2025/05/12 更新

お知らせ

 

写真a

イナダ　トモヒロ
稲田 知大
INADA TOMOHIRO
所属
先端素粒子物理研究センター 助教
職名
助教
外部リンク

学位

  • 博士(理学) （ 2020年3月 東京大学 ）

  • 修士(理学) （ 2017年3月 東京大学 ）

経歴

  • 欧州原子核研究機構  学術研究員 

    2023年11月 - 2024年11月

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    国名：スイス連邦

  • 清華大学  学術研究員 

    2021年9月 - 2023年10月

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    国名：中華人民共和国

  • 東京大学  学術研究員 

    2020年4月 - 2021年8月

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    国名：日本国

研究テーマ・研究キーワード

  • 研究テーマ： 素粒子物理学

    研究キーワード： ダークマター、加速器、シリコン検出器

    研究期間： 2015年4月 - 現在

受賞

  • 第19回 (2025年) 日本物理学会若手奨励賞

    2024年10月   日本物理学会  

    稲田知大

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    受賞区分：国内外の国際的学術賞  受賞国：日本国

  • 最優秀博士研究員入選

    2024年7月   清華大学  

    Tomohiro Inada

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    受賞区分：国内外の国際的学術賞  受賞国：中華人民共和国

  • 第24回 高エネルギー物理学奨励賞

    2022年10月   高エネルギー研究者会議  

    稲田知大

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    受賞区分：国内外の国際的学術賞  受賞国：日本国

  • 日本物理学会学生優秀発表賞

    2019年3月   日本物理学会  

    稲田知大

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    受賞区分：国内学会・会議・シンポジウム等の賞 

  • Award for outstanding contributions of poster presentation

    2018年8月   The Ettore Majorana Centre  

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    受賞区分：国際学会・会議・シンポジウム等の賞  受賞国：イタリア共和国

論文

  • Shining light on the dark sector: search for axion-like particles and other new physics in photonic final states with FASER

    Abraham R.M., Ai X., Anders J., Antel C., Ariga A., Ariga T., Atkinson J., Bernlochner F.U., Bianchi E., Boeckh T., Boyd J., Brenner L., Burger A., Cadoux F., Cardella R., Casper D.W., Cavanagh C., Chen X., Cho E., Chouhan D., Coccaro A., Débieux S., D’Onofrio M., Desai A., Dmitrievsky S., Dobre R., Eley S., Favre Y., Fellers D., Feng J.L., Fenoglio C.A., Ferrere D., Fieg M., Filali W., Firu E., Galantay E., Garabaglu A., Gibson S., Gonzalez-Sevilla S., Gornushkin Y., Gwilliam C., Hayakawa D., Holzbock M., Hsu S.C., Hu Z., Iacobucci G., Inada T., Iodice L., Jakobsen S., Joos H., Kajomovitz E., Kawahara H., Keyken A., Kling F., Köck D., Kontaxakis P., Kose U., Kotitsa R., Kuehn S., Kugathasan T., Levinson L., Li K., Liu J., Liu Y., Lutz M.S., MacDonald J., Magliocca C., Mäkelä T., McCoy L., McFayden J., Medina A.P., Milanesio M., Moretti T., Nakamura M., Nakano T., Nevay L., Ohashi K., Otono H., Paolozzi L., Petersen B., Preda T., Prim M., Queitsch-Maitland M., Rokujo H., Rubbia A., Sabater-Iglesias J., Sato O., Scampoli P., Schmieden K., Schott M., Sfyrla A., Sgalaberna D., Shamim M., Shively S., Takubo Y., Tarannum N., Theiner O., Torrence E., Valdes Martinez O.I., Vasina S.

    Journal of High Energy Physics   2025 ( 1 )   2025年1月   （ eISSN:1029-8479 ）

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    掲載種別：研究論文（学術雑誌）   出版者・発行元：Journal of High Energy Physics  

    The first FASER search for a light, long-lived particle decaying into a pair of photons is reported. The search uses LHC proton-proton collision data at s = 13.6 TeV collected in 2022 and 2023, corresponding to an integrated luminosity of 57.7 fb−1. A model with axion-like particles (ALPs) dominantly coupled to weak gauge bosons is the primary target. Signal events are characterised by high-energy deposits in the electromagnetic calorimeter and no signal in the veto scintillators. One event is observed, compared to a background expectation of 0.44 ± 0.39 events, which is entirely dominated by neutrino interactions. World-leading constraints on ALPs are obtained for masses up to 300 MeV and couplings to the Standard Model W gauge boson, gaWW, around 10−4 GeV−1, testing a previously unexplored region of parameter space. Other new particle models that lead to the same experimental signature, including ALPs coupled to gluons or photons, U(1)B gauge bosons, up-philic scalars, and a Type-I two-Higgs doublet model, are also considered for interpretation, and new constraints on previously viable parameter space are presented in this paper.

    DOI： 10.1007/jhep01(2025)199

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    その他リンク： https://link.springer.com/article/10.1007/JHEP01(2025)199/fulltext.html

  • Prospects for γ-ray observations of the Perseus galaxy cluster with the Cherenkov Telescope Array

    Abe, K. and others

    JCAP   10   004 - 004   2024年10月

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    掲載種別：研究論文（学術雑誌）  

    DOI： 10.1088/1475-7516/2024/10/004

    arXiv

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  • Early performance of the tracking detector for the FASER experiment 査読

    Tomohiro Inada

    Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment   1034   166825 - 166825   2024年8月   （ ISSN:0168-9002 ）

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    担当区分：筆頭著者,　責任著者   記述言語：英語   掲載種別：研究論文（学術雑誌）   出版者・発行元：Elsevier {BV}  

    DOI： 10.1016/j.nima.2024.169547

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  • Dark matter line searches with the Cherenkov Telescope Array

    Abe, S. and others

    JCAP   07   047 - 047   2024年7月

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    掲載種別：研究論文（学術雑誌）  

    DOI： 10.1088/1475-7516/2024/07/047

    arXiv

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  • First Measurement of the ν<sub>e</sub> and ν<sub>μ</sub> Interaction Cross Sections at the LHC with FASER's Emulsion Detector 査読 国際共著

    Abraham, RM; Anders, J; Antel, C; Ariga, A; Ariga, T; Atkinson, J; Bernlochner, FU; Boeckh, T; Boyd, J; Brenner, L; Burger, A; Cadoux, F; Cardella, R; Casper, DW; Cavanagh, C; Chen, X; Coccaro, A; Debieux, S; D'Onofrio, M; Desai, A; Dmitrievsky, S; Eley, S; Favre, Y; Fellers, D; Feng, JL; Fenoglio, CA; Ferrere, D; Fieg, M; Filali, W; Fujimori, H; Garabaglu, A; Gibson, S; Gonzalez-Sevilla, S; Gornushkin, Y; Gwilliam, C; Hayakawa, D; Hsu, SC; Hu, Z; Iacobucci, G; Inada, T; Iodice, L; Jakobsen, S; Joos, H; Kajomovitz, E; Kanai, T; Kawahara, H; Keyken, A; Kling, F; Koeck, D; Kontaxakis, P; Kose, U; Kotitsa, R; Kuehn, S; Kugathasan, T; Lefebvre, H; Levinson, L; Li, K; Liu, JF; Lutz, MS; Macdonald, J; Magliocca, C; Martinelli, F; Mccoy, L; Mcfayden, J; Medina, AP; Milanesio, M; Moretti, T; Munker, M; Nakamura, M; Nakano, T; Neuhaus, F; Nevay, L; Nonaka, M; Okui, K; Ohashi, K; Otono, H; Pang, H; Paolozzi, L; Petersen, B; Prim, M; Queitsch-Maitland, M; Rokujo, H; Ruiz-Choliz, E; Rubbia, A; Sabater-Iglesias, J; Sato, O; Scampoli, P; Schmieden, K; Schott, M; Sfyrla, A; Shamim, M; Shively, S; Takubo, Y; Tarannum, N; Theiner, O; Torrence, E; Vasina, S; Vormwald, B; Wang, D; Wang, YX; Welch, E; Zahorec, S; Zambito, S; Zhang, SL; FASER Collaboration

    PHYSICAL REVIEW LETTERS   133 ( 2 )   021802   2024年7月   （ ISSN:0031-9007 eISSN:1079-7114 ）

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    記述言語：英語   掲載種別：研究論文（学術雑誌）   出版者・発行元：Physical Review Letters  

    The first results of the study of high-energy electron neutrino (νe) and muon neutrino (νμ) charged-current interactions in the FASERν emulsion-tungsten detector of the FASER experiment at the LHC are presented. A 128.8 kg subset of the FASERν volume was analyzed after exposure to 9.5 fb-1 of s=13.6 TeV pp data. Four (eight) νe (νμ) interaction candidate events are observed with a statistical significance of 5.2σ (5.7σ). This is the first direct observation of νe interactions at a particle collider and includes the highest-energy νe and νμ ever detected from an artificial source. The interaction cross section per nucleon σ/Eν is measured over an energy range of 560-1740 GeV (520-1760 GeV) for νe (νμ) to be (1.2-0.7+0.8)×10-38 cm2 GeV-1 [(0.5±0.2)×10-38 cm2 GeV-1], consistent with standard model predictions. These are the first measurements of neutrino interaction cross sections in those energy ranges.

    DOI： 10.1103/PhysRevLett.133.021802

    Web of Science

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    その他リンク： http://harvest.aps.org/v2/journals/articles/10.1103/PhysRevLett.133.021802/fulltext

  • Neutrino rate predictions for FASER 査読 国際共著

    Abraham R.M., Anders J., Antel C., Ariga A., Ariga T., Atkinson J., Bernlochner F.U., Boeckh T., Boyd J., Brenner L., Burger A., Cadoux F., Cardella R., Casper D.W., Cavanagh C., Chen X., Coccaro A., Débieux S., D'Onofrio M., Desai A., Dmitrievsky S., Eley S., Favre Y., Fellers D., Feng J.L., Fenoglio C.A., Ferrere D., Fieg M., Filali W., Gibson S., Gonzalez-Sevilla S., Gornushkin Y., Gwilliam C., Hayakawa D., Hsu S.C., Hu Z., Iacobucci G., Inada T., Iodice L., Jakobsen S., Joos H., Kajomovitz E., Kawahara H., Keyken A., Kling F., Köck D., Kontaxakis P., Kose U., Kotitsa R., Kuehn S., Kugathasan T., Lefebvre H., Levinson L., Li K., Liu J., Lutz M.S., Macdonald J., Magliocca C., Martinelli F., McCoy L., McFayden J., Medina A.P., Milanesio M., Moretti T., Munker M., Nakamura M., Nakano T., Neuhaus F., Nevay L., Ohashi K., Otono H., Pang H., Paolozzi L., Petersen B., Prim M., Queitsch-Maitland M., Rokujo H., Ruiz-Choliz E., Rubbia A., Sabater-Iglesias J., Sato O., Scampoli P., Schmieden K., Schott M., Sfyrla A., Shamim M., Shively S., Takubo Y., Tarannum N., Theiner O., Torrence E., Vasina S., Vormwald B., Wang D., Wang Y., Welch E., Zahorec S., Zambito S., Zhang S.

    Physical Review D   110 ( 1 )   012009 - 012009   2024年7月   （ ISSN:24700010 eISSN:2470-0029 ）

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    掲載種別：研究論文（学術雑誌）   出版者・発行元：Physical Review D  

    The Forward Search Experiment (FASER) at CERN's Large Hadron Collider (LHC) has recently directly detected the first collider neutrinos. Neutrinos play an important role in all FASER analyses, either as signal or background, and it is therefore essential to understand the neutrino event rates. In this study, we update previous simulations and present prescriptions for theoretical predictions of neutrino fluxes and cross sections, together with their associated uncertainties. With these results, we discuss the potential for possible measurements that could be carried out in the coming years with the FASER neutrino data to be collected in LHC Run 3 and Run 4.

    DOI： 10.1103/PhysRevD.110.012009

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  • The FASER detector 査読 国際共著

    Abreu H., Mansour E.A., Antel C., Ariga A., Ariga T., Bernlochner F., Boeckh T., Boyd J., Brenner L., Cadoux F., Casper D.W., Cavanagh C., Chen X., Coccaro A., Crespo-Lopez O., Débieux S., Dmitrievsky S., D'Onofrio M., Dougherty L., Dozen C., Ezzat A., Favre Y., Fellers D., Feng J.L., Ferrere D., Galantay E.K., Gall J., Gamberini E., Gibson S., Gonzalez-Sevilla S., Gornushkin Y., Gwilliam C., Hayakawa D., Hsu S.C., Hu Z., Iacobucci G., Inada T., Jakobsen S., Johnson E., Kajomovitz E., Kawahara H., Kling F., Kose U., Kotitsa R., Krusse J., Kuehn S., Lefebvre H., Levinson L., Li K., Liu J., Magliocca C., Martinelli F., McFayden J., Meehan S., Milanesio M., Miura M., Mladenov D., Moretti T., Munker M., Nakamura M., Nakano T., Nessi M., Neuhaus F., Nevay L., Osborne J., Otono H., Pandini C., Pang H., Paolozzi L., Petersen B., Pietropaolo F., Prim M., Queitsch-Maitland M., Resnati F., Rizzi C., Rokujo H., Ruiz-Choliz E., Salfeld-Nebgen J., Galan F.S., Sato O., Scampoli P., Schmieden K., Schott M., Sfyrla A., Shively S., Sipos R., Spencer J., Takubo Y., Tarannum N., Theiner O., Thonet P., Torrence E., Tufanli S., Vasina S., Vendeuvre C., Vormwald B., Wang D., Zambito S., Zhang G.

    Journal of Instrumentation   19 ( 5 )   2024年5月

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    掲載種別：研究論文（学術雑誌）   出版者・発行元：Journal of Instrumentation  

    FASER, the ForwArd Search ExpeRiment, is an experiment dedicated to searching for light, extremely weakly-interacting particles at CERN's Large Hadron Collider (LHC). Such particles may be produced in the very forward direction of the LHC's high-energy collisions and then decay to visible particles inside the FASER detector, which is placed 480 m downstream of the ATLAS interaction point, aligned with the beam collisions axis. FASER also includes a sub-detector, FASERν, designed to detect neutrinos produced in the LHC collisions and to study their properties. In this paper, each component of the FASER detector is described in detail, as well as the installation of the experiment system and its commissioning using cosmic-rays collected in September 2021 and during the LHC pilot beam test carried out in October 2021. FASER has successfully started taking LHC collision data in 2022, and will run throughout LHC Run 3.

