Zobrazeno 1 - 10
of 16
pro vyhledávání: '"G. H. Heald"'
Autor:
S. Vanderwoude, J. L. West, B. M. Gaensler, L. Rudnick, C. L. Van Eck, A. J. M. Thomson, H. Andernach, C. S. Anderson, E. Carretti, G. H. Heald, J. P. Leahy, N. M. McClure-Griffiths, S. P. O’Sullivan, M. Tahani, A. G. Willis
Publikováno v:
The Astronomical Journal, Vol 167, Iss 5, p 226 (2024)
The Polarisation Sky Survey of the Universe’s Magnetism (POSSUM) will conduct a sensitive ∼1 GHz radio polarization survey covering 20,000 deg ^2 of the southern sky with the Australian Square Kilometre Array Pathfinder. In anticipation of the fu
Externí odkaz:
https://doaj.org/article/d2e4de9e984646d9b93b25fd21d34f35
Autor:
V P Pomakov, S P O’Sullivan, M Brüggen, F Vazza, E Carretti, G H Heald, C Horellou, T Shimwell, A Shulevski, T Vernstrom
Publikováno v:
Monthly Notices of the Royal Astronomical Society, 515(1), 256-270
Faraday rotation studies of distant radio sources can constrain the evolution and the origin of cosmic magnetism. We use data from the LOFAR Two Metre Sky Survey: Data Release 2 (LoTSS DR2) to study the dependence of the Faraday rotation measure (RM)
Autor:
Ettore Carretti, V Vacca, S P O’Sullivan, G H Heald, C Horellou, H J A Röttgering, A M M Scaife, T W Shimwell, A Shulevski, C Stuardi, T Vernstrom
Publikováno v:
Monthly Notices of the Royal Astronomical Society, 512(1), 945-959
We used the Rotation Measure (RM) catalogue derived from the LOFAR Two-metre Sky Survey Data Release 2 (LoTSS DR2) at 144-MHz to measure the evolution with redshift of the extragalactic RM (RRM: Residual RM) and the polarization fraction ($p$) of sou
Autor:
N. Hurley-Walker, X. Zhang, A. Bahramian, S. J. McSweeney, T. N. O’Doherty, P. J. Hancock, J. S. Morgan, G. E. Anderson, G. H. Heald, T. J. Galvin
Publikováno v:
Nature. 601:526-530
Autor:
V. Heesen, S. P. O’Sullivan, M. Brüggen, A. Basu, R. Beck, A. Seta, E. Carretti, M. G. H. Krause, M. Haverkorn, S. Hutschenreuter, A. Bracco, M. Stein, D. J. Bomans, R.-J. Dettmar, K. T. Chyży, G. H. Heald, R. Paladino, C. Horellou
Publikováno v:
Astronomy & Astrophysics, 670, pp. 1-5
Astronomy & Astrophysics, 670, 1-5
Astronomy & Astrophysics, 670, 1-5
Context. The existence of magnetic fields in the circumgalactic medium (CGM) is largely unconstrained. Their detection is important as magnetic fields can have a significant impact on the evolution of the CGM and, in turn, the fields can serve as tra
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::0fe40abcc103b3cabb857ac9bf79dd0c
https://repository.ubn.ru.nl/handle/2066/290178
https://repository.ubn.ru.nl/handle/2066/290178
Autor:
V. Heesen, M. Staffehl, A. Basu, R. Beck, M. Stein, F. S. Tabatabaei, M. J. Hardcastle, K. T. Chyży, T. W. Shimwell, B. Adebahr, R. Beswick, D. J. Bomans, A. Botteon, E. Brinks, M. Brüggen, R.-J. Dettmar, A. Drabent, F. de Gasperin, G. Gürkan, G. H. Heald, C. Horellou, B. Nikiel-Wroczynski, R. Paladino, J. Piotrowska, H. J. A. Röttgering, D. J. B. Smith, C. Tasse
Publikováno v:
Astronomy & Astrophysics, 664:A83
Context. Cosmic rays and magnetic fields are key ingredients in galaxy evolution, regulating both stellar feedback and star formation. Their properties can be studied with low-frequency radio continuum observations that are free from thermal contamin
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::adac660be5e6e3be2e4e81f317e0960f
https://ui.adsabs.harvard.edu/abs/2022A&A...664A..83H
https://ui.adsabs.harvard.edu/abs/2022A&A...664A..83H
Autor:
J. W. Broderick, G. Drouart, N. Seymour, T. J. Galvin, N. Wright, A. Carnero Rosell, R. Chhetri, H. Dannerbauer, S. P. Driver, J. S. Morgan, V. A. Moss, S. Prabu, J. M. Afonso, C. De Breuck, B. H. C. Emonts, T. M. O. Franzen, C. M. Gutiérrez, P. J. Hancock, G. H. Heald, N. Hurley-Walker, R. J. Ivison, M. D. Lehnert, G. Noirot, M. Read, S. S. Shabala, D. Stern, W. J. Sutherland, E. Sutorius, R. J. Turner, J. Vernet
Publikováno v:
Publications of the Astronomical Society of Australia. 39
While unobscured and radio-quiet active galactic nuclei are regularly being found at redshifts $z > 6$, their obscured and radio-loud counterparts remain elusive. We build upon our successful pilot study, presenting a new sample of low-frequency-sele
Autor:
N, Hurley-Walker, X, Zhang, A, Bahramian, S J, McSweeney, T N, O'Doherty, P J, Hancock, J S, Morgan, G E, Anderson, G H, Heald, T J, Galvin
Publikováno v:
Nature. 601(7894)
The high-frequency radio sky is bursting with synchrotron transients from massive stellar explosions and accretion events, but the low-frequency radio sky has, so far, been quiet beyond the Galactic pulsar population and the long-term scintillation o
Autor:
Catherine L. Hale, D. McConnell, A. J. M. Thomson, E. Lenc, G. H. Heald, A. W. Hotan, J. K. Leung, V. A. Moss, T. Murphy, J. Pritchard, E. M. Sadler, A. J. Stewart, M. T. Whiting
The Rapid ASKAP Continuum Survey (RACS) is the first large sky survey using the Australian Square Kilometre Array Pathfinder (ASKAP), covering the sky south of +41$^\circ$ declination. With ASKAP's large, instantaneous field of view, $\sim 31$ deg$^2
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::14135f9e6aed068282ab9f318aaa1bc6
Autor:
V. Heesen, L. Whitler, P. Schmidt, A. Miskolczi, S. S. Sridhar, C. Horellou, R. Beck, G. Gürkan, E. Scannapieco, M. Brüggen, G. H. Heald, M. Krause, R. Paladino, B. Nikiel-Wroczyński, A. Wilber, R.-J. Dettmar
Publikováno v:
Astronomy and astrophysics, 628:L3. EDP Sciences
Cosmic rays play a pivotal role in launching galactic winds, particularly in quiescently star-forming galaxies where the hot gas alone is not sufficient to drive a wind. Except for the Milky Way, not much is known about the transport of cosmic rays i
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::7883c71d877830f6837eef24f449bb7c
https://ruj.uj.edu.pl/xmlui/handle/item/82853
https://ruj.uj.edu.pl/xmlui/handle/item/82853