JPS 77th Annual Meeting

1: XMASS: Dark matter search by using XMASS full data; ICRR The University of Tokyo^A, Kavli IPMU (WPI) The University of Tokyo^B; K. Abe^A,B, for the XMASS Collaboration
2: Progress report on PICOLON project; Tokushima Univ., Univ. of Alabama^A, RCNP Osaka Univ.^B, RCNS Tohoku Univ.^C, Osaka Sangyo Univ.^D, Tukuba Univ.^E, Kobe Univ.^G, ICRR Univ. Tokyo^H, Dept. Sci. Osaka Univ.^I, MEPhI^J, Osaka Butsuryo Univ.^K, Kavli IPMU Univ. Tokyo^L; K.Fushimi, D.Charnyak^A, H.Ejiri^B, K.Hata^C, R.Hazama^D, T.Iida^E, H.Ikeda^C, K.Imagawa^F, K.Inoue^C, H.Ishiura^G, H.Ito^H, T.Kisimoto^I, M.Koga^C, K.Kotera, A.Kozlov^J, K.Nakamura^K,L, R.Orito, T.Shima^B, Y.Takemoto^H,L, S.Umehara^B, Y.Urano, K.Yasuda^F, S.Yoshida^I
3: Background measurement results of PICOLON high-purity NaI (Tl) crystals; Tokushima Univ., Univ. of Alabama^A, RCNP Osaka Univ.^B, RCNS Tohoku Univ.^C, Osaka Sangyo Univ.^D, Tukuba Univ.^E, Kobe Univ.^G, ICRR Univ. Tokyo^H, Dept. Sci. Osaka Univ.^I, MEPhI^J, Osaka Butsuryo Univ.^K, Kavli IPMU Univ. Tokyo^L; K.Kotera, K.Fushimi, D.Charnyak^A, H.Ejiri^B, K.Hata^C, R.Hazama^D, T.Iida^E, H.Ikeda^C, K.Imagawa^F, K.Inoue^C, H.Ishiura^G, H.Ito^H, T.Kisimoto^I, M.Koga^C, A.Kozlov^J, K.Nakamura^K,L, R.Orito, T.Shima^B, Y.Takemoto^H,L, S.Umehara^B, Y.Urano, K.Yasuda^F, S.Yoshida^I
4: NEWAGE65: Direction-sensitive dark matter search in a surface laboratory using large volume gaseous TPC; Kobe Univ.; Satoshi Higashino, Kentaro Miuchi, Hirohisa Ishiura, Ryo Kubota, Ayaka Nakayama
5: NEWAGE66:Shield Development for Reducing Background Events in Dark Matter Search Using Large Gas TPC; Kobe University; Ayaka Nakayama, Kentaro Miuchi, Satoshi Higashino, Hirohisa Ishiura, Ryo Kubota
6: NEWAGE67: Development of a Low BG μ-PIC for internal background reduction of NEWAGE; Kobe Univ., Kyoto Univ.^A, ICRR^B, Tokyo Univ. of Scie.^C, Tohoku Univ.^D, Waseda Univ.^E; ISHIURA Hirohisa, MIUCHI Kentaro, IKEDA Tomonori^A, HIGASHINO Satoshi, KUBOTA Ryo,NAKAYAMA Ayaka, ABE Ko^B, ITO Hiroshi^C, NAKAMURA Kiseki^D, ICHIMURA Koichi^D, KOBAYASHI Kazuyoshi^E

7: Directional Dark Matter Search Project NEWSdm(1)～overall status～; Toho University, Nagoya University^A, IMASS Nagoya University^B, Gran Sasso National Laboratory^C, Tsukuba University^D, Isotope center Chiba University^E, Kanagawa University^F; Tatsuhiro Naka, Ryuta Kobayashi^A, Takuya Shiraishi, Hitoshi Oshima, Kana Saeki, Saya Akamatsu, Hiroaki Morisaki,Takashi Asada^C, Atsuhiro Umemoto^D, Osamu Sato^B, Toshiyuki Nakano^A, Ken'ichi Kuge^E, Yasushi Hoshino^F and NEWSdm collaboration
8: Directional Dark Matter Search Project NEWSdm(2)～data taking status of underground experiment～; Graduate School of Science Nagoya University, Graduate School of Science Toho University^A, Laboratori Nazionali del Gran Sasso^B, Graduate School of Science Kanagawa University^C, IMASS Nagoya University^D, Tsukuba University^E, Chiba University Isotope^F; Ryuta Kobayashi, Tatsuhiro Naka^A, Hitoshi Oshima^A, Takashi Asada^B, Takuya Shiraishi^A, Kana Saeki^A, Hiroaki Morisaki^A, Saya Akamatsu^A, Yasushi Hoshino^C, Osamu Sato^D, Atsuhiro Umemoto^E, Ken'ichi Kuge^F, Toshiyuki Nakano, and NEWSdm collaboration
9: Directional Dark Matter Search Project NEWSdm(3)～Data analysis report of the LNGS underground experiment～; Graduate School of Science Toho University, Graduate School of Science Nagoya University^A, Laboratori Nazionali del Gran Sasso^B, Graduate School of Science Kanagawa University^C, IMASS Nagoya University^D, Tsukuba University^E, Chiba University Isotope^F; Hitoshi Oshima, Tatsuhiro Naka, Ryuta Kobayashi^A, Takashi Asada^B, Takuya Shiraishi, Kana Saeki, Hiroaki Morisaki, Saya Akamatsu, Yasushi Hoshino^C, Osamu Sato^D, Atsuhiro Umemoto^E, Ken'ichi Kuge^F, Toshiyuki Nakano^A, and NEWSdm collaboration
10: Environmental Neutron Measurement with Ultra Fine-grained Nuclear Emulsion (1) - Improvement of recoil proton analysis and status report of Gran Sasso run; Graduate School of Science Toho University, Laboratori Nazionali del Gran Sasso^A, Graduate School of Science Nagoya University^B, IMASS Nagoya University^C, Chiba University Isotope^D, and NEWSdm collaboration; Saya Akamatsu, Takuya Shiraishi, Tatsuhiro Naka, Takashi Asada^A, Ryuta Kobayashi^B, Kana Saeki, Hiroaki Morisaki, Osamu Sato^C, Ken'ichi Kuge^D, and NEWSdm collaboration
11: Environmental Neutron Measurement with Ultra Fine-grained Nuclear Emulsion (2) - Physical analysis of Gran Sasso run; Graduate School of Science Toho University, Laboratori Nazionali del Gran Sasso^A, Graduate School of Science Nagoya University^B, IMASS Nagoya University^C, Chiba University Isotope^D, and NEWSdm collaboration; Takuya Shiraishi, Saya Akamatsu, Tatsuhiro Naka, Takashi Asada^A, Ryuta Kobayashi^B, Kana Saeki, Hiroaki Morisaki, Osamu Sato^C, Ken'ichi Kuge^D, and NEWSdm collaboration
12: Model dependence of directional direct detection of up-scattered dark matter; Okayama Univ. of Sci., Kobe Univ.^A, Toho Univ.^B; Keiko I. Nagao, Satoshi Higashino^A, Tatsuhiro Naka^B, Kentaro Miuchi^A
13: Dark matter indirect detection using Radio and Gamma ray; School of Science UTokyo, ICEPP UTokyo^A; Chikara Kawai, Shoji Asai, Toshio Namba^A

1: Parametrized Post-Newtonian test of strong gravity around the massive black hole at our galactic center, II; Daido Univ., Miyagi U. of Edu.^A, Nat'l Astro. Obs. of Jpn.^B, Wakayama NCT^C, Aichi U. of Edu.^D; Hiromi SAIDA, Shogo NISHIYAMA^A, Takayuki OHGAMI^B, Yosuke TAKAMORI^C, Masaaki TAKAHASHI^D, Members of our KAKENHIs and Subaru telescope proposals
2: Superradiant instability of Myers-Perry black strings; Rikkyo University, University of Southampton^A, Nihon University^B, University of Cambridge^C, University of Barcelona^D; Takaaki Ishii, Oscar J. C. Dias^A, ^○Keiju Murata^B, Jorge E. Santos^C, Benson Way^D
3: Helical black strings from superradiant instability; Rikkyo University, University of Southampton^A, Nihon University^B, University of Cambridge^C, University of Barcelona^D; Takaaki Ishii, Oscar J. C. Dias^A, Keiju Murata^B, Jorge E. Santos^C, Benson Way^D
4: Gravastars as nontopological soliton stars; Osaka City University; Tatsuya Ogawa, Hideki Ishihara, Yota Endo, Ryo Kato
5: Stability Analysis of Non-Topological Soliton Stars; Dept. of Phys. Osaka City Univ.^A, NITEP^B, OCAMI^C; Y.Endo^A，T.Ogawa^A,C，R.Kato^A,C，H.Ishihara^A,B,C
6: Circular propagation of sound in gravitational analogy of Superfluid ⁴He Suction Vortex; Osaka City University; Ayaka Sata, Tatsuya Ogawa, Hideki Ishihara

7: On gravity-induced decoherence; OCAMI^A, Kobe U.^B; Hirotaka Yoshino^A,B, Jiro Soda^B
8: Formal Solutions of Any-Order Mass, Angular-Momentum, and Dipole Perturbations on the Schwarzschild Background Spacetime; NAOJ; Kouji Nakamura
9: Generalized Sultana-Dyer spacetime; Rikkyo Univ.^A, Hokkai-Gakuen^B; Takuma Sato^A, Tomohiro Harada^A, Hideki Maeda^B
10: Behavior of deflection angle of light around a photon sphere; Hirosaki Univ.; Ryuya Kudo, Hideki Asada
11: Pair Creation and Entanglement Structure in the Analogous Spacetime; Nagoya University, Nagoya University^A; Yuki Osawa, Yasusada Nambu^A
12: Asymptotic behavior of photon surface near future null infinity; YITP Kyoto Univ., KMI Nagoya Univ.^A, Grad. Sch. of Math. Nagoya Univ.^B, Matsuyama Univ.^C, OCAMI^D, Kobe Univ.^E; Masaya Amo, Keisuke Izumi^A,B, Tetsuya Shiromizu^B,A, Yoshimune Tomikawa^C, Hirotaka Yoshino^D,E
13: Gravothermal instabilities in AdS spacetime; Dept. of Phys., Nagoya Univ.; Hiroki Asami

1: Inflationary phase transient process -a possible connection with dark energy-; Ochanomizu University; Masahiro Morikawa
^●2: Geometrical destabilization of multi-scalar-gauge inflation; Kobe University; Chong-Bin Chen, Jiro Soda
3: Nature of Kerr AdS₅ Black Hole based on the Numerical Analysis of the Quasi Normal Mode; Kyushu Univ., Riken^A; Issei Koga, Naritaka Oshita^A, ^○Kazushige Ueda
4: Catalysis of 5D rotating black hole and creation of inflationary universe; Kyushu Univ.，Riken^A; Issei Koga，Naritaka Oshita^A，Kazushige Ueda
5: Distribution of effective spins and mass ratios for PBH binaries with effects of critical phenomena; Nagoya U., Rikkyo U.^A, Nagoya U. KMI^B; Yasutaka Koga, Tomohiro Harada^A, Yuichiro Tada, Shuichiro Yokoyama^B, Chul-Moon Yoo
6: Gravitational lens on de Sitter backgrounds; Hirosaki Univ.; Keita Takizawa, Hideki Asada