    DOI： 10.1088/1748-0221/19/05/P05066

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  • The variability patterns of the TeV blazar PG 1553 + 113 from a decade of MAGIC and multiband observations

    H. Abe, S. Abe, J. Abhir, V. A. Acciari, I. Agudo, T. Aniello, S. Ansoldi, L. A. Antonelli, A. Arbet Engels, C. Arcaro, M. Artero, K. Asano, D. Baack, A. Babić, A. Baquero, U. Barres de Almeida, I. Batković, J. Baxter, J. Becerra González, E. Bernardini, J. Bernete, A. Berti, J. Besenrieder, C. Bigongiari, A. Biland, O. Blanch, G. Bonnoli, Bošnjak, I. Burelli, G. Busetto, A. Campoy-Ordaz, A. Carosi, R. Carosi, M. Carretero-Castrillo, A. J. Castro-Tirado, Y. Chai, A. Cifuentes, S. Cikota, E. Colombo, J. L. Contreras, J. Cortina, S. Covino, G. D’Amico, V. D’Elia, P. Da Vela, F. Dazzi, A. De Angelis, B. De Lotto, A. Del Popolo, M. Delfino, J. Delgado, C. Delgado Mendez, D. Depaoli, F. Di Pierro, L. Di Venere, D. Dominis Prester, A. Donini, D. Dorner, M. Doro, D. Elsaesser, G. Emery, J. Escudero, L. Fariña, A. Fattorini, L. Foffano, L. Font, S. Fukami, Y. Fukazawa, R. J. García López, S. Gasparyan, M. Gaug, J. G. Giesbrecht Paiva, N. Giglietto, F. Giordano, P. Gliwny, R. Grau, J. G. Green, D. Hadasch, A. Hahn, L. Heckmann, J. Herrera, T. Hovatta, D. Hrupec, M. Hütten, R. Imazawa, T. Inada, R. Iotov, K. Ishio, I. Jimenez Martínez, J. Jormanainen, D. Kerszberg, G. W. Kluge, Y. Kobayashi, P. M. Kouch, H. Kubo, J. Kushida, M. Láinez Lezáun, A. Lamastra, F. Leone, E. Lindfors

    Monthly Notices of the Royal Astronomical Society   529 ( 4 )   3894 - 3911   2024年4月   （ ISSN:0035-8711 eISSN:1365-2966 ）

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    掲載種別：研究論文（学術雑誌）  

    PG 1553 + 113 is one of the few blazars with a convincing quasi-periodic emission in the gamma-ray band. The source is also a very high energy (VHE; >100 GeV) gamma-ray emitter. To better understand its properties and identify the underlying physical processes driving its variability, the MAGIC Collaboration initiated a multiyear, multiwavelength monitoring campaign in 2015 involving the OVRO 40-m and Medicina radio telescopes, REM, KVA, and the MAGIC telescopes, Swift and Fermi satellites, and the WEBT network. The analysis presented in this paper uses data until 2017 and focuses on the characterization of the variability. The gamma-ray data show a (hint of a) periodic signal compatible with literature, but the X-ray and VHE gamma-ray data do not show statistical evidence for a periodic signal. In other bands, the data are compatible with the gamma-ray period, but with a relatively high p-value. The complex connection between the low- and high-energy emission and the non-monochromatic modulation and changes in flux suggests that a simple one-zone model is unable to explain all the variability. Instead, a model including a periodic component along with multiple emission zones is required.

    DOI： 10.1093/mnras/stae649

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  • First characterization of the emission behavior of Mrk 421 from radio to very high-energy gamma rays with simultaneous X-ray polarization measurements

    Abe, S. and others

    Astron.Astrophys.   684   A127   2024年4月

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    掲載種別：研究論文（学術雑誌）  

    DOI： 10.1051/0004-6361/202347988

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  • Multi-year characterisation of the broad-band emission from the intermittent extreme BL Lac 1ES 2344+514

    H. Abe, S. Abe, V. A. Acciari, I. Agudo, T. Aniello, S. Ansoldi, L. A. Antonelli, A. Arbet Engels, C. Arcaro, M. Artero, K. Asano, D. Baack, A. Babić, A. Baquero, U. Barres De Almeida, I. Batković, J. Baxter, J. Becerra González, E. Bernardini, J. Bernete, A. Berti, J. Besenrieder, C. Bigongiari, A. Biland, O. Blanch, G. Bonnoli, Bošnjak, I. Burelli, G. Busetto, A. Campoy-Ordaz, A. Carosi, R. Carosi, M. Carretero-Castrillo, A. J. Castro-Tirado, Y. Chai, A. Cifuentes, S. Cikota, E. Colombo, J. L. Contreras, J. Cortina, S. Covino, G. D'Amico, F. D'Ammando, V. D'Elia, P. Da Vela, F. Dazzi, A. De Angelis, B. De Lotto, A. Del Popolo, M. Delfino, J. Delgado, C. Delgado Mendez, D. Depaoli, F. Di Pierro, L. Di Venere, D. Dominis Prester, D. Dorner, M. Doro, D. Elsaesser, G. Emery, J. Escudero, L. Fariña, A. Fattorini, L. Foffano, L. Font, S. Fukami, Y. Fukazawa, R. J. García López, S. Gasparyan, M. Gaug, J. G. Giesbrecht Paiva, N. Giglietto, F. Giordano, P. Gliwny, R. Grau, J. G. Green, D. Hadasch, A. Hahn, L. Heckmann, J. Herrera, D. Hrupec, M. Hütten, R. Imazawa, T. Inada, R. Iotov, K. Ishio, I. Jiménez Martínez, J. Jormanainen, D. Kerszberg, G. W. Kluge, Y. Kobayashi, P. M. Kouch, H. Kubo, J. Kushida, M. Láinez Lezáun, A. Lamastra, F. Leone, E. Lindfors, L. Linhoff, S. Lombardi

    Astronomy and Astrophysics   682   2024年2月   （ ISSN:0004-6361 eISSN:1432-0746 ）

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    掲載種別：研究論文（学術雑誌）  

    Aims. The BL Lac 1ES 2344+514 is known for temporary extreme properties characterised by a shift of the synchrotron spectral energy distribution (SED) peak energy νsynch;p above 1 keV. While those extreme states have only been observed during high flux levels thus far, additional multi-year observing campaigns are required to achieve a coherent picture. Here, we report the longest investigation of the source from radio to very high energy (VHE) performed so far, focussing on a systematic characterisation of the intermittent extreme states. Methods.We organised a monitoring campaign covering a 3-year period from 2019 to 2021.Morethan ten instruments participated in the observations in order to cover the emission from radio to VHE. In particular, sensitive X-ray measurements by XMM-Newton, NuSTAR, and AstroSat took place simultaneously with multi-hour MAGIC observations, providing an unprecedented constraint of the two SED components for this blazar. Results. While our results confirm that 1ES 2344+514 typically exhibits νsynch;p > 1 keV during elevated flux periods, we also find periods where the extreme state coincides with low flux activity. A strong spectral variability thus happens in the quiescent state, and is likely caused by an increase in the electron acceleration efficiency without a change in the electron injection luminosity. On the other hand, we also report a strong X-ray flare (among the brightest for 1ES 2344+514) without a significant shift of νsynch;p. During this particular flare, the X-ray spectrum is among the softest of the campaign. It unveils complexity in the spectral evolution, where the common harder-when-brighter trend observed in BL Lacs is violated. By combining Swift-XRT and Swift-UVOT measurements during a low and hard X-ray state, we find an excess of the UV flux with respect to an extrapolation of the X-ray spectrum to lower energies. This UV excess implies that at least two regions significantly contribute to the infrared/optical/ultraviolet/X-ray emission. Using the simultaneous MAGIC, XMM-Newton, NuSTAR, and AstroSat observations, we argue that a region possibly associated with the 10 GHz radio core may explain such an excess. Finally, we investigate a VHE flare, showing an absence of simultaneous variability in the 0.3-2 keV band. Using time-dependent leptonic modelling, we show that this behaviour, in contradiction to single-zone scenarios, can instead be explained by a two-component model.

    DOI： 10.1051/0004-6361/202347845

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  • Constraints on axion-like particles with the Perseus Galaxy Cluster with MAGIC

    Abe, H. and others

    Phys.Dark Univ.   44   101425 - 101425   2024年1月

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    掲載種別：研究論文（学術雑誌）  

    DOI： 10.1016/j.dark.2024.101425

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  • Search for dark photons with the FASER detector at the LHC 査読 国際共著

    Abreu, H; Anders, J; Antel, C; Ariga, A; Ariga, T; Atkinson, J; Bernlochner, FU; Boeckh, T; Boyd, J; Brenner, L; Cadouxc, F; Casper, DW; Cavanaghj, C; Chen, X; Coccaro, A; D'Onofrioj, M; Desai, A; Dmitrievsky, S; Dozen, C; Favre, Y; Fellersm, D; Feng, JL; Fenoglio, CA; Ferrere, D; Galon, I; Gibson, S; Gonzalez-Sevillac, S; Gornushkin, Y; Gwilliam, C; Hayakawa, D; Hsu, SC; Hu, Z; Iacobucci, G; Inada, T; Jakobsen, S; Joos, H; Kajomovitz, E; Kawahara, H; Keyken, A; Kling, F; Köck, D; Kose, U; Kotitsa, R; Kuehn, S; Lefebvre, H; Levinson, L; Li, K; Liu, JF; MacDonald, J; Magliocca, C; Martinelli, F; McFayden, J; Meehan, S; Milanesio, M; Moretti, T; Munker, M; Nakamura, M; Nakano, T; Neuhaus, F; Nevay, L; Ohashi, K; Otono, H; Pang, H; Paolozzi, L; Petersen, B; Prim, M; Queitsch-Maitland, M; Rokujo, H; Ruiz-Choliz, E; Sabater-Iglesias, J; Salfeld-Nebgen, J; Sato, O; Scampoli, P; Schmieden, K; Schott, M; Sfyrla, A; Shively, S; Takubo, Y; Tarannum, N; Theiner, O; Torrence, E; Trojanowski, S; Vasina, S; Vormwald, B; Wang, D; Welch, E; Zahorec, S; Zambito, S

    PHYSICS LETTERS B   848   138378 - 138378   2024年1月   （ ISSN:0370-2693 eISSN:1873-2445 ）

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    記述言語：英語   掲載種別：研究論文（学術雑誌）   出版者・発行元：Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics  

    The FASER experiment at the LHC is designed to search for light, weakly-interacting particles produced in proton-proton collisions at the ATLAS interaction point that travel in the far-forward direction. The first results from a search for dark photons decaying to an electron-positron pair, using a dataset corresponding to an integrated luminosity of 27.0 fb−1 collected at centre-of-mass energy s=13.6 TeV in 2022 in LHC Run 3, are presented. No events are seen in an almost background-free analysis, yielding world-leading constraints on dark photons with couplings ϵ∼2×10−5−1×10−4 and masses ∼17 MeV−70 MeV. The analysis is also used to probe the parameter space of a massive gauge boson from a U(1)B−L model, with couplings gB−L∼5×10−6−2×10−5 and masses ∼15 MeV−40 MeV excluded for the first time.

    DOI： 10.1016/j.physletb.2023.138378

    Web of Science

    Scopus

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  • Performance of the joint LST-1 and MAGIC observations evaluated with Crab Nebula data

    Abe, H. and others

    Astron.Astrophys.   680   A66   2023年12月

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    掲載種別：研究論文（学術雑誌）  

    DOI： 10.1051/0004-6361/202346927

    arXiv

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  • MAGIC detection of GRB 201216C at $z$ = 1.1

    Abe, H. and others

    Mon.Not.Roy.Astron.Soc.   527 ( 3 )   5856 - 5867   2023年11月

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    掲載種別：研究論文（学術雑誌）  

    DOI： 10.1093/mnras/stad2958

    arXiv

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  • Observations of the Crab Nebula and Pulsar with the Large-sized Telescope Prototype of the Cherenkov Telescope Array

    Abe, H. and others

    Astrophys.J.   956 ( 2 )   80 - 80   2023年10月

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    掲載種別：研究論文（学術雑誌）  

    DOI： 10.3847/1538-4357/ace89d

    arXiv

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  • Potential of the Cherenkov Telescope Array for studying the young nearby supernova remnants

