Zobrazeno 1 - 10
of 168
pro vyhledávání: '"Michael P. Rupen"'
Autor:
Wanga Mulaudzi, Marco Toliman Lucchini, Diego Altamirano, Aastha S. Parikh, Roberto Soria, Sera Markoff, G. R. Sivakoff, Nathalie Degenaar, Rudy Wijnands, Stephane Corbel, Maria Cristina Baglio, D. M. Russell, D. Maitra, Chiara Ceccobello, Thomas D. Russell, Simone Migliari, Michael P. Rupen, Rob Fender, Karri I. I. Koljonen, J. van den Eijnden, Felicia Krauß, Sebastian Heinz, Craig L. Sarazin, James Miller-Jones, Richard M. Plotkin, Alexandra J. Tetarenko
Publikováno v:
Mon.Not.Roy.Astron.Soc.
Mon.Not.Roy.Astron.Soc., 2020, 498 (4), pp.5772-5785. ⟨10.1093/mnras/staa2650⟩
Monthly Notices of the Royal Astronomical Society, 498(4), 5772-5785. Oxford University Press
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, 2020, 498 (4), pp.5772-5785. ⟨10.1093/mnras/staa2650⟩
Mon.Not.Roy.Astron.Soc., 2020, 498 (4), pp.5772-5785. ⟨10.1093/mnras/staa2650⟩
Monthly Notices of the Royal Astronomical Society, 498(4), 5772-5785. Oxford University Press
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, 2020, 498 (4), pp.5772-5785. ⟨10.1093/mnras/staa2650⟩
We present results from six epochs of quasi-simultaneous radio, (sub-)millimetre, infrared, optical, and X-ray observations of the black hole X-ray binary MAXI~J1535$-$571. These observations show that as the source transitioned through the hard-inte
Autor:
Kirill V Sokolovsky, Kwan-Lok Li, Raimundo Lopes de Oliveira, Jan-Uwe Ness, Koji Mukai, Laura Chomiuk, Elias Aydi, Elad Steinberg, Indrek Vurm, Brian D Metzger, Aliya-Nur Babul, Adam Kawash, Justin D Linford, Thomas Nelson, Kim L Page, Michael P Rupen, Jennifer L Sokoloski, Jay Strader, David Kilkenny
Peaking at 3.7 mag on 2020 July 11, YZ Ret was the second-brightest nova of the decade. The nova's moderate proximity (2.7 kpc from Gaia) provided an opportunity to explore its multi-wavelength properties in great detail. Here we report on YZ Ret as
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a9b69c997236629ceecdfbca18e4af11
http://arxiv.org/abs/2108.03241
http://arxiv.org/abs/2108.03241
Publikováno v:
Modeling, Systems Engineering, and Project Management for Astronomy IX.
We present an end-to-end model of the signal-chain of the correlator and beamformer of the Square Kilometre Array Phase 1 Mid telescope. The objective of this model is to determine whether the proposed signal processing architecture can meet the SKA
Autor:
Elias Aydi, J. D. Linford, Jennifer L. Sokoloski, Jay Strader, Kirill Sokolovsky, Jan-Uwe Ness, Brian D. Metzger, K. L. Page, Michael P. Rupen, Koji Mukai, Adam Kawash, Kwan-Lok Li, Raimundo Lopes de Oliveira, Indrek Vurm, Elad Steinberg, Amy J. Mioduszewski, Laura Chomiuk, T. J. N. Nelson
Shocks in gamma-ray emitting classical novae are expected to produce bright thermal and non-thermal X-rays. We test this prediction with simultaneous NuSTAR and Fermi/LAT observations of nova V906 Car, which exhibited the brightest GeV gamma-ray emis
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::dada26afe83dd4e6a720d56750032561
Autor:
Kazumi Kashiyama, Sarah Burke-Spolaor, Bryan J. Butler, Geoffrey C. Bower, Justin D. Linford, Kohta Murase, T. J. W. Lazio, Kshitij Aggarwal, Michael P. Rupen, Paul Demorest, Conor Omand, Casey J. Law, Shriharsh P. Tendulkar