1: CTA Report 188: General Report; ICRR, U. Tokyo^A, Max-Planck-Inst. Phys.^B, Grad. Sch. Sci., Kyoto U.^C, Grad. Sch. Sci., U. Tokyo^D, Sch. Sci., Tokai U.^E, ISEE, Nagoya U.^F, RIKEN^G, Fac. Sci.&Eng., Konan U.^H, Grad. Sch. Advanced Sci.&Eng., Hiroshima U.^I, Grad. Sch. Sci., Nagoya U.^J, Fac. Sci., Yamagata U.^K, LEDC., Yamanashi Gakuin U.^L, Col. Sci., Ibaraki U.^M, Col. Sci., Rikkyo U.^N, Grad. Sch. Sci., Osaka U.^O, YITP, Kyoto U.^P, Astrophys, U. Lodz^Q, WISE, Waseda U.^R, Grad. Sch. Sci.&Eng., Saitama U.^S, IPNS, KEK^T, HASC, Hiroshima U.^U, Fac. Eng., U. Miyazaki^V, Fac. Med. Eng.&Tech., Kitasato U.^W, KMI, Nagoya U.^X, Grad. Sch. Sci.&Tech., Tokushima U^Y, Fac. Sci.&Eng., Aoyama Gakuin U.^Z, Grad. Sch. Sci.&Tech., Kumamoto U.^AA, Astro. Inst., Tohoku U.^AB; Koji Noda^A, Masahiro Teshima^A,B, Hidetoshi Kubo^C, Tomonori Totani^D, Hyuga Abe^A, Kazuki Abe^E, Shotaro Abe^A, Katsuaki Asano^A, Kyosuke Awai^A, Aya Bamba^D, Bang Sunghyun^F, Maxim Barkov^G, Joshua Ryo Baxter^A, Giovanni Ceribella^A, K. S. Cheng^A, Michiyuki Chikawa^H, Xiaohong Cui^A, Timur Dzhatdoev^A, Gilles Ferrand^G, Yutaka Fujita^A, Satoshi Fukami^A, Yasushi Fukazawa^I, Yasuo Fukui^J, Shuichi Gunji^K, Daniela Hadasch^A, Junya Haga^F, Satoshi Hara^L, Kazuaki Hashiyama^A, Yudai Hatsutori^M, Takahiro Hayakawa^J, Katsuhiro Hayashi^A, Kohei Hayashi^A, Masaaki Hayashida^N, Haoning He^G, Akihide Hiramatsu^E, Nagisa Hiroshima^A, Kouichi Hirotani^A, David C. Y. Hui^A, Moritz Hütten^A, Ryo Imazawa^I, Tomohiro Inada^A, Yusuke Inome^A, Susumu Inoue^G, Tsuyoshi Inoue^H, Yoshiyuki Inoue^O, Kunihito Ioka^P, Kazuma Ishio^A,Q, Wataru Ishizaki^P, Yuki Iwamura^A, Hiromu Iwasaki^C, Jumpei Takata^A, Mika Kagaya^A, Shotaro Kanamori^A, Hideaki Katagiri^M, Jun Kataoka^R, Satoru Katsuda^S, Norita Kawanaka^C, Emil Khalikov^A, Shota Kisaka^I, Yukiho Kobayashi^A, Kazunori Kohri^T, Albert K. H. Kong^A, Junko Kushida^E, Shiu-Hang (Herman) Lee^C, Pratik Majumdar^A, Hironori Matsumoto^O, Daniel Mazin^A,B, Masataka Miwa^A, Masaya Mizote^H, Tsunefumi Mizuno^U, Koji Mori^V, Hiroshi Muraishi^W, Kohta Murase^A, Hiromu Nagasawa^C, Shigehiro Nagataki^G, Tsuguya Naito^L, Takeshi Nakamori^K, Kazunori Nakayama^D, Kyoshi Nishijima^E, Seiya Nozaki^C, Yutaka Ohira^D, Michiko Ohishi^A, Hideyuki Ohoka^A, Yoshiki Ohtani^A, Tomohiko Oka^C, Nao Okazaki^A, Akira Okumura^F,X, Reiko Orito^Y, Ellis R. Owen^A, Takayuki Saito^A, Naoto Sakaki^G, Kanta Sakamoto^K, Shunsuke Sakurai^A, Hidetoshi Sano^A, Nobuaki Sasaki^S, Yuri Sato^Z, Makoto Sawada^G, Marcel Strzys^A, Yusuke Suda^I, Yuji Sunada^S, Hiromasa Suzuki^H, Kengo Tachihara^J, Hiroyasu Tajima^F, Hiromitsu Takahashi^I, Keitaro Takahashi^AA, Mitsunari Takahashi^F, Ryuji Takeishi^A, Thomas P. H. Tam^A, Kiji Tanabe^M, Manobu Tanaka^T, Shuta Tanaka^Z, Takaaki Tanaka^H, Dai Tateishi^S, Yukikatsu Terada^S, Kenta Terauchi^C, Wenwu Tian^A, Fuyuki Tokanai^K, Kenji Toma^AB, Takeshi Tsuru^C, Yasunobu Uchiyama^N, Ievgen Vovk^A, Kaori Wakazono^F, Donald Warren^G, Hiroaki Yamamoto^J, Tokonatsu Yamamoto^H, Yumiko Yamane^J, Ryo Yamazaki^Z, Shohei Yanagita^M, Atsumasa Yoshida^Z, Tatsuo Yoshida^M, Takanori Yoshikoshi^A
2: CTA Report 189: Detection of the gamma-ray signal above 20 GeV with the LST-1 for the Cherenkov Telescope Array; Grad. Sch. Sci., Kyoto U., ICRR, U. Tokyo^A, Fac. Sci.&Eng., Konan U.^B, Fac. Sci., Yamagata U.^C, ISEE, Nagoya U.^D, Sch. Sci., Tokai U.^E, Grad. Sch. Advanced Sci.&Eng., Hiroshima U.^F, Col. Sci., Ibaraki U.^G, Max-Planck-Inst. Phys.^H, KMI, Nagoya U.^I, Grad. Sch. Sci.&Tech., Tokushima U.^J, Grad. Sch. Sci.&Eng., Saitama U.^K; Seiya Nozaki, Hyuga Abe^A, Shotaro Abe^A, Joshua Ryo Baxter^A, Michiyuki Chikawa^B, Satoshi Fukami^A, Shuichi Gunji^C, Daniela Hadasch^A, Junya Haga^D, Kazuaki Hashiyama^A, Akihide Hiramatsu^E, Moritz Hütten^A, Ryo Imazawa^F, Tomohiro Inada^A, Yuki Iwamura^A, Hideaki Katagiri^G, Yukiho Kobayashi^A, Hidetoshi Kubo, Junko Kushida^E, Daniel Mazin^A,H, Takeshi Nakamori^C, Kyoshi Nishijima^E, Koji Noda^A, Michiko Ohishi^A, Yoshiki Ohtani^A, Tomohiko Oka, Akira Okumura^D,I, Reiko Orito^J, Takayuki Saito^A, Shunsuke Sakurai^A, Marcel Strzys^A, Yusuke Suda^F, Hiroyasu Tajima^D, Mitsunari Takahashi^D, Ryuji Takeishi^A, Dai Tateishi^K, Yukikatsu Terada^K, Kenta Terauchi, Masahiro Teshima^A,H, Ievgen Vovk^A, Tokonatsu Yamamoto^B, Tatsuo Yoshida^G, Takanori Yoshikoshi^A, for the CTA LST Project
3: CTA report 190: Analysis of the CTA-LST prototype observations of the nova RS Ophiuchi; ICRR, U. Tokyo^A, Fac. Sci., Yamagata U.^B, ISEE, Nagoya U.^C, Sch. Sci., Tokai U.^D, Grad. Sch. Advanced Sci. & Eng., Hiroshima U.^E, Col. Sci., Ibaraki U.^F, Grad. Sch. Sci., Kyoto U.^G, Max-Planck-Inst. Phys.^H, KMI, Nagoya U.^I, Grad. Sch. Sci. & Tech., Tokushima U.^J, Grad. Sch. Sci. & Eng., Saitama U.^K, Fac. Sci. & Eng., Konan U.^L; Yukiho Kobayashi^A, Hyuga Abe^A, Shotaro Abe^A, Joshua Ryo Baxter^A, Michiyuki Chikawa^A, Satoshi Fukami^A, Shuichi Gunji^B, Daniela Hadasch^A, Junya Haga^C, Kazuaki Hashiyama^A, Akihide Hiramatsu^D, Moritz Hütten^A, Ryo Imazawa^E, Tomohiro Inada^A, Yuki Iwamura^A, Hideaki Katagiri^F, Hidetoshi Kubo^G, Junko Kushida^D, Daniel Mazin^A,H, Takeshi Nakamori^B, Kyoshi Nishijima^D, Koji Noda^A, Seiya Nozaki^G, Michiko Ohishi^A, Yoshiki Ohtani^A, Tomohiko Oka^G, Akira Okumura^C,I, Reiko Orito^J, Takayuki Saito^A, Shunsuke Sakurai^A, Marcel Strzys^A, Yusuke Suda^E, Hiroyasu Tajima^C, Mitsunari Takahashi^A, Ryuji Takeishi^A, Dai Tateishi^K, Yukikatsu Terada^K, Kenta Terauchi, Masahiro Teshima^A,H, Ievgen Vovk^A, Tokonatsu Yamamoto^L, Tatsuo Yoshida^F, Takanori Yoshikoshi^A, for the CTA LST Project
4: CTA Report 191: Performance Study of CTA-LST-1 Large-Zenith-Angle Technique; ICRR, U. Tokyo^A, Fac. Sci., Yamagata U.^B, ISEE, Nagoya U.^C, Sch. Sci., Tokai U.^D, Grad. Sch. Advanced Sci. & Eng., Hiroshima U.^E, Col. Sci., Ibaraki U.^F, Grad. Sch. Sci., Kyoto U.^G, Max-Planck-Inst. Phys.^H, KMI, Nagoya U.^I, Grad. Sch. Sci. & Tech., Tokushima U.^J, Grad. Sch. Sci. & Eng., Saitama U.^K, Fac. Sci. & Eng., Konan U.^L; Shotaro Abe^A, Hyuga Abe^A, Joshua Ryo Baxter^A, Michiyuki Chikawa^A, Satoshi Fukami^A, Shuichi Gunji^B, Daniela Hadasch^A, Junya Haga^C, Kazuaki Hashiyama^A, Akihide Hiramatsu^D, Moritz Hütten^A, Ryo Imazawa^E, Tomohiro Inada^A, Yuki Iwamura^A, Hideaki Katagiri^F, Yukiho Kobayashi^A, Hidetoshi Kubo^G, Junko Kushida^D, Daniel Mazin^A,H, Takeshi Nakamori^B, Kyoshi Nishijima^D, Koji Noda^A, Seiya Nozaki^G, Michiko Ohishi^A, Yoshiki Ohtani^A, Tomohiko Oka^G, Akira Okumura^C,I, Reiko Orito^J, Takayuki Saito^A, Shunsuke Sakurai^A, Marcel Strzys^A, Yusuke Suda^E, Hiroyasu Tajima^C, Mitsunari Takahashi^A, Ryuji Takeishi^A, Dai Tateishi^K, Yukikatsu Terada^K, Kenta Terauchi, Masahiro Teshima^A,H, Ievgen Vovk^A, Tokonatsu Yamamoto^L, Tatsuo Yoshida^F, Takanori Yoshikoshi^A, for the CTA LST Project
5: CTA Report 192: Study of the combined analysis method of the CTA-LST prototype and the MAGIC telescopes (2); ICRR, U. Tokyo^A, Fac. Sci., Yamagata U.^B, ISEE, Nagoya U.^C, Sch. Sci., Tokai U.^D, Grad. Sch. Advanced Sci.&Eng., Hiroshima U.^E, Col. Sci., Ibaraki U.^F, Grad. Sch. Sci., Kyoto U.^G, Max-Planck-Inst. Phys.^H, KMI, Nagoya U.^I, Grad. Sch. Sci.&Tech., Tokushima U.^J, Grad. Sch. Sci.&Eng., Saitama U.^K, Fac. Sci.&Eng., Konan U.^L; Yoshiki Ohtani^A, Hyuga Abe^A, Shotaro Abe^A, Joshua Ryo Baxter^A, Michiyuki Chikawa^A, Satoshi Fukami^A, Shuichi Gunji^B, Daniela Hadasch^A, Junya Haga^C, Kazuaki Hashiyama^A, Akihide Hiramatsu^D, Moriz Hütten^A, Ryo Imazawa^E, Tomohiro Inada^A, Yuki Iwamura^A, Hideaki Katagiri^F, Yukiho Kobayashi^A, Hidetoshi Kubo^G, Junko Kushida^D, Daniel Mazin^A,H, Takeshi Nakamori^B, Kyoshi Nishijima^D, Koji Noda^A, Seiya Nozaki^G, Michiko Ohishi^A, Tomohiko Oka^G, Akira Okumura^C,I, Reiko Orito^J, Takayuki Saito^A, Shunsuke Sakurai^A, Marcel Strzys^A, Yusuke Suda^E, Hiroyasu Tajima^C, Mitsunari Takahashi^A, Ryuji Takeishi^A, Dai Tateishi^K, Yukikatsu Terada^K, Kenta Terauchi^G, Masahiro Teshima^A,H, Ievgen Vovk^A, Tokonatsu Yamamoto^L, Tatsuo Yoshida^F, Takanori Yoshikoshi^A, for the CTA LST Project and the MAGIC Collaboration
6: CTA Report 193: Implementation status report and performance estimation of the new hardware trigger-based system between the first CTA large size telescope and the MAGIC telescopes; ICRR, U. Tokyo^A, Fac. Sci., Yamagata U.^B, ISEE, Nagoya U.^C, Sch. Sci., Tokai U.^D, Grad. Sch. Advanced Sci. & Eng., Hiroshima U.^E, Col. Sci., Ibaraki U.^F, Grad. Sch. Sci., Kyoto U.^G, Max-Planck-Inst. Phys.^H, KMI, Nagoya U.^I, Grad. Sch. Sci. & Tech., Tokushima U.^J, Grad. Sch. Sci. & Eng., Saitama U.^K, Fac. Sci. & Eng., Konan U.^L, UCM. Madrid, Spain.^M, INFN. Pisa, Italy^N; Joshua Ryo Baxter^A, Shotaro Abe^A, Hyuga Abe^A, Alejandro Perez Aguilera^M, Juan Abel Barrio^M, Massimiliano Bitossi^N, Michiyuki Chikawa^A, Satoshi Fukami^A, Shuichi Gunji^B, Daniela Hadasch^A, Junya Haga^C, Kazuaki Hashiyama^A, Akihide Hiramatsu^D, Moritz Hütten^A, Ryo Imazawa^E, Tomohiro Inada^A, Yuki Iwamura^A, Hideaki Katagiri^F, Yukiho Kobayashi^A, Hidetoshi Kubo^G, Junko Kushida^D, Daniel Mazin^A,H, Takeshi Nakamori^B, Kyoshi Nishijima^D, Koji Noda^A, Seiya Nozaki^G, Michiko Ohishi^A, Yoshiki Ohtani^A, Tomohiko Oka^G, Akira Okumura^C,I, Reiko Orito^J, Riccardo Paoletti^N, Takayuki Saito^A, Shunsuke Sakurai^A, Marcel Strzys^A, Yusuke Suda^E, Hiroyasu Tajima^C, Mitsunari Takahashi^A, Ryuji Takeishi^A, Dai Tateishi^K, Yukikatsu Terada^K, Kenta Terauchi, Masahiro Teshima^A,H, Ievgen Vovk^A, Tokonatsu Yamamoto^L, Tatsuo Yoshida^F, Seokhyum Yoo^G, Takanori Yoshikoshi^A, for the CTA LST Project, the MAGIC Collaboration

