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CALET Search for Electromagnetic Counterparts of Gravitational Waves During the LIGO/Virgo O3 Run

التفاصيل البيبلوغرافية
العنوان: CALET Search for Electromagnetic Counterparts of Gravitational Waves During the LIGO/Virgo O3 Run
المؤلفون: O Adriani, Y Akaike, K Asano, Y Asaoka, E Berti, G Bigongiari, W R Binns, M Bongi, P Brogi, A Bruno, J H Buckley, N Cannady, G Castellini, C Checchia, M L Cherry, G Collazuol, K Ebisawa, A W Ficklin, H Fuke, S Gonzi, T G Guzik, T Hams, K Hibino, M Ichimura, K Ioka, W Ishizak, M H Israel, K Kasahara, J Kataoka, R Kataoka, Y Katayose, C Kato, N Kawanaka, Y Kawakubo, K Kobayashi, K Kohri, H S Krawczynski, J F Krizmanic, P Maestro, P S Marrocches, A M Messineo, J W Mitchell, S Miyake, A A Moiseev, M Mori, N Mori, H M Motz, K Munakata, S Nakahira, J Nishimura, G A de Nolfo, S Okuno, J F Ormes, N Ospina, S Ozawa, L Pacini, P Papini, B F Rauch, S B Ricciarini, K Sakai, T Sakamoto, M Sasaki, Y Shimizu, A Shiomi, P Spillantini, F Stolzi, S Sugita, A Sulaj, M Takita, T Tamura, T Terasawa, S Torii, Y Tsunesada, Y Uchihori, E Vannuccini, J P Wefel, K Yamaoka, S Yanagita, A Yoshida, K Yoshida, W V Zober
المصدر: Astrophysical Journal. 933(1)
بيانات النشر: United States: NASA Center for Aerospace Information (CASI), 2022.
سنة النشر: 2022
مصطلحات موضوعية: Astronomy
الوصف: The CALorimetric Electron Telescope (CALET)on the International Space Station consists of a high-energy cosmic-ray CALorimeter (CAL)and a lower-energy CALET Gamma-ray Burst Monitor (CGBM). CAL is sensitive to electrons up to 20 TeV, cosmic-ray nuclei from Z=1 throughZ∼40, and gamma rays over the range1 GeV–10 TeV. CGBM observes gamma rays from 7 keV to 20 MeV. The combined CAL-CGBM instrument has conducted a search for gamma-ray bursts (GRBs)since 2015 October. We report here on the results of a search for X-ray/gamma-ray counterparts to gravitational-wave events reported during the LIGO/Virgo observing run O3. No events have been detected that pass all acceptance criteria. We describe the components, performance, and triggering algorithms of the CGBM—the two Hard X-ray Monitors consisting of LaBr3(Ce)scintillators sensitive to 7 keV–1 MeV gamma rays and a Soft Gamma-ray Monitor BGO scintillator sensitive to 40 keV–20 MeV—and the high-energy CAL consisting of a charge detection module, imaging calorimeter, and the fully active total absorption calorimeter. The analysis procedure is described and upper limits to the time-averaged fluxes are presented.
نوع الوثيقة: Report
اللغة: English
تدمد: 1538-4357
0004-637X
DOI: 10.3847/1538-4357/ac6f53
URL الوصول: https://ntrs.nasa.gov/citations/20230001723
ملاحظات: 80NSSC20K0397

80NSSC20K0399
رقم الأكسشن: edsnas.20230001723
قاعدة البيانات: NASA Technical Reports
الوصف
تدمد:15384357
0004637X
DOI:10.3847/1538-4357/ac6f53