Zobrazeno 1 - 10
of 77
pro vyhledávání: '"Bright, Joe"'
Autor:
Bright, Joe S., Carotenuto, Francesco, Fender, Rob, Choza, Carmen, Mummery, Andrew, Jonker, Peter G., Smartt, Stephen J., DeBoer, David R., Farah, Wael, Matthews, James, Pollak, Alexander W., Rhodes, Lauren, Siemion, Andrew
Despite being operational for only a short time, the Einstein Probe mission has already significantly advanced the study of rapid variability in the soft X-ray sky. We report the discovery of luminous and variable radio emission from the Einstein Pro
Externí odkaz:
http://arxiv.org/abs/2409.19055
Autor:
Orlowski-Scherer, John, Maccarone, Thomas J., Bright, Joe, Kaminski, Tomasz, Koss, Michael, Mohan, Atul, Montenegro-Montes, Francisco Miguel, Næss, Sig urd, Ricci, Claudio, Severgnini, Paola, Stanke, Thomas, Vignali, Cristian, Wedemeyer, Sven, Booth, Mark, Cicone, Claudia, Di Mascolo, Luca, Johnstone, Doug, Mroczkowski, Tony, Cordiner, Martin A., Greiner, Jochen, Hatziminaoglou, Evanthia, van Kampen, Eelco, Klaassen, Pamela, Lee, Minju M., Liu, Daizhong, Saintonge, Amelie, Smith, Matthew, Thelen, Alexander E.
The study of transient and variable events, including novae, active galactic nuclei, and black hole binaries, has historically been a fruitful path for elucidating the evolutionary mechanisms of our universe. The study of such events in the millimete
Externí odkaz:
http://arxiv.org/abs/2404.13133
Publikováno v:
Published in RAS Astronomy and Geophysic, Vol 64, p 6.24 (December 2023)
In this short paper we outline the case for a small radio telescope array in the southern hemisphere with operations dedicated to rapid follow-up and monitoring of astrophysical transients. We argue that the science harvest from such a facility would
Externí odkaz:
http://arxiv.org/abs/2402.04698
Autor:
Sfaradi, Itai, Horesh, Assaf, Sollerman, Jesper, Fender, Rob, Rhodes, Lauren, Williams, David R. A., Bright, Joe, Green, Dave A., Schulze, Steve, Gal-Yam, Avishay
Publikováno v:
A&A 686, A129 (2024)
We present here broadband radio observations of the CSM interacting SN2019oys. SN2019oys was first detected in the optical and was classified as a Type Ib SN. Then, about $\sim 100$ days after discovery, it showed an optical rebrightening and a spect
Externí odkaz:
http://arxiv.org/abs/2312.00131
Autor:
Echiburú-Trujillo, Constanza, Tetarenko, Alexandra J., Haggard, Daryl, Russell, Thomas D., Koljonen, Karri I. I., Bahramian, Arash, Wang, Jingyi, Bremer, Michael, Bright, Joe, Casella, Piergiorgio, Russell, David M., Altamirano, Diego, Baglio, M. Cristina, Belloni, Tomaso, Ceccobello, Chiara, Corbel, Stephane, Trigo, Maria Diaz, Maitra, Dipankar, Gabuya, Aldrin, Gallo, Elena, Heinz, Sebastian, Homan, Jeroen, Kara, Erin, Körding, Elmar, Lewis, Fraser, Lucchini, Matteo, Markoff, Sera, Migliari, Simone, Miller-Jones, James C. A., Rodriguez, Jerome, Saikia, Payaswini, Sarazin, Craig L., Shahbaz, Tariq, Sivakoff, Gregory, Soria, Roberto, Testa, Vincenzo, Tetarenko, Bailey E., Tudose, Valeriu
Publikováno v:
2024 ApJ 962 116
Black hole X-ray binaries (BH XRBs) are ideal targets to study the connection between accretion inflow and jet outflow. Here we present quasi-simultaneous, multi-wavelength observations of the Galactic black hole system MAXI J1820+070, throughout its
Externí odkaz:
http://arxiv.org/abs/2311.11523
Autor:
Sfaradi, Itai, Beniamini, Paz, Horesh, Assaf, Piran, Tsvi, Bright, Joe, Rhodes, Lauren, Willians, David R. A., Fender, Rob, Leung, James K., Murphy, Tara, Green, Dave A.