^●7: MAGIC report 82: A robust lower bound on intergalactic magnetic fields from Fermi/LAT and MAGIC observations of 1ES 0229+200; ICRR，U. Tokyo^A，Grad. Sch. Advanced Sci. and Eng.，Hiroshima U.^B，Grad. Sch. Sci.，Kyoto U.^C，Sch. Sci.，Tokai U.^D，Max-Planck-Inst. Phys.^E，Fac. Sci.，Yamagata U.^F，Fac. Sci. and Eng.，Konan U.^G，Universite de Paris，CNRS^H，Laboratory of Astrophysics，EPFL^I，Institute for Nuclear Research of the Russian Academy of Sciences^J，National Research Nuclear University MEPHI^K，Novosibirsk State University^L，INAF^M，INFN^N，Innsbruck U.^O; I. Vovk^A，A. Stamerra^M，P. Da Vela^N，O，A. Neronov^H，I，D. Semikoz^H，J，K，A. Korochkin^H，J，L，K. Asano^A，G. Ceribella^A，Y. Fukazawa^B，D. Hadasch^A，M. Huetten^A，T. Inada^A，Y. Iwamura^A，Y. Kobayashi^A，H. Kubo^C，J. Kushida^D，D. Mazin^A，E，T. Nakamori^F，K. Nishijima^D，K. Noda^A，S. Nozaki^C，Y. Ohtani^A，T. Oka^C，T. Saito^A，S. Sakurai^A，J. Sitarek^A，M. Strzys^A，Y. Suda^B，M. Takahashi^A，R. Takeishi^A，M. Teshima^A，E，T. Yamamoto^G，The MAGIC Collaboration
8: Recent Activity of the H.E.S.S. Japan Team; Konan Univ., Rikkyo Univ.^A, Kavli IPMU^B, RIKEN^C; Takaaki Tanaka, Dmitry Khangulyan^A, Hiromasa Suzuki, Tadayuki Takahashi^B, Naomi Tsuji^C, Yasunobu Uchiyama^A
9: Multiwavelength observations of the massive stellar cluster W43/HESS J1848−018; RIKEN, Konan Univ.^A, MPIK^B, IFJ-PAN^C, DESY^D, DIAS^E; Naomi Tsuji, Takaaki Tanaka^A, Felix Aharonian^B, Giada Peron^B, Sabrina Casanova^C, Emma de Ona Wilhelmi^D, Davit Zargaryan^E, H.E.S.S. Collaboration
^●10: Study of new transient gamma-ray sources with H.E.S.S.; Rikkyo Univ.; Dmitry Khangulyan，H.E.S.S. Collaboration
11: Gas and Cosmic-Ray Properties in the MBM 53, 54, and 55 Molecular Clouds and the Pegasus Loop as Revealed by HI Line Profiles, Dust, and Gamma-Ray Data; Hiroshima University, ISAS/JAXA^A，Chicago University^B, Stanford University^C，MPE^D，Nagoya University^E; Tsunefumi Mizuno，Katsuhiro Hayashi^A，Jessica Metzger^B，Igor Moskalenko^C，Elena Orlando^C，Andrew Strong^D, Hiroaki Yamamoto^E
12: CTA report 194: Status of the development of the PMT camera for CTA LST2-4; ICRR, U.of Tokyo^A, Fac. Sci., Yamagata U.^B, Col. Sci., Ibaraki U.^C, Grad. Sch. Sci., Kyoto U.^D, Sch. Sci.,Tokai U.^E, Max-Planck-Inst. Phys.^F, ISEE, Nagoya U.^G, KMI, Nagoya U.^H, Grad. Sch. Sci. Tech., Tokushima U.^I, Grad. Sch. Sci. and Eng., Saitama U.^J, IPNS, KEK^K, Fac. Sci. Eng., Konan U.^L; H. Abe^A, K. Hashiyama^A, S. Gunji^B, D. Hadasch^A, Y. Inome^A, Y. Iwamura^A, H. Iwasaki^D, H. Katagiri^C, H. Kubo^D, J. Kushida^E, D. Mazin^A,F, T. Nakamori^B, K. Nishijima^E, K. Noda^A, Y. Nogami^C, S. Nozaki^D, H. Ohoka^A, T. Oka^D, N. Okazaki^A, A. Okumura^G,H, R. Orito^I, T. Saito^A, S. Sakurai^A, N. Sasaki^J, Y. Sunada^J, Mitsunari Takahashi^A, M. Tanaka^K, D. Tateishi^J, Y. Terada^J, K. Terauchi^D, M. Teshima^A,F, F. Tokanai^B, T. Yamamoto^L, T. Yoshida^C, for the CTA-Japan Consortium
13: CTA report 195: Measurement of the magnetic field dependence of the response of the PMT for the CTA Large Size Telescope; Grad. Sch. Sci. &Eng., Saitama U^A, ICRR, U.of Tokyo^B, Fac. Sci., Yamagata U.^C, Col. Sci., Ibaraki U.^D, Grad. Sch. Sci., Kyoto U.^E, Grad. Sch. Sci. &Tech., Tokai U^F, Max-Planck-Inst. Phys.^G, ISEE, Nagoya U.^H, KMI, Nagoya U.^I, Grad. Sch. Sci. Tech., Tokushima U.^J, IPNS, KEK^K, Fac. Sci. &Eng., Konan U.^L; D. Tateishi^A, Y. Kobayashi^B, Y. Sunada^A, N. Sasaki^A, T. Saito^B, Y. Terada^A, S. Katsuda^A, S. Gunji^C, D. Hadasch^B, Y. Inome^B, Y. Iwamura^B, H. Katagiri^D, H. Kubo^E, J. Kushida^F, D. Mazin^B, T. Nakamori^C, K. Nishijima^F, K. Noda^B, Y. Nogami^D, S. Nozaki^E, H. Ohoka^B, T. Oka^E, N. Okazaki^B, A. Okumura^H,I, R. Orito^J, S. Sakurai^B, M. Takahashi^B, R. Takeishi^B, M. Tanaka^K, M. Teshima^B,G, F. Tokanai^C, T. Yamamoto^L, and T.Yoshida^D for the CTA-Japan Consortium

1: Current status and future of SK-Gd; ICRR; Kei Ieki on behalf of the SK collaboration
^●2: EGADS/HEIMDALL - a galactic core collapse supernova detector.; Yokohama National University; Lluis Marti-Magro
3: Calibration of energy scale uncertainly based on understanding of Super-Kamiokande detector elements; ICRR; K. Shimizu，K. Hiraide，Y. Nakano，M. Shiozawa，Super-Kamiokande Collaboration
4: Study for top-bottom-asymmetry of detector response in Super-Kamiokande; Tokyo U. of Science, ICRR, U. of Tokyo^A; N.Shigeta, M.Ishitsuka, H.Sekiya, Y.Nakano, Super-Kamiokande Collaboration
5: Evaluation of the energy scale for Super-Kamiokande Gadolinium experiment by Nitrogen-16 decay; ICRR; Y.Kanemura, H.Sekiya, Y.Nakano, Super-Kamiokande collaboration
6: Study of energy scale calibration using spallation neutron capture signals from cosmic ray muons in SK-Gd; UTokyo, TUS, ICRR; Shizuka Shima, Yasuhiro Nakajima, Masataka Shinoki, Super-Kamiokande Collaboration

7: Evaluation of the neutron detection efficiency for the SK-Gd experiment using Am/Be source; Okayama Univ., ICRR^A, Univ. of Tokyo^B, Kyoto Univ.^C; Masayuki Harada, Yusuke Koshio, Han Seungho^A, Shuhei Watanabe^A, Takatomi Yano^A, Kimihiro Okumura^A, Hiroyuki Sekiya^A, Shigetaka Moriyama^A, Yasuhiro Nakajima^B, Roger Wendell^C, for the Super-Kamiokande Collaboration
8: A quenching factor measurement for BGO scintillators; Tokyo Univ. of Science, Yokohama National Univ.^A, ICRR^B; Y.Ommura, M.Ishizuka, H.Ito, A.Minamino^A, K.Wada^A, T.Yano^B
9: A study of AmBe neutron source using NaI(Tl) scintillation detector; Yokohama National Univ., Tokyo Univ. of Science^A, ICRR^B; K.Wada, A.Minamino, H.Ito^A, M.Ishizuka^A, Y.Ommura^A, T.Yano^B
10: Status of the spin-polarization measurement of cosmic-ray muons with the Super-Kamiokande detector; Okayama Univ., ICRR^A; Hussain Kitagawa, Yuuki Nakano^A, Yusuke Koshio, for the Super-Kamiokande collaboration
^●11: Super-Kamiokande Supernova monitoring upgrade with Gd neutron capture; University of Tokyo，Okayama University^A; Guillaume Pronost，Yuri Kashiwagi，Hiroyuki Sekiya，Yusuke Koshio^A，Motoyasu Ikeda，for the Super-Kamiokande Collaboration
12: Detector Simulation using Supernova Models for Supernova Burst Alert by Super-Kamiokande; ICRR, Okayama Univ.^A; Yuri Kashiwagi, Hiroyuki Sekiya, Yusuke Koshio^A, Guillaume Pronost, Motoyasu Ikeda, for the Super-Kamiokande Collaboration
13: Study of the reaction between supernova neutrinos and oxygen nuclei in SK-Gd; Okayama Univ., ICRR^A; Fumi Nakanishi, Yusuke Koshio, Hiroyuki Sekiya^A, Yuri Kashiwagi^A, Guillaume Pronost^A, Motoyasu Ikeda^A, for the Super-Kamiokande Collaboration

1: （Invited Presentation.）; Mitsuhiro Kato
2: （Invited Presentation.） A new search method for axion dark matter by using the birefringence effect; MPA; Ippei Obata
3: （Invited Presentation.） Topology-changing horizons at large D as Ricci flows; Toyota Tech. Inst.; Ryotaku Suzuki
4: （Invited Presentation.） 't Hooft surface operators in five dimensions and elliptic ruijsenaars operators; Tokyo Inst. Tech.; Yutaka Yoshida

5: （Lecture of the Young Scientist Award of JPS） Report of the Selection Committee; Univ. Tokyo; Yoshio Kikukawa
6: （Lecture of the Young Scientist Award of JPS） AdS/CFT Correspondence from Surface/State; Univ. California, Berkely; Masamichi Miyaji
7: （Lecture of the Young Scientist Award of JPS） Studies on defect C-theorem; Tohoku U.; Yoshiki Sato
8: （Lecture of the Young Scientist Award of JPS） Generalized Higgs effective field theory and perturbative unitarity; Osaka U.; Ryo Nagai

1: Development of ultra-low radioactivity type 5A zeolite for removing radon; CST-Nihon-U, U-Tokyo^A, ICRR^B, Kobe-U^C, Osaka-U^D; Hiroshi Ogawa, Kenta Iyogi^A, Minoru Matsukura^A, Toru Wakihara^A, Ko Abe^B, Kentaro Miuchi^C, Saori Umehara^D
^●2: XENONnT and its Neutron Veto Technology; Kavli IPMU，The University of Tokyo; Kai Martens
3: XENONnT: measurement of environmental tritium for further understanding of low energy ER background; ISEE, Nagoya University; Masatoshi Kobayashi^A，Ko Abe^B，Yoshitaka Itow^A,C, Shingo Kazama^A,C，Nobuyuki Kato^B，Yasuo Takeuchi^D，Atsushi Takeda^B,E，Tuan Khai Bui^E，Takeshi Maeda^D，Kai Martens^E，Kentaro Miuchi^D，Keita Mizukoshi^D，Shigetaka Moriyama^B,E，Masaki Yamashita^B,E，Hideki Kakiuchi^F for XENON Collaboration
4: Neutron beam test results for observation of Migdal effect using xenon gas detector; Tohoku University, Kobe University^A, Kyoto University^B; Kiseki Nakamura, Kei Kanezaki^A, Takeki Uchiyama, Kentaro Miuchi^A, Satoshi Higashino^A, Keita Mizukoshi^A, Tomonori Ikeda^B
5: Neutron beam test results for observation of Migdal effect using argon gas TPC; Kobe University, Tohoku University^A, Kyoto University^B; Kei Kanezaki, Kiseki Nakamura^A, Takeki Uchiyama^A, Kentaro Miuchi, Satoshi Higashino, Keita Mizukoshi, Tomonori Ikeda^B
6: Development of hermetic LXe TPC for the DARWIN experiment; Nagoya University, KMI; Shingo Kazama
7: Development of new electrodes with low quantum efficiency for the DARWIN experiment; Nagoya University, ISEE; Naoki Aoyama

1: Evolution of Primordial Fluctuations in Squeezed States; Kobe U, Kyushu U^A; Jiro Soda, Sugumi Kanno^A
2: Indirect detection of gravitons through quantum entanglement; Kyushu, Kobe^A; Sugumi Kanno, Jiro Soda, Junsei Tokuda
3: Particle motion in AdS spacetime and its Holographic dual; Rikkyo University, Waseda University^A, Takushoku University^B; Tomotaka Kitamura, ^○Shoichiro Miyashita^A, Yasuhiro Sekino^B
4: Quantum gravity witness using quantum clock; Nagoya Univ.; Youka Kaku, Yuhki Osawa, Shin'ya Maeda, Yasusada Nambu
5: Quantum gravity witness by Leggett-Garg inequality for oscillator; NU; Shin'ya Maeda, Yasusada Nambu, Youka Kaku, Yuki Osawa
6: False Vacuum Decay with Stationary Shells in Kerr Spacetimes; Dept. of Phys. Nagoya U.; Daiki Saito, Chul-Moon Yoo

7: Classification of the conformal boundaries of the FLRW solutions: linear equations of state II; Rikkyo U, KEK^A, QMUL^B; Tomohiro Harada, Takahisa Igata^A, Takuma Sato, Bernard Carr^B
8: Propagation of perturbations for a stealth black hole in DHOST theories; NIT, Kochi College^A，Rikkyo Univ.^B，Kogakuin Univ.^C，YITP^D; Keisuke Nakashi^A,B，Masashi Kimura^B，Hayato Motohashi^C，Kazufumi Takahashi^D
9: New analysis on gravitational perturbations of higher-dimensional rotating black holes; National Institute of Technology, Maizuru College, Chuo University^A, Setsunan University^B; Tsuyoshi Houri, Norihiro Tanahashi^A, Yukinori Yasui^B
10: Periapsis/apoapsis shift in static clouds around a black hole; KEK IPNS, Rikkyo U.^A, Daido U.^B, Wakayama KOSEN^C; Takahisa Igata, Tomohiro Harada^A, Hiromi Saida^B, Yohsuke Takamori^C
11: Squashed black holes at large D; Toyota Technological Institute; Ryotaku Suzuki, Shinya Tomizawa
12: Can we detect the signature of axion clouds in black hole binaries?; Kyoto University; T.Takahashi, H.Omiya, T.Tanaka
13: Charged hairy anti-de Sitter black holes in the Robin boundary; Department of Physics, Rikkyo University, Faculty of Science and Engineering, Chuo University^A; Takaaki Ishii, ^○Takuya Katagiri, Norihiro Tanahashi^A, Tomohiro Harada

1: Topological defects in nonlocal field theories; Tokyo Tech, NORDITA^A; Luca Buoninfante^A, ^○Yuichi Miyashita, Masahide Yamaguchi
2: Gravitational waves of Cartan formalism in F(R) modified gravity theory; Hiroshima Univ. Adv Sci and Eng., Hiroshima Univ. IMC.^A; Taniguchi Masahiko, Inagaki Tomohiro^A
3: Photon multiple scatterings in relativistic flows; NIT, Tomakomai College^A, University of Tsukuba^B; Rohta Takahashi^A, Masayuki Umemura^B, Ken Ohsuga^B, Yuta Asahina^B
4: Fundamental tone and overtones of quasinormal modes in ringdown gravitatiional waves; Kyoto Univ., Osaka City Univ., Univ. of Southampton^A, Ryukoku Univ.^B; Norichika Sago, Soichiro Isoyama^A, Hiroyuki Nakano^B
5: General-relativistic neutrino-radiation magnetohydrodynamics simulation of black hole-neutron star mergers for seconds; YITP^A, AEI^B, Kyoto Univ.^C, Toho Univ.^D; Kota Hayashi^A, Sho Fujibayashi^B, Kenta Kiuchi^B, Koutarou Kyutoku^C, Yuichiro Sekiguchi^D, Masaru Shibata^A,B
6: Dependence of the nuclear composition of the ejecta from binary neutron star mergers on the binary mass ratio; AEI, Toho U^A; Sho Fujibayashi, Shinya Wanajo, Kenta Kiuchi, Masaru Shibata, Yuichiro Sekiguchi^A

7: The r-process in the ejecta from binary neutron star or neutron star-black hole mergers; AEI^A, Kyoto U^B, Toho U^C; Shinya Wanajo^A, Sho Fujibayashi^A, Kota Hayashi^B, Kenta Kiuchi^A, Koutarou Kyutoku^B, Yuichiro Sekiguchi^C, Masaru Shibata^A
8: Theoretical interpretation of very-high-energy gamma-ray afterglows for low-luminosity GRB 190829A; Aoyama Gakuin U., Penn State^A, Grad. Sch. Sci., U. Tokyo^B; Y. Sato, K. Obayashi, R. Yamazaki, K. Murase^A, Y. Ohira^B, S.J. Tanaka
9: Strong magnetic field sustained by the elastic force in neutron star crust; Dept. of Phys., Ad. Sci. and Eng., Hiroshima Univ., RESCU, Univ. of Tokyo^A; Yasufumi Kojima, Shota Kisaka, Kotaro Fujisawa^A
10: Dynamics of solar magnetic field described by the macroscopic spin model; Kyoto Sangyo Univ., Ochanomizu Univ.^A; Akika NAKAMICHI, Masahiro MORIKAWA^A

