Zobrazeno 1 - 10
of 10
pro vyhledávání: '"R. L. Tunnicliffe"'
Autor:
R. L. Tunnicliffe, A. L. Ganesan, R. J. Parker, H. Boesch, N. Gedney, B. Poulter, Z. Zhang, J. V. Lavrič, D. Walter, M. Rigby, S. Henne, D. Young, S. O'Doherty
Publikováno v:
Atmospheric Chemistry and Physics, Vol 20, Pp 13041-13067 (2020)
Brazil's CH4 emissions over the period 2010–2018 were derived for the three main sectors of activity: anthropogenic, wetland and biomass burning. Our inverse modelling estimates were derived from GOSAT (Greenhouse gases Observing SATellite) satelli
Externí odkaz:
https://doaj.org/article/0e538465bcc44f2b966df0158f106e82
Autor:
David N. Burrows, N. Lyons, Antonino Cucchiara, Antonia Rowlinson, P. T. O'Brien, R. L. Tunnicliffe, Jens Hjorth, Richard Willingale, K. L. Page, A. S. Fruchter, Andrew J. Levan, Phil Evans, O. Onal, A. P. Beardmore, Nial R. Tanvir, T. N. Ukwatta, Derek B. Fox, Edo Berger, Bing Zhang
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 409:531-540
The majority of short gamma-ray bursts (SGRBs) are thought to originate from the merger of compact binary systems collapsing directly to form a black hole. However, it has been proposed that both SGRBs and long gamma-ray bursts (LGRBs) may, on rare o
Autor:
Joao Bento, J. W. Rostron, Elmé Breedt, Steven G. Parsons, Madelon C. P. Bours, C. D. J. Savoury, S. P. Littlefair, V. S. Dhillon, T. R. Marsh, R. L. Tunnicliffe, P. Kerry, Isabelle Baraffe, D. I. Sahman, Chris M. Copperwheat, M. J. McAllister, L. K. Hardy, J. Bochinski
We present high-speed, three-colour photometry of the eclipsing dwarf nova PHL 1445, which, with an orbital period of 76.3 min, lies just below the period minimum of ~82 min for cataclysmic variable stars. Averaging four eclipses reveals resolved ecl
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a4cc134f62f08635363fe8625d1920d7
http://wrap.warwick.ac.uk/83091/1/WRAP_MNRAS-2015-McAllister-114-25.pdf
http://wrap.warwick.ac.uk/83091/1/WRAP_MNRAS-2015-McAllister-114-25.pdf
Autor:
A. S. Fruchter, Andrew J. Levan, Rebekah Hounsell, Jens Hjorth, R. L. Tunnicliffe, K. Wiersema, Nial R. Tanvir
Publikováno v:
Nature. 500:547-549
Short-duration γ-ray bursts are intense flashes of cosmic γ-rays, lasting less than about two seconds, whose origin is unclear1, 2. The favoured hypothesis is that they are produced by a relativistic jet created by the merger of two compact stellar
Autor:
Andrew J. Levan, Pall Jakobsson, S. B. Cenko, D. Malesani, Ovidiu Vaduvescu, Ryan Chornock, R. Karjalainen, Stefano Covino, Daniel A. Perley, Darach Watson, I. Skillen, Graham A. Wynn, Ralph A. M. J. Wijers, J. P. Osborne, Christina C. Thöne, P. Goldoni, A. de Ugarte Postigo, B. A. Zauderer, Edo Berger, Elena Pian, T. Kruehler, D. Bersier, G. Tagliaferri, J. Gorosabel, Lex Kaper, Avishay Gal-Yam, Steve Schulze, A. Cucchiara, K. L. Page, G. C. Brown, A. S. Fruchter, Klaas Wiersema, R. L. Tunnicliffe, B. E. Cobb, R. Sanchez-Ramirez, R. L. C. Starling, Jens Hjorth, P. T. O'Brien, Brian P. Schmidt, Nial R. Tanvir, D. B. Fox
Publikováno v:
The Astrophysical Journal
The Astrophysical Journal, American Astronomical Society, 2014, 781 (1), pp.13. ⟨10.1088/0004-637X/781/1/13⟩
Artículos CONICYT
CONICYT Chile
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The Astrophysical Journal, 2014, 781 (1), pp.13. ⟨10.1088/0004-637X/781/1/13⟩
Astrophysical Journal, 781(1):13. IOP Publishing Ltd.
The Astrophysical Journal, American Astronomical Society, 2014, 781 (1), pp.13. ⟨10.1088/0004-637X/781/1/13⟩
Artículos CONICYT
CONICYT Chile
instacron:CONICYT
The Astrophysical Journal, 2014, 781 (1), pp.13. ⟨10.1088/0004-637X/781/1/13⟩
Astrophysical Journal, 781(1):13. IOP Publishing Ltd.