    Dmitry A Prokhorov, Shiu-Hang Lee, Shigehiro Nagataki, Jacco Vink, Donald Ellison, Gilles Ferrand, Daniel Patnaude, Friedrich Roepke, Ivo Seitenzahl, Patrick Slane, Kazuki Abe, Shotaro Abe, Atreya Acharyya, Remi Adam, Arnau Aguasca-Cabot, Ivan Agudo, Jorge Alfaro, Nuria Alvarez-Crespo, Rafael Alves Batista, Jean-Philippe Amans, Elena Amato, Filippo Ambrosino, Ekrem Oguzhan Angüner, Lucio Angelo Antonelli, Carla Aramo, Cornelia Arcaro, Luisa Arrabito, Katsuaki Asano, Jann Aschersleben, Halim Ashkar, Luiz Augusto Stuani, Dominik Baack, Michael Backes, Csaba Balazs, Matteo Balbo, Andres Baquero Larriva, Victor Barbosa Martins, Ulisses Barres de Almeida, Juan Abel Barrio, Denis Bastieri, Pedro Ivo Batista, Ivana Batković, Rowan William Batzofin, Joshua Ryo Baxter, Geoffrey Beck, Julia Becker Tjus, Lukas Beiske, Daniele Belardinelli, Wystan Benbow, Elisa Bernardini, Juan Bernete Medrano, Konrad Bernlöhr, Alessio Berti, Vasyl Beshley, Pooja Bhattacharjee, Saptashwa Bhattacharyya, Baiyang Bi, Noah Biederbeck, Adrian Biland, Elisabetta Bissaldi, Oscar Blanch, Jiri Blazek, Catherine Boisson, Julien Bolmont, Giacomo Bonnoli, Pol Bordas, Željka Bošnjak, Federica Bradascio, Catherine Braiding, Ettore Bronzini, Robert Brose, Anthony M. Brown, Francois Brun, Giulia Brunelli, Andrea Bulgarelli, Irene Burelli, Leonid Burmistrov, Michael Burton, Tomas Bylund, Paolo Gherardo Calisse, Anna Campoy-Ordaz, Brandon Khan Cantlay, Milvia Capalbi, Anderson Caproni, Roberto Capuzzo-Dolcetta, Colin Carlile, Sami Caroff, Alessandro Carosi, Roberto Carosi, Marie-Sophie Carrasco, Enrico Cascone, Franca Cassol, Noelia Castrejon, Fernando Catalani, Davide Cerasole, Matteo Cerruti, Sylvain Chaty, Andrew W Chen, Maria Chernyakova, Andrea Chiavassa, Jiří Chudoba, Carlos Henrique Coimbra Araujo, Vito Conforti, Francesco Conte, Jose Luis Contreras, Christophe Cossou, Alessandro Costa, Heide Costantini, Pierre Cristofari, Omar Cuevas, Zachary Curtis-Ginsberg, Giacomo D'Amico, Filippo D'Ammando, Mauro Dadina, Mykhailo Dalchenko, Ludovic David, Isak Delberth Davids, Francesco Dazzi, Alessandro De Angelis, Mathieu de Bony de Lavergne, Vincenzo De Caprio, Giovanni De Cesare, Elisabete M. de Gouveia Dal Pino, Barbara De Lotto, Mario de Lucia, Raniere de Menezes, Mathieu de Naurois, Emma de Oña Wilhelmi, Nicola De Simone, Vitor de Souza, Luis Del Peral, Maria Victoria del Valle, Eric Delagnes, Andres Gabriel Delgado Giler, Carlos Delgado, Michael Dell'aiera, Roberto Della Ceca, Massimo Della Valle, Domenico Della Volpe, Davide Depaoli, Antonios Dettlaff, Tristano Di Girolamo, Ambra Di Piano, Federico Di Pierro, Riccardo Di Tria, Leonardo Di Venere, Christian Díaz-Bahamondes, Claudio Dib, Sebastian Diebold, Razvan Dima, Adithiya Dinesh, Arache Djannati-Ataï, Julia Isabel Djuvsland, Alberto Dominguez, Rune Michael Dominik, Alice Donini, Daniela Dorner, Julien Dörner, Michele Doro, Rita de Cassia dos Anjos, Jean-Laurent Dournaux, Dainis Dravins, Chaimongkol Duangchan, Coline Dubos, Lozenzo Ducci, Vikram V. Dwarkadas, Jan Ebr, Christopher Eckner, Kathrin Egberts, Sabrina Einecke, Dominik Elsässer, Gabriel Emery, Miguel Escobar Godoy, Juan Escudero, Paolo Esposito, Diego Falceta-Gonçalves, Vandad Fallah Ramazani, Alice Faure, Elena Fedorova, Stephen Fegan, Kirsty Feijen, Qi Feng, Fabio Ferrarotto, Emanuele Fiandrini, Armand Fiasson, Valentina Fioretti, Luca Foffano, Lluis Font Guiteras, Gerard Fontaine, Stefan Fröse, Satoshi Fukami, Yasuo Fukui, Stefan Funk, Daniele Gaggero, Giorgio Galanti, Gaspar Galaz, Yves A. Gallant, Stefano Gallozzi, Viviana Gammaldi, Claudio Gasbarra, Markus Gaug, Arsen Ghalumyan, Fulvio Gianotti, Marina Giarrusso, Nicola Giglietto, Francesco Giordano, Andrea Giuliani, Jean-Francois Glicenstein, Jonas Glombitza, Paolo Goldoni, José Mauricio González, Maria Magdalena González, Jaziel Goulart Coelho, Jonathan Granot, Dario Grasso, Roger Grau, David Green, Jarred Gershon Green, Tim Greenshaw, Guillaume Grolleron, Jeff Grube, Orel Gueta, Shuichi Gunji, Daniela Hadasch, Petr Hamal, William Hanlon, Satoshi Hara, Violet M. Harvey, Kazuaki Hashiyama, Tarek Hassan, Matthieu Heller, Sergio Hernández Cadena, Jonathan Hie, Nagisa Hiroshima, Bohdan Hnatyk, Roman Hnatyk, Dirk Hoffmann, Werner Hofmann, Markus Holler, Deirdre Horan, Pavel Horvath, Talvikki Hovatta, Dario Hrupec, Saqib Hussain, Marco Iarlori, Tomohiro Inada, Federico Incardona, Yusuke Inome, Susumu Inoue, Fabio Iocco, Kazuma Ishio, Marek Jamrozy, Petr Janecek, Felix Jankowsky, Christian Jarnot, Pierre Jean, Irene Jiménez Martínez, Weidong Jin, Laurent Jocou, Claire Juramy-Gilles, Jakub Jurysek, Oleg KALEKIN, Dimitrios Kantzas, Vladimir Karas, Sarah Kaufmann, Daniel Kerszberg, Bruno Khelifi, David B Kieda, Tobias Kai Kleiner, Włodzimierz Kluźniak, Yukiho Kobayashi, Kazunori Kohri, Nukri Komin, Paula Kornecki, Karl Kosack, Hidetoshi Kubo, Junko Kushida, Antonino La Barbera, Nicola La Palombara, Maria Lainez, Alessandra Lamastra, Jon S Lapington, Sanja Lazarevic, Jasmina Lazendic-Galloway, Steven Leach, Marianne Lemoine-Goumard, Jean-Philippe Lenain, Giuseppe Leto, Fabian Leuschner, Elina Lindfors, Maximilian Linhoff, Ioannis Liodakis, Lozach Loïc, Saverio Lombardi, Francesco Longo, Rubén López-Coto, Marcos López-Moya, Alicia López-Oramas, Serena Loporchio, Julio Lozano Bahilo, Pedro L. Luque-Escamilla, Oscar Macias, Gernot Maier, Pratik Majumdar, Denys Malyshev, Dmitry Malyshev, Dusan Mandat, Giulio Manicò, Peter David Marinos, Sera Markoff, Isabel Márquez, Patricia Marquez, Giovanni Marsella, Josep Martí, Pierrick Martin, Gustavo Augusto Martínez, Manel Martínez, Oibar Martinez, Christophe Marty, Alvaro Mas-Aguilar, Michele Mastropietro, Gilles Maurin, Walter Max-Moerbeck, Daniel Mazin, David Melkumyan, Stefano Menchiari, Enrique Mestre, Jean-Luc Meunier, Dominique M.-A. Meyer, Davide Miceli, Miltiadis Michailidis, Jerzy Michałowski, Tjark Miener, Jose Miguel Miranda, Alison Mitchell, Masaya Mizote, Tsunefumi Mizuno, Rafal Moderski, Lars Mohrmann, Miguel Molero, Cesare Molfese, Edgar Molina, Teresa Montaruli, Abelardo Moralejo, Daniel Morcuende, Katharina Morik, Aldo Morselli, Emmanuel Moulin, Victor Moya Zamanillo, Reshmi Mukherjee, Kevin Munari, Adam Muraczewski, Hiroshi Muraishi, Takeshi Nakamori, Lara Nava, Amrit Nayak, Rodrigo Nemmen, Lukas Nickel, Jacek Niemiec, Daniel Nieto, Mireia Nievas Rosillo, Marek Nikołajuk, Kyoshi Nishijima, Koji Noda, Dalibor Nosek, Bohdan Novosyadlyj, Vladimír Novotný, Seiya Nozaki, Paul O'Brien, Michiko Ohishi, Yoshiki Ohtani, Akira Okumura, Jean-François Olive, Barbara Olmi, Rene A. Ong, Monica Orienti, Reiko Orito, Mauro Orlandini, Elena Orlando, Michal Ostrowski, Nepomuk Otte, Igor Oya, Isabella Pagano, Antonio Pagliaro, Michele Palatiello, Gabriele Panebianco, Josep M. Paredes, Nicolò Parmiggiani, Sonal Ramesh Patel, Barbara Patricelli, Dijana Pavlović, Asaf Pe'er, Miroslav Pech, Mario Pecimotika, Michele Peresano, Judit Pérez-Romero, Giada Peron, Massimo Persic, Pierre-Olivier Petrucci, Oleh Petruk, Felix Pfeifle, Fabio Pintore, Giorgio Pirola, Carlotta Pittori, Cyann Plard, Franjo Podobnik, Martin Pohl, Estelle Pons, Elisa Prandini, Julie Prast, Giacomo Principe, Chaitanya Priyadarshi, Nicolas Produit, Elisa Pueschel, Gerd Pühlhofer, Maria Letizia Pumo, Michael Punch, Andreas Quirrenbach, Silvia Raino, Nunzio Randazzo, Riccardo Rando, Thierry Ravel, Soebur Razzaque, Maxime Regeard, Patrick Reichherzer, Anita Reimer, Olaf Reimer, Andreas Reisenegger, Thierry Reposeur, Brian Reville, Wolfgang Rhode, Marc Ribó, Tom Richtler, Frank Rieger, Emmet Roache, Gonzalo Rodriguez Fernandez, Maria Dolores Rodríguez Frías, Juan José Rodríguez-Vázquez, Patrizia Romano, Giuseppe Romeo, Jaime Rosado, Gavin P Rowell, Bronislaw Rudak, Ashley J. Ruiter, Cameron Boyd Rulten, Federico Russo, Iftach Sadeh, Lab Saha, Takayuki Saito, Shunsuke Sakurai, Heiko Salzmann, David Sanchez, Miguel Sanchez-Conde, Pierluca Sangiorgi, Hidetoshi Sano, Marcos Santander, Andrea Santangelo, Reinaldo Santos-Lima, Andreu Sanuy, Toni Šarić, Arkadipta Sarkar, Subir Sarkar, Francesco Gabriele Saturni, Volodymyr Savchenko, Andres Scherer, Pietro Schipani, Bernd Schleicher, Petr Schovanek, Jan Lukas Schubert, Fabian Schüssler, Ullrich Schwanke, Georg Schwefer, Salvatore Scuderi, Monica Seglar Arroyo, Olga Sergijenko, Vito Sguera, Ruo Yu Shang, Pooja Sharma, Guereguin Der Sylvestre Sidibe, Lara Sidoli, Hubert Siejkowski, Clarissa Siqueira, Patrick Sizun, Vitalii Sliusar, Agnieszka Slowikowska, Helene Sol, Andreas Specovius, Samuel Timothy Spencer, Daniele Spiga, Antonio Stamerra, Samo Stanič, Tomasz Starecki, Rhaana Starling, Constantin Steppa, Thierry Stolarczyk, Jelena Strišković, Marcel C. Strzys, Yusuke Suda, Tiina Suomijarvi, Donggeun Tak, Mitsunari Takahashi, Ryuji Takeishi, Pak-Hin Thomas Tam, Shuta J Tanaka, Takaaki Tanaka, Kenta Terauchi, Vincenzo Testa, Luigi Tibaldo, Omar Tibolla, Francesc Torradeflot, Diego F. Torres, Eleonora Torresi, Nick Tothill, Francois Toussenel, Victoria Touzard, Andrea Tramacere, Petr Travnicek, Giovanni Tripodo, Stefano Truzzi, Adellain Tsiahina, Antonio Tutone, Martin Vacula, Bertrand Vallage, Piero Vallania, Ramon Vallés, Christopher van Eldik, Juliane van Scherpenberg, Justin Vandenbroucke, Vladimir Vassiliev, Philippe Venault, Sofia Ventura, Stefano Vercellone, Gaia Verna, Aion Viana, Nicolás Viaux, Alessandro Vigliano, Jonatan Vignatti, Carlo francesco Vigorito, Vincenzo Vitale, Veronika Vodeb, Vincent Voisin, Serguei Vorobiov, Georgios Gerasimos Voutsinas, Ievgen Vovk, Vincent Waegebaert, Stefan Joachim Wagner, Roland Walter, Martin Ward, Maneenate Wechakama, Richard White, Alicja Wierzcholska, Martin Will, David A. Williams, Frederik Wohlleben, Anna Wolter, Tokonatsu Yamamoto, Ryo Yamazaki, Lili Yang, Tatsuo Yoshida, Takanori Yoshikoshi, Michael Zacharias, Ricardo Zanmar Sanchez, Danilo Zavrtanik, Marko Zavrtanik, Andrzej A. Zdziarski, Andreas Zech, Valery I. Zhdanov, Krzysztof Ziȩtara, Miha Živec, Jaume Zuriaga-Puig

    Proceedings of 38th International Cosmic Ray Conference — PoS(ICRC2023)   2023年8月

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    掲載種別：研究論文（国際会議プロシーディングス）   出版者・発行元：Sissa Medialab  

    DOI： 10.22323/1.444.0824

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  • Sensitivity of the Cherenkov Telescope Array to spectral signatures of hadronic PeVatrons with application to Galactic Supernova Remnants