1: Observation of very-high-energy gamma-ray sources with the Tibet air shower array (5); ICRR, Univ. of Tokyo, Dept. of Phys., Hirosaki Univ.^A, Dept. of Phys., Shinshu Univ.^B, Fac. of Engn., Yokohama Natl. Univ.^C, Fac. of Engn., Kanagawa Univ.^D, Utsunomiya Univ.^E, Shibaura Inst. of Tech.^F, ROIS^H, Coll. of Ind. Tech., Nihon Univ.^I, NII^J, NICT^K, Tokyo Metro. Coll. of Ind. Tech.^L, Dept. of Phys., Konan Univ.^M, Shonan Inst. of Tech.^N, Res. Inst. for Sci. and Engn., Waseda^O, JAEA^P; S. Kato, M. Amenomori^A, S. Asano^B, A. Gomi^C, K. Hibino^D, N. Hotta^E, K. Kasahara^F, Y. Katayose^C, C. Kato^B, T. Kawashima, K. Kawata, M. Kozai^H, D. Kurashige^C, K. Munakata^B, K. Nagaya^C, Y. Nakamura, Y. Nakazawa^I, H. Nanjo^A, M. Nishizawa^J, M. Ohnishi, S. Okukawa^C, S. Ozawa^K, T. Saito^L, Y. Sakakibara^C, M. Sakata^M, T. Sako, T. K. Sako, M. Shibata^C, A. Shiomi^I, H. Sugimoto^N, W. Takano^D, M. Takita, N. Tateyama^D, S. Torii^O, H. Tsuchiya^P, S. Udo^D, Y. Yokoe et al. (The Tibet ASγ Collaboration)
2: ALPACA experiment 24 : Current status and construction plan in 2022; ICRR, Univ. of Tokyo^A, Dept. of Phys., Shinshu Univ.^B, IIF, UMSA^C, Univ. de Guadalajara^D, Fac. of Engn., Yokohama Natl. Univ.^E, Fac. of Engn., Kanagawa Univ.^F, Utsunomiya Univ.^G, Coll. of Engn., Chubu Univ.^H, Astro. Obs., Chubu Univ.^I, Grad. Sch. of Sci., Osaka City Univ.^J, NITEP, Osaka City Univ.^K, Coll. of Ind. Tech., Nihon Univ.^L, NII^M, Tokyo Metro. Coll. of Ind. Tech.^N, RIKEN^O, Fac. of Engn., Osaka Electro-Comm. Univ.^P, Fac. of Info. Sci., Hiroshima City Univ.^Q, JAEA^R; T. Sako^A, M. Anzorena^A, S. Asano^B, C. A. H. Condori^C, E. de la Fuente^D, A. Gomi^E, K. Hibino^F, N. Hotta^G, Y. Katayose^E, C. Kato^B, S. Kato^A, T. Kawashima^A, K. Kawata^A, T. Koi^H, H. Kojima^I, D. Kurashige^E, J. Lozoya^D, R. Mayta^J,K, P. Miranda^C, K. Munakata^B, K. Nagaya^E, Y. Nakamura^A, Y. Nakazawa^L, C. Nina^C, M. Nishizawa^M, S. Ogio^J,K, M. Ohnishi^A, S. Okukawa^E, F. Orozco^D, A. Oshima^H, M. Raljevich^C, H. Rivera^C, T. Saito^N, Y. Sakakibara^E, T. K. Sako^A, S. Shibata^I, A. Shiomi^L, M. Subieta^C, N. Tajima^O, W. Takano^F, M. Takita^A, Y. Tameda^P, K. Tanaka^Q, R. Ticona^C, I. Toledano-Juarez^D, H. Torres^D, H. Tsuchiya^R, Y. Tsunesada^J,K, S. Udo^F, K. Yamazaki^H, Y. Yokoe^A et al. (The ALPACA Collaboration)
3: ALPACA experiment 25 : Simulation study for the ALPACA experiment; ICRR, Univ. of Tokyo^A, Dept. of Phys., Shinshu Univ.^B, IIF, UMSA^C, Univ. de Guadalajara^D, Fac. of Engn., Yokohama Natl. Univ.^E, Fac. of Engn., Kanagawa Univ.^F, Utsunomiya Univ.^G, Coll. of Engn., Chubu Univ.^H, Astro. Obs., Chubu Univ.^I, Grad. Sch. of Sci., Osaka City Univ.^J, NITEP, Osaka City Univ.^K, Coll. of Ind. Tech., Nihon Univ.^L, NII^M, Tokyo Metro. Coll. of Ind. Tech.^N, RIKEN^O, Fac. of Engn., Osaka Electro-Comm. Univ.^P, Fac. of Info. Sci., Hiroshima City Univ.^Q, JAEA^R; Y. Yokoe^A, M. Anzorena^A, S. Asano^B, C. A. H. Condori^C, E. de la Fuente^D, A. Gomi^E, K. Hibino^F, N. Hotta^G, Y. Katayose^E, C. Kato^B, S. Kato^A, T. Kawashima^A, K. Kawata^A, T. Koi^H, H. Kojima^I, D. Kurashige^E, J. Lozoya^D, R. Mayta^J,K, P. Miranda^C, K. Munakata^B, K. Nagaya^E, Y. Nakamura^A, Y. Nakazawa^L, C. Nina^C, M. Nishizawa^M, S. Ogio^J,K, M. Ohnishi^A, S. Okukawa^E, F. Orozco^D, A. Oshima^H, M. Raljevich^C, H. Rivera^C, T. Saito^N, Y. Sakakibara^E, T. Sako^A, T. K. Sako^A, S. Shibata^I, A. Shiomi^L, M. Subieta^C, N. Tajima^O, W. Takano^F, M. Takita^A, Y. Tameda^P, K. Tanaka^Q, R. Ticona^C, I. Toledano-Juarez^D, H. Torres^D, H. Tsuchiya^R, Y. Tsunesada^J,K, S. Udo^F, K. Yamazaki^H, et al. (The ALPACA Collaboration)
4: ALPACA experiment 26 : Systematic uncertainty in cosmic gamma ray flux depending on hadronic interaction model; Fac. of Engn., Yokohama Natl. Univ., ICRR, Univ. of Tokyo^A, Dept. of Phys., Shinshu Univ.^B, IIF, UMSA^C, Univ. de Guadalajara^D, Fac. of Engn., Kanagawa Univ.^F, Utsunomiya Univ.^G, Coll. of Engn., Chubu Univ.^H, Astro. Obs., Chubu Univ.^I, Grad. Sch. of Sci., Osaka City Univ.^J, NITEP, Osaka City Univ.^K, Coll. of Ind. Tech., Nihon Univ.^L, NII^M, Tokyo Metro. Coll. of Ind. Tech.^N, RIKEN^O, Fac. of Engn., Osaka Electro-Comm. Univ.^P, Fac. of Info. Sci., Hiroshima City Univ.^Q, JAEA^R; S. Okukawa, M. Anzorena^A, S. Asano^B, C. A. H. Condori^C, E. de la Fuente^D, A. Gomi, K. Hibino^F, N. Hotta^G, Y. Katayose, C. Kato^B, S. Kato^A, T. Kawashima^A, K. Kawata^A, T. Koi^H, H. Kojima^I, D. Kurashige, J. Lozoya^D, R. Mayta^J,K, P. Miranda^C, K. Munakata^B, K. Nagaya, Y. Nakamura^A, Y. Nakazawa^L, C. Nina^C, M. Nishizawa^M, S. Ogio^J,K, M. Ohnishi^A, F. Orozco^D, A. Oshima^H, M. Raljevich^C, H. Rivera^C, T. Saito^N, Y. Sakakibara, T. Sako^A, T. K. Sako^A, S. Shibata^I, A. Shiomi^L, M. Subieta^C, N. Tajima^O, W. Takano^F, M. Takita^A, Y. Tameda^P, K. Tanaka^Q, R. Ticona^C, I. Toledano-Juarez^D, H. Torres^D, H. Tsuchiya^R, Y. Tsunesada^J,K, S. Udo^F, K. Yamazaki^H, Y. Yokoe^A et al. (The ALPACA Collaboration)
5: ALPACA experiment 27：Expanding the dynamic range of photomultiplier tube; ICRR, Univ. of Tokyo, Dept. of Phys., Shinshu Univ.^A, IIF, UMSA^B, Univ. de Guadalajara^C, Fac. of Engn., Yokohama Natl. Univ.^D, Fac. of Engn., Kanagawa Univ.^E, Utsunomiya Univ.^F, Coll. of Engn., Chubu Univ.^G, Astro. Obs., Chubu Univ.^H, Grad. Sch. of Sci., Osaka City Univ.^I, NITEP, Osaka City Univ.^J, Coll. of Ind. Tech., Nihon Univ.^K, NII^L, Tokyo Metro. Coll. of Ind. Tech.^M, RIKEN^N, Fac. of Engn., Osaka Electro-Comm. Univ.^O, Fac. of Info. Sci., Hiroshima City Univ.^P, JAEA^Q; T. Kawashima, M. Anzorena, S. Asano^A, C. A. H. Condori^B, E. de la Fuente^C, A. Gomi^D, K. Hibino^E, N. Hotta^F, Y. Katayose^D, C. Kato^A, S. Kato, K. Kawata, T. Koi^G, H. Kojima^H, D. Kurashige^D, J. Lozoya^C, R. Mayta^I,J, P. Miranda^B, K. Munakata^A, K. Nagaya^D, Y. Nakamura, Y. Nakazawa^K, C. Nina^B, M. Nishizawa^L, S. Ogio^I,J, M. Ohnishi, S. Okukawa^D, F. Orozco^C, A. Oshima^G, M. Raljevich^B, H. Rivera^B, T. Saito^M, Y. Sakakibara^D, T. Sako, T. K. Sako, S. Shibata^H, A. Shiomi^K, M. Subieta^B, N. Tajima^N, W. Takano^E, M. Takita, Y. Tameda^O, K. Tanaka^P, R. Ticona^B, I. Toledano-Juarez^C, H. Torres^C, H. Tsuchiya^Q, Y. Tsunesada^I,J, S. Udo^E, K. Yamazaki^G, Y. Yokoe et al. (The ALPACA Collaboration)
6: Calibration of 50-cm HK-PMTs in the Super-Kamiokande detector for improved single-photoelecton distribution; Nagoya Univ., ISEE Nagoya Univ., ISEE Nagoya Univ., ICRR Univ. of Tokyo, Keio Univ., Kamioka Observatory; Kotaro Ninomiya, Yoshitaka Itow, Hiroaki Menjo, Kazufumi Sato, Yasuhiro Nishimura, Yano Takatomi, The Super-Kamiokande Collaboration

7: CTA Report 196: Development of SiPM Modules for the CTA Large-Sized Telescopes; ICRR, U.of Tokyo^A, Fac. Sci., Yamagata U.^B, Col. Sci., Ibaraki U.^C, Grad. Sch. Sci., Kyoto U.^D, Sch. Sci., Tokai U.^E, Max-Planck-Inst. Phys.^F, ISEE, Nagoya U.^G, KMI, Nagoya U.^H, Grad. Sch. Sci. Tech., Tokushima U.^I, Grad. Sch. Sci. and Eng., Saitama U.^J, IPNS, KEK^K, Fac. Sci. and Eng., Konan U.^L; K. Hashiyama^A, S. Gunji^B, D. Hadasch^A, Y. Inome^A, Y. Iwamura^A, H. Iwasaki^D, H. Katagiri^C, H. Kubo^D, J. Kushida^E, D. Mazin^A,F, T. Nakamori^B, K. Nishijima^E, K. Noda^A, Y. Nogami^C, S. Nozaki^D, H. Ohoka^A, T. Oka^D, N. Okazaki^A, A. Okumura^G,H, R. Orito^I, T. Saito^A, S. Sakurai^A, N. Sasaki^J, Y. Sunada^J, Mitsunari Takahashi^A, M. Tanaka^K, D. Tateishi^J, Y. Terada^J, K. Terauchi^D, M. Teshima^A,F, F. Tokanai^B, T. Yamamoto^L, T. Yoshida^C, for the CTA-Japan Consortium
8: CTA Report 197: Simulation study of multilayer coating on light concentrators for future SiPM cameras for the CTA Large- and Medium-Sized Telescopes(2); ISEE, Nagoya U.^A, KMI, Nagoya U.^B, Tokushima U.^C, Sch. Sci. and Eng., Ibaraki U.^D, Grad. Sch. Sci., Tokai U.^E, Kyoto U.^F, Sch. Sci., Yamagata U.^G, Col. Sci., ICRR, U.of Tokyo^H, Fac. Sci., Saitama U.^I, IPNS, KEK^J, Max-Planck-Inst. Phys.^K, Konan U.^L; J. Haga^A, A. Okumura^A,B, H. Tajima^A, R. Orito^C, H. Katagiri^D, J. Kushida^E, H. Kubo^F, S. Gunji^G, T. Saito^H, N. Sasaki^H, N. Sasaki^I, Y. Sunada^I, Mitsunari Takahashi^H, D. Tateishi^I, M. Tanaka^J, M. Teshima^H,K, K. Terauchi^F, Y. Terada^I, T. Nakamori^G, K. Nishijima^E, Y. Nogami^D, S. Nozaki^F, K. Noda^H, D. Hadasch^H, D. Mazin^H,K, T. Yamamoto^L, T. Yoshida^D, for the CTA-Japan Consortium
9: CTA Report 198 : Evaluation of SiPM for the CTA Small Sized-Telescopes with the background light under the moon night observations; ISEE, Nagoya U.^A, KMI, Nagoya U.^B; Kaori Wakazono^A, Hiroyasu Tajima^A, Akira Okumura^A,B
10: Neutrino Multiplet -- A new approach to identify high-energy neutrino sources.; ICEHAP; Shigeru Yoshida, Nobuhiro Shimizu, Aya Ishihara, Kohta Murase, Masaomi Tanaka
11: Studies of the online multiplet signal for the follow up observation by optical telescopes at the IceCube neutrino observatory; Chiba Univ.; N.Shimizu, C.Hill, A.Ishihara, M.Meier, Y.Morii, R.Nagai, K.Niwano, Y.Takemasa, S.Yoshida
12: Neutrino, gamma-ray and radio emission from winds and tori of active galactic nuclei; Bunkyo U.^A, RIKEN^B, APC^C, Penn State U.^D, Nanjing U.^E; Susumu Inoue^A,B, Matteo Cerruti^C, Kohta Murase^D, Ruo-Yu Liu^E
13: Clear identification of very high energy particle sources by NTA; Univ. Tokyo ICRR, Toho Univ.^A, Univ. Hawaii Manoa^B, Univ. Hawaii Hilo^C, Nagoya Univ.^D, Chiba Univ. CEReS^E, Ibaraki Univ.^F, Kanagawa Univ.^G, Okayama Univ.^H,KEK^I, Univ. Wisconsin-Madison^J, Univ. Torino^K, NTU^L, NCTU^M, Academia Sinica^N, UIP^O; T. Aoki, P. Binder^C, T.E.Browder^C, Y. Fukasaku^A, J. Golden^C, J. Hamilton^C, T. Kimura^F, K. Kori^H, H. Kuze^E, J. Learned^B, H. Mashiyama^A, S. Matsuno^B, H. Oshima^A, ^○S. Ogawa^A, P.Doetinchem^C, M. Sasaki, H. Shibuya^A, N. Sugiyama^D, R. M. Tanaka^H, S. Yamada^A,K. Yoshimura^I, Y. Watanabe^G, F. Halzen^J,R. Mussa^K, Y.B. Hsiung^L, M.-Z. Wang^M, G.-L. Lin^M, S. Haino^N, H.A. Huang^O
14: Development of NTA for clear identification of very high energy particle sources; Univ. Tokyo ICRR, Toho Univ.^A, Univ. Hawaii Manoa^B, Univ. Hawaii Hilo^C, Nagoya Univ.^D, Chiba Univ. CEReS^E, Ibaraki Univ.^F, Kanagawa Univ.^G, Okayama Univ.^H,KEK^I, Univ. Wisconsin-Madison^J, Univ. Torino^K, NTU^L, NCTU^M, Academia Sinica^N, UIP^O; T. Aoki, P. Binder^C, T.E. Browder^C, Y. Fukasaku^A, J. Golden^C, J. Hamilton^C, T. Kimura^F,K. Kori^H, H. Kuze^E, J. Learned^B, H. Mashiyama^A, S. Matsuno^B, H. Oshima^A, ^○S. Ogawa^A, P.Doetinchem^C, M. Sasaki, H. Shibuya^A, N. Sugiyama^D, R. M. Tanaka^H, S. Yamada^A,K. Yoshimura^I, Y. Watanabe^G, F. Halzen^J, R. Mussa^K, Y.B. Hsiung^L, M.-Z. Wang^M, G.-L. Lin^M, S. Haino^N, H.A. Huang^O

