Zobrazeno 1 - 10
of 67
pro vyhledávání: '"Dong, Fengqiu Adam"'
Autor:
Curtin, Alice P., Sand, Ketan R., Pleunis, Ziggy, Jain, Naman, Kaspi, Victoria, Michilli, Daniele, Fonseca, Emmanuel, Shin, Kaitlyn, Nimmo, Kenzie, Brar, Charanjot, Dong, Fengqiu Adam, Eadie, Gwendolyn M., Gaensler, B. M., Herrera-Martin, Antonio, Ibik, Adaeze L., Joseph, Ronny C., Kaczmarek, Jane, Leung, Calvin, Main, Robert, Masui, Kiyoshi W., McKinven, Ryan, Mena-Parra, Juan, Ng, Cherry, Pandhi, Ayush, Pearlman, Aaron B., Rafiei-Ravandi, Masoud, Sammons, Mawson W., Scholz, Paul, Smith, Kendrick, Stairs, Ingrid
The Canadian Hydrogen Intensity Mapping Experiment Fast Radio Burst (CHIME/FRB) project has discovered the most repeating fast radio burst (FRB) sources of any telescope. However, most of the physical conclusions derived from this sample are based on
Externí odkaz:
http://arxiv.org/abs/2411.02870
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:
Dong, Fengqiu Adam, Herrera-Martin, Antonio, Stairs, Ingrid, Craiu, Radu V., Crowter, Kathryn, Eadie, Gwendolyn M., Fonseca, Emmanuel, Good, Deborah, Mckee, James W., Meyers, Bradley W., Pearlman, Aaron B., Stenning, David C.
Studying transient phenomena, such as individual pulses from pulsars, has garnered considerable attention in the era of astronomical big data. Of specific interest to this study are Rotating Radio Transients (RRATs), nulling, and intermittent pulsars
Externí odkaz:
http://arxiv.org/abs/2406.04597
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:
Tan, Chia Min, Fonseca, Emmanuel, Crowter, Kathryn, Dong, Fengqiu Adam, Kaspi, Victoria M., Masui, Kiyoshi W., McKee, James W., Meyers, Bradley W., Ransom, Scott M., Stairs, Ingrid H.
We performed near-daily observations on the binary pulsars PSR J0218+4232, PSR J1518+4904 and PSR J2023+2853 with the Canadian Hydrogen Intensity Mapping Experiment (CHIME). For the first time, we detected the Shapiro time delay in all three pulsar-b
Externí odkaz:
http://arxiv.org/abs/2402.08188
Autor:
Lanman, Adam E., Andrew, Shion, Lazda, Mattias, Shah, Vishwangi, Amiri, Mandana, Balasubramanian, Arvind, Bandura, Kevin, Boyle, P. J., Brar, Charanjot, Carlson, Mark, Cliche, Jean-François, Gusinskaia, Nina, Hendricksen, Ian T., Kaczmarek, J. F., Landecker, Tom, Leung, Calvin, Mckinven, Ryan, Mena-Parra, Juan, Milutinovic, Nikola, Nimmo, Kenzie, Pearlman, Aaron B., Renard, Andre, Rahman, Mubdi, Shaw, J. Richard, Siegel, Seth R., Smegal, Rick J., Cassanelli, Tomas, Chatterjee, Shami, Curtin, Alice P., Dobbs, Matt, Dong, Fengqiu Adam, Halpern, Mark, Hopkins, Hans, Kaspi, Victoria M., Khairy, Kholoud, Masui, Kiyoshi W., Meyers, Bradley W., Michilli, Daniele, Petroff, Emily, Pinsonneault-Marotte, Tristan, Pleunis, Ziggy, Rafiei-Ravandi, Masoud, Shin, Kaitlyn, Smith, Kendrick, Vanderlinde, Keith, Zegmott, Tarik J.
Localizing fast radio bursts (FRBs) to their host galaxies is an essential step to better understanding their origins and using them as cosmic probes. The CHIME/FRB Outrigger program aims to add VLBI-localization capabilities to CHIME, such that FRBs
Externí odkaz:
http://arxiv.org/abs/2402.07898
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
Autor:
Pearlman, Aaron B., Scholz, Paul, Bethapudi, Suryarao, Hessels, Jason W. T., Kaspi, Victoria M., Kirsten, Franz, Nimmo, Kenzie, Spitler, Laura G., Fonseca, Emmanuel, Meyers, Bradley W., Stairs, Ingrid, Tan, Chia Min, Bhardwaj, Mohit, Chatterjee, Shami, Cook, Amanda M., Curtin, Alice P., Dong, Fengqiu Adam, Eftekhari, Tarraneh, Gaensler, B. M., Güver, Tolga, Kaczmarek, Jane, Leung, Calvin, Masui, Kiyoshi W., Michilli, Daniele, Prince, Thomas A., Sand, Ketan R., Shin, Kaitlyn, Smith, Kendrick M., Tendulkar, Shriharsh P.
Since fast radio bursts (FRBs) were discovered, their precise origins have remained a mystery. Multiwavelength observations of nearby FRB sources provide one of the best ways to make rapid progress in our understanding of the enigmatic FRB phenomenon
Externí odkaz:
http://arxiv.org/abs/2308.10930