    F. Acero, A. Acharyya, R. Adam, A. Aguasca-Cabot, I. Agudo, A. Aguirre-Santaella, J. Alfaro, R. Aloisio, N. Álvarez Crespo, R. Alves Batista, L. Amati, E. Amato, G. Ambrosi, E.O. Angüner, C. Aramo, C. Arcaro, T. Armstrong, K. Asano, Y. Ascasibar, J. Aschersleben, M. Backes, A. Baktash, C. Balazs, M. Balbo, J. Ballet, A. Baquero Larriva, V. Barbosa Martins, U. Barres de Almeida, J.A. Barrio, D. Bastieri, J.R. Baxter, J. Becker Tjus, W. Benbow, M.I. Bernardos-Martín, J. Bernete, A. Berti, B. Bertucci, V. Beshley, P. Bhattacharjee, S. Bhattacharyya, A. Biland, E. Bissaldi, J. Biteau, O. Blanch, P. Bordas, E. Bottacini, J. Bregeon, R. Brose, N. Bucciantini, A. Bulgarelli, M. Capasso, R.A. Capuzzo Dolcetta, P. Caraveo, M. Cardillo, R. Carosi, S. Casanova, E. Cascone, F. Cassol, F. Catalani, M. Cerruti, P. Chadwick, S. Chaty, A. Chen, M. Chernyakova, A. Chiavassa, J. Chudoba, C. Coimbra-Araujo, V. Conforti, J.L. Contreras, A. Costa, H. Costantini, P. Cristofari, R. Crocker, G. D’Amico, F. D’Ammando, A. De Angelis, V. De Caprio, E.M. de Gouveia Dal Pino, E. de Ona Wilhelmi, V. de Souza, C. Delgado, D. della Volpe, D. Depaoli, T. Di Girolamo, F. Di Pierro, R. Di Tria, L. Di Venere, S. Diebold, J.I. Djuvsland, A. Donini, M. Doro, R.d.C. Dos Anjos, V.V. Dwarkadas, S. Einecke, D. Elsässer, G. Emery, C. Evoli, D. Falceta-Goncalves, E. Fedorova, S. Fegan, G. Ferrand, E. Fiandrini, M. Filipovic, V. Fioretti, M. Fiori, L. Foffano, G. Fontaine, S. Fukami, G. Galanti, G. Galaz, V. Gammaldi, C. Gasbarra, A. Ghalumyan, G. Ghirlanda, M. Giarrusso, G. Giavitto, N. Giglietto, F. Giordano, M. Giroletti, A. Giuliani, L. Giunti, N. Godinovic, J. Goulart Coelho, L. Gréaux, D. Green, M.-H. Grondin, O. Gueta, S. Gunji, T. Hassan, M. Heller, S. Hernández-Cadena, J. Hinton, B. Hnatyk, R. Hnatyk, D. Hoffmann, W. Hofmann, J. Holder, D. Horan, P. Horvath, M. Hrabovsky, D. Hrupec, T. Inada, F. Incardona, S. Inoue, K. Ishio, M. Jamrozy, P. Janecek, I. Jiménez Martínez, W. Jin, I. Jung-Richardt, J. Jurysek, P. Kaaret, V. Karas, U. Katz, D. Kerszberg, B. Khélifi, D.B. Kieda, R. Kissmann, T. Kleiner, G. Kluge, W. Kluzniak, J. Knödlseder, Y. Kobayashi, K. Kohri, N. Komin, P. Kornecki, H. Kubo, N. La Palombara, M. Láinez, A. Lamastra, J. Lapington, M. Lemoine-Goumard, J.-P. Lenain, F. Leone, G. Leto, F. Leuschner, E. Lindfors, I. Liodakis, T. Lohse, S. Lombardi, F. Longo, R. López-Coto, M. López-Moya, A. López-Oramas, S. Loporchio, P.L. Luque-Escamilla, O. Macias, J. Mackey, P. Majumdar, D. Mandat, M. Manganaro, G. Manicò, M. Marconi, J. Martí, G. Martínez, M. Martinez, O. Martinez, A.J.T.S. Mello, S. Menchiari, D.M.-A. Meyer, S. Micanovic, D. Miceli, M. Miceli, J. Michalowski, T. Miener, J.M. Miranda, A. Mitchell, B. Mode, R. Moderski, L. Mohrmann, E. Molina, T. Montaruli, D. Morcuende, G. Morlino, A. Morselli, M. Mosè, E. Moulin, R. Mukherjee, K. Munari, T. Murach, A. Nagai, S. Nagataki, R. Nemmen, J. Niemiec, D. Nieto, M. Nievas Rosillo, M. Nikolajuk, K. Nishijima, K. Noda, B. Novosyadlyj, S. Nozaki, M. Ohishi, S. Ohm, Y. Ohtani, A. Okumura, B. Olmi, R.A. Ong, M. Orienti, R. Orito, M. Orlandini, E. Orlando, S. Orlando, M. Ostrowski, I. Oya, F.R. Pantaleo, J.M. Paredes, B. Patricelli, M. Pecimotika, M. Peresano, J. Pérez-Romero, M. Persic, O. Petruk, G. Piano, E. Pietropaolo, G. Pirola, C. Pittori, M. Pohl, G. Ponti, E. Prandini, G. Principe, C. Priyadarshi, E. Pueschel, G. Pühlhofer, M.L. Pumo, A. Quirrenbach, R. Rando, S. Razzaque, P. Reichherzer, A. Reimer, O. Reimer, M. Renaud, T. Reposeur, M. Ribó, T. Richtler, J. Rico, F. Rieger, M. Rigoselli, L. Riitano, V. Rizi, E. Roache, P. Romano, G. Romeo, J. Rosado, G. Rowell, B. Rudak, I. Sadeh, S. Safi-Harb, L. Saha, S. Sailer, M. Sánchez-Conde, S. Sarkar, K. Satalecka, F.G. Saturni, A. Scherer, P. Schovánek, F. Schussler, U. Schwanke, S. Scuderi, M. Seglar-Arroyo, O. Sergijenko, M. Servillat, R.-Y. Shang, P. Sharma, H. Siejkowski, V. Sliusar, A. Słowikowska, H. Sol, A. Specovius, S.T. Spencer, G. Spengler, A. Stamerra, S. Stanič, T. Starecki, R. Starling, T. Stolarczyk, L.A. Stuani Pereira, Y. Suda, T. Suomijarvi, I. Sushch, H. Tajima, P.-H.T. Tam, S.J. Tanaka, F. Tavecchio, V. Testa, W. Tian, L. Tibaldo, D.F. Torres, N. Tothill, B. Vallage, P. Vallania, C. van Eldik, J. van Scherpenberg, J. Vandenbroucke, M. Vazquez Acosta, M. Vecchi, S. Vercellone, G. Verna, A. Viana, J. Vignatti, V. Vitale, V. Vodeb, S. Vorobiov, T. Vuillaume, S.J. Wagner, R. Walter, M. White, A. Wierzcholska, M. Will, D. Williams, L. Yang, T. Yoshida, T. Yoshikoshi, G. Zaharijas, L. Zampieri, D. Zavrtanik, M. Zavrtanik, V.I. Zhdanov, M. Z̆ivec

    Astroparticle Physics   150   102850 - 102850   2023年8月   （ ISSN:0927-6505 ）

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    掲載種別：研究論文（学術雑誌）   出版者・発行元：Elsevier BV  

    DOI： 10.1016/j.astropartphys.2023.102850

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  • First Direct Observation of Collider Neutrinos with FASER at the LHC 査読 国際共著

    Abreu, H; Anders, J; Antel, C; Ariga, A; Ariga, T; Atkinson, J; Bernlochner, FU; Blesgen, T; Boeckh, T; Boyd, J; Brenner, L; Cadoux, F; Casper, DW; Cavanagh, C; Chen, X; Coccaro, A; Desai, A; Dmitrievsky, S; D'Onofrio, M; Favre, Y; Fellers, D; Feng, JL; Fenoglio, CA; Ferrere, D; Gibson, S; Gonzalez-Sevilla, S; Gornushkin, Y; Gwilliam, C; Hayakawa, D; Hsu, SC; Hu, Z; Iacobucci, G; Inada, T; Jakobsen, S; Joos, H; Kajomovitz, E; Kawahara, H; Keyken, A; Kling, F; Köck, D; Kose, U; Kotitsa, R; Kuehn, S; Lefebvre, H; Levinson, L; Li, K; Liu, JF; Macdonald, J; Magliocca, C; Martinelli, F; Mcfayden, J; Milanesio, M; Mladenov, D; Moretti, T; Munker, M; Nakamura, M; Nakano, T; Nessi, M; Neuhaus, F; Nevay, L; Otono, H; Pang, H; Paolozzi, L; Petersen, B; Pietropaolo, F; Prim, M; Queitsch-Maitland, M; Resnati, F; Rokujo, H; Ruiz-Choliz, E; Sabater-Iglesias, J; Sato, O; Scampoli, P; Schmieden, K; Schott, M; Sfyrla, A; Shively, S; Takubo, Y; Tarannum, N; Theiner, O; Torrence, E; Tufanli, S; Vasina, S; Vormwald, B; Wang, D; Welch, E

    PHYSICAL REVIEW LETTERS   131 ( 3 )   031801   2023年7月   （ ISSN:0031-9007 eISSN:1079-7114 ）

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    担当区分：責任著者   記述言語：英語   掲載種別：研究論文（学術雑誌）   出版者・発行元：Physical Review Letters  

    We report the first direct observation of neutrino interactions at a particle collider experiment. Neutrino candidate events are identified in a 13.6 TeV center-of-mass energy pp collision dataset of 35.4 fb-1 using the active electronic components of the FASER detector at the Large Hadron Collider. The candidates are required to have a track propagating through the entire length of the FASER detector and be consistent with a muon neutrino charged-current interaction. We infer 153-13+12 neutrino interactions with a significance of 16 standard deviations above the background-only hypothesis. These events are consistent with the characteristics expected from neutrino interactions in terms of secondary particle production and spatial distribution, and they imply the observation of both neutrinos and anti-neutrinos with an incident neutrino energy of significantly above 200 GeV.

    DOI： 10.1103/PhysRevLett.131.031801

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    その他リンク： http://harvest.aps.org/v2/journals/articles/10.1103/PhysRevLett.131.031801/fulltext

  • Multimessenger Characterization of Markarian 501 during Historically Low X-Ray and γ-Ray Activity

    Abe, H. and others

    Astrophys.J.Suppl.   266 ( 2 )   37 - 37   2023年6月

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    掲載種別：研究論文（学術雑誌）  

    DOI： 10.3847/1538-4365/acc181

    arXiv

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  • Sensitivity of the Cherenkov Telescope Array to TeV photon emission from the Large Magellanic Cloud 査読

    Acharyya, A. and others

    Mon.Not.Roy.Astron.Soc.   523 ( 4 )   5353 - 5387   2023年5月   （ ISSN:0035-8711 eISSN:1365-2966 ）

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    掲載種別：研究論文（学術雑誌）   出版者・発行元：Oxford University Press (OUP)  

    A deep survey of the Large Magellanic Cloud at ~0.1-100 TeV photon energies with the Cherenkov Telescope Array is planned. We assess the detection prospects based on a model for the emission of the galaxy, comprising the four known TeV emitters, mock populations of sources, and interstellar emission on galactic scales. We also assess the detectability of 30 Doradus and SN 1987A, and the constraints that can be derived on the nature of dark matter. The survey will allow for fine spectral studies of N 157B, N 132D, LMC P3, and 30 Doradus C, and half a dozen other sources should be revealed, mainly pulsar-powered objects. The remnant from SN 1987A could be detected if it produces cosmic-ray nuclei with a flat power-law spectrum at high energies, or with a steeper index 2.3-2.4 pending a flux increase by a factor &gt;3-4 over ~2015-2035. Large-scale interstellar emission remains mostly out of reach of the survey if its &gt;10 GeV spectrum has a soft photon index ~2.7, but degree-scale 0.1-10 TeV pion-decay emission could be detected if the cosmic-ray spectrum hardens above &gt;100 GeV. The 30 Doradus star-forming region is detectable if acceleration efficiency is on the order of 1 - 10 per cent of the mechanical luminosity and diffusion is suppressed by two orders of magnitude within &lt;100 pc. Finally, the survey could probe the canonical velocity-averaged cross section for self-annihilation of weakly interacting massive particles for cuspy Navarro-Frenk-White profiles....

    DOI： 10.1093/mnras/stad1576

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    その他リンク： https://academic.oup.com/mnras/article-pdf/523/4/5353/50733482/stad1576.pdf

  • Multi-wavelength study of the galactic PeVatron candidate LHAASO J2108+5157

    Abe, S. and others

    Astron.Astrophys.   673   A75   2023年5月

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    掲載種別：研究論文（学術雑誌）  

    DOI： 10.1051/0004-6361/202245086

    arXiv

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  • MAGIC observations provide compelling evidence of hadronic multi-TeV emission from the putative PeVatron SNR G106.3+2.7

    Abe, H. and others

    Astron.Astrophys.   671   A12   2023年3月

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    掲載種別：研究論文（学術雑誌）  

    DOI： 10.1051/0004-6361/202244931

    arXiv

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  • Search for Gamma-Ray Spectral Lines from Dark Matter Annihilation up to 100 TeV toward the Galactic Center with MAGIC 査読 国際共著

    H. Abe, S. Abe, V. A. Acciari, T. Aniello, S. Ansoldi, L. A. Antonelli, A. Arbet Engels, C. Arcaro, M. Artero, K. Asano, D. Baack, A. Babić, A. Baquero, U. Barres de Almeida, J. A. Barrio, I. Batković, J. Baxter, J. Becerra González, W. Bednarek, E. Bernardini, M. Bernardos, A. Berti, J. Besenrieder, W. Bhattacharyya, C. Bigongiari, A. Biland, O. Blanch, G. Bonnoli, Ž. Bošnjak, I. Burelli, G. Busetto, R. Carosi, M. Carretero-Castrillo, G. Ceribella, Y. Chai, A. Chilingarian, S. Cikota, E. Colombo, J. L. Contreras, J. Cortina, S. Covino, G. D’Amico, V. D’Elia, P. Da Vela, F. Dazzi, A. De Angelis, B. De Lotto, A. Del Popolo, M. Delfino, J. Delgado, C. Delgado Mendez, D. Depaoli, F. Di Pierro, L. Di Venere, E. Do Souto Espiñeira, D. Dominis Prester, A. Donini, D. Dorner, M. Doro, D. Elsaesser, G. Emery, V. Fallah Ramazani, L. Fariña, A. Fattorini, L. Font, C. Fruck, S. Fukami, Y. Fukazawa, R. J. García López, M. Garczarczyk, S. Gasparyan, M. Gaug, J. G. Giesbrecht Paiva, N. Giglietto, F. Giordano, P. Gliwny, N. Godinović, J. G. Green, D. Green, D. Hadasch, A. Hahn, T. Hassan, L. Heckmann, J. Herrera, D. Hrupec, M. Hütten, R. Imazawa, T. Inada, R. Iotov, K. Ishio, I. Jiménez Martínez, J. Jormanainen, D. Kerszberg, Y. Kobayashi, H. Kubo, J. Kushida, A. Lamastra, D. Lelas, F. Leone, E. Lindfors, L. Linhoff, S. Lombardi, F. Longo, R. López-Coto, M. López-Moya, A. López-Oramas, S. Loporchio, A. Lorini, E. Lyard, B. Machado de Oliveira Fraga, P. Majumdar, M. Makariev, G. Maneva, N. Mang, M. Manganaro, S. Mangano, K. Mannheim, M. Mariotti, M. Martínez, A. Mas Aguilar, D. Mazin, S. Menchiari, S. Mender, S. Mićanović, D. Miceli, T. Miener, J. M. Miranda, R. Mirzoyan, E. Molina, H. A. Mondal, A. Moralejo, D. Morcuende, V. Moreno, T. Nakamori, C. Nanci, L. Nava, V. Neustroev, M. Nievas Rosillo, C. Nigro, K. Nilsson, K. Nishijima, T. Njoh Ekoume, K. Noda, S. Nozaki, Y. Ohtani, T. Oka, J. Otero-Santos, S. Paiano, M. Palatiello, D. Paneque, R. Paoletti, J. M. Paredes, L. Pavletić, M. Persic, M. Pihet, F. Podobnik, P. G. Prada Moroni, E. Prandini, G. Principe, C. Priyadarshi, I. Puljak, W. Rhode, M. Ribó, J. Rico, C. Righi, A. Rugliancich, N. Sahakyan, T. Saito, S. Sakurai, K. Satalecka, F. G. Saturni, B. Schleicher, K. Schmidt, F. Schmuckermaier, J. L. Schubert, T. Schweizer, J. Sitarek, V. Sliusar, D. Sobczynska, A. Spolon, A. Stamerra, J. Strišković, D. Strom, M. Strzys, Y. Suda, T. Surić, M. Takahashi, R. Takeishi, F. Tavecchio, P. Temnikov, K. Terauchi, T. Terzić, M. Teshima, L. Tosti, S. Truzzi, A. Tutone, S. Ubach, J. van Scherpenberg, M. Vazquez Acosta, S. Ventura, V. Verguilov, I. Viale, C. F. Vigorito, V. Vitale, I. Vovk, R. Walter, M. Will, C. Wunderlich, T. Yamamoto, D. Zarić, N. Hiroshima, K. Kohri

    Physical Review Letters   130 ( 6 )   061002   2023年2月   （ ISSN:0031-9007 eISSN:1079-7114 ）

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    担当区分：責任著者   記述言語：英語   掲載種別：研究論文（学術雑誌）   出版者・発行元：American Physical Society  