1: Measurement of Gd³⁺ ion emission lifetime in aqueous solution of Gd sulfate; Japan Atomic Energy Agency, Institute for Cosmic Ray Research, the University of Tokyo^A; Yoshihiro Iwata, Hiroyuki Sekiya^A, Chikara Ito
2: Development and performance evaluation of light propagation model in water using Geant4 based simulation in Super-Kamiokande; Okayama University，Super-Kamiokande Collaboration; Tomoaki Tada, Yusuke Koshio, Super-Kamiokande Collaboration
3: Trigger optimization towards search for supernovae relic neutrinos in Super-Kamiokande experiment; Tokyo Tech, ICRR^A, Univ. of Tokyo^B; Shota Izumiyama, Yoshinari Hayato^A, Yasuhiro Nakajima^B, Masahiro Kuze, Super-Kamiokande Collaboration
4: Development of high-sensitivity radon detector in water for astroparticle physics; CRR, Kobe University^A; A.Takeda, K.Okamoto, Y.Takeuchi^A, Y.Nakano
5: Search for supernova neutrino at KamLAND; RCNS, Tohoku Univ.; Minori Eizuka, for KamLAND Collaboration
6: Long time simulation of neutrino emission from core-collapse; University of Tokyo; Masamitsu Mori, Yudai Suwa

1: Leggett-Garg inequalities in hybrid system due to gravitational interaction; Department of Physics Kyushu University, Department of Physics Nagoya University^A; Akira Matsumura, Yasusada Nambu, ^○Kazuhiro Yamamoto
2: Coherence and inseparable evolution in non-classical gravity; Faculty of Science, Kyushu Univ.; Akira Matsumura
3: Invertible disformal transformations with higher derivatives; YITP, Kogakuin Univ.^A, Univ. of Lisbon^B; Kazufumi Takahashi, Hayato Motohashi^A, Masato Minamitsuji^B
^●4: Parity-violating single-field inflation; Kobe U., TITec^A, NTHU^A, YITP^B; Pengyuan Gao, Asuka Ito^A, Jiro Soda, Kazufumi Takahashi^B
5: Mimetic K-essence; Czech Academy of Sciences^A, Tokyo Institute of Technology^B; Pavel Jirousek^A, Keigo Shimada^B, Alexander Vikman^A, Masahide Yamaguchi^B

1: Development and Milestones of the Sparse Wire Grid, polarization angle calibrator for the Simons Observatory Experiment; KyotoU, UTokyo^A, JAXA^B; H.Nakata, M.Masaaki, K.Iijima, S.Adachi, Y.Seino, K.Kiuchi, F.Matsuda, A.Kusaka, O.Tajima, SO Collaboration
2: Development status of the polarization angle calibrator for Simons Observatory; Univ. of Tokyo^A, Kyoto Univ.^B, JAXA^C, LBNL^D; Kengo Iijima^A, Masaaki Murata^A, Hironobu Nakata^B, Shunsuke Adachi^B, Kenji Kiuchi^A, Frederick Matsuda^C, Akito Kusaka^A,D, Osamu Tajima^B, Simons Observatory Collaboration
3: Optical test result of sparse wire grid calibrator for Simons Observatory experiment; UTokyo^A, KyotoU^B, JAXA^C, LBNL^D; Masaaki Murata^A, Hironobu Nakata^B, Kengo Iijima^A, Shunsuke Adachi^B, Yudai Seino^B, Kenji Kiuchi^A, Frederick Matsuda^C, Akito Kusaka^A,D, Osamu Tajima^B, Simons Observatory Collaboration
4: Evaluating HWP for search for CMB circular polarization at the POLARBEAR experiment 3; YNU, Kavil IPMU^A, NIES^B, Univ. of Tokyo^C, JASRI^D, KEK^E; Takuro Fujino, Nobuhiko Katayama^A, Satoru Takakura^B, Yuji Chinone^C, Haruki Nishino^D, Masaya Hasegawa^E, POLARBEAR Collaboration
5: Simons Array experiment, commissioning at the observation site; KEK, Kyoto U^A, NCU^B, IPMU^C, UTokyo^D, LBNL^E, SOKENDAI^F, NIES^G, NIFS^H, NAOJ^G, JASRI^H, AIST^I, YNU^J, ISAS^K, RCNP^L; Daisuke Kaneko, Shunsuke Adachi^A, Yuki Inoue^B, Nobuhiko Katayama^C, Akito Kusaka^D, Aritoki Suzuki^E, Junichi suzuki, Yudai Seino^A, Yuuko Segawa^F, Satoru Takakura^G, Suguru Takada^H, Sayuri Takatori^F, Osamu Tajima^A, Daiki Tanabe^B, Yuji Chinone^D, Takayuki Tomaru^G, Haruki Nichino^H, Yumie Nishinomiya^D, Masashi Hazumi, Masaya Hasegawa, Kaori Hattori^I, Haruaki Hirose^J, Takuro Fujino^J, Frederick Matsuda^K, Tomotake Matsumura^C, Yuto Minami^L, Masaaki Murata^D, Kyohei Yamada^D, and POLARBEAR Colllaboration
6: A noise reduction method using a broadband black-body calibration source for the Simons Array Cosmic Microwave Background Experiment; SOKENDAI, Univ. of Tokyo^A, UCB^B, KEK^C, LBNL^D, NIST^E, Kavli IPMU^F, NIES^G; S. Takatori, Y. Chinone^A, K. Crowley^B, T. de Haan^C, T. Elleflot^D, J. Groh^E, M. Hasegawa^C, M. Hazumi^C, D. Kaneko^C, N. Katayama^F, A. Suzuki^D, A. T. Lee^B, S. Takakura^G, K. Yamada^A, POLARBEAR Collaboration
7: Evaluation for the telescope boresight pointing by the observations of radio sources in Simons Array experiment; UTokyo, KEK^A, Sokendai^B, MRI^C, JASRI^D, JAXA^E; Yume Nishinomiya, Daisuke Kaneko, Akito Kusaka, Sayuri Takatori, Satoru Takakura, Yuji Chinone, Haruki Nishino, Masashi Hazumi, Masaya Hasegawa, Frederick Matsuda, Kyohei Yamada
8: The development of a polarization modulator for CMB polarimetry; UTokyo, KEK^A, Okayama Univ.^B, Kavli IPMU^C; Junna Sugiyama, Kana Sakaguri, Kyohei Yamada, Masaya Hasegawa^A, Yuki Sakurai^B, Akito Kusaka, SO collaboration

1: （Lecture of the Young Scientist Award of JPS） Explanation of JPS Young Scientist Award Selection; Hiroshima University, Hiroshima Astrophysical Science Center; Tsunefumi MIZUNO
2: （Lecture of the Young Scientist Award of JPS） Frequency-Dependent Squeezed Vacuum Source with Filter Cavity Control using Coherent Control Sidebands for Gravitational-Wave Detectors; Gravitational Wave Project Office, National Astronomical Observatory of Japan; Naoki ARITOMI
3: （Lecture of the Young Scientist Award of JPS） Study on ultrasoft outflows from active galactic nuclei and associated absorption structure in their X-ray spectra; Department of Physics, Faculty of Science and Engineering, Tokyo University of Science; Koichi HAGINO
4: （Lecture of the Young Scientist Award of JPS） Cosmological roles of gauge fields; Waseda Institute for Advanced Study, Waseda University; Tomohito FUJITA

5: Preparation status for next LHCf operation at pp collisions; ISEE, Nagoya Univ.^A，KMI, Nagoya Univ.^B，ICRR,Univ. of Tokyo^C，Shibaura Inst.Tech.^D，RISE, Waseda Univ.^E，Kanagawa Univ.^F，Tokushima Univ.^G，INFN Firenze^H，Firenze Univ.^I，Ecole Polytechnique^J，INFN Catania^K，Catania Univ.^L，LBNL^M; H. Menjo^A，Y. Itow^A,B，M. Kondo^A，K. Ohashi^A，Y. Matsubara^A，Y. Muraki^A，T. Sako^C，K. Yoshida^D，K. Kasahara^D，S. Torii^E，Y. Shimizu^F，T. Tamura^F，N. Sakurai^G, O. Adriani^H,I，E. Berti^H, L. Bonechi^H，M. Bongi^H,I，R. D'Alessandro^H,I，S. Detti^H，M. Haguenauer^J，P. Papini^H，G. Piparo^K,L，S. Ricciarini^H，M. Scaringella^H，A. Tiberio^H，A. Tricomi^K,L，W.C. Turner^M
6: Effects of experimental uncertainties in diffractive dissociation on predictions of X_MAX; ISEE, Nagoya Univ.^A, KMI, Nagoya Univ.^B, ICRR, Univ. of Tokyo^C; K. Ohashi^A, H. Menjo^A, Y. Itow^A,B, T. Sako^C
7: Estimating the statistics needed to search for mass composition anisotropy in ultra-high energy cosmic rays; Shinshu Univ., Kanagawa Univ.^A; R.Saito, T.Tomida, D.Ikeda^A
8: Observation of the proton spectrum around 100 TeV using Tibet-III and MD; Fac. of Engn., Yokohama Natl. Univ., Dept. of Phys., Hirosaki Univ.^A, Dept. of Phys., Shinshu Univ.^B, Fac. of Engn., Kanagawa Univ.^D, Utsunomiya Univ.^E, Shibaura Inst. of Tech.^F, ICRR, Univ. of Tokyo^G, ROIS^H, Coll. of Ind. Tech., Nihon Univ.^I, NII^J, NICT^K, Tokyo Metro. Coll. of Ind. Tech.^L, Dept. of Phys., Konan Univ.^M, Shonan Inst. of Tech.^N, Res. Inst. for Sci. and Engn., Waseda^O, JAEA^P; D. Kurashige, M. Amenomori^A, S. Asano^B, A. Gomi^C, K. Hibino^D, N. Hotta^E, K. Kasahara^F, Y. Katayose^C, C. Kato^B, S. Kato^G, T. Kawashima^G, K. Kawata^G, M. Kozai^H, K. Munakata^B, K. Nagaya^C, Y. Nakamura^G, Y. Nakazawa^I, H. Nanjo^A, M. Nishizawa^J, M. Ohnishi^G, S. Okukawa^C, S. Ozawa^K, T. Saito^L, Y. Sakakibara^C, M. Sakata^M, T. Sako^G, T. K. Sako^G, M. Shibata^C, A. Shiomi^I, H. Sugimoto^N, W. Takano^D, M. Takita^G, N. Tateyama^D, S. Torii^O, H. Tsuchiya^P, S. Udo^D, Y. Yokoe^G et al. (The Tibet ASγ Collaboration)
9: Large volume NaI detectors of the GRAPES-3 for detection of atmospheric gamma rays accompanying with lightning; Hiroshima City Univ., Grad. Sch. of Sci. Osaka City Univ.^A, Fac. of Engn. Aichi Inst. of Tech.^B, Tata Inst. India^C, ICRR. Univ. of Tokyo^D, Grad. Sch. of Inf. Coll. of Engn. Chubu Univ.^E, Fac. of Sci., Kochi Univ.^F, IPMU^G, Fac. Econ. Asahi Univ.^H; Taketo Hikino, N. Ito^A, T. Ueoka, T. Ueda, S. Ogio^A, S. Kawakami^A, H. Kojima^B, S. Shibata^E, H. Takamaru^E, A. Oshima^E, K. Tanaka, H. Tanaka^G
10: Arrival time distribution of electron components in the gamma-induced shower predicted by the cascade shower theory; Okayama Shoka University, Kawasaki Medical School^A; Takao Nakatsuka, Kazuhide Okei^A

1: Status of KAGRA; ICRR; Takahiro Yamamoto on behalf of the KAGRA collaboration
2: Investigation for the noise budget of KAGRA detector in the joint observation O3GK; NAOJ; Tatsuki Washimi, on behalf of the KAGRA collaboration
3: Simulation of the angular change of the mirror of the input mode cleaner in the gravitational wave telescope KAGRA; Niigata Univ., ICRR^A, Cardiff Univ.^B; Chiaki Hirose, Kenta Tanaka^A, Keiko Kokeyama^B, Osamu Miyakawa^A, Takamasa Suzuki, KAGRA collaboration
4: Alignment Sensing and Control of the input mode cleaner of KAGRA; ICRR, Grad. Sch. of Sci. and Tech., Niigata Univ.^A; K. Tanaka, C. Hirose^A, O. Miyakawa on the behalf of KAGRA collaboration
5: Improvement of vibration isolation system for KAGRA test mass towards O4　Ⅲ; ICRR, NAOJ^A; T. Sugiyama, R. Takahashi^A, N. Sato^A, T. Uchiyama, KAGRA collaboration
6: Sapphire mirror suspension control of KAGRA; Phys. S. Univ. of Tokyo, ICRR, Univ. of Tokyo^A, NAOJ^B, KAGRA collaboration^C; M. Tamaki^A, S. Miyoki^A, T. Ushiba^A, T. Yamamoto^A, K. Miyo^A, T. Tomaru^B, R. Takahashi^B, S. Ikeda^B, KAGRA collaboration^C

