Zobrazeno 1 - 10
of 33
pro vyhledávání: '"Bright, Joe S."'
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:
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
Autor:
Veledina, Alexandra, Muleri, Fabio, Poutanen, Juri, Podgorný, Jakub, Dovčiak, Michal, Capitanio, Fiamma, Churazov, Eugene, De Rosa, Alessandra, Di Marco, Alessandro, Forsblom, Sofia, Kaaret, Philip, Krawczynski, Henric, La Monaca, Fabio, Loktev, Vladislav, Lutovinov, Alexander A., Molkov, Sergey V., Mushtukov, Alexander A., Ratheesh, Ajay, Cavero, Nicole Rodriguez, Steiner, James F., Sunyaev, Rashid A., Tsygankov, Sergey S., Zdziarski, Andrzej A., Bianchi, Stefano, Bright, Joe S., Bursov, Nikolaj, Costa, Enrico, Egron, Elise, Garcia, Javier A., Green, David A., Gurwell, Mark, Ingram, Adam, Kajava, Jari J. E., Kale, Ruta, Kraus, Alex, Malyshev, Denys, Marin, Frédéric, Matt, Giorgio, McCollough, Michael, Mereminskiy, Ilia A., Nizhelsky, Nikolaj, Piano, Giovanni, Pilia, Maura, Pittori, Carlotta, Rao, Ramprasad, Righini, Simona, Soffitta, Paolo, Shevchenko, Anton, Svoboda, Jiri, Tombesi, Francesco, Trushkin, Sergei, Tsybulev, Peter, Ursini, Francesco, Weisskopf, Martin C., Wu, Kinwah, Agudo, Iván, Antonelli, Lucio A., Bachetti, Matteo, Baldini, Luca, Baumgartner, Wayne H., Bellazzini, Ronaldo, Bongiorno, Stephen D., Bonino, Raffaella, Brez, Alessandro, Bucciantini, Niccolò, Castellano, Simone, Cavazzuti, Elisabetta, Chen, Chien-Ting, Ciprini, Stefano, Del Monte, Ettore, Di Gesu, Laura, Di Lalla, Niccolò, Donnarumma, Immacolata, Doroshenko, Victor, Ehlert, Steven R., Enoto, Teruaki, Evangelista, Yuri, Fabiani, Sergio, Ferrazzoli, Riccardo, Gunji, Shuichi, Hayashida, Kiyoshi, Heyl, Jeremy, Iwakiri, Wataru, Jorstad, Svetlana G., Karas, Vladimir, Kislat, Fabian, Kitaguchi, Takao, Kolodziejczak, Jeffery J., Latronico, Luca, Liodakis, Ioannis, Maldera, Simone, Manfreda, Alberto, Marinucci, Andrea, Marscher, Alan P., Marshall, Herman L., Massaro, Francesco, Mitsuishi, Ikuyuki, Mizuno, Tsunefumi, Negro, Michela, Ng, Chi-Yung, O'Dell, Stephen L., Omodei, Nicola, Oppedisano, Chiara, Papitto, Alessandro, Pavlov, George G., Peirson, Abel L., Perri, Matteo, Pesce-Rollins, Melissa, Petrucci, Pierre-Olivier, Possenti, Andrea, Puccetti, Simonetta, Ramsey, Brian D., Rankin, John, Roberts, Oliver, Romani, Roger W., Sgrò, Carmelo, Slane, Patrick, Spandre, Gloria, Swartz, Doug, Tamagawa, Toru, Tavecchio, Fabrizio, Taverna, Roberto, Tawara, Yuzuru, Tennant, Allyn F., Thomas, Nicholas E., Trois, Alessio, Turolla, Roberto, Vink, Jacco, Xie, Fei, Zane, Silvia
The accretion of matter by compact objects can be inhibited by radiation pressure if the luminosity exceeds the critical value, known as the Eddington limit. Discovery of ultraluminous X-ray sources has shown that accretion can proceed even when the
Externí odkaz:
http://arxiv.org/abs/2303.01174
Autor:
Polzin, Ava, Margutti, Raffaella, Coppejans, Deanne, Auchettl, Katie, Page, Kim L., Vasilopoulos, Georgios, Bright, Joe S., Esposito, Paolo, Williams, Peter K. G., Mukai, Koji, Berger, Edo
We present a detailed compilation and analysis of the X-ray phase space of low- to intermediate-redshift ($ 0\le z \le 1$) transients that consolidates observed light curves (and theory where necessary) for a large variety of classes of transient/var
Externí odkaz:
http://arxiv.org/abs/2211.01232
Autor:
Zenati, Yossef, Wang, Qinan, Bobrick, Alexey, DeMarchi, Lindsay, Glanz, Hila, Rozner, Mor, Rest, Armin, Metzger, Brian D., Margutti, Raffaella, Gomez, Sebastian, Smith, Nathan, Toonen, Silvia, Bright, Joe S., Norman, Colin, Foley, Ryan J., Gagliano, Alexander, Krolik, Julian H., Smartt, Stephen J., Villar, Ashley V., Narayan, Gautham, Fox, Ori, Auchettl, Katie, Brethauer, Daniel, Clocchiatti, Alejandro, Coelln, Sophie V., Coppejans, Deanne L., Dimitriadis, Georgios, Doroszmai, Andris, Drout, Maria, Jacobson-Galan, Wynn, Gao, Bore, Ridden-Harper, Ryan, Kilpatrick, Charles Donald, Laskar, Tanmoy, Matthews, David, Rest, Sofia, Smith, Ken W., Stauffer, Candice McKenzie, Stroh, Michael C., Strolger, Louis-Gregory, Terreran, Giacomo, Pierel, Justin D. R., Piro, Anthony L.