We present comprehensive multiwavelength observations of three gamma-ray bursts (GRBs) with durations of several thousand seconds. We demonstrate that these events are extragalactic transients; in particular we resolve the long-standing conundrum of
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a744689ec1325b8b8f888d83059f03c9
https://resolver.caltech.edu/CaltechAUTHORS:20140211-130807949
https://resolver.caltech.edu/CaltechAUTHORS:20140211-130807949
Autor:
R. L. Tunnicliffe, A. de Ugarte Postigo, Antonia Rowlinson, Josh Bloom, D. Malesani, Andrew J. Levan, Jens Hjorth, Daniel A. Perley, Nial R. Tanvir, Klaas Wiersema, Pall Jakobsson, S. B. Cenko, Johan P. U. Fynbo, P. T. O'Brien, B. E. Cobb
Publikováno v:
Monthly Notices of the Royal Astronomical Society, 437(2), 1495-1510. Oxford University Press
A significant proportion ($\sim30\%$) of the short-duration gamma-ray bursts (SGRBs) localised by Swift have no detected host galaxy coincident with the burst location to deep limits, and also no high-likelihood association with proximate galaxies on
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a893c6371ad3a5c1f54f356140dd597e
Autor:
R. Margutti, W. Fong, Ryan Chornock, Tanmoy Laskar, Edo Berger, Nial R. Tanvir, Karl M. Menten, Jens Hjorth, Katherine C. Roth, B. A. Zauderer, Derek B. Fox, Trent J. Dupuy, R. L. Tunnicliffe, V. Mangano, Andrew J. Levan
We present the optical discovery and sub-arcsecond optical and X-ray localization of the afterglow of the short GRB 120804A, as well as optical, near-IR, and radio detections of its host galaxy. X-ray observations with Swift/XRT, Chandra, and XMM-New
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::ee1f5557ddaf0bedc6ee53264c2f54b2
Autor:
R. L. Tunnicliffe, Andrew J. Levan
Publikováno v:
Proceedings of the International Astronomical Union. 7:415-416
Gamma-ray bursts are normally split into two classes, primarily determined by their observed duration, so called long (> 2s) and short (< 2s) GRBs. There have been many claims of a third duration class, with emission lasting for intermediate periods
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Autor:
Geoffrey C. Bower, J. C. Tello, A. S. Fruchter, Duncan A. Forbes, Pall Jakobsson, Giorgos Leloudas, Richard G. Strom, Christina C. Thöne, S. B. Cenko, Klaas Wiersema, Robert M. Quimby, Daniel Kocevski, N. Singh, L. van Spaandonk, D. Xu, John D. Graham, Chryssa Kouveliotou, Mansi M. Kasliwal, Antonino Cucchiara, T. Kerr, Johan P. U. Fynbo, Andrew J. Levan, P. A. Curran, A. de Ugarte Postigo, Jay Farihi, Aaron J. Romanowsky, Sergei Guziy, M. Bremer, R. M. Cutri, Kuntal Misra, Peter Nugent, Eran O. Ofek, Maryam Modjaz, R. L. Tunnicliffe, Jean P. Brodie, J. M. Castro Cerón, Jacob A. Arnold, Nathaniel R. Butler, A. J. Castro-Tirado, E. Rol, J. Ehle, Dovi Poznanski, J. M. Winters, Steve Schulze, Michael C. Cooper, Ralph A. M. J. Wijers, Javier Gorosabel, Ovidiu Vaduvescu, D. I. Hoffman, Jens Hjorth, R. Sanchez-Ramirez, Atish Kamble, Peter J. Wheatley, J. M. Silverman, Daniel A. Perley, T. Carroll, Nicholas M. Law, A. J. van der Horst, Nial R. Tanvir, Adam N. Morgan, Josh Bloom, R. L. C. Starling, P. T. O'Brien
Publikováno v:
Science
Science, American Association for the Advancement of Science, 2011, 333 (6039), pp.199-202. ⟨10.1126/science.1207143⟩
Science, 333, 199-202. American Association for the Advancement of Science
Science, 2011, 333 (6039), pp.199-202. ⟨10.1126/science.1207143⟩
Science, American Association for the Advancement of Science, 2011, 333 (6039), pp.199-202. ⟨10.1126/science.1207143⟩
Science, 333, 199-202. American Association for the Advancement of Science
Science, 2011, 333 (6039), pp.199-202. ⟨10.1126/science.1207143⟩
Variable X-ray and gamma-ray emission is characteristic of the most extreme physical processes in the Universe, and studying the sources of these energetic photons has been a major driver in astronomy for the past 50 years. Here we present multiwavel
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::2bdc87466dff447e458c191b74f0baec
https://researchonline.ljmu.ac.uk/id/eprint/6568/1/1104.3356.pdf
https://researchonline.ljmu.ac.uk/id/eprint/6568/1/1104.3356.pdf