Zobrazeno 1 - 9
of 9
pro vyhledávání: '"Kieran J. Luken"'
Autor:
Quentin Roper, Michael G. Burton, Ain De Horta, Kieran J. Luken, Gavin Rowell, T. J. Galvin, Nicholas O Ralph, Natasha Hurley-Walker, Miroslav Filipovic, Graeme F Wong, Ray P. Norris, Denis Leahy, Lisa Harvey-Smith, N. Maxted, Dejan Urošević, I. Sushch, Catherine Braiding, Rebecca Blackwell, Roland Kothes, James R. Allison, Robert Brose
Publikováno v:
Monthly notices of the Royal Astronomical Society 492(2), 2606-2621 (2020). doi:10.1093/mnras/stz3439
Monthly notices of the Royal Astronomical Society 492(2), 2606 - 2621 (2020). doi:10.1093/mnras/stz3439
We present 1–10 GHz radio continuum flux density, spectral index, polarization, and rotation measure (RM) images of the youngest known Gala
We present 1–10 GHz radio continuum flux density, spectral index, polarization, and rotation measure (RM) images of the youngest known Gala
Autor:
Aidan Hotan, Devika Shobhana, Timothy J Galvin, Roland M. Crocker, Vanessa A. Moss, Huib Intema, Kieran J. Luken, R. Z. E. Alsaberi, Tiziana Venturi, Evan J Crawford, Wasim Raja, J. Marvil, P. Manojlovic, Andrew M. Hopkins, Anna D. Kapińska, Ray P. Norris, Peter J. Macgregor, B. S. Koribalski, Craig S Anderson, Jordan D. Collier, G. E. Anderson, Matthew Whiting, Laurence A. F. Park, Miroslav Filipovic, C. L. Hale, Andrew O'Brien, Lawrence Rudnick, Natasha Hurley-Walker, Emil Lenc, Susumu Inoue, Jayanne English
Publikováno v:
Publications of the Astronomical Society of Australia, 38
We have found a class of circular radio objects in the Evolutionary Map of the Universe Pilot Survey, using the Australian Square Kilometre Array Pathfinder telescope. The objects appear in radio images as circular edge-brightened discs, about one ar
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::11e19cdd6ece7027d755439ec649c6f9
http://hdl.handle.net/1887/3275247
http://hdl.handle.net/1887/3275247
Autor:
E. J. Crawford, Elizabeth K. Mahony, Ray P. Norris, G. Gürkan, Kieran J. Luken, Andrew M. Hopkins, Michael J. I. Brown, Neeraj Gupta, Andrew O'Brien, J. Marvil, David Parkinson, John D. Bunton, Jacobo Asorey, Stanislav S. Shabala, C. J. Riseley, Syed Faisal ur Rahman, Jordan D. Collier, Anna D. Kapińska, C. L. Hale, Maxim Voronkov, C. E. Jacka, Baerbel Koribalski, Kim HyeongHan, Martin Bell, Tessa Vernstrom, M. Huynh, Wasim Raja, M. James Jee, Umberto Maio, M. Pandey-Pommier, Emil Lenc, James R. Allison, I. Prandoni, Matthew Whiting, Marcus Brüggen, Tim J. Galvin, Vanessa A. Moss, Lewis Ball, Lawrence Rudnick, Aidan Hotan, Yjan A. Gordon, Jaimie R. Sheil, Peter J. Macgregor, Thomas H. Reiprich, Christy Anderson, Heinz Andernach, Jayanne English, Miroslav Filipovic
Publikováno v:
Norris, R P, Marvil, J, Collier, J D, Kapinska, A D, O'Brien, A N, Rudnick, L, Andernach, H, Asorey, J, Brown, M J I, Bruggen, M, Crawford, E, English, J, Rahman, S F U, Filipovic, M D, Gordon, Y, Gurkan, G, Hale, C, Hopkins, A M, Huynh, M T, HyeongHan, K, Jee, M J, Koribalski, B S, Lenc, E, Luken, K, Parkinson, D, Prandoni, I, Raja, W, Reiprich, T H, Riseley, C J, Shabala, S S, Sheil, J R, Vernstrom, T, Whiting, M T, Allison, J R, Anderson, C S, Ball, L, Bell, M, Bunton, J, Galvin, T J, Gupta, N, Hotan, A, Jacka, C, Macgregor, P J, Mahony, E K, Maio, U, Moss, V, Pandey-Pommier, M & Voronkov, M A 2021, ' The Evolutionary Map of the Universe Pilot Survey ', Publications of the Astronomical Society of Australia, vol. 38, e046, pp. 1-26 . https://doi.org/10.1017/pasa.2021.42
We present the data and initial results from the first Pilot Survey of the Evolutionary Map of the Universe (EMU), observed at 944 MHz with the Australian Square Kilometre Array Pathfinder (ASKAP) telescope. The survey covers 270 \sqdeg of an area co
Autor:
Miroslav Filipovic, Kieran J. Luken, Thomas G. Pannuti, Graeme F Wong, N. Maxted, P. Manojlovic, Quentin Roper
