Zobrazeno 1 - 10
of 17 394
pro vyhledávání: '"Brar, A"'
Autor:
Sand, Ketan R., Curtin, Alice P., Michilli, Daniele, Kaspi, Victoria M., Fonseca, Emmanuel, Nimmo, Kenzie, Pleunis, Ziggy, Shin, Kaitlyn, Bhardwaj, Mohit, Brar, Charanjot, Dobbs, Matt, Eadie, Gwendolyn, Gaensler, B. M., Joseph, Ronniy C., Leung, Calvin, Main, Robert, Masui, Kiyoshi W., Mckinven, Ryan, Pandhi, Ayush, Pearlman, Aaron B., Rafiei-Ravandi, Masoud, Sammons, Mawson W., Smith, Kendrick, Stairs, Ingrid H.
We present a spectro-temporal analysis of 137 fast radio bursts (FRBs) from the first CHIME/FRB baseband catalog, including 125 one-off bursts and 12 repeat bursts, down to microsecond resolution using the least-squares optimization fitting routine:
Externí odkaz:
http://arxiv.org/abs/2408.13215
Autor:
Pant, Himanshu, Singh, Saurabh, Brar, Jaskirat, Sharma, Priyamedha, Bharath, M., Kuga, Kentaro, Takeuchi, Tsunehiro, Bindu, R.
We have studied the origin of zero volume expansion below the Curie temperature (Tc), variable range hopping (VRH) behaviour using structural, magnetic, transport and thermal studies on the oxygen deficient double perovskite NdBaCo_2O_{5+{\delta}} ({
Externí odkaz:
http://arxiv.org/abs/2408.02974
Traditional round-trip car rental systems mandate users to return vehicles to their point of origin, limiting the system adaptability to meet diverse mobility demands. This constraint often leads to fleet under-utilization and incurs high parking cos
Externí odkaz:
http://arxiv.org/abs/2407.08238
Domain probe lists--used to determine which URLs to probe for Web censorship--play a critical role in Internet censorship measurement studies. Indeed, the size and accuracy of the domain probe list limits the set of censored pages that can be detecte
Externí odkaz:
http://arxiv.org/abs/2407.08185
Autor:
Feng, Demeng, Kumar, Tanuj, Yin, Shenwei, Mah, Merlin, Lin, Phyo, Fortman, Margaret, Jaffe, Gabriel R., Wan, Chenghao, Mei, Hongyan, Xiao, Yuzhe, Synowicki, Ron, Warzoha, Ronald J., Brar, Victor W., Talghader, Joseph J., Kats, Mikhail A.
Laser-light sails are a spacecraft concept wherein lightweight "sails" are propelled to high speeds by lasers with high intensities. The sails must comprise materials with low optical loss, to minimize the risk of laser damage. Stoichiometric silicon
Externí odkaz:
http://arxiv.org/abs/2404.04449
Autor:
Leung, Calvin, Andrew, Shion, Masui, Kiyoshi W., Brar, Charanjot, Cassanelli, Tomas, Chatterjee, Shami, Kaspi, Victoria, Khairy, Kholoud, Lanman, Adam E., Lazda, Mattias, Mena-Parra, Juan, Noble, Gavin, Pearlman, Aaron B., Rahman, Mubdi, Sanghavi, Pranav, Shah, Vishwangi
One major goal in fast radio burst science is to detect fast radio bursts (FRBs) over a wide field of view without sacrificing the angular resolution required to pinpoint them to their host galaxies. Wide-field detection and localization capabilities
Externí odkaz:
http://arxiv.org/abs/2403.05631
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
Extensive research has been conducted to explore vehicle lane changes, while the study on cut-ins has not received sufficient attention. The existing studies have not addressed the fundamental question of why studying cut-ins is crucial, despite the
Externí odkaz:
http://arxiv.org/abs/2402.08289
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:
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