The Tidal Disruption Event (TDE) AT 2018hyz exhibited a delayed radio flare almost three years after the stellar disruption. Here we report new radio observations of the TDE AT 2018hyz with the AMI-LA and ATCA spanning from a month to more than four
Externí odkaz:
http://arxiv.org/abs/2308.01965
Autor:
Makrygianni, Lydia, Trakhtenbrot, Benny, Arcavi, Iair, Ricci, Claudio, Lam, Marco C., Horesh, Assaf, Sfaradi, Itai, Bostroem, K. Azalee, Hosseinzadeh, Griffin, Howell, D. Andrew, Pellegrino, Craig, Fender, Rob, Green, David A., Williams, David R. A., Bright, Joe
AT 2021loi is an optical-ultraviolet transient located at the center of its host galaxy. Its spectral features identify it as a member of the ``Bowen Fluorescence Flare'' (BFF) class. The first member of this class was considered to be related to a t
Externí odkaz:
http://arxiv.org/abs/2305.01694
Autor:
Andersson, Alex, Lintott, Chris, Fender, Rob, Bright, Joe, Carotenuto, Francesco, Driessen, Laura, Espinasse, Mathilde, Gaseahalwe, Kelebogile, Heywood, Ian, van der Horst, Alexander J., Motta, Sara, Rhodes, Lauren, Tremou, Evangelia, Williams, David R. A., Woudt, Patrick, Zhang, Xian, Bloemen, Steven, Groot, Paul, Vreeswijk, Paul, Giarratana, Stefano, Saikia, Payaswini, Andersson, Jonas, Arroyo, Lizzeth Ruiz, Baert, Loïc, Baumann, Matthew, Domainko, Wilfried, Eschweiler, Thorsten, Forsythe, Tim, Gaudenzi, Sauro, Grenier, Rachel Ann, Iannone, Davide, Lahoz, Karla, Melville, Kyle J., Nascimento, Marianne De Sousa, Navarro, Leticia, Parthasarathi, Sai, Piilonen, Rahman, Najma, Smith, Jeffrey, Stewart, B., Temoke, Newton, Tworek, Chloe, Whittle, Isabelle
The newest generation of radio telescopes are able to survey large areas with high sensitivity and cadence, producing data volumes that require new methods to better understand the transient sky. Here we describe the results from the first citizen sc
Externí odkaz:
http://arxiv.org/abs/2304.14157
Autor:
Zdziarski, Andrzej A., Veledina, Alexandra, Szanecki, Michal, Green, David A., Bright, Joe S., Williams, David R. A.
Recently, the accretion geometry of the black-hole X-ray binary Cyg X-1 was probed with the X-ray polarization. The position angle of the X-ray emitting flow was found to be aligned with the position angle of the radio jet in the plane of the sky. At
Externí odkaz:
http://arxiv.org/abs/2304.07553
Autor:
Bright, Joe S., Rhodes, Lauren, Farah, Wael, Fender, Rob, van der Horst, Alexander J., Leung, James K., Williams, David R. A., Anderson, Gemma E., Atri, Pikky, DeBoer, David R., Giarratana, Stefano, Green, David A., Heywood, Ian, Lenc, Emil, Murphy, Tara, Pollak, Alexander W., Premnath, Pranav H., Scott, Paul F., Sheikh, Sofia Z., Siemion, Andrew, Titterington, David J.
The deaths of massive stars are sometimes accompanied by the launch of highly relativistic and collimated jets. If the jet is pointed towards Earth, we observe a "prompt" gamma-ray burst due to internal shocks or magnetic reconnection events within t
Externí odkaz:
http://arxiv.org/abs/2303.13583