Zobrazeno 1 - 3
of 3
pro vyhledávání: '"Pleunis, Ziggy"'
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:
Rafiei-Ravandi, Masoud, Smith, Kendrick M., Michilli, D., Pleunis, Ziggy, Bhardwaj, Mohit, Dobbs, Matt, Eadie, Gwendolyn M., Fonseca, Emmanuel, Gaensler, B. M., Kaczmarek, Jane, Kaspi, Victoria M., Leung, Calvin, Li, Dongzi, Masui, Kiyoshi W., Pandhi, Ayush, Pearlman, Aaron B., Petroff, Emily, Rahman, Mubdi, Scholz, Paul, Stenning, David C.
We present results from angular cross-correlations between select samples of CHIME/FRB repeaters and galaxies in three photometric galaxy surveys, which have shown correlations with the first CHIME/FRB catalog containing repeating and nonrepeating so
Externí odkaz:
http://arxiv.org/abs/2308.09608
Autor:
Cook, Amanda M., Bhardwaj, Mohit, Gaensler, B. M., Scholz, Paul, Eadie, Gwendolyn M., Hill, Alex S., Kaspi, Victoria M., Masui, Kiyoshi W., Curtin, Alice P., Dong, Fengqiu Adam, Fonseca, Emmanuel, Herrera-Martin, Antonio, Kaczmarek, Jane, Lanman, Adam E., Lazda, Mattias, Leung, Calvin, Meyers, Bradley W., Michilli, Daniele, Pandhi, Ayush, Pearlman, Aaron B., Pleunis, Ziggy, Ransom, Scott, Rahman, Mubdi, Sand, Ketan R., Shin, Kaitlyn, Smith, Kendrick, Stairs, Ingrid, Stenning, David C.
The CHIME/FRB project has detected hundreds of fast radio bursts (FRBs), providing an unparalleled population to probe statistically the foreground media that they illuminate. One such foreground medium is the ionized halo of the Milky Way (MW). We e
Externí odkaz:
http://arxiv.org/abs/2301.03502