Zobrazeno 1 - 10
of 191
pro vyhledávání: '"Burns, Eric"'
Autor:
Negro, Michela, Younes, George, Wadiasingh, Zorawar, Burns, Eric, Trigg, Aaron, Baring, Matthew
Time-domain and multimessenger astronomy (TDAMM) involves the study of transient and time-variable phenomena across various wavelengths and messengers. The Astro2020 Decadal Survey has identified TDAMM as the top priority for NASA in this decade, emp
Externí odkaz:
http://arxiv.org/abs/2406.04967
Autor:
Negro, Michela, Cibrario, Nicoló, Burns, Eric, Wood, Joshua, Goldstein, Adam, Canton, Tito Dal
Gamma-ray Bursts (GRBs) are one of the most energetic phenomena in the cosmos, whose study probes physics extremes beyond the reach of laboratories on Earth. Our quest to unravel the origin of these events and understand their underlying physics is f
Externí odkaz:
http://arxiv.org/abs/2406.03643
Autor:
Ronchini, Samuele, Bala, Suman, Wood, Joshua, Delaunay, James, Dichiara, Simone, Kennea, Jamie A., Parsotan, Tyler, Raman, Gayathri, Tohuvavohu, Aaron, Adhikari, Naresh, Bhat, Narayana P., Biscoveanu, Sylvia, Bissaldi, Elisabetta, Burns, Eric, Campana, Sergio, Chandra, Koustav, Cleveland, William H., Dalessi, Sarah, De Pasquale, Massimiliano, García-Bellido, Juan, Gasbarra, Claudio, Giles, Misty M., Gupta, Ish, Hartmann, Dieter, Hristov, Boyan A., Hui, Michelle C., Kashyap, Rahul, Kocevski, Daniel, Mailyan, Bagrat, Malacaria, Christian, Nakano, Hiroyuki, Principe, Giacomo, Roberts, Oliver J., Sathyaprakash, Bangalore, Shao, Lijing, Troja, Eleonora, Veres, Péter, Wilson-Hodge, Colleen A.
GW230529 is the first compact binary coalescence detected by the LIGO-Virgo-KAGRA collaboration with at least one component mass confidently in the lower mass-gap, corresponding to the range 3-5$M_{\odot}$. If interpreted as a neutron star-black hole
Externí odkaz:
http://arxiv.org/abs/2405.10752
Autor:
Lagos, Macarena, Jenks, Leah, Isi, Maximiliano, Hotokezaka, Kenta, Metzger, Brian D., Burns, Eric, Farr, Will M., Perkins, Scott, Wong, Kaze W. K., Yunes, Nicolas
Extensions to General Relativity (GR) allow the polarization of gravitational waves (GW) from astrophysical sources to suffer from amplitude and velocity birefringence, which respectively induce changes in the ellipticity and orientation of the polar
Externí odkaz:
http://arxiv.org/abs/2402.05316
Autor:
Perley, Daniel A., Ho, Anna Y. Q., Fausnaugh, Michael, Lamb, Gavin P., Kasliwal, Mansi M., Ahumada, Tomas, Anand, Shreya, Andreoni, Igor, Bellm, Eric, Bhalerao, Varun, Bolin, Bryce, Brink, Thomas G., Burns, Eric, Cenko, S. Bradley, Corsi, Alessandra, Filippenko, Alexei V., Frederiks, Dmitry, Goldstein, Adam, Hamburg, Rachel, Jayaraman, Rahul, Jonker, Peter G., Kool, Erik C., Kulkarni, Shrinivas, Kumar, Harsh, Laher, Russ, Levan, Andrew, Lysenko, Alexandra, Perley, Richard A., Ricker, George R., Riddle, Reed, Ridnaia, Anna, Rusholme, Ben, Smith, Roger, Svinkin, Dmitry, Ulanov, Mikhail, Waratkar, Gaurav, Yao, Yuhan
Classical gamma-ray bursts (GRBs) have two distinct emission episodes: prompt emission from ultra-relativistic ejecta and afterglow from shocked circumstellar material. While both components are extremely luminous in known GRBs, a variety of scenario
Externí odkaz:
http://arxiv.org/abs/2401.16470
Autor:
Trigg, Aaron C., Burns, Eric, Roberts, Oliver J., Negro, Michela, Svinkin, Dmitry S., Baring, Matthew G., Wadiasingh, Zorawar, Christensen, Nelson L., Andreoni, Igor, Briggs, Michael S., Di Lalla, Niccolo, Frederiks, Dmitry D., Lipunov, Vladimir M., Omodei, Nicola, Ridnaia, Anna V., Veres, Peter, Lysenko, Alexandra L.