    DOI： 10.1103/physrevlett.130.061002

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    その他リンク： http://harvest.aps.org/v2/journals/articles/10.1103/PhysRevLett.130.061002/fulltext

  • A lower bound on intergalactic magnetic fields from time variability of 1ES 0229+200 from MAGIC and Fermi/LAT observations

    Acciari, V. A. and others

    Astron.Astrophys.   670   A145   2023年2月   （ ISSN:1432-0746 ）

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    掲載種別：研究論文（学術雑誌）  

    DOI： 10.1051/0004-6361/202244126

    Scopus

    arXiv

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  • The Forward Physics Facility at the High-Luminosity LHC 査読 国際共著

    Feng, JL; Kling, F; Reno, MH; Rojo, J; Soldin, D; Anchordoqui, LA; Boyd, J; Ismail, A; Harland-Lang, L; Kelly, KJ; Pandey, V; Trojanowski, S; Tsai, YD; Alameddine, JM; Araki, T; Ariga, A; Ariga, T; Asai, K; Bacchetta, A; Balazs, K; Barr, AJ; Battistin, M; Bian, JM; Bertone, C; Bai, WD; Bakhti, P; Balantekin, AB; Barman, B; Batell, B; Bauer, M; Bauer, B; Becker, M; Berlin, A; Bertuzzo, E; Bhattacharya, A; Bonvini, M; Boogert, ST; Boyarsky, A; Bramante, J; Brdar, V; Carmona, A; Casper, DW; Celiberto, FG; Cerutti, F; Chachamis, G; Chauhan, G; Citron, M; Copello, E; Corso, JP; Darmé, L; D'Agnolo, RT; Darvishi, N; Das, A; De Lellis, G; De Roeck, A; de Vries, J; Dembinski, HP; Demidov, S; DeNiverville, P; Denton, PB; Deppisch, FF; Dev, PSB; Di Crescenzo, A; Dienes, KR; Diwan, M; Dreiner, HK; Du, Y; Dutta, B; Duwentäster, P; Elie, L; Ellis, SAR; Enberg, R; Farzan, Y; Fieg, M; Foguel, AL; Foldenauer, P; Foroughi-Abari, S; Fortin, JF; Friedland, A; Fuchs, E; Fucilla, M; Gallmeister, K; Garcia, A; Canal, CAG; Garzelli, MV; Gauld, R; Ghosh, S; Ghoshal, A; Gibson, S; Giuli, F; Gonçalves, VP; Gorbunov, D; Goswami, S; Grau, S; Günther, JY; Guzzi, M; Haas, A; Hakulinen, T; Harris, SP; Harz, J; Herrera, JCH; Hill, CS; Hirsch, M; Hobbs, TJ; Höche, S; Hryczuk, A; Huang, F; Inada, T; Infantino, A; Ismail, A; Jacobsson, R; Jana, S; Jeong, YS; Jho, Y; Kalashnikov, D; Kärkkäinen, TJ; Keppel, C; Kim, J; Klasen, M; Klein, SR; Ko, P; Köhler, D; Komatsu, M; Kovarík, K; Kulkarni, S; Kumar, J; Kumar, K; Kuo, JL; Krauss, F; Kusina, A; Laletin, M; Le Roux, C; Lee, SJ; Lee, HS; Lefebvre, H; Li, JM; Li, SL; Li, YC; Liu, W; Liu, Z; Lonjon, M; Lyu, KF; Maciula, R; Abraham, RM; Masouminia, MR; McFayden, J; Mikulenko, O; Mohammed, MMA; Mohan, KA; Morfín, JG; Mosel, U; Mosny, M; Muzakka, KF; Nadolsky, P; Nakano, T; Nangia, S; Cornago, AN; Nevay, LJ; Ninin, P; Nocera, ER; Nomura, T; Nunes, R; Okada, N; Olness, F; Osborne, J; Otono, H; Ovchynnikov, M; Papa, A; Pei, JL; Peon, G; Perez, G; Pickering, L; Plätzer, S; Plestid, R; Poddar, TK; Quílez, P; Rai, M; Rajaee, M; Raut, D; Reimitz, P; Resnati, F; Rhode, W; Richardson, P; Ritz, A; Rokujo, H; Roszkowski, L; Ruhe, T; Ruiz, R; Sabate-Gilarte, M; Sandrock, A; Sarcevic, I; Sarkar, S; Sato, O; Scherb, C; Schienbein, I; Schulz, H; Schwaller, P; Sciutto, SJ; Sengupta, D; Shchutska, L; Shimomura, T; Silvetti, F; Sinha, K; Sjöstrand, T; Sobczyk, JT; Song, HY; Soriano, JF; Soreq, Y; Stasto, A; Stuart, D; Su, SF; Su, W; Szczurek, A; Tabrizi, Z; Takubo, Y; Taoso, M; Thomas, B; Thonet, P; Tuckler, D; Vera, AS; Vincke, H; Vishnudath, KN; Wang, ZS; Winkler, MW; Wu, WJ; Xie, KP; Xu, XJ; You, T; Yu, JY; Yu, JH; Zapp, K; Zhang, YC; Zhang, Y; Zhou, GH; Funchal, RZ

    JOURNAL OF PHYSICS G-NUCLEAR AND PARTICLE PHYSICS   50 ( 3 )   030501 - 030501   2023年1月   （ ISSN:0954-3899 eISSN:1361-6471 ）

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    記述言語：英語   掲載種別：研究論文（学術雑誌）   出版者・発行元：Journal of Physics G: Nuclear and Particle Physics  

    High energy collisions at the High-Luminosity Large Hadron Collider (LHC) produce a large number of particles along the beam collision axis, outside of the acceptance of existing LHC experiments. The proposed Forward Physics Facility (FPF), to be located several hundred meters from the ATLAS interaction point and shielded by concrete and rock, will host a suite of experiments to probe standard model (SM) processes and search for physics beyond the standard model (BSM). In this report, we review the status of the civil engineering plans and the experiments to explore the diverse physics signals that can be uniquely probed in the forward region. FPF experiments will be sensitive to a broad range of BSM physics through searches for new particle scattering or decay signatures and deviations from SM expectations in high statistics analyses with TeV neutrinos in this low-background environment. High statistics neutrino detection will also provide valuable data for fundamental topics in perturbative and non-perturbative QCD and in weak interactions. Experiments at the FPF will enable synergies between forward particle production at the LHC and astroparticle physics to be exploited. We report here on these physics topics, on infrastructure, detector, and simulation studies, and on future directions to realize the FPF's physics potential.

    DOI： 10.1088/1361-6471/ac865e

    Web of Science

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  • Long-term multi-wavelength study of 1ES 0647+250

    Acciari, V. A. and others

    Astron.Astrophys.   670   A49   2023年

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    掲載種別：研究論文（学術雑誌）  

    DOI： 10.1051/0004-6361/202244477

    arXiv

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  • The recent status of the FASER detector

    Tomohiro Inada

    Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment   2022年10月

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    掲載種別：研究論文（学術雑誌）  

    DOI： 10.1016/j.nima.2022.167185

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  • Gamma-ray observations of MAXI J1820+070 during the 2018 outburst

    Abe, H. and others

    Mon.Not.Roy.Astron.Soc.   517 ( 4 )   4736 - 4751   2022年9月   （ ISSN:0035-8711 eISSN:1365-2966 ）

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    記述言語：英語   掲載種別：研究論文（学術雑誌）   出版者・発行元：OXFORD UNIV PRESS  

    MAXIJ1820+070 is a low-mass X-ray binary with a black hole (BH) as a compact object. This binary underwent an exceptionally bright X-ray outburst from 2018 March to October, showing evidence of a non-thermal particle population through its radio emission during this whole period. The combined results of 59.5 h of observations of the MAXI J1820+070 outburst with the H.E.S.S., MAGIC and VERITAS experiments at energies above 200 GeV are presented, together with Fermi-LAT data between 0.1 and 500 GeV, and multiwavelength observations from radio to X-rays. Gamma-ray emission is not detected from MAXI J1820+070, but the obtained upper limits and the multiwavelength data allow us to put meaningful constraints on the source properties under reasonable assumptions regarding the non-thermal particle population and the jet synchrotron spectrum. In particular, it is possible to show that, if a high-energy (HE) gamma-ray emitting region is present during the hard state of the source, its predicted flux should be at most a factor of 20 below the obtained Fermi-LAT upper limits, and closer to them for magnetic fields significantly below equipartition. During the state transitions, under the plausible assumption that electrons are accelerated up to similar to 500 GeV, the multiwavelength data and the gamma-ray upper limits lead consistently to the conclusion that a potential HE and very-HE gamma-ray emitting region should be located at a distance from the BH ranging between 10(11) and 10(13) cm. Similar outbursts from low-mass X-ray binaries might be detectable in the near future with upcoming instruments such as CTA.

    DOI： 10.1093/mnras/stac2686

    Web of Science

    arXiv

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  • The tracking detector of the FASER experiment 査読 国際共著

    Abreu H., Antel C., Ariga A., Ariga T., Bernlochner F., Boeckh T., Boyd J., Brenner L., Cadoux F., Casper D.W., Cavanagh C., Chen X., Coccaro A., Crespo-Lopez O., Dmitrievsky S., D'Onofrio M., Dozen C., Ezzat A., Favre Y., Fellers D., Feng J.L., Ferrere D., Gibson S., Gonzalez-Sevilla S., Gornushkin Y., Gwilliam C., Hsu S.C., Hu Z., Iacobucci G., Inada T., Jakobsen S., Kajomovitz E., Kling F., Kose U., Kuehn S., Lefebvre H., Levinson L., Li K., Liu J., Magliocca C., McFayden J., Milanesio M., Meehan S., Mladenov D., Moretti T., Munker M., Nakamura M., Nakano T., Nessi M., Neuhaus F., Nevay L., Otono H., Pandini C., Pang H., Paolozzi L., Petersen B., Pietropaolo F., Prim M., Queitsch-Maitland M., Resnati F., Rizzi C., Rokujo H., Ruiz-Choliz E., Salfeld-Nebgen J., Sato O., Scampoli P., Schmieden K., Schott M., Sfyrla A., Shively S., Spencer J., Takubo Y., Tarannum N., Theiner O., Torrence E., Tufanli S., Vasina S., Vormwald B., Wang D.

    Nuclear Instruments and Methods in Physics Research, Section A: Accelerators, Spectrometers, Detectors and Associated Equipment   1034   166825   2022年7月   （ ISSN:01689002 ）

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    記述言語：英語   掲載種別：研究論文（学術雑誌）   出版者・発行元：Nuclear Instruments and Methods in Physics Research, Section A: Accelerators, Spectrometers, Detectors and Associated Equipment  

    FASER is a new experiment designed to search for new light weakly-interacting long-lived particles (LLPs) and study high-energy neutrino interactions in the very forward region of the LHC collisions at CERN. The experimental apparatus is situated 480 m downstream of the ATLAS interaction-point aligned with the beam collision axis. The FASER detector includes four identical tracker stations constructed from silicon microstrip detectors. Three of the tracker stations form a tracking spectrometer, and enable FASER to detect the decay products of LLPs decaying inside the apparatus, whereas the fourth station is used for the neutrino analysis. The spectrometer has been installed in the LHC complex since March 2021, while the fourth station is not yet installed. FASER will start physics data taking when the LHC resumes operation in early 2022. This paper describes the design, construction and testing of the tracking spectrometer, including the associated components such as the mechanics, readout electronics, power supplies and cooling system.

    DOI： 10.1016/j.nima.2022.166825

    Scopus

  • Multiwavelength Observations of the Blazar VER J0521+211 during an Elevated TeV Gamma-Ray State 査読

    Adams, C. B. and others

    Astrophys.J.   932 ( 2 )   129 - 129   2022年6月   （ ISSN:0004-637X eISSN:1538-4357 ）

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    掲載種別：研究論文（学術雑誌）   出版者・発行元：American Astronomical Society  

    Abstract

    We report on a long-lasting, elevated gamma-ray flux state from VER J0521+211 observed by VERITAS, MAGIC, and Fermi-LAT in 2013 and 2014. The peak integral flux above 200 GeV measured with the nightly binned light curve is (8.8 ± 0.4) × 10<sup>−7</sup> photons m<sup>−2</sup> s<sup>−1</sup>, or ∼37% of the Crab Nebula flux. Multiwavelength observations from X-ray, UV, and optical instruments are also presented. A moderate correlation between the X-ray and TeV gamma-ray fluxes was observed, and the X-ray spectrum appeared harder when the flux was higher. Using the gamma-ray spectrum and four models of the extragalactic background light (EBL), a conservative 95% confidence upper limit on the redshift of the source was found to be z ≤ 0.31. Unlike the gamma-ray and X-ray bands, the optical flux did not increase significantly during the studied period compared to the archival low-state flux. The spectral variability from optical to X-ray bands suggests that the synchrotron peak of the spectral energy distribution (SED) may become broader during flaring states, which can be adequately described with a one-zone synchrotron self-Compton model varying the high-energy end of the underlying particle spectrum. The synchrotron peak frequency of the SED and the radio morphology of the jet from the MOJAVE program are consistent with the source being an intermediate-frequency-peaked BL Lac object.