We present multi-band ATLAS photometry for SN 2019tsf, a stripped-envelope Type Ib supernova (SESN). The SN shows a triple-peaked light curve and a late (re-)brightening, making it unique among stripped-envelope systems. The re-brightening observatio
Externí odkaz:
http://arxiv.org/abs/2207.07146
Autor:
DeMarchi, Lindsay, Margutti, R., Dittman, J., Brunthaler, A., Milisavljevic, D., Bietenholz, Michael F., Stauffer, C., Brethauer, D., Coppejans, D., Auchettl, K., Alexander, K. D., Kilpatrick, C. D., Bright, Joe S., Kelley, L. Z., Stroh, Michael C., Jacobson-Galan, W. V.
We present extensive multi-frequency VLA and VLBA observations of the radio-bright supernova (SN) IIb SN 2004C that span $\sim(40-2793)$ days post-explosion. We interpret the temporal evolution of the radio spectral energy distribution (SED) in the c
Externí odkaz:
http://arxiv.org/abs/2203.07388
Autor:
Jacobson-Galán, Wynn, Venkatraman, Padma, Margutti, Raffaella, Khatami, David, Terreran, Giacomo, Foley, Ryan J., Angulo, Rodrigo, Angus, Charlotte R., Auchettl, Katie, Blanchard, Peter K., Bobrick, Alexey, Bright, Joe S., Couch, Cirilla D., Coulter, David A., Clever, Karoli, Davis, Kyle W., de Boer, Thomas, DeMarchi, Lindsay, Dodd, Sierra A., Jones, David O., Johnson, Jessica, Kilpatrick, Charles D., Khetan, Nandita, Lai, Zhisen, Langeroodi, Danial, Lin, Chien-Cheng, Magnier, Eugene A., Milisavljevic, Dan, Perets, Hagai B., Pierel, Justin D. R., Raymond, John, Rest, Sofia, Rest, Armin, Ridden-Harper, Ryan, Shen, Ken J., Siebert, Matthew R., Smith, Carli, Taggart, Kirsty, Tinyanont, Samaporn, Valdes, Frank, Villar, Victoria A., Wang, Qinan, Yadavalli, S. Karthik, Zenati, Yossef, Zenteno, Alfredo
We present panchromatic observations and modeling of calcium-strong supernovae (SNe) 2021gno in the star-forming host galaxy NGC 4165 (D = 30.5 Mpc) and 2021inl in the outskirts of elliptical galaxy NGC 4923 (D = 80 Mpc), both monitored through the Y
Externí odkaz:
http://arxiv.org/abs/2203.03785
Autor:
Bright, Joe S., Margutti, Raffaella, Matthews, David, Brethauer, Daniel, Coppejans, Deanne, Wieringa, Mark H., Metzger, Brian D., DeMarchi, Lindsay, Laskar, Tanmoy, Romero, Charles, Alexander, Kate D., Horesh, Assaf, Migliori, Giulia, Chornock, Ryan, Berger, E., Bietenholz, Michael, Devlin, Mark J., Dicker, Simon R., Jacobson-Galán, W. V., Mason, Brian S., Milisavljevic, Dan, Motta, Sara E., Mroczkowski, Tony, Ramirez-Ruiz, Enrico, Rhodes, Lauren, Sarazin, Craig L., Sfaradi, Itai, Sievers, Jonathan
We present deep X-ray and radio observations of the Fast Blue Optical Transient (FBOT) AT2020xnd/ZTF20acigmel at $z=0.2433$ from $13$d to $269$d after explosion. AT2020xnd belongs to the category of optically luminous FBOTs with similarities to the a
Externí odkaz:
http://arxiv.org/abs/2110.05514
Autor:
Ho, Anna Y. Q., Goldstein, Daniel A., Schulze, Steve, Khatami, David K., Perley, Daniel A., Ergon, Mattias, Gal-Yam, Avishay, Corsi, Alessandra, Andreoni, Igor, Barbarino, Cristina, Bellm, Eric C., Blagorodnova, Nadia, Bright, Joe S., Burns, Eric, Cenko, S. Bradley, Cunningham, Virginia, De, Kishalay, Dekany, Richard, Dugas, Alison, Fender, Rob P., Fransson, Claes, Fremling, Christoffer, Goldstein, Adam, Graham, Matthew J., Hale, David, Horesh, Assaf, Hung, Tiara, Kasliwal, Mansi M., Kuin, N. Paul M., Kulkarni, Shri R., Kupfer, Thomas, Lunnan, Ragnhild, Masci, Frank J., Ngeow, Chow-Choong, Nugent, Peter E., Ofek, Eran O., Patterson, Maria T., Petitpas, Glen, Rusholme, Ben, Sai, Hanna, Sfaradi, Itai, Shupe, David L., Sollerman, Jesper, Soumagnac, Maayane T., Tachibana, Yutaro, Taddia, Francesco, Walters, Richard, Wang, Xiaofeng, Yao, Yuhan, Zhang, Xinhan
We present detailed observations of ZTF18abukavn (SN2018gep), discovered in high-cadence data from the Zwicky Transient Facility as a rapidly rising ($1.4\pm0.1$ mag/hr) and luminous ($M_{g,\mathrm{peak}}=-20$ mag) transient. It is spectroscopically
Externí odkaz:
http://arxiv.org/abs/1904.11009