Zobrazeno 1 - 2
of 2
pro vyhledávání: '"McGrath, C. E"'
Autor:
Adams, C. B., Batshoun, J., Farrell, K. A., Feng, Q., Finley, J. P., Foote, G. M., Fortson, L., Furniss, A., Gent, A., Giuri, Chiara, Hanna, D., Hassan Collado, Tarek, Benbow, W., Hervet, O., Holder, J., Houck, M., Humensky, T. B., Jin, W., Kaaret, P., Kertzman, M., Kieda, D., Krennrich, F., Kumar, S., Brill, A., Lundy, M., Maier, G., McGrath, C. E., Moriarty, P., Mukherjee, R., Nieto, D., Nievas Rosillo, Mireia, O'Brien, S., Ong, R. A., Oppenheimer, A., Buckley, J. H., Otte, A. N., Patel, S., Pfrang, Konstantin Johannes, Pohl, M., Prado, R. R., Pueschel, E., Quinn, J., Ragan, K., Reynolds, P. T., Rhatigan, A., Capasso, M., Ribeiro, D., Roache, E., Ryan, J. L., Santander, M., Sembroski, G. H., Williams, D. A., Williamson, T. J., Valverde, J., Horan, D., Buson, S., Cavins, B., Cheung, C. C., Ciprini, S., Gasparrini, D., Ojha, R., van Zyl, P., Sironi, L., VERITAS Collaboration, Fermi-LAT Collaboration, Christiansen, J. L., Coppi, P., Errando, M.
Publikováno v:
The astrophysical journal / 2 924(2), 95 (2022). doi:10.3847/1538-4357/ac32bd
The astrophysical journal 924(2), 95 (2022). doi:10.3847/1538-4357/ac32bd
Flat-spectrum radio quasars (FSRQs) are the most luminous blazars at GeV energies but only rarely emit detectable fluxes of TeV gamma rays, typically during bright GeV fla
Flat-spectrum radio quasars (FSRQs) are the most luminous blazars at GeV energies but only rarely emit detectable fluxes of TeV gamma rays, typically during bright GeV fla
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::7baa560f7eaa848b2b60ce7d7a6e6473
https://bib-pubdb1.desy.de/record/474567
https://bib-pubdb1.desy.de/record/474567
Autor:
Benbow, Wystan, Brill, A., Buckley, James, Capasso, M, Chromey, A, Errando, M., Falcone, Abraham, Farrell, K. A., Feng, Qi, Finley, J, Foote, G. M., Fortson, Lucy, Furniss, Amy, Gent, Alasdair, Giuri, C, Hanna, David, Hassan, Tarek, Hervet, Olivier, Holder, Jamie, Hughes, G, Humensky, T. B., Jin, Weidong, Kaaret, Philip, Kargaltsev, Oleg, Kertzman, Mary P., Kieda, David, Klingler, Noel, Kumar, Sajan, Lang, M, Lundy, M, Maier, Gernot, McGrath, C. E., Moriarty, Patrick, Mukherjee, Reshmi, Nieto, D, Nievas-Rosillo, M, O'Brien, S, Ong, Rene A., Otte, A. N., Patel, S., Pfrang, Konstantin, Pohl, Martin, Prado, Raul, Quinn, John, Ragan, Kenneth J., Reynolds, T., Ribeiro, D, Richards, G. T., Roache, Emmet Thomas, Ryan, James, Santander, Marcos, Sembroski, Glenn H, Shang, R, Volkov, Igor, Wakely, S. P, Weinstein, Amanda, Wilcox, P., Williams, D. A.
We report on the search for very-high-energy gamma-ray emission from the regions around three nearby supersonic pulsars (PSR B0355+54, PSR J0357+3205 and PSR J1740+1000) that exhibit long X-ray tails. To date there is no clear detection of TeV emissi
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::4447cecc30ebb07f5ebbf9339d0bb094