Zobrazeno 1 - 10
of 94
pro vyhledávání: '"Mckinven R"'
Autor:
Mckinven, R., Gaensler, B. M., Michilli, D., Masui, K., Kaspi, V. M., Su, J., Bhardwaj, M., Cassanelli, T., Chawla, P., Dong, Fonseca, E., Leung, C., Petroff, E., Pleunis, Z., Rafiei-Ravandi, M., Stairs, I. H., Tendulkar, S., Li, D. Z., Ng, C., Patel, C., Pearlman, A. B., Rahman, M., Sand, K. R., Shin, K.
Fast radio bursts (FRBs) display a confounding variety of burst properties and host galaxy associations. Repeating FRBs offer insight into the FRB population by enabling spectral, temporal and polarimetric properties to be tracked over time. Here, we
Externí odkaz:
http://arxiv.org/abs/2302.08386
Autor:
Mckinven, R., Gaensler, B. M., Michilli, D., Masui, K., Kaspi, V. M., Bhardwaj, M., Cassanelli, T., Chawla, P., Dong, F. Adam, Fonseca, E., Leung, C., Li, D. Z., Ng, C., Patel, C., Petroff, E., Pearlman, A. B., Pleunis, Z., Rafiei-Ravandi, M., Rahman, M., Sand, K. R., Shin, K., Scholz, P., Stairs, I. H., Smith, K., Su, J., Tendulkar, S.
Fast radio burst (FRB) source 20180916B exhibits a 16.33-day periodicity in its burst activity. It is as of yet unclear what proposed mechanism produces the activity, but polarization information is a key diagnostic. Here, we report on the polarizati
Externí odkaz:
http://arxiv.org/abs/2205.09221
Autor:
Josephy, A., Chawla, P., Curtin, A. P., Kaspi, V. M., Bhardwaj, M., Boyle, P. J., Brar, C., Cassanelli, T., Fonseca, E., Gaensler, B. M., Leung, C., Lin, H. -H., Masui, K. W., McKinven, R., Mena-Parra, J., Michilli, D., Ng, C., Pleunis, Z., Rafiei-Ravandi, M., Rahman, M., Sanghavi, P., Scholz, P., Smith, K. M., Stairs, I. H., Tendulkar, S. P., Zwaniga, A. V.
We investigate whether the sky rate of Fast Radio Bursts depends on Galactic latitude using the first catalog of Fast Radio Bursts (FRBs) detected by the Canadian Hydrogen Intensity Mapping Experiment Fast Radio Burst (CHIME/FRB) Project. We first se
Externí odkaz:
http://arxiv.org/abs/2106.04353
Autor:
Nimmo, K., Hessels, J. W. T., Kirsten, F., Keimpema, A., Cordes, J. M., Snelders, M. P., Hewitt, D. M., Karuppusamy, R., Archibald, A. M., Bezukovs, V., Bhardwaj, M., Blaauw, R., Buttaccio, S. T., Cassanelli, T., Conway, J. E., Corongiu, A., Feiler, R., Fonseca, E., Forssen, O., Gawronski, M., Giroletti, M., Kharinov, M. A., Leung, C., Lindqvist, M., Maccaferri, G., Marcote, B., Masui, K. W., Mckinven, R., Melnikov, A., Michilli, D., Mikhailov, A., Ng, C., Orbidans, A., Ould-Boukattine, O. S., Paragi, Z., Pearlman, A. B., Petroff, E., Rahman, M., Scholz, P., Shin, K., Smith, K. M., Stairs, I. H., Surcis, G., Tendulkar, S. P., Vlemmings, W., Wang, N., Yang, J., Yuan, J.
Fast radio bursts (FRBs) are extragalactic radio flashes of unknown physical origin. Their high luminosities and short durations require extreme energy densities, like those found in the vicinity of neutron stars and black holes. Studying the burst i
Externí odkaz:
http://arxiv.org/abs/2105.11446
Autor:
Kirsten, F., Marcote, B., Nimmo, K., Hessels, J. W. T., Bhardwaj, M., Tendulkar, S. P., Keimpema, A., Yang, J., Snelders, M. P., Scholz, P., Pearlman, A. B., Law, C. J., Peters, W. M., Giroletti, M., Paragi, Z., Bassa, C., Hewitt, D. M., Bach, U., Bezrukovs, V., Burgay, M., Buttaccio, S. T., Conway, J. E., Corongiu, A., Feiler, R., Forssén, O., Gawroński, M. P., Karuppusamy, R., Kharinov, M. A., Lindqvist, M., Maccaferri, G., Melnikov, A., Ould-Boukattine, O. S., Possenti, A., Surcis, G., Wang, N., Yuan, J., Aggarwal, K., Anna-Thomas, R., Bower, G. C., Blaauw, R., Burke-Spolaor, S., Cassanelli, T., Clarke, T. E., Fonseca, E., Gaensler, B. M., Gopinath, A., Kaspi, V. M., Kassim, N., Lazio, T. J. W., Leung, C., Li, D. Z., Lin, H. H., Masui, K. W., Mckinven, R., Michilli, D., Mikhailov, A., Ng, C., Orbidans, A., Pen, U. L., Petroff, E., Rahman, M., Ransom, S. M., Shin, K., Smith, K. M., Stairs, I. H., Vlemmings, W.