We present results of a search for late-time radio emission and Fast Radio Bursts (FRBs) from a sample of type-I superluminous supernovae (SLSNe-I). We used the Karl G. Jansky Very Large Array to observe ten SLSN-I more than 5 years old at a frequenc
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::0dda3b8745f2756c59f2c89b7676d97e
https://resolver.caltech.edu/CaltechAUTHORS:20191115-091128751
https://resolver.caltech.edu/CaltechAUTHORS:20191115-091128751
Autor:
Mark Gurwell, Dipankar Maitra, Rob Fender, Sera Markoff, Michael P. Rupen, Alexandra J. Tetarenko, Erik Rosolowsky, Simone Migliari, Gregory R. Sivakoff, James Miller-Jones, Glen Petitpas, Craig L. Sarazin, D. M. Russell, J. G. A. Wouterloot, Sebastian Heinz, A. Rushton, Thomas D. Russell
Publikováno v:
Monthly Notices of the Royal Astronomical Society, 469(3), 3141-3162. Oxford University Press
We present simultaneous radio through sub-mm observations of the black hole X-ray binary (BHXB) V404 Cygni during the most active phase of its June 2015 outburst. Our $4$ hour long set of overlapping observations with the Very Large Array, the Sub-mi
Autor:
Jason W. T. Hessels, Matthew W. Abruzzo, Michael P. Rupen, H. J. van Langevelde, Scott M. Ransom, Paul Demorest, Sarah Burke-Spolaor, Bryan J. Butler, Zsolt Paragi, P. Scholz, Shami Chatterjee, Benito Marcote, V. M. Kaspi, Maura McLaughlin, A. Keimpema, Slavko Bogdanov, Laura Spitler, Andrew Seymour, Geoffrey C. Bower, C. G. Bassa, James M. Cordes, T. J. W. Lazio, Robert Wharton, Casey J. Law, Shriharsh P. Tendulkar
Publikováno v:
Nature
NASA Astrophysics Data System
Nature, 541, 58-61
Nature, 541(7635), 58-61. Nature Publishing Group
NASA Astrophysics Data System
Nature, 541, 58-61
Nature, 541(7635), 58-61. Nature Publishing Group
Fast radio bursts are astronomical radio flashes of unknown physical nature with durations of milliseconds. Their dispersive arrival times suggest an extragalactic origin and imply radio luminosities orders of magnitude larger than any other kind of
Autor:
Frederick M. Walter, R. Mark Wagner, Takahiro Sumi, Yong Zheng, Michael P. Rupen, C. C. Cheung, Fumio Abe, Daisuke Suzuki, J. Weston, Koji Mukai, G. B. Taylor, Jennifer L. Sokoloski, Jennifer C. Yee, Paul J. Tristram, J. L. Prieto, G. W. Christie, T. J. N. Nelson, Jennie McCormick, Amy J. Mioduszewski, Subo Dong, Ian A. Bond, David P. Bennett, Brian D. Metzger, Tim Natusch, Charles E. Woodward, Laura Chomiuk, C. Buil, Sumner Starrfield, Thomas Finzell, Andrew Gould, Naoki Koshimoto, Thomas Bensby, Terry Bohlsen, Justin D. Linford
Publikováno v:
The Astrophysical Journal. 903:153
Autor:
J. L. Sokoloski, Amy J. Mioduszewski, Justin D. Linford, Frederick M. Walter, Laura Chomiuk, T. Finzell, Jennifer Weston, T. J. N. Nelson, Michael P. Rupen, Koji Mukai
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 460:2687-2697
Since the Fermi discovery of $\gamma$-rays from novae, one of the biggest questions in the field has been how novae generate such high-energy emission. Shocks must be a fundamental ingredient. Six months of radio observations of the 2012 nova V5589 S
Autor:
Jon M. Miller, Mark Reynolds, Kayhan Gültekin, Amy J. Mioduszewski, Michael Bietenholz, Norbert Bartel, A. L. King, Michael P. Rupen
Publikováno v:
Nature Physics. 12:772-777
Observational constraints of relativistic jets from black holes has largely come from the most powerful and extended jets\cite{Jorstad05,Asada14}, leaving the nature of the low luminosity jets a mystery\cite{Falcke04}. M81* is one of the nearest low-