor, A. Russ, Thomson, Alec, Van Eck, Cameron L., Vazza, Franco, West, Jennifer L., Group, the SKA Magnetism Science Working
The Square Kilometre Array (SKA) will answer fundamental questions about the origin, evolution, properties, and influence of magnetic fields throughout the Universe. Magnetic fields can illuminate and influence phenomena as diverse as star formation,
Externí odkaz:
http://arxiv.org/abs/2006.03172
Autor:
Smith, David A., Bruel, Philippe, Cognard, Ismaël, Cameron, Andrew D., Camilo, Fernando, Dai, Shi, Guillemot, Lucas, Johnson, Tyrel J., Johnston, Simon, Keith, Michael J., Kerr, Matthew, Kramer, Michael, Lyne, Andrew G., Manchester, Richard N., Shannon, Ryan, Sobey, Charlotte, Stappers, Benjamin W., Weltevrede, Patrick
Identifying as many gamma-ray pulsars as possible in the Fermi Large Area Telescope (LAT) data helps test pulsar emission models by comparing predicted and observed properties for a large, varied sample with as little selection bias as possible. It a
Externí odkaz:
http://arxiv.org/abs/1812.00719
Autor:
Geyer, Marisa, Karastergiou, Aris, Kondratiev, Vladislav I., Zagkouris, Kimon, Kramer, Michael, Stappers, Benjamin W., Grießmeier, Jean-Mathias, Hessels, Jason W. T., Michilli, Daniele, Pilia, Maura, Sobey, Charlotte
We measure the effects of interstellar scattering on average pulse profiles from 13 radio pulsars with simple pulse shapes. We use data from the LOFAR High Band Antennas, at frequencies between 110 and 190~MHz. We apply a forward fitting technique, a
Externí odkaz:
http://arxiv.org/abs/1706.04205
Akademický článek
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.
K zobrazení výsledku je třeba se přihlásit.
Autor:
SOBEY, CHARLOTTE
Publikováno v:
Australasian Science; May/Jun2018, Vol. 39 Issue 3, p14-16, 3p, 2 Color Photographs