Publikováno v:
Serbian Astronomical Journal, Vol 2017, Iss 195, Pp 23-31 (2017)
We present an analysis of X-ray observations made with ASCA and XMM-Newton of the Galactic supernova remnant (SNR) G311.5−0.3. Prior infrared and radio observations of this SNR have revealed a shell-like morphology at both wavelengths. The spectral
Discovery of a Pulsar-powered Bow Shock Nebula in the Small Magellanic Cloud Supernova Remnant DEMS5
Autor:
Roland Kothes, Thomas G. Pannuti, Kieran J. Luken, V. Velović, Andrew O'Brien, P. Maggi, Ray P. Norris, R. Z. E. Alsaberi, Nicholas F. H Tothill, Sebastián Gurovich, N. Maxted, Hidetoshi Sano, T. J. Galvin, Luke M Bozzetto, Dejan Urošević, Patrick J. Kavanagh, Natasha Hurley-Walker, B. Q. For, Miroslav Filipovic, H. Dénes, Evan J Crawford, Graeme F Wong, Yasuo Fukui, Thomas H. Jarrett, Manami Sasaki, D. Onić, Ivan S. Bojičić, Miranda Yew, Shi Dai, Lister Staveley-Smith, Naomi McClure-Griffiths, Gavin Rowell, P. Manjolović, Frank Haberl, Chandreyee Maitra
Publikováno v:
Mon.Not.Roy.Astron.Soc.
Mon.Not.Roy.Astron.Soc., 2019, 486 (2), pp.2507-2524. ⟨10.1093/mnras/stz971⟩
CONICET Digital (CONICET)
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
Mon.Not.Roy.Astron.Soc., 2019, 486 (2), pp.2507-2524. ⟨10.1093/mnras/stz971⟩
CONICET Digital (CONICET)
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
We report the discovery of a new Small Magellanic Cloud Pulsar Wind Nebula (PWN) at the edge of the Supernova Remnant (SNR)-DEM S5. The pulsar powered object has a cometary morphology similar to the Galactic PWN analogs PSR B1951+32 and 'the mouse'.
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d19e93dd20e3ad90efb2657b1ec843a2
http://arxiv.org/abs/1903.03226
http://arxiv.org/abs/1903.03226
Publikováno v:
Astron.Astrophys.
Astron.Astrophys., 2019, 627, pp.A166. ⟨10.1051/0004-6361/201834430⟩
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2019, 627, pp.A166. ⟨10.1051/0004-6361/201834430⟩
Astronomy and astrophysics 627, A166-(2019). doi:10.1051/0004-6361/201834430
Astron.Astrophys., 2019, 627, pp.A166. ⟨10.1051/0004-6361/201834430⟩
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2019, 627, pp.A166. ⟨10.1051/0004-6361/201834430⟩
Astronomy and astrophysics 627, A166-(2019). doi:10.1051/0004-6361/201834430
Context. The youngest Galactic supernova remnant G1.9+0.3 is an interesting target for next generation gamma-ray observatories. So far, the remnant is only detected in the radio and the X-ray bands, but its young age of ~100 yrs and inferred shock sp
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c6ccdcd559b27b2d71ec6124f2a2bb17
https://hal.archives-ouvertes.fr/hal-02279078
https://hal.archives-ouvertes.fr/hal-02279078
Publikováno v:
Publications of the Astronomical Society of the Pacific. 131:108003
In the near future, all-sky radio surveys are set to produce catalogues of tens of millions of sources with limited multi-wavelength photometry. Spectroscopic redshifts will only be possible for a small fraction of these new-found sources. In this pa
Autor:
James E. Geach, Giuseppe Longo, Kai Lars Polsterer, Ray P. Norris, Kieran J. Luken, Stefano Cavuoti, Vernesa Smolčić, Nick Seymour, Mattia Vaccari, Peter-Christian Zinn, Duncan Farrah, Giuseppe Riccio, Massimo Brescia, Tamás Budavári, Samuel Carliles, A. Musaeva, Mara Salvato
Publikováno v:
Publications of the Astronomical Society of the Pacific. 131:108004
Future radio surveys will generate catalogues of tens of millions of radio sources, for which redshift estimates will be essential to achieve many of the science goals. However, spectroscopic data will be available for only a small fraction of these
Publikováno v:
Publications of the Astronomical Society of the Pacific; Oct2019, Vol. 131 Issue 1004, p1-1, 1p