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

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. Ishizaki; 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. Marrocchesi; 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

doi:10.3847/1538-4357/ac6f53

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

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. GonziT. G. Guzik, T. Hams, K. Hibino, M. Ichimura, K. Ioka, W. Ishizaki, 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. Marrocchesi, 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

研究成果: Article › 査読

1 被引用数 (Scopus)

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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 through Z ∼40, and gamma rays over the range 1 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.

本文言語	English
論文番号	85
ジャーナル	Astrophysical Journal
巻	933
号	1
DOI	https://doi.org/10.3847/1538-4357/ac6f53
出版ステータス	Published - 2022 7月 1

ASJC Scopus subject areas

天文学と天体物理学
宇宙惑星科学

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10.3847/1538-4357/ac6f53

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Adriani, O., Akaike, Y., Asano, K., Asaoka, Y., Berti, E., Bigongiari, G., Binns, W. R., Bongi, M., Brogi, P., Bruno, A., Buckley, J. H., Cannady, N., Castellini, G., Checchia, C., Cherry, M. L., Collazuol, G., Ebisawa, K., Ficklin, A. W., Fuke, H., ... Zober, W. V. (2022). CALET Search for Electromagnetic Counterparts of Gravitational Waves during the LIGO/Virgo O3 Run. Astrophysical Journal, 933(1), [85]. https://doi.org/10.3847/1538-4357/ac6f53

Adriani, O, Akaike, Y, Asano, K, Asaoka, Y, Berti, E, Bigongiari, G, Binns, WR, Bongi, M, Brogi, P, Bruno, A, Buckley, JH, Cannady, N, Castellini, G, Checchia, C, Cherry, ML, Collazuol, G, Ebisawa, K, Ficklin, AW, Fuke, H, Gonzi, S, Guzik, TG, Hams, T, Hibino, K, Ichimura, M, Ioka, K, Ishizaki, W, Israel, MH, Kasahara, K, Kataoka, J, Kataoka, R, Katayose, Y, Kato, C, Kawanaka, N, Kawakubo, Y, Kobayashi, K, Kohri, K, Krawczynski, HS, Krizmanic, JF, Maestro, P, Marrocchesi, PS, Messineo, AM, Mitchell, JW, Miyake, S, Moiseev, AA, Mori, M, Mori, N, Motz, HM, Munakata, K, Nakahira, S, Nishimura, J, Nolfo, GAD, Okuno, S, Ormes, JF, Ospina, N, Ozawa, S, Pacini, L, Papini, P, Rauch, BF, Ricciarini, SB, Sakai, K, Sakamoto, T, Sasaki, M, Shimizu, Y, Shiomi, A, Spillantini, P, Stolzi, F, Sugita, S, Sulaj, A, Takita, M, Tamura, T, Terasawa, T, Torii, S, Tsunesada, Y, Uchihori, Y, Vannuccini, E, Wefel, JP, Yamaoka, K, Yanagita, S, Yoshida, A, Yoshida, K & Zober, WV 2022, 'CALET Search for Electromagnetic Counterparts of Gravitational Waves during the LIGO/Virgo O3 Run', Astrophysical Journal, vol. 933, no. 1, 85. https://doi.org/10.3847/1538-4357/ac6f53

@article{0b8ecbce890d4d2cb16f74adf432548b,

title = "CALET Search for Electromagnetic Counterparts of Gravitational Waves during the LIGO/Virgo O3 Run",

abstract = "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 through Z ∼40, and gamma rays over the range 1 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.",

author = "O. Adriani and Y. Akaike and K. Asano and Y. Asaoka and E. Berti and G. Bigongiari and Binns, {W. R.} and M. Bongi and P. Brogi and A. Bruno and Buckley, {J. H.} and N. Cannady and G. Castellini and C. Checchia and Cherry, {M. L.} and G. Collazuol and K. Ebisawa and Ficklin, {A. W.} and H. Fuke and S. Gonzi and Guzik, {T. G.} and T. Hams and K. Hibino and M. Ichimura and K. Ioka and W. Ishizaki and Israel, {M. H.} and K. Kasahara and J. Kataoka and R. Kataoka and Y. Katayose and C. Kato and N. Kawanaka and Y. Kawakubo and K. Kobayashi and K. Kohri and Krawczynski, {H. S.} and Krizmanic, {J. F.} and P. Maestro and Marrocchesi, {P. S.} and Messineo, {A. M.} and Mitchell, {J. W.} and S. Miyake and Moiseev, {A. A.} and M. Mori and N. Mori and Motz, {H. M.} and K. Munakata and S. Nakahira and J. Nishimura and Nolfo, {G. A.De} and S. Okuno and Ormes, {J. F.} and N. Ospina and S. Ozawa and L. Pacini and P. Papini and Rauch, {B. F.} and Ricciarini, {S. B.} and K. Sakai and T. Sakamoto and M. Sasaki and Y. Shimizu and A. Shiomi and P. Spillantini and F. Stolzi and S. Sugita and A. Sulaj and M. Takita and T. Tamura and T. Terasawa and S. Torii and Y. Tsunesada and Y. Uchihori and E. Vannuccini and Wefel, {J. P.} and K. Yamaoka and S. Yanagita and A. Yoshida and K. Yoshida and Zober, {W. V.}",