    DOI： 10.3847/1538-4357/ac6dd9

    arXiv

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    その他リンク： https://iopscience.iop.org/article/10.3847/1538-4357/ac6dd9/pdf

  • Proton acceleration in thermonuclear nova explosions revealed by gamma rays 査読 国際共著

    V. A. Acciari, S. Ansoldi, L. A. Antonelli, A. Arbet Engels, M. Artero, K. Asano, D. Baack, A. Babić, A. Baquero, U. Barres de Almeida, J. A. Barrio, I. Batković, J. Becerra González, W. Bednarek, L. Bellizzi, E. Bernardini, M. Bernardos, A. Berti, J. Besenrieder, W. Bhattacharyya, C. Bigongiari, A. Biland, O. Blanch, H. Bökenkamp, G. Bonnoli, Ž. Bošnjak, G. Busetto, R. Carosi, G. Ceribella, M. Cerruti, Y. Chai, A. Chilingarian, S. Cikota, S. M. Colak, E. Colombo, J. L. Contreras, J. Cortina, S. Covino, G. D’Amico, V. D’Elia, P. Da Vela, F. Dazzi, A. De Angelis, B. De Lotto, A. Del Popolo, M. Delfino, J. Delgado, C. Delgado Mendez, D. Depaoli, F. Di Pierro, L. Di Venere, E. Do Souto Espiñeira, D. Dominis Prester, A. Donini, D. Dorner, M. Doro, D. Elsaesser, V. Fallah Ramazani, L. Fariña Alonso, A. Fattorini, M. V. Fonseca, L. Font, C. Fruck, S. Fukami, Y. Fukazawa, R. J. García López, M. Garczarczyk, S. Gasparyan, M. Gaug, N. Giglietto, F. Giordano, P. Gliwny, N. Godinović, J. G. Green, D. Green, D. Hadasch, A. Hahn, T. Hassan, L. Heckmann, J. Herrera, J. Hoang, D. Hrupec, M. Hütten, T. Inada, K. Ishio, Y. Iwamura, I. Jiménez Martínez, J. Jormanainen, L. Jouvin, D. Kerszberg, Y. Kobayashi, H. Kubo, J. Kushida, A. Lamastra, D. Lelas, F. Leone, E. Lindfors, L. Linhoff, S. Lombardi, F. Longo, R. López-Coto, M. López-Moya, A. López-Oramas, S. Loporchio, B. Machado de Oliveira Fraga, C. Maggio, P. Majumdar, M. Makariev, M. Mallamaci, G. Maneva, M. Manganaro, K. Mannheim, L. Maraschi, M. Mariotti, M. Martínez, A. Mas Aguilar, D. Mazin, S. Menchiari, S. Mender, S. Mićanović, D. Miceli, T. Miener, J. M. Miranda, R. Mirzoyan, E. Molina, A. Moralejo, D. Morcuende, V. Moreno, E. Moretti, T. Nakamori, L. Nava, V. Neustroev, M. Nievas Rosillo, C. Nigro, K. Nilsson, K. Nishijima, K. Noda, S. Nozaki, Y. Ohtani, T. Oka, J. Otero-Santos, S. Paiano, M. Palatiello, D. Paneque, R. Paoletti, J. M. Paredes, L. Pavletić, P. Peñil, M. Persic, M. Pihet, P. G. Prada Moroni, E. Prandini, C. Priyadarshi, I. Puljak, W. Rhode, M. Ribó, J. Rico, C. Righi, A. Rugliancich, N. Sahakyan, T. Saito, S. Sakurai, K. Satalecka, F. G. Saturni, B. Schleicher, K. Schmidt, T. Schweizer, J. Sitarek, I. Šnidarić, D. Sobczynska, A. Spolon, A. Stamerra, J. Strišković, D. Strom, M. Strzys, Y. Suda, T. Surić, M. Takahashi, R. Takeishi, F. Tavecchio, P. Temnikov, T. Terzić, M. Teshima, L. Tosti, S. Truzzi, A. Tutone, S. Ubach, J. van Scherpenberg, G. Vanzo, M. Vazquez Acosta, S. Ventura, V. Verguilov, C. F. Vigorito, V. Vitale, I. Vovk, M. Will, C. Wunderlich, T. Yamamoto, D. Zarić, F. Ambrosino, M. Cecconi, G. Catanzaro, C. Ferrara, A. Frasca, M. Munari, L. Giustolisi, J. Alonso-Santiago, M. Giarrusso, U. Munari, P. Valisa

    Nature Astronomy   6 ( 6 )   689 - 697   2022年4月   （ ISSN:2397-3366 eISSN:2397-3366 ）

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    記述言語：英語   掲載種別：研究論文（学術雑誌）   出版者・発行元：Springer Science and Business Media LLC  

    DOI： 10.1038/s41550-022-01640-z

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    その他リンク： https://www.nature.com/articles/s41550-022-01640-z

  • Deep-learning-driven event reconstruction applied to simulated data from a single Large-Sized Telescope of CTA

    Pietro Grespan, Ruben Lopez-Coto, Daniel Nieto-Castaño, Hyuga Abe, Arnau Aguasca, Ivan Agudo, Lucio Angelo Antonelli, Carla Aramo, Thomas Armstrong, Manuel Artero, Katsuaki Asano, Halim Ashkar, Pierre Aubert, Ali Baktash, Aya Bamba, Andres Baquero Larriva, Leonardo Baroncelli, Ulisses Barres de Almeida, Juan Abel Barrio, Ivana Batković, Josefa Becerra González, Mabel Bernardos, Alessio Berti, Noah Biederbeck, Ciro Bigongiari, Oscar Blanch, Giacomo Bonnoli, Pol Bordas, Debanjan Bose, Andrea Bulgarelli, Irene Burelli, Mario Buscemi, Martina Cardillo, Sami Caroff, Alessandro Carosi, Franca Cassol, Matteo Cerruti, Yating Chai, Ks Cheng, Michiyuki Chikawa, Ladislav Chytka, Jose Luis Contreras, Juan Cortina, Heide Costantini, Mykhailo Dalchenko, Alessandro De Angelis, Mathieu de Bony de Lavergne, Guillaume Deleglise, Carlos Delgado, Jordi Delgado Mengual, Domenico Della Volpe, Davide Depaoli, Federico Di Pierro, Leonardo Di Venere, Carlos Díaz, Rune Michael Dominik, Dijana Dominis Prester, Alice Donini, Daniela Dorner, Michele Doro, Dominik Elsässer, Gabriel Emery, Juan Escudero, Armand Fiasson, Luca Foffano, Maria Victoria Fonseca, Lluis Freixas Coromina, Satoshi Fukami, Yasushi Fukazawa, Enrique Garcia, Ramon Garcia López, Nicola Giglietto, Francesco Giordano, Pawel Gliwny, Nikola Godinović, David Green, Shuichi Gunji, Jonas Hackfeld, Daniela Hadasch, Alexander Hahn, Tarek Hassan, Kohei Hayashi, Lea Heckmann, Matthieu Heller, Javier Herrera Llorente, Kouichi Hirotani, Dirk Hoffmann, Dieter Horns, Julien Houles, Miroslav Hrabovsky, Dario Hrupec, David Hui, Moritz Hütten, Tomohiro Inada, Yusuke Inome, Maurizio Iori, Kazuma Ishio, Yuki Iwamura, Mikael Jacquemont, Irene Jimenez-Martinez, Léa Jouvin, Jakub Jurysek, Mika Kagaya, Vladimir Karas, Hideaki Katagiri, Jun Kataoka, Daniel Kerszberg, Yukiho Kobayashi, Albert Kong, Hidetoshi Kubo, Junko Kushida, Giovanni Lamanna, Alessandra Lamastra, Thierry Le Flour, Francesco Longo, Rubén López-Coto, Marcos López-Moya, Alicia López-Oramas, Pedro L. Luque-Escamilla, Pratik Majumdar, Martin MAKARIEV, Dusan Mandat, Marina Manganaro, Karl Mannheim, Mosè Mariotti, Patricia Marquez, Giovanni Marsella, Josep Martí, Oibar Martinez, Gustavo Martínez, Manel Martínez, Petra Marusevec, Alvaro Mas, Gilles Maurin, Daniel Mazin, David Medina Miranda, Enrique Mestre Guillen, Saša Mićanović, Davide Miceli, Tjark Miener, Jose Miguel Miranda, Razmik Mirzoyan, Tsunefumi Mizuno, Edgar Molina, Teresa Montaruli, Inocencio Monteiro, Abelardo Moralejo, Daniel Morcuende, Elena Moretti, Aldo Morselli, Karlo Mrakovcic, Kohta Murase, Andrii Nagai, Takeshi Nakamori, Lukas Nickel, Daniel Nieto, Mireia Nievas, Kyoshi Nishijima, Koji Noda, Dalibor Nosek, Maximilian Nöthe, Seiya Nozaki, Michiko Ohishi, Yoshiki Ohtani, Tomohiko Oka, Nao Okazaki, Akira Okumura, Reiko Orito, Jorge Otero-Santos, Michele Palatiello, David Paneque, Riccardo Paoletti, Josep Maria Paredes, Lovro Pavletić, Miroslav Pech, Mario Pecimotika, Vincent Poireau, Miguel Polo, Elisa Prandini, Julie Prast, Chaitanya Priyadarshi, Michael Prouza, Riccardo Rando, Wolgang Rhode, Marc Ribó, Vincenzo Rizi, Andrea Rugliancich, Jose Enrique Ruiz, Takayuki Saito, Shunsuke Sakurai, David Sanchez, Toni Šarić, Francesco Gabriele Saturni, Juliane Scherpenberg, Bernd Schleicher, Jan Lukas Schubert, Fabian Schüssler, Thomas Schweizer, Monica Seglar Arroyo, Ronald Cintra Shellard, Julian Sitarek, Vitalii Sliusar, Alessia Spolon, Jelena Strišković, Marcel C. Strzys, Yusuke Suda, Yuji Sunada, Hiroyasu Tajima, Mitsunari Takahashi, Hiromitsu Takahashi, Jumpei Takata, Ryuji Takeishi, P. Thomas Tam, Shuta Tanaka, Dai Tateishi, Luis Ángel Tejedor, Petar Temnikov, Yukikatsu Terada, Tomislav Terzić, Masahiro Teshima, Martin Tluczykont, Fuyuki Tokanai, Diego F. Torres, Petr Travnicek, Stefano Truzzi, Martin Vacula, Monica VAZQUEZ ACOSTA, Vassil VERGUILOV, Gaia Verna, Ilaria Viale, Carlo francesco Vigorito, Vincenzo Vitale, Ievgen Vovk, Thomas Vuillaume, Roland Walter, Martin Will, Tokonatsu Yamamoto, Ryo Yamazaki, Tatsuo Yoshida, Takanori Yoshikoshi, Darko Zarić

    Proceedings of 37th International Cosmic Ray Conference — PoS(ICRC2021)   771   2022年3月

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  • Investigating the Blazar TXS 0506+056 through Sharp Multiwavelength Eyes During 2017–2019

    Acciari, V. A. and others

    Astrophys.J.   927 ( 2 )   197 - 197   2022年3月   （ ISSN:0004-637X eISSN:1538-4357 ）

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    掲載種別：研究論文（学術雑誌）   出版者・発行元：American Astronomical Society  

    Abstract

    The blazar TXS 0506+056 got into the spotlight of the astrophysical community in 2017 September, when a high-energy neutrino detected by IceCube (IceCube-170922A) was associated at the 3σ level with a γ-ray flare from this source. This multi-messenger photon-neutrino association remains, as per today, the most significant association ever observed. TXS 0506+056 was a poorly studied object before the IceCube-170922A event. To better characterize its broadband emission, we organized a multiwavelength campaign lasting 16 months (2017 November to 2019 February), covering the radio band (Metsähovi, OVRO), the optical/UV (ASAS-SN, KVA, REM, Swift/UVOT), the X-rays (Swift/XRT, NuSTAR), the high-energy γ rays (Fermi/LAT), and the very high-energy (VHE) γ rays (MAGIC). In γ rays, the behavior of the source was significantly different from the behavior in 2017: MAGIC observations show the presence of flaring activity during 2018 December, while the source only shows an excess at the 4σ level during the rest of the campaign (74 hr of accumulated exposure); Fermi/LAT observations show several short (on a timescale of days to a week) flares, different from the long-term brightening of 2017. No significant flares are detected at lower energies. The radio light curve shows an increasing flux trend that is not seen in other wavelengths. We model the multiwavelength spectral energy distributions in a lepto-hadronic scenario, in which the hadronic emission emerges as Bethe-Heitler and pion-decay cascade in the X-rays and VHE γ rays. According to the model presented here, the 2018 December γ-ray flare was connected to a neutrino emission that was too brief and not bright enough to be detected by current neutrino instruments.

    DOI： 10.3847/1538-4357/ac531d

    arXiv

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    その他リンク： https://iopscience.iop.org/article/10.3847/1538-4357/ac531d/pdf

  • Combined searches for dark matter in dwarf spheroidal galaxies observed with the MAGIC telescopes, including new data from Coma Berenices and Draco

    V.A. Acciari, S. Ansoldi, L.A. Antonelli, A. Arbet Engels, M. Artero, K. Asano, D. Baack, A. Babić, A. Baquero, U. Barres de Almeida, J.A. Barrio, I. Batković, J. Becerra González, W. Bednarek, L. Bellizzi, E. Bernardini, M. Bernardos, A. Berti, J. Besenrieder, W. Bhattacharyya, C. Bigongiari, A. Biland, O. Blanch, H. Bökenkamp, G. Bonnoli, Ž. Bošnjak, G. Busetto, R. Carosi, G. Ceribella, M. Cerruti, Y. Chai, A. Chilingarian, S. Cikota, S.M. Colak, E. Colombo, J.L. Contreras, J. Cortina, S. Covino, G. D’Amico, V. D’Elia, P. Da Vela, F. Dazzi, A. De Angelis, B. De Lotto, M. Delfino, J. Delgado, C. Delgado Mendez, D. Depaoli, F. Di Pierro, L. Di Venere, E. Do Souto Espiñeira, D. Dominis Prester, A. Donini, D. Dorner, M. Doro, D. Elsaesser, V. Fallah Ramazani, A. Fattorini, M.V. Fonseca, L. Font, C. Fruck, S. Fukami, R.J. García López, M. Garczarczyk, S. Gasparyan, M. Gaug, N. Giglietto, F. Giordano, P. Gliwny, N. Godinović, J.G. Green, D. Green, D. Hadasch, A. Hahn, L. Heckmann, J. Herrera, J. Hoang, D. Hrupec, M. Hütten, T. Inada, K. Ishio, Y. Iwamura, I. Jiménez, J. Jormanainen, L. Jouvin, M. Karjalainen, D. Kerszberg, Y. Kobayashi, H. Kubo, J. Kushida, A. Lamastra, D. Lelas, F. Leone, E. Lindfors, L. Linhoff, S. Lombardi, F. Longo, R. López-Coto, M. López-Moya, A. López-Oramas, S. Loporchio, B. Machado de Oliveira Fraga, C. Maggio, P. Majumdar, M. Makariev, M. Mallamaci, G. Maneva, M. Manganaro, K. Mannheim, L. Maraschi, M. Mariotti, M. Martínez, D. Mazin, S. Menchiari, S. Mender, S. Mićanović, D. Miceli, T. Miener, J.M. Miranda, R. Mirzoyan, E. Molina, A. Moralejo, D. Morcuende, V. Moreno, E. Moretti, V. Neustroev, C. Nigro, K. Nilsson, D. Ninci, K. Nishijima, K. Noda, S. Nozaki, Y. Ohtani, T. Oka, J. Otero-Santos, S. Paiano, M. Palatiello, D. Paneque, R. Paoletti, J.M. Paredes, L. Pavletić, P. Peñil, M. Persic, M. Pihet, P.G. Prada Moroni, E. Prandini, C. Priyadarshi, I. Puljak, W. Rhode, M. Ribó, J. Rico, C. Righi, A. Rugliancich, L. Saha, N. Sahakyan, T. Saito, S. Sakurai, K. Satalecka, F.G. Saturni, B. Schleicher, K. Schmidt, T. Schweizer, J. Sitarek, I. Šnidarić, D. Sobczynska, A. Spolon, A. Stamerra, J. Strišković, D. Strom, M. Strzys, Y. Suda, T. Surić, M. Takahashi, R. Takeishi, F. Tavecchio, P. Temnikov, T. Terzić, M. Teshima, L. Tosti, S. Truzzi, A. Tutone, S. Ubach, J. van Scherpenberg, G. Vanzo, M. Vazquez Acosta, S. Ventura, V. Verguilov, C.F. Vigorito, V. Vitale, I. Vovk, M. Will, C. Wunderlich, D. Zarić

    Physics of the Dark Universe   35   100912 - 100912   2022年3月   （ ISSN:2212-6864 ）

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    掲載種別：研究論文（学術雑誌）   出版者・発行元：Elsevier BV  

    DOI： 10.1016/j.dark.2021.100912

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  • Multiwavelength study of the gravitationally lensed blazar QSO B0218+357 between 2016 and 2020

    Acciari, V. A. and others

    Mon.Not.Roy.Astron.Soc.   510 ( 2 )   2344 - 2362   2022年1月   （ ISSN:0035-8711 eISSN:1365-2966 ）

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    記述言語：英語   掲載種別：研究論文（学術雑誌）   出版者・発行元：Oxford University Press (OUP)  

    <title>ABSTRACT</title>
    We report multiwavelength observations of the gravitationally lensed blazar QSO B0218+357 in 2016–2020. Optical, X-ray, and GeV flares were detected. The contemporaneous MAGIC observations do not show significant very high energy (VHE; ≳100 GeV) gamma-ray emission. The lack of enhancement in radio emission measured by The Owens Valley Radio Observatory indicates the multizone nature of the emission from this object. We constrain the VHE duty cycle of the source to be &amp;lt;16 2014-like flares per year (95 per cent confidence). For the first time for this source, a broad-band low-state spectral energy distribution is constructed with a deep exposure up to the VHE range. A flux upper limit on the low-state VHE gamma-ray emission of an order of magnitude below that of the 2014 flare is determined. The X-ray data are used to fit the column density of (8.10 ± 0.93stat) × 1021 cm−2 of the dust in the lensing galaxy. VLBI observations show a clear radio core and jet components in both lensed images, yet no significant movement of the components is seen. The radio measurements are used to model the source-lens-observer geometry and determine the magnifications and time delays for both components. The quiescent emission is modelled with the high-energy bump explained as a combination of synchrotron-self-Compton and external Compton emission from a region located outside of the broad-line region. The bulk of the low-energy emission is explained as originating from a tens-of-parsecs scale jet.