1: Relativistic star perturbations in Horndeski theories with a gauge-ready formulation; Waseda University, Tokyo University of Science^A; Shinji Tsujikawa, Ryotaro Kase^A
2: Distinguishing modified gravity with just two tensorial degrees of freedom from general relativity: cosmology; Rikkyo U.; Aya Iyonaga, Tsutomu Kobayashi
3: Tidal Deformation Phenomena under the F(R) Gravity; Nagoya U.^A, CCNU^B, KMI^C; K. Numajiri^A, T. Katsuragawa^B, S. Nojiri^A,C
4: cosmology with minimally modified gravity thoery; YITP; Taisuke Matsuda, Ryo Namba, Shinji Mukohyama, Paul Martens
5: Propagation of gravitational waves in Horndeski theory; YITP, KMI^A; Ke-ichiro Kubota, Shinji Mukohyama, Shun Arai^A
6: Vector-tensor theories in metric-affine formalism; Rikkyo U.; Tact Ikeda, Tsutomu Kobayashi

7: HSC cosmology: preparation of theoretical templates based on emulation; YITP Kyoto U.^A，Kavli IPMU^B，Hirosaki U.^C，NAOJ^D，Chiba U.^E，KMI Nagoya U.^F，U of Tokyo^G，Arizona U.^H; Takahiro Nishimichi^A,B，Masahiro Takada^B，Ryuichi Takahashi^C，Ken Osato^A，Masato Shirasaki^D，Taira Oogi^E，Hironao Miyatake^F，Masamune Oguri^G，Yosuke Kobayashi^H，Naoki Yoshida^G，Sunao Sugiyama^B，Satoshi Tanaka^A
8: HSC cosmology: joint analyses of galaxy-galaxy lensing and clustering of Subaru HSC and SDSS galaxy survey data; IPMU^A, Tokyo^B, Nagoya KMI^C, Nagoya IAR^D, Nagoya Phys.^E, Caltech Jet^F, Kyoto YITP^G, NAOJ^H, ISM^I, Arizona Astro.^J, IUCAA^K, Hirosaki Phys.^L, LPENS^M, RESCEU^N, Geneva^O, ASIAA^P, UC Santa Crutz Astro.^Q, CMU McWilliams Center for Cosmology^R, USTC Phys.^S, USTC Astro.^T, Princeton Astrophys.^U, UC Berkeley^V, LBNL^W, UCR^X, Tronto Stat.^Y, Tronto Dunlap Astro.^Z, Tronto David A. Dunlap Astro^AA, Princeton Astrophys.^BB; Sunao Sugiyama^A,B, Masahiro Takada^A, Hironao Miyatake^C,D,E,A,F, Takahiro Nishimichi^G, Masato Shirasaki^H,I, Yosuke Kobayashi^J,A, Rachel Mandelbaum^R, Surhud More^K,A, Ryuichi Takahashi^L, Ken Osato^G,M, Masamune Oguri^N,B,A, Jean Coupon^O, Chiaki Hikage^A, Bau-Ching Hsieh^P, Yutaka Komiyama^H, Alexie Leauthaud^Q, Xiangchong Li^R,A, Wentao Luo^S,T, Robert H. Lupton^U, Satoshi Miyazaki^H, Hitoshi Murayama^V,A,W, Atsushi J. Nishizawa^D, Youngsoo Park^A, Paul A. Price^U, Melanie Simet^X, Joshua S. Speagle^Y,Z,AA, Michael A. Strauss^BB, Masayuki Tanaka^H, Naoki Yoshida^B,A
9: HSC cosmology: Testing General Relativity with HSC-measured weak gravitational lensing; Nagoya U., KMI Nagoya U.^A, Kanagawa U.^B; Yuji Okochi, ^○Shun Arai^A, Hironao Miyatake^A, Shuichiro Yokoyama^A, Daisuke Yamauchi^B
10: HSC cosmology: toward a joint cosmology analysis of HSC weak lensing and SDSS redshift-space power spectrum; Kavli IPMU^A, Arizona U.^B, YITP Kyoto U.^C，KMI Nagoya U.^D; Masahiro Takada^A, Yosuke Kobayashi^B, Takahiro Nishimichi^C, Hironao Miyatake^D
11: Core-halo relation of fuzzy dark matter; YITP, IAP; Atsushi Taruya, Shohei Saga
12: Impacts of new small-scale N-body simulations on dark matter annihilations constrained from cosmological 21-cm line observations; U. of Toyama，iTHEMS RIKEN^A，IPNS KEK^B，SOKENDAI^C，Kavli IPMU^D，Hirosaki U.^E; Nagisa Hiroshima^A，Kazunori Kohri^B,C,D，Toyokazu Sekiguchi^B，Ryuichi Takahashi^E
13: Anisotropies in Cosmological 21 cm line Background by Oscillons of Ultra-light Axion-like Particle; Tokyo Univ. ICRR; Masahiro Kawasaki, ^○Kazuyoshi Miyazaki, Kai Murai, Hiromasa Nakatsuka, Eisuke Sonomoto

1: Development of a calibration device using blackbody radiation in the Simons Observatory experiment; Kyoto University, KEK^A; Yudai Seino, Junya Suzuki, Daisuke Kaneko^A, Masaya Hasegawa^A, Osamu Tajima, Simons Observatory collaboration
2: Full remote operation of CMB polarimeter GroundBIRD; IAC，Kyoto U^A，Tohoku U^B，RIKEN^C，SOKENDAI^D，KEK^E，JAXA^F，SRON^G，U Tokyo^H，Saitama U^I，NAOJ^J，KASI^K，Korea U^L; S. Honda，T. Ikemitsu^A，H. Ishida^B,C，H. Ishitsuka^D，T. Uchida^E,D，C. Otani^B,C，S. Oguri^F，K. Karatsu^G，K. Kiuchi^H，H. Kutsuma^B,C，J. Komine^A，R. Koyano^I，Y. Sueno^A，J. Suzuki^A，Y. Sekimoto^F，T. Taino^I，O. Tajima^A，Y. Tsuji^B,C，N. Tomita^H，M. Nagai^J，T. Nagasaki^E，M. Naruse^I，M. Hazumi^E,D，M. Hattori^B，M. Minowa^H，S. Mima^C，M. Yoshida^E,D，J. Choi^K，RT. Génova-Santos，Y. Jo^L，K. Lee^L，J. Moon^L，M. Peel，R. Rebolo，JA. Rubiño-Martín，E. Won^L
3: Calibration measurement at CMB polarization experiment “GroundBIRD” - Responsivity calibration of superconducting detector ‘MKID’.; Kyoto U，IAC^A，Tohoku U^B，RIKEN^C，SOKENDAI^D，KEK^E，JAXA^F，SRON^G，U Tokyo^H，Saitama U^I，NAOJ^J，KASI^K，Korea U^L, TU Delft^M; Y. Sueno，T. Ikemitsu，H. Ishida^B,C，H. Ishitsuka^D，T. Uchida^E,D，C. Otani^B,C，S. Oguri^F，K. Karatsu^G，K. Kiuchi^H,M，H. Kutsuma^B,C，J. Komine，R. Koyano^I，J. Suzuki，Y. Sekimoto^F，T. Taino^I，O. Tajima，Y. Tsuji^B,C，N. Tomita^H，M. Nagai^J，T. Nagasaki^E，M. Naruse^I，M. Hazumi^E,D，M. Hattori^B，S. Honda^A，S. Mima^C，M. Yoshida^E,D，J. Choi^K，RT. Génova-Santos^A，Y. Jo^L，K. Lee^L，J. Moon^L，M. Peel^A，R. Rebolo^A，JA. Rubiño-Martín^A，E. Won^L
4: Cryogenic performance evaluation of anti-reflection coatings used for Sapphire and Alumina for CMB polarimetry; UTokyo^A，KEK^B，Okayama Univ.^C，Kavli IPMU^D，Lawrence Berkeley Nat’l. Lab.^E; Kana Sakaguri^A, Junna Sugiyama^A, Masaya Hasegawa^B, Yuki Sakurai^C, Tomotake Matsumura^D, Akito Kusaka^A,D,E
5: Move
6: Analytical study of systematic errors due to gain and pointing in CMB polarization observation experiments at large angular scales; Okayama University; Koki Ishizaka, Naoya Doi, Yusuke Takase, Yuya Nagano, Hirokazu Ishino
7: A noise evaluation system of TES bolometers for the CMB polarization observation satellite LiteBIRD; Tokyo Tech^A, JAXA/ISAS^B; Ryo Masumura^A, Tadayasu Dotani^A,B, Shugo Oguri^B, Toyoaki Suzuki^B

8: Systematics study synchronized to continuously rotating half-wave plates in CMB observation satellite LiteBIRD; Okayama University, Kavli IPMU^A, The University of Tokyo^B, Saitama University^C; Yuki Sakurai, Tomotake Matsumura^A, Nobuhiko Katayama^A, Ryota Takaku^B, Kunimoto Komatsu, Shinya Sugiyama^C, Yurika Hoshino^C, Takashi Hasebe^A, Tommaso Ghigna^A
9: Effects for the CMB observation due to misalignment of crystal axis of half-wave plate installed in LiteBIRD low-frequency telescope; Saitama University, Kavli IPMU^A, Okayama University^B, University of Tokyo^C; Yurika Hoshino, Tomotake Matsumura^A, Yuki Sakurai^A, Takashi Hasebe^A, Tommaso Ghigna^A, Nobuhiko Katayama^A, Makoto Tashiro, Yukikatsu Terada, Kosuke Sato, Satoru Katsuda, Shinya Sugiyama, Kunimoto Komatsu^B, Ryota Takaku^C, LiteBIRD Joint Study Group
^●10: Cryogenic characterisation of Transition Edge Sensors for the LiteBIRD space mission and their susceptibility to cosmic rays; Okayama University^A，Kavli IPMU，the University of Tokyo^B，University of California，Berkeley^C; Samantha Lynn Stever^A,B，Tommaso Ghigna^B，Shawn Beckman^C，Ben Westbrook，Adrian Lee^C，Tomotake Matsumura^B，Hirokazu Ishino^A
11: Optimization of the full-sky observation methodology for the CMB polarimetry satellite LiteBIRD - Searching for a scanning strategy that enables systematic error suppression and calibration -; Okayama U., IRAP^A, Paris U.^B; Yusuke Takase, Léo Vacher^A, Hirokazu Ishino, Yuya Nagano, Ludovic Montier^A, Jonathan Aumont^A, Guillaume Patanchon^B, other LiteBIRD Joint Study Group
12: Study of systematic errors derived from asymmetric 4π beams and calibration accuracy in all-sky polarimetric CMB observations; Okayama Univ., IRAP^A, Paris Univ.^B; Yuya Nagano, Yusuke Takase, Hirokazu Ishino, Léo Vacher^A, L. Montier^A, J. Aumont^A, G. Patanchon^B, Other LiteBIRD Joint Study Group
13: Development of large diameter millimeter-wave low-pass filter made of alumina with laser ablated anti-reflection coating; The University of Tokyo, University of Minnesota/Twin Cities^A, University of Pennsylvania^B, i-space^C; Ryota Takaku, Qi Wen^A, Scott Cray^A, Mark Devlin^B, Simon Dicker^B, Shaul Hanany^A, Takashi Hasebe, Teruhito Iida^C, Nobuhiko Katayama, Kuniaki Konishi, Makoto Kuwata-Gonokami, Tomotake Matsumura, Norikatsu Mio, Haruyuki Sakurai, Yuki Sakurai, Ryohei Yamada, Junji Yumoto
14: A systematic effect study for the pointing error in CMB all-sky polarimetric observations with multiple detectors; Okayama University; Naoya Doi, Hirokazu Ishino, Yusuke Takase, Yuya Nagano, LiteBIRD Joint Study Group
15: Cosmic Birefringence Tomography with Ultralight Axion; ICRR, MPA^A, Kavli IPMU^B; Hiromasa Nakatsuka, Eiichiro Komatsu^A, Toshiya Namikawa^B

