Zobrazeno 1 - 10
of 203
pro vyhledávání: '"Scholz, Paul"'
Autor:
Dong, Fengqiu Adam, Clarke, Tracy, Curtin, Alice P., Kumar, Ajay, Stairs, Ingrid, Chatterjee, Shami, Cook, Amanda M., Fonseca, Emmanuel, Gaensler, B. M., Hessels, Jason W. T., Kaspi, Victoria M., Lazda, Mattias, Masui, Kiyoshi W., McKee, James W., Meyers, Bradley W., Pearlman, Aaron B., Ransom, Scott M., Scholz, Paul, Shin, Kaitlyn, Smith, Kendrick M., Tan, Chia Min
Neutron stars and white dwarfs are both dense remnants of post-main-sequence stars. Pulsars, magnetars and strongly magnetised white dwarfs have all been seen to been observed to exhibit coherent, pulsed radio emission in relation to their rotational
Externí odkaz:
http://arxiv.org/abs/2407.07480
Autor:
Curtin, Alice P., Sirota, Sloane, Kaspi, Victoria M., Tendulkar, Shriharsh P., Bhardwaj, Mohit, Cook, Amanda M., Fong, Wen-Fai, Gaensler, B. M., Main, Robert A., Masui, Kiyoshi W., Michilli, Daniele, Pandhi, Ayush, Pearlman, Aaron B., Scholz, Paul, Shin, Kaitlyn
We use the Canadian Hydrogen Intensity Mapping Experiment (CHIME) Fast Radio Burst (FRB) Project to search for FRBs that are temporally and spatially coincident with gamma-ray bursts (GRBs) occurring between 2018 July 7 and 2023 August 3. We do not f
Externí odkaz:
http://arxiv.org/abs/2404.09242
Autor:
Mckinven, Ryan, Bhardwaj, Mohit, Eftekhari, Tarraneh, Kilpatrick, Charles D., Kirichenko, Aida, Pal, Arpan, Cook, Amanda M., Gaensler, B. M., Giri, Utkarsh, Kaspi, Victoria M., Michilli, Daniele, Nimmo, Kenzie, Pearlman, Aaron B., Pleunis, Ziggy, Sand, Ketan R., Stairs, Ingrid, Andersen, Bridget C., Andrew, Shion, Bandura, Kevin, Brar, Charanjot, Cassanelli, Tomas, Chatterjee, Shami, Curtin, Alice P., Dong, Fengqiu Adam, Eadie, Gwendolyn, Fonseca, Emmanuel, Ibik, Adaeze L., Kaczmarek, Jane F., Kharel, Bikash, Lazda, Mattias, Leung, Calvin, Li, Dongzi, Main, Robert, Masui, Kiyoshi W., Mena-Parra, Juan, Ng, Cherry, Pandhi, Ayush, Patil, Swarali Shivraj, Prochaska, J. Xavier, Rafiei-Ravandi, Masoud, Scholz, Paul, Shah, Vishwangi, Shin, Kaitlyn, Smith, Kendrick
Fast radio bursts (FRBs) last for milliseconds and arrive at Earth from cosmological distances. While their origin(s) and emission mechanism(s) are presently unknown, their signals bear similarities with the much less luminous radio emission generate
Externí odkaz:
http://arxiv.org/abs/2402.09304
Autor:
Pandhi, Ayush, Pleunis, Ziggy, Mckinven, Ryan, Gaensler, B. M., Su, Jianing, Ng, Cherry, Bhardwaj, Mohit, Brar, Charanjot, Cassanelli, Tomas, Cook, Amanda M., Curtin, Alice P., Kaspi, Victoria M., Lazda, Mattias, Leung, Calvin, Li, Dongzi, Masui, Kiyoshi W., Michilli, Daniele, Nimmo, Kenzie, Pearlman, Aaron, Petroff, Emily, Rafiei-Ravandi, Masoud, Sand, Ketan R., Scholz, Paul, Shin, Kaitlyn, Smith, Kendrick, Stairs, Ingrid
We present a 400-800 MHz polarimetric analysis of 128 non-repeating fast radio bursts (FRBs) from the first CHIME/FRB baseband catalog, increasing the total number of FRB sources with polarization properties by a factor of ~3. 89 FRBs have >6${\sigma
Externí odkaz:
http://arxiv.org/abs/2401.17378
Autor:
Faber, Jakob T., Michilli, Daniele, Mckinven, Ryan, Su, Jianing, Pearlman, Aaron B., Nimmo, Kenzie, Main, Robert A., Kaspi, Victoria, Bhardwaj, Mohit, Chatterjee, Shami, Curtin, Alice P., Dobbs, Matt, Eadie, Gwendolyn, Gaensler, B. M., Kader, Zarif, Leung, Calvin, Masui, Kiyoshi W., Pandhi, Ayush, Petroff, Emily, Pleunis, Ziggy, Rafiei-Ravandi, Masoud, Sand, Ketan R., Scholz, Paul, Shin, Kaitlyn, Smith, Kendrick, Stairs, Ingrid