    DOI： 10.1093/mnras/stab3454

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    その他リンク： https://academic.oup.com/mnras/article-pdf/510/2/2344/42556105/stab3454.pdf

  • The FASER Detector

    {FASER Collaboration} and Abreu, Henso and Mansour, Elham Amin and Antel, Claire and Ariga, Akitaka and Ariga, Tomoko and Bernlochner, Florian and Boeckh, Tobias and Boyd, Jamie and Brenner, Lydia and Cadoux, Franck and Casper, David W. and Cavanagh, Charlotte and Chen, Xin and Coccaro, Andrea and Crespo-Lopez, Olivier and Debieux, Stephane and D'Onofrio, Monica and Dougherty, Liam and Dozen, Candan and Ezzat, Abdallah and Favre, Yannick and Fellers, Deion and Feng, Jonathan L. and Ferrere, Didier and Galantay, Edward Karl and Gall, Jonathan and Gamberini, Enrico and Gibson, Stephen and Gonzalez-Sevilla, Sergio and Gwilliam, Carl and Hayakawa, Daiki and Hsu, Shih-Chieh and Hu, Zhen and Iacobucci, Giuseppe and Inada, Tomohiro and Jakobsen, Sune and Johnson, Eliott and Kajomovitz, Enrique and Kawahara, Hiroaki and Kling, Felix and Kose, Umut and Kotitsa, Rafaella and Krusse, Jesse and Kuehn, Susanne and Lefebvre, Helena and Levinson, Lorne and Li, Ke and Liu, Jinfeng and Magliocca, Chiara and Martinelli, Fulvio and McFayden, Josh and Meehan, Sam and Milanesio, Matteo and Miura, Manato and Mladenov, Dimitar and Moretti, Theo and Munker, Magdalena and Nakamura, Mitsuhiro and Nakano, Toshiyuki and Nessi, Marzio and Neuhaus, Friedemann and Nevay, Laurie and Osborne, John and Otono, Hidetoshi and Pandini, Carlo and Pang, Hao and Paolozzi, Lorenzo and Petersen, Brian and Pietropaolo, Francesco and Prim, Markus and Queitsch-Maitland, Michaela and Resnati, Filippo and Rizzi, Chiara and Rokujo, Hiroki and Ruiz-Choliz, Elisa and Salfeld-Nebgen, Jakob and Galan, Francisco Sanchez and Sato, Osamu and Scampoli, Paola and Schmieden, Kristof and Schott, Matthias and Sfyrla, Anna and Shively, Savannah and Sipos, Roland and Spencer, John and Takubo, Yosuke and Tarannum, Noshin and Theiner, Ondrej and Thonet, Pierre and Torrence, Eric and Tufanli, Serhan and Vendeuvre, Camille and Vormwald, Benedikt and Wang, Di and Zambito, Stefano and Zhang, Gang

    2022年

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    出版者・発行元：arXiv  

    FASER, the ForwArd Search ExpeRiment, is an experiment dedicated to searching for light, extremely weakly-interacting particles at CERN's Large Hadron Collider (LHC). Such particles may be produced in the very forward direction of the LHC's high-energy collisions and then decay to visible particles inside the FASER detector, which is placed 480 m downstream of the ATLAS interaction point, aligned with the beam collisions axis. FASER also includes a sub-detector, FASER$ν$, designed to detect neutrinos produced in the LHC collisions and to study their properties. In this paper, each component of the FASER detector is described in detail, as well as the installation of the experiment system and its commissioning using cosmic-rays collected in September 2021 and during the LHC pilot beam test carried out in October 2021. FASER will start taking LHC collision data in 2022, and will run throughout LHC Run 3.

    DOI： 10.48550/ARXIV.2207.11427

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  • Author Correction: Proton acceleration in thermonuclear nova explosions revealed by gamma rays (Nature Astronomy, (2022), 6, 6, (689-697), 10.1038/s41550-022-01640-z)

    Acciari, V.A., Ansoldi, S., Antonelli, L.A., Engels, A.A., Artero, M., Asano, K., Baack, D., Babi?, A., Baquero, A., de Almeida, U.B., Barrio, J.A., Batkovi?, I., Gonz{\'a}lez, J.B., Bednarek, W., Bellizzi, L., Bernardini, E., Bernardos, M., Berti, A., Besenrieder, J., Bhattacharyya, W., Bigongiari, C., Bil, , A., Blanch, O., B{\"o}kenkamp, H., Bonnoli, G., Bo?njak, ?., Busetto, G., Carosi, R., Ceribella, G., Cerruti, M., Chai, Y., Chilingarian, A., Cikota, S., Colak, S.M., Colombo, E., Contreras, J.L., Cortina, J., Covino, S., D?Amico, G., D?Elia, V., Da Vela, P., Dazzi, F., De Angelis, A., De Lotto, B., Del Popolo, A., Delfino, M., Delgado, J., Mendez, C.D., Depaoli, D., Di Pierro, F., Di Venere, L., Espi{\~n}eira, E.D.S., Prester, D.D., Donini, A., Dorner, D., Doro, M., Elsaesser, D., Ramazani, V.F., Alonso, L.F., Fattorini, A., Fonseca, M.V., Font, L., Fruck, C., Fukami, S., Fukazawa, Y., L{\'o}pez, R.J.G., Garczarczyk, M., Gasparyan, S., Gaug, M., Giglietto, N., Giordano, F., Gliwny, P., Godinovi?, N., Green, J.G., Green, D., Hadasch, D., Hahn, A., Hassan, T., Heckmann, L., Herrera, J., Hoang, J., Hrupec, D., H{\"u}tten, M., Inada, T., Ishio, K., Iwamura, Y., Mart{\'i}nez, I.J., Jormanainen, J., Jouvin, L., Kerszberg, D., Kobayashi, Y., Kubo, H., Kushida, J., Lamastra, A., Lelas, D., Leone, F., Lindfors, E., Linhoff, L., Lombardi, S., Longo, F., L{\'o}pez-Coto, R., L{\'o}pez-Moya, M., L{\'o}pez-Oramas, A., Loporchio, S., de Oliveira Fraga, B.M., Maggio, C., Majumdar, P., Makariev, M., Mallamaci, M., Maneva, G., Manganaro, M., Mannheim, K., Maraschi, L., Mariotti, M., Mart{\'i}nez, M., Aguilar, A.M., Mazin, D., Menchiari, S., Mender, S., Mi?anovi?, S., Miceli, D., Miener, T., Mir, a, J.M., Mirzoyan, R., Molina, E., Moralejo, A., Morcuende, D., Moreno, V., Moretti, E., Nakamori, T., Nava, L., Neustroev, V., Rosillo, M.N., Nigro, C., Nilsson, K., Nishijima, K., Noda, K., Nozaki, S., Ohtani, Y., Oka, T., Otero-Santos, J., Paiano, S., Palatiello, M., Paneque, D., Paoletti, R., Paredes, J.M., Pavleti?, L., Pe{\~n}il, P., Persic, M., Pihet, M., Moroni, P.G.P., Pr, ini, E., Priyadarshi, C., Puljak, I., Rhode, W., Rib{\'o}, M., Rico, J., Righi, C., Rugliancich, A., Sahakyan, N., Saito, T., Sakurai, S., Satalecka, K., Saturni, F.G., Schleicher, B., Schmidt, K., Schweizer, T., Sitarek, J., ?nidari?, I., Sobczynska, D., Spolon, A., Stamerra, A., Stri?kovi?, J., Strom, D., Strzys, M., Suda, Y., Suri?, T., Takahashi, M., Takeishi, R., Tavecchio, F., Temnikov, P., Terzi?, T., Teshima, M., Tosti, L., Truzzi, S., Tutone, A., Ubach, S., van Scherpenberg, J., Vanzo, G., Acosta, M.V., Ventura, S., Verguilov, V., Vigorito, C.F., Vitale, V., Vovk, I., Will, M., Wunderlich, C., Yamamoto, T., Zari?, D., Ambrosino, F., Cecconi, M., Catanzaro, G., Ferrara, C., Frasca, A., Munari, M., Giustolisi, L., Alonso-Santiago, J., Giarrusso, M., Munari, U., Valisa, P.

    Nature Astronomy   6 ( 6 )   760 - 760   2022年   （ ISSN:2397-3366 ）

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    掲載種別：研究論文（学術雑誌）  

    DOI： 10.1038/s41550-022-01687-y

    Scopus

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  • Observation of inverse Compton emission from a long γ-ray burst 査読 国際共著

    V. A. Acciari, S. Ansoldi, L. A. Antonelli, A. Arbet Engels, D. Baack, A. Babic, B. Banerjee, U. Barres de Almeida, J. A. Barrio, J. Becerra Gonzalez, W. Bednarek, L. Bellizzi, E. Bernardini, A. Berti, J. Besenrieder, W. Bhattacharyya, C. Bigongiari, A. Biland, O. Blanch, G. Bonnoli, Z. Bosnjak, G. Busetto, A. Carosi, R. Carosi, G. Ceribella, Y. Chai, A. Chilingaryan, S. Cikota, S. M. Colak, U. Colin, E. Colombo, J. L. Contreras, J. Cortina, S. Covino, G. D'Amico, D'Elia, V, P. Da Vela, F. Dazzi, A. De Angelis, B. De Lotto, M. Delfino, J. Delgado, D. Depaoli, F. Di Pierro, L. Di Venere, E. Do Souto Espineira, D. Dominis Prester, A. Donini, D. Dorner, M. Doro, D. Elsaesser, V. Fallah Ramazani, A. Fattorini, A. Fernandez-Barral, G. Ferrara, D. Fidalgo, L. Foffano, M. Fonseca, L. Font, C. Fruck, S. Fukami, S. Gallozzi, R. J. Garcia Lopez, M. Garczarczyk, S. Gasparyan, M. Gaug, N. Giglietto, F. Giordano, N. Godinovic, D. Green, D. Guberman, D. Hadasch, A. Hahn, J. Herrera, J. Hoang, D. Hrupec, M. Huetten, T. Inada, S. Inoue, K. Ishio, Y. Iwamura, L. Jouvin, D. Kerszberg, H. Kubo, J. Kushida, A. Lamastra, D. Lelas, F. Leone, E. Lindfors, S. Lombardi, F. Longo, M. Lopez, R. Lopez-Coto, A. Lopez-Oramas, S. Loporchio, B. Machado de Oliveira Fraga, C. Maggio, P. Majumdar, M. Makariev, M. Mallamaci, G. Maneva, M. Manganaro, K. Mannheim, L. Maraschi, M. Mariotti, M. Martinez, S. Masuda, D. Mazin, S. Micanovic, D. Miceli, M. Minev, J. M. Miranda, R. Mirzoyan, E. Molina, A. Moralejo, D. Morcuende, Moreno, V, E. Moretti, P. Munar-Adrover, Neustroev, V, C. Nigro, K. Nilsson, D. Ninci, K. Nishijima, K. Noda, L. Nogues, M. Noethe, S. Nozaki, S. Paiano, J. Palacio, M. Palatiello, D. Paneque, R. Paoletti, J. M. Paredes, P. Penil, M. Peresano, M. Persic, P. G. Prada Moroni, E. Prandini, Puljak, I, W. Rhode, M. Ribo, J. Rico, C. Righi, A. Rugliancich, L. Saha, N. Sahakyan, T. Saito, S. Sakurai, K. Satalecka, K. Schmidt, T. Schweizer, J. Sitarek, Snidaric, I, D. Sobczynska, A. Somero, A. Stamerra, D. Strom, M. Strzys, Y. Suda, T. Suric, M. Takahashi, F. Tavecchio, P. Temnikov, T. Terzic, M. Teshima, N. Torres-Alba, L. Tosti, S. Tsujimoto, V. Vagelli, J. van Scherpenberg, G. Vanzo, M. Vazquez Acosta, C. F. Vigorito, V. Vitale, Vovk, I, M. Will, D. Zaric, L. Nava

    Nature   575 ( 7783 )   459 - 463   2019年11月

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    記述言語：英語   掲載種別：研究論文（学術雑誌）  