Fast radio bursts (FRBs) are exceptionally luminous flashes of unknown physical origin, reaching us from other galaxies (Petroff et al. 2019). Most FRBs have only ever been seen once, while others flash repeatedly, though sporadically (Spitler et al.
Externí odkaz:
http://arxiv.org/abs/2105.11445
Autor:
Bhardwaj, M., Gaensler, B. M., Kaspi, V. M., Landecker, T. L., Mckinven, R., Michilli, D., Pleunis, Z., Tendulkar, S. P., Andersen, B. C., Boyle, P. J., Cassanelli, T., Chawla, P., Cook, A., Dobbs, M., Fonseca, E., Kaczmarek, J., Leung, C., Masui, K., Münchmeyer, M., Ng, C., Rafiei-Ravandi, M., Scholz, P., Shin, K., Smith, K. M., Stairs, I. H., Zwaniga, A. V.
We report on the discovery of FRB 20200120E, a repeating fast radio burst (FRB) with low dispersion measure (DM), detected by the Canadian Hydrogen Intensity Mapping Experiment (CHIME)/FRB project. The source DM of 87.82 pc cm$^{-3}$ is the lowest re
Externí odkaz:
http://arxiv.org/abs/2103.01295
Autor:
Pleunis, Z., Michilli, D., Bassa, C. G., Hessels, J. W. T., Naidu, A., Andersen, B. C., Chawla, P., Fonseca, E., Gopinath, A., Kaspi, V. M., Kondratiev, V. I., Li, D. Z., Bhardwaj, M., Boyle, P. J., Brar, C., Cassanelli, T., Gupta, Y., Josephy, A., Karuppusamy, R., Keimpema, A., Kirsten, F., Leung, C., Marcote, B., Masui, K., Mckinven, R., Meyers, B. W., Ng, C., Nimmo, K., Paragi, Z., Rahman, M., Scholz, P., Shin, K., Smith, K. M., Stairs, I. H., Tendulkar, S. P.
FRB 20180916B is a well-studied repeating fast radio burst source. Its proximity (~150 Mpc), along with detailed studies of the bursts, have revealed many clues about its nature -- including a 16.3-day periodicity in its activity. Here we report on t
Externí odkaz:
http://arxiv.org/abs/2012.08372
Autor:
Michilli, D., Masui, K. W., Mckinven, R., Cubranic, D., Bruneault, M., Brar, C., Patel, C., Boyle, P. J., Stairs, I. H., Renard, A., Bandura, K., Berger, S., Breitman, D., Cassanelli, T., Dobbs, M., Kaspi, V. M., Leung, C., Mena-Parra, J., Pleunis, Z., Russell, L., Scholz, P., Siegel, S. R., Tendulkar, S. P., Vanderlinde, K.
The Canadian Hydrogen Intensity Mapping Experiment (CHIME) has become a leading facility for detecting fast radio bursts (FRBs) through the CHIME/FRB backend. CHIME/FRB searches for fast transients in polarization-summed intensity data streams that h
Externí odkaz:
http://arxiv.org/abs/2010.06748
Autor:
Hilmarsson, G. H., Michilli, D., Spitler, L. G., Wharton, R. S., Demorest, P., Desvignes, G., Gourdji, K., Hackstein, S., Hessels, J. W. T., Nimmo, K., Seymour, A. D., Kramer, M., McKinven, R.
The repeating fast radio burst source FRB 121102 has been shown to have an exceptionally high and variable Faraday rotation measure (RM), which must be imparted within its host galaxy and likely by or within its local environment. In the redshifted (
Externí odkaz:
http://arxiv.org/abs/2009.12135
Autor:
Law, C. J., Butler, B. J., Prochaska, J. X., Zackay, B., Burke-Spolaor, S., Mannings, A., Tejos, N., Josephy, A., Andersen, B., Chawla, P., Heintz, K. E., Aggarwal, K., Bower, G. C., Demorest, P. B., Kilpatrick, C. D., Lazio, T. J. W., Linford, J., Mckinven, R., Tendulkar, S., Simha, S.
We present the discovery and subarcsecond localization of a new Fast Radio Burst with the Karl G. Jansky Very Large Array and realfast search system. The FRB was discovered on 2019 June 14 with a dispersion measure of 959 pc/cm3. This is the highest
Externí odkaz:
http://arxiv.org/abs/2007.02155