Magnetars are slowly rotating neutron stars that possess the strongest magnetic fields ($10^{14}-10^{15} \mathrm{G}$) known in the cosmos. They display a range of transient high-energy electromagnetic activity. The brightest and most energetic of the
Externí odkaz:
http://arxiv.org/abs/2311.09362
Autor:
Tomsick, John A., Boggs, Steven E., Zoglauer, Andreas, Hartmann, Dieter, Ajello, Marco, Burns, Eric, Fryer, Chris, Karwin, Chris, Kierans, Carolyn, Lowell, Alexander, Malzac, Julien, Roberts, Jarred, Saint-Hilaire, Pascal, Shih, Albert, Siegert, Thomas, Sleator, Clio, Takahashi, Tadayuki, Tavecchio, Fabrizio, Wulf, Eric, Beechert, Jacqueline, Gulick, Hannah, Joens, Alyson, Lazar, Hadar, Neights, Eliza, Oliveros, Juan Carlos Martinez, Matsumoto, Shigeki, Melia, Tom, Yoneda, Hiroki, Amman, Mark, Bal, Dhruv, von Ballmoos, Peter, Bates, Hugh, Böttcher, Markus, Bulgarelli, Andrea, Cavazzuti, Elisabetta, Chang, Hsiang-Kuang, Chen, Claire, Chu, Che-Yen, Ciabattoni, Alex, Costamante, Luigi, Dreyer, Lente, Fioretti, Valentina, Fenu, Francesco, Gallego, Savitri, Ghirlanda, Giancarlo, Grove, Eric, Huang, Chien-You, Jean, Pierre, Khatiya, Nikita, Knödlseder, Jürgen, Krause, Martin, Leising, Mark, Lewis, Tiffany R., Lommler, Jan Peter, Marcotulli, Lea, Martinez-Castellanos, Israel, Mittal, Saurabh, Negro, Michela, Nussirat, Samer Al, Nakazawa, Kazuhiro, Oberlack, Uwe, Palmore, David, Panebianco, Gabriele, Parmiggiani, Nicolo, Parsotan, Tyler, Pike, Sean N., Rogers, Field, Schutte, Hester, Sheng, Yong, Smale, Alan P., Smith, Jacob, Trigg, Aaron, Venters, Tonia, Watanabe, Yu, Zhang, Haocheng
Publikováno v:
PoS(ICRC2023)745
The Compton Spectrometer and Imager (COSI) is a NASA Small Explorer (SMEX) satellite mission in development with a planned launch in 2027. COSI is a wide-field gamma-ray telescope designed to survey the entire sky at 0.2-5 MeV. It provides imaging, s
Externí odkaz:
http://arxiv.org/abs/2308.12362
Autor:
Martinez-Castellanos, Israel, Gallego, Savitri, Huang, Chien-You, Karwin, Chris, Kierans, Carolyn, Lommler, Jan Peter, Mittal, Saurabh, Negro, Michela, Neights, Eliza, Pike, Sean N., Sheng, Yong, Siegert, Thomas, Yoneda, Hiroki, Zoglauer, Andreas, Tomsick, John A., Boggs, Steven E., Hartmann, Dieter, Ajello, Marco, Burns, Eric, Fryer, Chris, Lowell, Alexander, Malzac, Julien, Roberts, Jarred, Saint-Hilaire, Pascal, Shih, Albert, Sleator, Clio, Takahashi, Tadayuki, Tavecchio, Fabrizio, Wulf, Eric, Beechert, Jacqueline, Gulick, Hannah, Joens, Alyson, Lazar, Hadar, Oliveros, Juan Carlos Martinez, Matsumoto, Shigeki, Melia, Tom, Amman, Mark, Bal, Dhruv, von Ballmoos, Peter, Bates, Hugh, Böttcher, Markus, Bulgarelli, Andrea, Cavazzuti, Elisabetta, Chang, Hsiang-Kuang, Chen, Claire, Chu, Che-Yen, Ciabattoni, Alex, Costamante, Luigi, Dreyer, Lente, Fioretti, Valentina, Fenu, Francesco, Ghirlanda, Giancarlo, Grove, Eric, Jean, Pierre, Khatiya, Nikita, Knödlseder, Jürgen, Krause, Martin, Leising, Mark, Lewis, Tiffany R., Marcotulli, Lea, Nussirat, Samer Al, Nakazawa, Kazuhiro, Oberlack, Uwe, Palmore, David, Panebianco, Gabriele, Parmiggiani, Nicolo, Parsotan, Tyler, Rogers, Field, Schutte, Hester, Smale, Alan P., Smith, Jacob, Trigg, Aaron, Venters, Tonia, Watanabe, Yu, Zhang, Haocheng
Publikováno v:
Martinez, Israel. The cosipy library: COSI's high-level analysis software. PoS ICRC2023 (2023) 444-858
The Compton Spectrometer and Imager (COSI) is a selected Small Explorer (SMEX) mission launching in 2027. It consists of a large field-of-view Compton telescope that will probe with increased sensitivity the under-explored MeV gamma-ray sky (0.2-5 Me
Externí odkaz:
http://arxiv.org/abs/2308.11436
Autor:
Burns, Eric, Coughlin, Michael, Ackley, Kendall, Andreoni, Igor, Bizouard, Marie-Anne, Broekgaarden, Floor, Christensen, Nelson L., D'Ammando, Filippo, DeLaunay, James, Fleischhack, Henrike, Frey, Raymond, Fryer, Chris L., Goldstein, Adam, Grossan, Bruce, Hamburg, Rachel, Hartmann, Dieter H., Ho, Anna Y. Q., Howell, Eric J., Hui, C. Michelle, Jenks, Leah, Joens, Alyson, Lesage, Stephen, Levan, Andrew J., Lien, Amy, Meli, Athina, Negro, Michela, Parsotan, Tyler, Roberts, Oliver J., Santander, Marcos, Smith, Jacob R., Tohuvavohu, Aaron, Tomsick, John A., Wadiasingh, Zorawar, Veres, Peter, Villar, Ashley V., Zhang, Haocheng, Zhu, Sylvia J.
The Interplanetary Network (IPN) is a detection, localization and alert system that utilizes the arrival time of transient signals in gamma-ray detectors on spacecraft separated by planetary baselines to geometrically locate the origin of these trans
Externí odkaz:
http://arxiv.org/abs/2308.04485
Publikováno v:
Res. Notes AAS 7 136 (2023)
Compact-object binary mergers consisting of one neutron star and one black hole (NSBHs) have long been considered promising progenitors for gamma-ray bursts, whose central engine remains poorly understood. Using gravitational-wave constraints on the
Externí odkaz:
http://arxiv.org/abs/2306.14974