    DOI： 10.1038/s41586-019-1754-6

  • Teraelectronvolt emission from the γ-ray burst GRB 190114C 査読 国際共著

    V. A. Acciari, S. Ansoldi, L. A. Antonelli, A. Arbet Engels, D. Baack, A. Babic, B. Banerjee, U. Barres de Almeida, J. A. Barrio, J. Becerra Gonzalez, W. Bednarek, L. Bellizzi, E. Bernardini, A. Berti, J. Besenrieder, W. Bhattacharyya, C. Bigongiari, A. Biland, O. Blanch, G. Bonnoli, Z. Bosnjak, G. Busetto, A. Carosi, R. Carosi, G. Ceribella, Y. Chai, A. Chilingaryan, S. Cikota, S. M. Colak, U. Colin, E. Colombo, J. L. Contreras, J. Cortina, S. Covino, G. D'Amico, D'Elia, V, P. Da Vela, F. Dazzi, A. De Angelis, B. De Lotto, M. Delfino, J. Delgado, D. Depaoli, F. Di Pierro, L. Di Venere, E. Do Souto Espineira, D. Dominis Prester, A. Donini, D. Dorner, M. Doro, D. Elsaesser, V. Fallah Ramazani, A. Fattorini, A. Fernandez-Barral, G. Ferrara, D. Fidalgo, L. Foffano, M. Fonseca, L. Font, C. Fruck, S. Fukami, S. Gallozzi, R. J. Garcia Lopez, M. Garczarczyk, S. Gasparyan, M. Gaug, N. Giglietto, F. Giordano, N. Godinovic, D. Green, D. Guberman, D. Hadasch, A. Hahn, J. Herrera, J. Hoang, D. Hrupec, M. Huetten, T. Inada, S. Inoue, K. Ishio, Y. Iwamura, L. Jouvin, D. Kerszberg, H. Kubo, J. Kushida, A. Lamastra, D. Lelas, F. Leone, E. Lindfors, S. Lombardi, F. Longo, M. Lopez, R. Lopez-Coto, A. Lopez-Oramas, S. Loporchio, B. Machado de Oliveira Fraga, C. Maggio, P. Majumdar, M. Makariev, M. Mallamaci, G. Maneva, M. Manganaro, K. Mannheim, L. Maraschi, M. Mariotti, M. Martinez, S. Masuda, D. Mazin, S. Micanovic, D. Miceli, M. Minev, J. M. Miranda, R. Mirzoyan, E. Molina, A. Moralejo, D. Morcuende, Moreno, V, E. Moretti, P. Munar-Adrover, Neustroev, V, C. Nigro, K. Nilsson, D. Ninci, K. Nishijima, K. Noda, L. Nogues, M. Noethe, S. Nozaki, S. Paiano, J. Palacio, M. Palatiello, D. Paneque, R. Paoletti, J. M. Paredes, P. Penil, M. Peresano, M. Persic, P. G. Prada Moroni, E. Prandini, Puljak, I, W. Rhode, M. Ribo, J. Rico, C. Righi, A. Rugliancich, L. Saha, N. Sahakyan, T. Saito, S. Sakurai, K. Satalecka, K. Schmidt, T. Schweizer, J. Sitarek, Snidaric, I, D. Sobczynska, A. Somero, A. Stamerra, D. Strom, M. Strzys, Y. Suda, T. Suric, M. Takahashi, F. Tavecchio, P. Temnikov, T. Terzic, M. Teshima, N. Torres-Alba, L. Tosti, S. Tsujimoto, V. Vagelli, J. van Scherpenberg, G. Vanzo, M. Vazquez Acosta, C. F. Vigorito, V. Vitale, Vovk, I, M. Will, D. Zaric, L. Nava

    Nature   575 ( 7783 )   455 - 458   2019年11月

    　詳細を見る

    記述言語：英語   掲載種別：研究論文（学術雑誌）  

    DOI： 10.1038/s41586-019-1750-x

▼全件表示

講演・口頭発表等

  • Recent results from FASER at CERN 招待 国際会議

    Tomohiro Inada

    12th Neutrino Oscillation Workshop 2024 (NOW 2024)   2024年9月 

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    記述言語：英語   会議種別：口頭発表（招待・特別）  

  • Indirect dark matter searches with the MAGIC telescopes 招待 国際会議

    Tomohiro Inada

    58th Rencontres de Moriond 2024  2024年3月 

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    記述言語：英語   会議種別：口頭発表（招待・特別）  

  • Early performance of the tracking detector for the FASER experiment 国際会議

    Tomohiro Inada

    13th International "Hiroshima" Symposium on the Development and Application of Semiconductor Tracking Detectors (HSTD13)   2023年12月 

    　詳細を見る

    記述言語：英語   会議種別：口頭発表（一般）  

  • First neutrino physics at colliders with FASER 招待 国際会議

    Tomohiro Inada

    Searching for long-lived particles at the LHC and beyond: Thirteenth workshop of the LLP Community  2023年6月 

    　詳細を見る

    記述言語：英語   会議種別：口頭発表（招待・特別）  

  • 天の川銀河中心領域における暗黒物質対消滅からの高エネルギーガンマ線放射の探索 招待

    稲田 知大

    高エネルギー物理学奨励賞受賞講演, 日本物理学会 2023年春季大会  2023年3月 

    　詳細を見る

    記述言語：英語   会議種別：口頭発表（基調）  

  • Dark Matter and the Galactic Centre with MAGIC 招待 国際会議

    Tomohiro Inada

    19th Rencontres du Vietnam, Theory meeting experiment : Particle astrophysics and Cosmology (TMEX-2023)  2023年1月 

    　詳細を見る

    記述言語：英語   会議種別：口頭発表（招待・特別）  

  • Looking forward to New Physics and Neutrinos with FASER at the LHC

    Tomohiro Inada

    International Conference on the Physics of the Two Infinities  2023年3月 

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    会議種別：口頭発表（一般）  

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  • Looking forward to New Physics and neutrinos with FASER at the LHC

    Tomohiro Inada

    The 8th China LHC Physics Workshop  2022年11月 

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    会議種別：口頭発表（一般）  

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  • Looking forward to New Physics and neutrinos with FASER at the LHC 招待

    Tomohiro Inada

    16th Chinese TeV Physics Working Group Symposium  2022年11月 

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    会議種別：口頭発表（基調）  

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  • Looking forward to New Physics and Neutrinos with FASER at LHC - the latest results in LHC run3 招待

    Tomohiro Inada

    Laboratoire de Physique Nucléaire et des Hautes Énergies (LPNHE) Séminaires  2025年2月 

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  • Looking forward to New Physics and Neutrinos with FASER at LHC - the latest results in LHC run3 招待

    Tomohiro Inada

    Monash University, Australia, Seminar  2023年5月 

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    会議種別：公開講演，セミナー，チュートリアル，講習，講義等  

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  • Looking forward to New Physics and Neutrinos with FASER at LHC

    Tomohiro Inada

    IHEP-CAS, Beijing, China, Seminar  2022年12月 

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    会議種別：公開講演，セミナー，チュートリアル，講習，講義等  

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  • Looking forward to New Physics and Neutrinos with FASER at LHC

    Tomohiro Inada

    清華大学 セミナー  2022年10月 

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    会議種別：公開講演，セミナー，チュートリアル，講習，講義等  

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  • Looking forward to New Physics and Neutrinos with FASER at LHC 招待

    Tomohiro Inada

    Peking University-Shanghai Jiao tong University Collider Physics Forum for Junior Scholars  2022年10月 

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  • LHC-FASER実験における高エネルギーニュートリノを用いたハドロン相互作用研究のための準備状況

    稲田知大

    日本物理学会 2022年秋季大会  2022年9月 

    　詳細を見る

  • LHC-FASER実験における衝突型加速器起源ニュートリノの初観測 招待

    稲田知大

    若手奨励賞受賞講演, 日本物理学会 2025年春季大会  2025年3月 

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  • Indirect dark matter searches with the MAGIC telescopes 招待

    Tomohiro Inada

    58th Rencontres de Moriond 2024  2024年3月 

    　詳細を見る

    会議種別：口頭発表（招待・特別）  

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  • Gamma-ray monochromatic line emission search from dark matter annihilation up to 100 TeV towards the Galactic Centre with MAGIC

    Tomohiro Inada

    7th Heidelberg international Symposium on High energy Gamma-Ray Astronomy (Gamma 2022)  2022年7月 

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    会議種別：口頭発表（一般）  

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  • First neutrino physics at colliders with FASER 招待

    Tomohiro Inada

    Searching for long-lived particles at the LHC and beyond: Thirteenth workshop of the LLP Community  2023年6月 

    　詳細を見る

    会議種別：口頭発表（基調）  

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  • FASERnuとLHCでのニュートリノ測定の将来展望

    稲田知大

    第五回 空気シャワー観測による宇宙線の起源探索勉強会  2022年3月 

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  • FASER/FPF アップグレード計画

    稲田 知大

    第5回 ITDC プラットフォームA （光検出器、シンチレータ）研究会  2024年12月 

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    会議種別：口頭発表（一般）  

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  • Dark matter searches with high-energy gamma-ray: Latest results and future prospects 招待

    Tomohiro Inada

    DM3 - Deep insights and Multiple strategies for Deciphering the Mystery of Dark Matter  2022年9月 

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    会議種別：口頭発表（基調）  

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  • Dark Matter Particle Searches and Prospects with High-Energy Gamma Rays 招待

    Tomohiro inada

    KMI2025 : The 6th KMI International Symposium  2025年3月 

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  • Dark Matter and the Galactic Centre with MAGIC 招待

    Tomohiro Inada

    19th Rencontres du Vietnam, Theory meeting experiment : Particle astrophysics and Cosmology (TMEX-2023)  2023年1月 

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    会議種別：口頭発表（基調）  

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  • Dark Matter and Cosmic ray studies with colliders and telescopes 招待

    稲田知大

    理研/京都大 知の共有ゼミ  2023年5月 

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    会議種別：公開講演，セミナー，チュートリアル，講習，講義等  

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  • Neutrinos and beyond the standard model with the FASER experiment

    稲田知大

    神戸大 セミナー  2022年9月 

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    会議種別：公開講演，セミナー，チュートリアル，講習，講義等  

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  • Recent results from FASER at CERN 招待

    Tomohiro Inada

    12th Neutrino Oscillation Workshop 2024 (NOW 2024)  2024年9月 

    　詳細を見る

  • Search for gamma-ray spectral line emission from dark matter annihilation up to 100 TeV towards the Galactic Centre with MAGIC

    Tomohiro Inada

    38th International Cosmic Ray Conference (ICRC 2023)  2023年7月 

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    会議種別：ポスター発表  

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  • Search for gamma-ray spectral line emission from dark matter annihilation up to 100 TeV towards the Galactic Centre with MAGIC

    Tomohiro Inada

    41st International Conference on High Energy Physics (ICHEP 2022)  2022年7月 

    　詳細を見る

    会議種別：口頭発表（一般）  

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  • Search for TeV-scale WIMP Dark Matter by observing Gamma rays around the Galactic Centre with the MAGIC telescopes and future prospects 招待

    Tomohiro Inada

    RIKEN iTHEMS Dark Matter WG seminar  2023年4月 

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    会議種別：公開講演，セミナー，チュートリアル，講習，講義等  

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  • Search for TeV-scale WIMP Dark Matter with High-Energy Gamma rays 招待

    Tomohiro Inada

    UC Berkley BCTP seminar  2024年11月 

    　詳細を見る

  • Search for TeV-scale WIMP Dark Matter with High-Energy Gamma rays 招待

    Tomohiro Inada

    KIPAC seminar, Stanford University,  2024年11月 

    　詳細を見る

  • Searches for TeV Dark Matter at the Galactic Centre with the MAGIC and CTA gamma-ray telescopes 招待

    Tomohiro Inada

    ICEHAP seminar, Chiba University  2024年10月 

    　詳細を見る

  • Searches for TeV Dark Matter at the Galactic Centre with the MAGIC and CTA gamma-ray telescopes 招待

    Tomohiro Inada

    Institute for Theoretical Physics, Kanazawa University  2024年11月 

    　詳細を見る

  • TeV-scale Dark Matter Searches with High-Energy Gamma Rays 招待

    Tomohiro Inada

    Kashiwa-no-ha Dark Matter and Cosmology Symposium: Satellite workshop of COSMO 2024  2024年10月 

    　詳細を見る

  • TeV-scale WIMP Dark Matter Searches by observing Very-High-Energy Gamma rays around the Galactic Centre with the MAGIC telescopes 招待

    Tomohiro Inada

    IJClab, Paris-Orsay, France, Seminar  2023年3月 

    　詳細を見る

    会議種別：公開講演，セミナー，チュートリアル，講習，講義等  

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  • The challenge for TeV-scale WIMP Dark Matter by observing Very-High-Energy Gamma rays around the Galactic Centre with the MAGIC telescopes 招待

    Tomohiro Inada

    LAPP, Annecy, France, Seminar  2023年2月 

    　詳細を見る

    会議種別：公開講演，セミナー，チュートリアル，講習，講義等  

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  • The recent status of the FASER detector

    Tomohiro Inada

    18th Vienna Conference on Instrumentation (VCI 2022)  2022年2月 

    　詳細を見る

    会議種別：口頭発表（一般）  

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  • The Run3 highlight of the FASER experiment

    Tomohiro Inada

    Tsinghua University, seminar  2024年7月 

    　詳細を見る

  • WIMP or WIMPless miracle? : Searches for TeV-scale WIMPs Dark Matter with Gamma-ray telescopes and MeV-GeV Long-Lived Particles with the LHC forward beam 招待

    Tomohiro Inada

    Kavli IPMU APEC Seminar  2022年12月 

    　詳細を見る

    会議種別：公開講演，セミナー，チュートリアル，講習，講義等  

    researchmap

  • 天の川銀河中心領域における暗黒物質対消滅からの高エネルギーガンマ線放射の探索 招待

    稲田知大

    高エネルギー物理学奨励賞受賞講演, 日本物理学会 2023年春季大会  2023年3月 

    　詳細を見る

    会議種別：口頭発表（招待・特別）  

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  • 高エネルギー宇宙ガンマ線観測による暗黒物質探索 招待

    稲田知大

    奈良女子大学 コロキウム  2023年9月 

    　詳細を見る

  • 高エネルギー宇宙線を用いた暗黒物質探索 招待

    稲田 知大

    ICEPP 夏の学校  2024年8月 

    　詳細を見る

▼全件表示

MISC

  • CERN LHC Run3におけるFASER最新結果 ビーム軸超前方での物理研究の開拓と進展 査読

    早川大樹, 稲田知大, 河原宏晃, 大橋健

    高エネルギーニュース 43(2)   2024年12月

    　詳細を見る

    担当区分：責任著者  

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  • 大気チェレンコフ望遠鏡を用いた天の川銀河中心領域におけるTeVスケール暗黒物質探索

    稲田知大

    高エネルギーニュース   42 ( 1 )   2023年4月

    　詳細を見る

    担当区分：筆頭著者,　責任著者  

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所属学協会

  • 高エネルギー物理学研究者会議 (JAHEP)

    2021年10月 - 現在

  • 宇宙線研究者会議 (CRC)

    2017年4月

  • 日本物理学会

    2015年4月 - 現在

委員歴

  • 高エネルギー物理学研究者会議   高エネルギーニュース編集委員   国内

    2023年4月   

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