note = "Funding Information: CALET is currently approved to continue operating through 2024. We gratefully acknowledge JAXA's contributions to the development of CALET and to the operations aboard the JEM-EF on the International Space Station. We also wish to express our sincere gratitude to Agenzia Spaziale Italiana (ASI) and NASA for their support of the CALET project. In Japan, this work was supported in part by JSPS KAKENHI grant Nos. 26220708, 19H05608, 17H02901, 21K03592, and 20K22352 and by the MEXT-Supported Program for the Strategic Research Foundation at Private Universities (2011–2015) (No.S1101021) at Waseda University. The CALET effort in Italy is supported by ASI under agreement 2013-018-R.0 and its amendments. The CALET effort in the United States is supported by NASA through Grants 80NSSC20K0397, 80NSSC20K0399, and NNH18ZDA001N-APRA18-000. A part of this research is made possible by use of data obtained from DARTS at ISAS/JAXA. Publisher Copyright: {\textcopyright} 2022. The Author(s). Published by the American Astronomical Society.",

year = "2022",

month = jul,

day = "1",

doi = "10.3847/1538-4357/ac6f53",

language = "English",

volume = "933",

journal = "Astrophysical Journal",

issn = "0004-637X",

publisher = "IOP Publishing Ltd.",

number = "1",

}

TY - JOUR

T1 - CALET Search for Electromagnetic Counterparts of Gravitational Waves during the LIGO/Virgo O3 Run

AU - Adriani, O.

AU - Akaike, Y.

AU - Asano, K.

AU - Asaoka, Y.

AU - Berti, E.

AU - Bigongiari, G.

AU - Binns, W. R.

AU - Bongi, M.

AU - Brogi, P.

AU - Bruno, A.

AU - Buckley, J. H.

AU - Cannady, N.

AU - Castellini, G.

AU - Checchia, C.

AU - Cherry, M. L.

AU - Collazuol, G.

AU - Ebisawa, K.

AU - Ficklin, A. W.

AU - Fuke, H.

AU - Gonzi, S.

AU - Guzik, T. G.

AU - Hams, T.

AU - Hibino, K.

AU - Ichimura, M.

AU - Ioka, K.

AU - Ishizaki, W.

AU - Israel, M. H.

AU - Kasahara, K.

AU - Kataoka, J.

AU - Kataoka, R.

AU - Katayose, Y.

AU - Kato, C.

AU - Kawanaka, N.

AU - Kawakubo, Y.

AU - Kobayashi, K.

AU - Kohri, K.

AU - Krawczynski, H. S.

AU - Krizmanic, J. F.

AU - Maestro, P.

AU - Marrocchesi, P. S.

AU - Messineo, A. M.

AU - Mitchell, J. W.

AU - Miyake, S.

AU - Moiseev, A. A.

AU - Mori, M.

AU - Mori, N.

AU - Motz, H. M.

AU - Munakata, K.

AU - Nakahira, S.

AU - Nishimura, J.

AU - Nolfo, G. A.De

AU - Okuno, S.

AU - Ormes, J. F.

AU - Ospina, N.

AU - Ozawa, S.

AU - Pacini, L.

AU - Papini, P.

AU - Rauch, B. F.

AU - Ricciarini, S. B.

AU - Sakai, K.

AU - Sakamoto, T.

AU - Sasaki, M.

AU - Shimizu, Y.

AU - Shiomi, A.

AU - Spillantini, P.

AU - Stolzi, F.

AU - Sugita, S.

AU - Sulaj, A.

AU - Takita, M.

AU - Tamura, T.

AU - Terasawa, T.

AU - Torii, S.

AU - Tsunesada, Y.

AU - Uchihori, Y.

AU - Vannuccini, E.

AU - Wefel, J. P.

AU - Yamaoka, K.

AU - Yanagita, S.

AU - Yoshida, A.

AU - Yoshida, K.

AU - Zober, W. V.

N1 - Funding Information: CALET is currently approved to continue operating through 2024. We gratefully acknowledge JAXA's contributions to the development of CALET and to the operations aboard the JEM-EF on the International Space Station. We also wish to express our sincere gratitude to Agenzia Spaziale Italiana (ASI) and NASA for their support of the CALET project. In Japan, this work was supported in part by JSPS KAKENHI grant Nos. 26220708, 19H05608, 17H02901, 21K03592, and 20K22352 and by the MEXT-Supported Program for the Strategic Research Foundation at Private Universities (2011–2015) (No.S1101021) at Waseda University. The CALET effort in Italy is supported by ASI under agreement 2013-018-R.0 and its amendments. The CALET effort in the United States is supported by NASA through Grants 80NSSC20K0397, 80NSSC20K0399, and NNH18ZDA001N-APRA18-000. A part of this research is made possible by use of data obtained from DARTS at ISAS/JAXA. Publisher Copyright: © 2022. The Author(s). Published by the American Astronomical Society.

PY - 2022/7/1

Y1 - 2022/7/1

N2 - 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 through Z ∼40, and gamma rays over the range 1 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.

AB - 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 through Z ∼40, and gamma rays over the range 1 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.

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U2 - 10.3847/1538-4357/ac6f53

DO - 10.3847/1538-4357/ac6f53

M3 - Article

AN - SCOPUS:85134844723

SN - 0004-637X

VL - 933

JO - Astrophysical Journal

JF - Astrophysical Journal

IS - 1

M1 - 85

ER -

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

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