We present the discovery of twelve thus far non-repeating fast radio burst (FRB) sources, detected by the Canadian Hydrogen Intensity Mapping Experiment (CHIME) telescope. These sources were selected from a database comprising of order $10^3$ CHIME/F
Externí odkaz:
http://arxiv.org/abs/2312.14133
Autor:
Fonseca, Emmanuel, Pleunis, Ziggy, Breitman, Daniela, Sand, Ketan R., Kharel, Bikash, Boyle, Patrick J., Brar, Charanjot, Giri, Utkarsh, Kaspi, Victoria M., Masui, Kiyoshi W., Meyers, Bradley W., Patel, Chitrang, Scholz, Paul, Smith, Kendrick
We present a framework for modeling astrophysical pulses from radio pulsars and fast radio bursts (FRBs). This framework, called fitburst, generates synthetic representations of dynamic spectra that are functions of several physical and heuristic par
Externí odkaz:
http://arxiv.org/abs/2311.05829
Autor:
Collaboration, The CHIME/FRB, Amiri, Mandana, Andersen, Bridget C., Andrew, Shion, Bandura, Kevin, Bhardwaj, Mohit, Boyle, P. J., Brar, Charanjot, Breitman, Daniela, Cassanelli, Tomas, Chawla, Pragya, Cook, Amanda M., Curtin, Alice P., Dobbs, Matt, Dong, Fengqiu Adam, Eadie, Gwendolyn, Fonseca, Emmanuel, Gaensler, B. M., Giri, Utkarsh, Herrera-Martin, Antonio, Hopkins, Hans, Ibik, Adaeze L., Joseph, Ronniy C., Kaczmarek, J. F., Kader, Zarif, Kaspi, Victoria M., Lanman, Adam E., Lazda, Mattias, Leung, Calvin, Liu, Siqi, Masui, Kiyoshi W., Mckinven, Ryan, Mena-Parra, Juan, Merryfield, Marcus, Michilli, Daniele, Ng, Cherry, Nimmo, Kenzie, Noble, Gavin, Pandhi, Ayush, Patel, Chitrang, Pearlman, Aaron B., Pen, Ue-Li, Petroff, Emily, Pleunis, Ziggy, Rafiei-Ravandi, Masoud, Rahman, Mubdi, Ransom, Scott M., Sand, Ketan R., Scholz, Paul, Shah, Vishwangi, Shin, Kaitlyn, Shpunarska, Yuliya, Siegel, Seth R., Smith, Kendrick, Stairs, Ingrid, Stenning, David C., Vanderlinde, Keith, Wang, Haochen, White, Henry, Wulf, Dallas
In 2021, a catalog of 536 fast radio bursts (FRBs) detected with the Canadian Hydrogen Intensity Mapping Experiment (CHIME) radio telescope was released by the CHIME/FRB Collaboration. This large collection of bursts, observed with a single instrumen
Externí odkaz:
http://arxiv.org/abs/2311.00111
Autor:
Giri, Utkarsh, Andersen, Bridget C., Chawla, Pragya, Curtin, Alice P., Fonseca, Emmanuel, Kaspi, Victoria M., Lin, Hsiu-Hsien, Masui, Kiyoshi W., Sand, Ketan R., Scholz, Paul, Abbott, Thomas C., Dong, Fengqiu Adam, Gaensler, B. M., Leung, Calvin, Michilli, Daniele, Bhardwaj, Mohit, Münchmeyer, Moritz, Pandhi, Ayush, Pearlman, Aaron B., Pleunis, Ziggy, Rafiei-Ravandi, Masoud, Reda, Alex, Shin, Kaitlyn, Smith, Kendrick, Stairs, Ingrid H., Stenning, David C., Tendulkar, Shriharsh P.
The bright millisecond-duration radio burst from the Galactic magnetar SGR 1935+2154 in 2020 April was a landmark event, demonstrating that at least some fast radio burst (FRB) sources could be magnetars. The two-component burst was temporally coinci
Externí odkaz:
http://arxiv.org/abs/2310.16932
Autor:
Bhardwaj, Mohit, Michilli, Daniele, Kirichenko, Aida Yu., Modilim, Obinna, Shin, Kaitlyn, Kaspi, Victoria M., Andersen, Bridget C., Cassanelli, Tomas, Brar, Charanjot, Chatterjee, Shami, Cook, Amanda M., Dong, Fengqiu Adam, Fonseca, Emmanuel, Gaensler, B. M., Ibik, Adaeze L., Kaczmarek, J. F., Lanman, Adam E., Leung, Calvin, Masui, K. W., Pandhi, Ayush, Pearlman, Aaron B., Pleunis, Ziggy, Prochaska, J. Xavier, Rafiei-Ravandi, Masoud, Sand, Ketan R., Scholz, Paul, Smith, Kendrick M.
We present the host galaxies of four apparently non-repeating fast radio bursts (FRBs), FRBs 20181223C, 20190418A, 20191220A, and 20190425A, reported in the first Canadian Hydrogen Intensity Mapping Experiment (CHIME/FRB) catalog. Our selection of th
Externí odkaz:
http://arxiv.org/abs/2310.10018