1: TA experiment 374：Report on the TAx4 experiment 10; RIKEN，Shinshu Univ.^A，Osaka City Univ.^B，Kanagawa Univ.^C，Yamanashi Univ.^D，Saitama Univ.^E，Kochi Univ.^F，NIRS^G，ICRR Univ. of Tokyo^H，Chubu Univ.^I，Ritsumeikan Univ.^J，Osaka Electro-Comm. Univ.^K，NICT^L，Kyushu Univ.^M，Shibaura Inst. of Tech.^N，Tokyo City Univ.^O，Chiba Univ.^P，KEK^Q，Tokyo Univ. of Science^R，ERI^S，Hiroshima City Univ.^T，Kindai^U，Kyoto Univ.^V，Ehime Univ.^W，Univ. of Utah^X，Ewha Womans Univ.^Y，Hanyang Univ.^Z，Yonsei Univ.^a，INR^b，Ulsan Nat'l. Inst. of Sci. and Tech.^c，Sungkyunkwan Univ.^d，Univ. Libre de Bruxelles^e，Rutgers Univ.^f; E. Kido，Y. Abe^A，R. Arimura^B，D. Ikeda^C，T. Ishii^D，Y. Ito，N. Inoue^E，D. Inadomi^A，K. Imaoka^F，H. Iwakura^A，A. Iwasaki^B，T. Uehama^A，Y. Uchihori^G，S. Udo^C，H. Ohoka^H，A. Oshima^I，M. Ohnishi^H，R. Onogi^B，S. Ogio^B，N. Okimoto^H，T. Okuda^J，Y. Oku^K，S. Ozawa^L，H. Oda^B，K. Ono^M，Y. Omura^B，F. Kakimoto^C，K. Kasahara^N，S. Kasami^K，K. Kadota^O，K. Kamei^F，H. Kawai^P，S. Kawakami^B，K. Kawata^H，S. Kawana^E，S. Kishigami^B，J. H. Kim^B，Y. Kubota^A，K. Saito，R. Saito^A，N. Sakaki，H. Sagawa^H，N. Sakurai^B，T. Sako^H，R. Sahara^B，Y. Shibasaki^A，T. Shibata^Q，N. Shibata^K，H. Shimodaira^H，H. Shin^H，D. Shinto^K，T. Suzawa^E，T. Seki^A，K. Sekino^H，Y. Takagi^B，K. Takahashi^H，Y. Takahashi^B，M. Takamura^R，M. Takita^H，K. Takakuwa^A，R. Takeishi^H，A. Taketa^S，M. Takeda^H，K. Tanaka^T，H. Tanaka^B，M. Tanaka^Q，Y. Tanoue^B，Y. Tameda^K，M. Chikawa^H，J. Chiba^R，M. Tsujimoto^R，Y. Tsunesada^B，H. Tokuno^H，T. Tomida^A，K. Nakai^B，A. Nakazawa^A，S. Nagataki，K. Nakada^E，T. Nakamura^A，T. Nakamura^F，R. Nakamura^A，E. Nishio^K，D. Nishimoto^A，A. Nozato^U，T. Nonaka^H，M. Hayashi^A，Y. Hayashi^B，N. Hayashida^C，R. Higuchi^H，R. Hibi^A，K. Hibino^C，M. Fukushima^H，T. Fujii^V，K. Fujisue^H，K. Fujita^B，R. Fujiwara^B，K. Honda^D，R. Mayta^B，H. Mashiyama^E, T. Matsudaira^F，H. Matsumiya^B，T. Matuyama^B，K. Yashiro^R，K. Yada^H，H.;Yamaoka^Q，K. Yamazaki^I，M. Yamamoto^A，M. Yosei^K, N. Yoshii^W，F. Yoshida^K，R. U. Abbasi^X，T. Abu-Zayyad^X，M. Allen^X，R. Anderson^X，E. Barcikowski^X，J. W. Belz^X，D. R. Bergman^X，S. A. Blake^X，R. Cady^X，B. G. Cheon^Z，A. di Matteo^e，W. Hanlon^X，D. Ivanov^X，H. M. Jeong^d，S. Jeong^d，C. C. H. Jui^X，O. Kalashev^b，H. B. Kim^Z，J. H. Kim^X，V. Kuzmin^b，M. Kuznetsov^b，Y. J. Kwon^Z，K. H. Lee^d，B.;Lubsandorzhiev^b，J. P. Lundquist^X，J. N. Matthews^X，I. Myers^X，I. H. Park^d，M. S. Piskunov^d，M. S. Pshirkov^e，J. Remington^X，D. C. Rodriguez^X，G. I. Rubtsov^b，D. Ryu^c，L. M. Scott^f，P. D. Shah^X，B. K. Shin^Z，J. D. Smith^X，P. Sokolsky^X，B. T. Stokes^X，S. R. Stratton^X,f，T. A. Stroman^X，S. B. Thomas^X，G. B. Thomson^X，P. Tinyakov^b,e，I. Tkachev^b，S. Troitsky^b，F. Urban^e，T. Wong^X，J. Yang^Y，Y. Zhezher^b，Z. Zundel^X
2: TA experiment 375 : Monte Carlo simulation for TAx4-SD array analysis 4; ICRR, Osaka City Univ.^A, Ritsumeikan Univ.^B, Riken^C, Sungkyunkwan Univ.^D, etc.; K. Fujisue, H. Ohoka, S. Ogio^A, T. Okuda^B, K. Kawata, E. Kido^C, N. Sakaki^C, H. Sagawa, T. Sako, T. Nonaka, H. Jeong^D, and Telescope Array Collaboration
3: TA experiment 376: General report 7 of TALE experiment; Osaka City Univ., ICRR^A, Osaka Electro-Communication Univ.^B, Shinsyu U.^C, Kanagawa Univ.^D, Kyoto Univ.^E, Riken^F, Ritsumeikan Univ.^G; R. Arimura, K. Fujita, S. Ogio, M. Takeda^A, Y. Tameda^B, T. Tomida^C, S. Udo^D, T. Fujii^E, D. Ikeda^D, E. Kido^F, T. Nonaka^A, H. Ohoka^A, T. Okuda^G, H. Sagawa^A, N. Sakaki^F, Y. Tsunesada for the Telescope Array Collaboration
4: TA experiment 377: Current status of the TALE infill SD production and measurement accuracy of the TALE infill hybrid detector; Osaka City Univ., ICRR^A, Osaka Electro-Communication Univ.^B, Shinsyu U.^C, Kanagawa Univ.^D, Kyoto Univ.^E, Riken^F, Ritsumeikan Univ.^G; A. Iwasaki, K. Fujita, S. Ogio, Y. Tameda^B, T. Tomida^C, S. Udo^D, T. Fujii^E, D. Ikeda^D, E. Kido^F, T. Nonaka^A, H. Ohoka^A, T. Okuda^G, H. Sagawa^A, N. Sakaki^F and Y. Tsunesada for the Telescope Array Collaboration
5: TA experiment 378: Measurement of optical properties of atmospheric fluorescence telescope using UAV-mounted light source; Shinsyu U., Osaka Electro-Communication Univ.^A, Kanagawa Univ.^B; T. Tomida, A. Nakazawa, Y Tameda^A, R. Hibi, M. Kai, D. Ikeda^B, for the Telescope Array Collaboration
6: TA experiment 379 : Analysis of Fluorescence Detector events with Hybrid trigger (V); ICRR Univ. of Tokyo, etc.; H.S.Shin, for the Telescope Array Collaboration

7: TA experiment 380: The Cosmic Ray Spectrum and Mass Composition as measured by the TALE Hybrid Detector (2); Osaka City Univ., Kanagawa Univ.^A, ICRR^B, Osaka Electro-Communication Univ.^C, Ritsumeikan Univ.^D, Kyoto Univ.^E Riken^F, Shinsyu U.^G; K.Fujita, S.Ogio, Y.Tsunesada, S.Udo^A, D.Ikeda^A, H.Ohoka^B, H.Sagawa^B, T.Nonaka^B, Y.Tameda^C, T.Okuda^D, T.Fujii^E, E.Kido^F, N.Sakaki^F, T.Tomida^G, for the Telescope Array Collaboration
8: TA experiment 381: jNICHE - Energy spectrum and composition analysis of cosmic rays measured with the NICHE detectors at the TA site; Osaka City Univ., Univ. of Utah^A, UMD^B; Y. Omura, R. Tsuda, Y. Tsunesada, Shin BokKyun, T. Nonaka^A, Douglas Bergman^B, John Krizmanic^C, for the Telescope Array Collaboration
9: TA experiment 382：Search for temporal and directional coincidence between UHECR and transient events in other wavelengths; ICRR Univ. of Tokyo^A, Kyoto Univ.^B; K. Takahashi, T. Sako^A, T. Fujii^B, Telescope Array Collaboration
10: TA experiment 383: Development of UHECR anisotropy analysis method convoluting galaxy magnetic field; ICRR Univ. of Tokyo^A, Riken^B, Kyoto Univ.^C, 他; R. Higuchi, T. Sako^A, E. Kido^B, K. Kazumasa^A, T. Fujii^C, Telescope Array Collaboration
11: TA experiment 384 : Ultra-high-energy cosmic ray observed by the surface detector array on 27th May 2021; Kyoto Univ.，ICRR Univ. of Tokyo^A，Osaka City Univ.^B; T. Fujii，R. Higuchi^A，T. Sako^A，R. Mayta^B，for Telescope Array Collaboration
12: CRAFFT12 : Future observation plan and status of preparation; Osaka Electro-Comm. Univ., Shinshu Univ.^A, Kanagawa Univ.^B，Chubu Univ.^C; Y. Tameda, N. Shibata, E. Nishio, T. Takayuki^A, Y. Kubota^A, Y. Nakamura^A, D. Ikeda^B, K. Yamazaki^C
13: JEM-EUSO(184) The EUSO program to study UHECR from space: results and perspectives; RIKEN; Yoshiyuki TAKIZAWA, the JEM-EUSO collaboration

1: Estimation of birefringence distribution for sapphire mirror using transmitted wavefront error map; Tokyo Institute of Technology School of Science, National Astronomical Observatory of Japan^A, National Astronomical Observatory of Japan^B, The University of Tokyo School of Science^C; Homare Abe, Yoichi Aso^A, Matteo Leonardi^B, Wang Haoyu^C
2: Status of KAGRA calibration; NAOJ; Dan Chen, KAGRA collaboration
3: Study of the environmental noise for the KAGRA gravitational wave detector; ICRR; Takaaki Yokozawa, on the behalf of the KAGRA collaboration
4: Estimating the Newtonian noise of groundwater at the KAGRA; Tokyo Tech, etc; Takanori Suzuki，KAGRA collaboration
5: Applying linear Independent Component Analysis to KAGRA data; Osaka City University, etc.; Yuichiro Kobayashi, KAGRA collaboration
6: Non-linear noise subtraction from KAGRA data using Independent Component Analysis; Univ. of Tokyo, KAGRA collaboration; Jun'ya Kume, KAGRA collaboration

7: KAGRA : Development of data quality system toward O4 observing run; ICRR UTokyo; Hirotaka Yuzurihara, on behalf of the KAGRA collaboration
8: Exploration of glitches in KAGRA; Phys. S. Univ. of Tokyo, ICRR. Univ. of Tokyo^A, KAGRA collaboration^B; R. Chiba^A, T. Uchiyama^A, T. Yamamoto^A, KAGRA collaboration^B
9: Parameter orthonormalization on data analysis of gravitational waves; Kyoto Univ.^A, Osaka City Univ.^B, YITP^C; Kei Yamada^A, Norichika Sago^A,B, Takahiro Tanaka^A,C
10: Deep learning for non-Gaussian background gravitational waves; Nagoya University^A, IFT Madrid^B, Tamkang University^C; Takahiro S. Yamamoto, Sachiko Kuroyanagi, Guo Chin Liu
11: Development of a machine learning based monitor for gravitational waves from binary neutron star coalescences; Graduate School of Science, Osaka City University, etc.; Tomoya Ohashi
12: Sky localization of gravitational waves using machine learning; Dept. of Phys. Tokyo Tech，Tokyo City Univ.^A; Seiya Sasaoka，Yilun Hou，Kentaro Somiya，Hirotaka Takahashi^A
^●13: Sky localization of gravitational wave sources with one-dimensional residual neural network; ICRR，The University of Tokyo; Bin-Hua Hsieh，Hideyuki Tagoshi

1: AXEL: Result of the 180L large-sized prototype detector; Kyoto Univ.^A, Tohoku Univ.^B, Tohoku Univ. FRIS^C, UTokyo^D; Kazuhiro NAKAMURA^A, Atsuko K. ICHIKAWA^B, Tsuyoshi NAKAYA^A, Kiseki NAKAMURA^B, Shuhei OBARA^C, Sei BAN^D, Masashi YOSHIDA^A, Bungo SUGASHIMA^A, Yukimasa KASHINO^A, and the AXEL collaboration
2: AXEL: Efforts to develop a large gas Xe TPC; Kyoto Univ.^A, Tohoku Univ.^B, Tohoku Univ. FRIS^C, KEK^D, UTokyo^E; Bungo SUGASHIMA^A, Atsuko K. ICHIKAWA^B, Tsuyoshi NAKAYA^A, Kiseki NAKAMURA^B, Shuhei OBARA^C, Yoshihisa IWASHITA^A，Ken SAKASHITA^D, Sei BAN^D, Kazuhiro NAKAMURA^A, Masashi YOSHIDA^A, Yukimasa KASHINO^A, and the AXEL collaboration
3: KamLAND-Zen: Summary of Background Estimation; RCNS, Tohoku Univ.; KAMEI Yuto, for KamLAND-Zen Collaboration
4: KamLAND-Zen: Particle Identification Technique with Machine Learning; RCNS, Tohoku Univ.; Haruhiko Miyake, for KamLAND-Zen Collaboration
5: KamLAND-Zen: New result from the neutrino-less double beta decay search; RCNS, Tohoku Univ.; Hideyoshi Ozaki, for KamLAND-Zen Collaboration
6: KamLAND-Zen: Identification and track reconstruction of muon bundle; RCNS, Tohoku Univ.; Tomomi Gima, for KamLAND-Zen Collaboration
7: Development of liquid scintillator with wavelength shifter for KamLAND2-Zen; RCNS, Tohoku Univ.; Anna Goto, for KamLAND-Zen Collaboration

8: A search for double beta decay of Gd-160 by PIKACHU experiment; University of Tsukuba, Tokushima University^A, Tohoku University IMR^B, Tohoku University NICHe^C, Tokyo University^D, Fukui University^E, Kobe University^F; Takashi Iida, Ken-ichi Fushimi^A, Masao Yoshino^B, Kei Kamada^C, Keishi Hosokawa^D, Kyohei Nakajima^E, Nobuo Hinohara, Keita Mizukoshi^F
9: Purification of CaF₂ Crystals for Double-beta experiment III; NICHe Tohoku Univ.^A，IMR Tohoku Univ.^B，IMR, RCNP Osaka Univ.^C, Tokushima Univ.^D，I.S.C.Lab.^E; Shunsuke Kurosawa^A,B, Saori Umehara^C, Ken-ichi Fushimi^D, Yumiko Kishida^D, Akitoshi Sakaue^D, Tomomi Yoshida^C, Kyoshiro Imagawa^E, Kensuke Yasuda^E, Akihiro Yamaji^A,B
10: Improvement of pulse shape discrimination analysis for background rdduction in CANDLES; Osaka Univ., RCNP, OSaka Univ.^A, Univ. of Fukui^B, Tokushima Univ.^C, Tsukuba Univ.^D, Osaka Sangyo Univ.^E, WERC^F, Saga Univ.^G; Yoshioka Atsushi, Miyoshi Go, Minami Yuto^A, Umehara Saori^A, Yoshida Sei, Anawat Rittirong^E, Fushimi Ken-ichi^C, Harada Takaaki, Hashimoto Akihiro^B, Hazama Ryuta^E, Hiraiwa Tasuku^B, Iida Takashi^D, Matsuoka Kenji^A, Kishida Yumiko^C, Kishimoto Tadafumi^A, Muramatsu Yoshiki^B, Nakajima Kyohei^B, Nomachi Masaharu^A, Ogawa Izumi^B, Osumi Hideaki^G, Sakagami Akitoshi^C, Sakai Toshiki, Suzuki Kohtaku^F, Takihira Yukichi^A, Tamagawa Yoichi^B, Tozawa Masashi^B, Yamamoto Asahi, Yoshida Tomomi
11: Analysis for reducing backgrounds by ²⁰⁸Tl decays in CANDLES experiment; Osaka Univ.，Osaka Univ.RCNP^A; Miyoshi Go，Yoshioka Atsushi，Minami Yuto^A，Umehara Saori^A，Yoshida Sei，for CANDLES collaboration
12: Development of low radioactive Germanium detector for trace analysis; Osaka Univ., Osaka Univ. RCNP^A; Yoshida Tomomi, Harada Takuaki, Yamamoto Asahi, Umehara Saori^A, Minami Yuto^A, Yoshida Sei
13: Improvement of ⁴⁸Sc Detection Efficiency for ⁴⁸Ca Half-life Measurement and Evaluation of Sc Collection Efficiency by Chelate Resin; University of Osaka, RCNP^A; Harada Takaaki, Yamamoto Asahi, Yoshida Sei, Umehara Saori^A

1: Vainshtein screening in scalar-tensor theories nonminimally and kinetically coupled to matter; Tokyo University of Science; Kitaro Taniguchi, Ryotaro Kase
2: Can EDE with interacting DE-DM model solve the H₀ and S₈ tensions simultaneously?; Yamaguchi University; Mai Yashiki
3: Preferred frame effects for nonluminal propagetion speeds of GWs in pulsar timing arrays; Rikkyo Univ.; Yosuke Mishima，Hiroaki Tahara
4: CMB constraints on DHOST theories; Rikkyo Univ.; Takashi Hiramatsu
5: The Effective Field Theory of Vector-Tensor Theories; YITP; Katsuki Aoki, Mohammad Ali Gorji, Shinji Mukohyama, Kazufumi Takahashi
6: Toward Completion of EFT in Cosmology and UV Consistency Conditions; RIKEN iTHEMS, YITP Kyoto^A; Ryo Namba, Katsuki Aoki^A, Shinji Mukohyama^A

7: Positivity Bounds on Dark Photon Models; Kobe Univ.; Toshifumi Noumi, Sota Sato, Junsei Tokuda
8: On UV-completion of Palatini-Higgs inflation; Nagoya U., IAR^A; Yusuke Mikura, Yuichiro Tada^A
9: Relaxing inflation models with non-minimal coupling: A general study; Saga University; Tatsuki Kodama
10: H₀ tension in the extended frameworks and its implications to models beyond ΛCDM; Saga University; Fumiya Okamatsu, Tomo Takahashi
11: Hubble tension with an extra radiation and neutrino degeneracy; Dept. of Phys., Hokkaido U., IAHE, Hokkaido U.^A; Yo Toda，Osamu Seto^A
12: DeWitt boundary condition is consistent in Hořava-Lifshitz quantum gravity; YITP; Hiroki Matsui, Shinji Mukohyama, Atsushi Naruko
13: Wheeler-De Witt equation with radiative corrections and minisuperspace models; CST, Nihon Univ.; Koichi Iwamoto

1: Preparation status of the science operations for XRISM (X-ray Imaging and Spectroscopy Mission); ISAS/JAXA^A, Saitama University^B, Hiroshima University^C, Nara University of Education^D, Nihon Fukushi University^E, Shibaura Institute of Technology^F, Nagoya University^G, NASA/GSFC^H, Fukuoka University^I, Riken^J, The University of Tokyo^K, Nara Women’s University^L, Ehime University^M, Chuo University^N, Shizuoka University^O; Katsuhiro Hayashi^A, Makoto Tashiro^A,B, Yukikatsu Terada^A,B, Hiromitsu Takahashi^C, Masayoshi Nobukawa^D, Tsunefumi Mizuno^C, Shin’ichiro Uno^E, Aya Kubota^F, Kazuhiro Nakazawa^G, Shin Watanabe^A, Ryo Iizuka^A, Rie Sato^A, Tomokage Yoneyama^A, Chris Baluta^H, Ken Ebisawa^A, Satoshi Eguchi^I, Yasushi Fukazawa^C, So Kato^B, Satoru Katsuda^B, Takao Kitaguchi^J, Hirokazu Odaka^K, Masanori Ohno^C, Naomi Ota^L, Minami Sakama^B, Ryohei Sato^B, Megumi Shidatsu^M, Yasuharu Sugawara^A, Tsubasa Tamba^K, Atsushi Tanimoto^K, Yuichi Terashima^M, Yoko Tsuboi^N, Nagomi Uchida^A, Yuusuke Uchida^C, Hideki Uchiyama^O, Shigeo Yamauchi^L
2: Status of the Development of the X-ray Mirror Assembly (XMA) onboard the X-ray Imaging and Spectroscopy Mission (6); ISAS/JAXA, NASA's GSFC^A, Rikkyo Univ.^B, Tokyo Metropolitan Univ.^C, Kanazawa Univ.^D, Miyazaki Univ.^E; Manabu Ishida, Takayuki Hayashi^A, Takashi Okajima^A, Keisuke Tamura^A, Rozenn Boissay-Malaquin^A, Danielle N.Gurgew^A, Larry Olsen^A, Richard Koenecke^A, Leor Bleier^A, Richard Kelley^A, Gary Sneiderman^A, Meng Chiao^A, Toshiki Sato^B, Hideyuki Mori, Yoshitomo Maeda, Ryo Iizuka, Yoshitaka Ishisaki^C, Ryuichi Fujimoto^D, Koji Mori^E
3: Development status of Resolve instrument onboard X-Ray Imaging and Spectroscopy Mission IX; Tokyo Metro-U^A，NASA^B，SRON^C，Ehime-U^D，LLNL^E，U-Geneva^F，Kanazawa-U^G，Fujita Health-U^H，JAXA^I，Nagoya-U^J，Rikkyo-U^K，U-Wisconsin^L，RIKEN^M，Tohoku-U^N，Saitama-U^O，Yale-U^P，Kyoto-U^Q，Hiroshima-U^R; Y. Ishisaki^A,I，R.L. Kelley^B，H. Akamatsu^C，H. Awaki^D，T.G. Bialas^B，G.V. Brown^E，M.P. Chiao^B，E. Costantini^C，J.-W. den Herder^C，M.J. Dipirro^B，M.E. Eckart^E，Y. Ezoe^A，C. Ferrigno^F，R. Fujimoto^G,I，A. Furuzawa^H，S.M. Graham^B，M. Grim^C，T. Hayashi^B，A. Hoshino^I，Y. Ichinohe^K，R. Iizuka^I，M. Ishida^I，K. Ishikawa^A，C.A. Kilbourne^B，S. Kitamoto^K，M.A. Leutenegger^B，Y. Maeda^I，D. McCammon^L，I. Mitsuishi^J，M. Mizumoto^Q，T. Okajima^B，S. Paltani^F，F.S. Porter^B，K. Sato^O，T. Sato^K，M. Sawada^M，H. Seta^A，P.J. Shirron^B，G.A. Sneiderman^B，Y. Soong^B，A.E. Szymkowiak^P，Y. Takei^I，T. Tamagawa^M，M. Tsujimoto^I，Y. Uchida^R，C.P. de Vries^C，S. Yamada^K，N.Y. Yamasaki^I，S. Yasuda^I，N. Yoshioka^I
4: Development status of the soft X-ray imaging telescope “Xtend” for X-ray Imaging and Spectroscopy Mission “XRISM” (IX); Kyoto Univ., Osaka Univ.^A, ISAS/JAXA^B, Univ. of Miyazaki^C, Kanto Gakuin Univ.^D, Konan Univ.^E, NASA/GSFC^F, Tohoku Gakuin Univ.^G, Nara Univ. of Education^H, Kindai Univ.^I, Tokyo Univ. of Science^J, Tokyo Univ. of Science^K, Kwansei Gakuin Univ.^L, Shizuoka Univ.^M, Nagoya Univ.^N, Hiroshima Univ.^O; H. Uchida, K. Hagino^J, H. Noda^A, K. Hayashida^A,B, H. Tomida^B, K. Mori^C,B, H. Nakajima^D, T. Tanaka^E, T. G. Tsuru, H. Matsumoto^A, T. Okajima^F, T. Yoshida^B, T. Yoneyama^B, M. Ishida^B, Y. Maeda^B, H. Murakami^G, M. Yamauchi^C, I. Hatsukade^C, M. Nobukawa^H, K. K. Nobukawa^I, T. Kohmura^J, S. B. Kobayashi^K, H. Suzuki^E, J. S. Hiraga^L, H. Uchiyama^M, K. Yamaoka^N, M. Ozaki^B, T. Dotani^B, H. Tsunemi^A, Tsunefumi Mizuno^O, and the XRISM/Xtend team
5: Spectral analysis of pile-up data of X-ray CCD based on Monte Carlo simulation; Univ. of Tokyo, Tohoku Gakuin Univ.^A, Univ. of Miyazaki^B, Osaka Univ.^C, Saitama Univ.^D, Hiroshima Univ.^E, Nara Univ. of Education^F; T. Tamba, H. Odaka, A. Bamba, H. Murakami^A, K. Mori^B, K. Hayashida^C, Y. Terada^D, T. Mizuno^E, M. Nobukawa^F, XRISM MOPT
6: A wide-band X-ray observatory FORCE: Attitude determination system analysis and consideration for Observatory-type contribution; Nagoya-U, Miyazaki-U^A, Tohoku-gakuin^B, Shibaura-IT^C, Tokyo-U. of Science^D, Univ.-Tokyo^E, Saitama-U^F, RIKEN^G, Rikkyo-U^H, Waseda-U^I, Toho-U^J, TITEC^K, Tokyo Metro-U^L, ISAS/JAXA^M, Kantogakuin-U^N, Fujita-Health-U^O, Nara-U of Education^P, Nara-Women's-U^Q, Kyoto-U^R, Kindai-U^S, Osaka-U^T, Konan-U^U, Kobe-U^V, Ehime-U^W, Hiroshima-U^X, Eoetvoes U.^Y, SRON^Z, NASA/GSFC^AA; K. Nakazawa, K. Mori^A, H. Murakami^B, A. Kubota^C, S.B. Kobayashi^D, T. Kohmura^D, K. Hagino^D, T. Takahashi^E, A. Bamba^E, H. Odaka^E, Y. Terada^F, T. Enoto^G, Y. Uchiyama^H, T. Sato^H, T. K. Ishimura^I, Kitayama^J, Y. Yatsu^K, Y. Fujita^L, M. Ishida^M, S. Watanabe^M, H. Yamaguchi^M, M. Nakajima^N, A. Furuzawa^O, M. Nobukawa^P, N. Ota^Q, T.G. Tsuru^R, Y. Ueda^R, H. Uchida^R, K. Nobukawa^S, H. Matsumoto^T, H. Noda^T, H. Tsunemi^T, T. Tanaka^U, H. Suzuki^U, M. Itoh^V, H. Awaki^W, Y. Terashima^W, M. Shidatsu^W, Y. Fukazawa^X, T. Mizuno^X, H. Takahashi^X, A. Takeda^A, M. Ohno^Y, H. Akamatsu^Z, Hornschemeier,A.E^AA, T. Okajima^AA, Zhang,W.W.^AA, and the FORCE WG

7: GRAINE project, for the next balloon-borne experiments; Kobe University，Aichi University of Education^A，Okayama University of Science^B，Gifu University^C，Nagoya University^D; Satoru Takahashi, Shigeki Aoki, Takashi Azuma, Ayaka Karasuno, Takumi Kato, Kenji Kuretsubo, Toshitsugu Marushima, Syota Matsuda, Shogo Nagahara, Takafumi Nakamura, Motoya Nakamura, Miyuki Oda, Atsumu Suzuki, Mayu Yamashita, Kohichi Kodama^A, Atsushi Iyono^B, Kazuma Nakazawa^C, Masahiro Yoshimoto^C, Hirotaka Hayashi^D, Ryosuke Komatani^D, Masahiro Komatsu^D, Masahiro Komiyama^D, Hideyuki Minami^D, Kunihiro Morishima^D, Misaki Morishita^D, Naotaka Naganawa^D, Mitsuhiro Nakamura^D, Tomoaki Nakamura^D, Yuya Nakamura^D, Noboru Nakano^D, Toshiyuki Nakano^D, Akira Nishio^D, Hiroki Rokujo^D, Osamu Sato^D, Kai Shimizu^D, Amon Suganami^D, Kou Sugimura^D, Mayu Torii^D, Ikuya Usuda^D, Saya Yamamoto^D
8: GRAINE project, performance evaluation of nuclear emulsion films for next balloon experiment; Nagoya University, Aichi University of Education^A, Okayama University of Science^B, Gifu University^C, Kobe University^D; Ikuya Usuda, Osamu Sato, Kai Shimizu, Amon Suganami, Kou Sugimura, Toshiyuki Nakano, Tomoaki Nakamura, Mitsuhiro Nakamura, Yuya Nakamura, Hirotaka Hayashi, Hideyuki Minami, Saya Yamamoto, Hiroki Rokujo, GRAINE collaboration^A,B,C,D
9: GRAINE project：performance evaluation of next generation multi-stage shifter by cosmic ray tracks; Kobe University，Aichi University of Education^A，Okayama University of Science^B，Gifu University^C，Nagoya University^D; Miyuki Oda, Shigeki Aoki, Takashi Azuma, Takumi Kato, Satoru Takahashi, Shogo Ngahara, Mayu Yamashita, GRAINE collaboration^A,B,C,D
10: GRAINE project: Development of track-angle calibration system for next balloon experiment; Nagoya University, Aichi University of Education^A, Okayama University of Science^B, Gifu University^C, Kobe University^D; Tomoaki Nakamura, Ikuya Usuda, Osamu Sato, Kai Shimizu, Amon Suganami, Kou Sugimura, Toshiyuki Nakano, Mitsuhiro Nakamura, Yuya Nakamura, Hirotaka Hayashi, Hideyuki Minami, Saya Yamamoto, Hiroki Rokujo, GRAINE collaboration^A,B,C,D
11: Development of new emulsion read-out system for cosmic gamma-ray observation; Nagoya University, Aichi University of Education^A, Okayama University of Science^B, Gifu University^C, Kobe University^D; Yuya Nakamura, Ryosuke Komatani, Masahiro Komatsu, Masahiro Komiyama, Osamu Sato, Kou Sugimura, Mayu Torii, Naotaka Naganawa, Toshiyuki Nakano, Noboru Nakano, Mitsuhiro Nakamura, Akira Nishio, Misaki Morishita, Kunihiro Morishima, Hiroki Rokujo, Kohichi Kodama^A, Atsushi Iyono^B, Saya Yamamoto^B, Masahiro Yoshimoto^C, Shigeki Aoki^D, Miyuki Oda^D, Ayaka Karasuno^D, Kenji Kuretsubo^D, Atsumu Suzuki^D, Satoru Takahashi^D, Takafumi Nakamura^D, Motoya Nakamura^D, Syota Matsuda^D, Toshitsugu Marushima^D
12: The New Window of Imaging Polarization Observations opened by IXPE; Yamagata Univ., RIKEN^A, Tokyo Univ. of Science^B, Nagoya Univ.^C, Hiroshima Univ.^D, Chuo Univ.^E, Osaka Univ.^F, NASA/MSFC^G, IAPS/Rome^H, INFN/Pisa^I; Shuichi Gunji, Eri Watanabe, Masanobu Terashima, Yuma Kan, Yo Saito, Toru Tamagawa^A, Takao Kitaguchi^A, Teruaki Enoto^A, Keisuke Uchiyama^A,B, Tomoshi Takeda^A,B, Ikuyuki Mitsuishi^C, Kazuto Kashiwagura^C, Yuzuru Tawara^C, Yasushi Fukazawa^D, Tsunefumi Mizuno^D, Hiromitsu Takahashi^D, Nagomi Uchida^D, Zhang Sixuan^D, Wataru Iwakiri^E, Kiyoshi Hayashida^F, Kazunori Asakura^F, Martin Weisskopf^G, Brian Ramsey^G, Stephen O’Dell^G, Paolo Soffitta^H, Luca Baldini^I and IXPE Team
13: Study of X-ray polarimetry analysis with the Crab Nebula using IXPE and Chandra; Yamagata Univ., RIKEN^A, Tokyo Univ. of Science^B, Nagoya Univ.^C, Hiroshima Univ.^D, Chuo Univ.^E, Osaka Univ.^F, NASA/MSFC^G, IAPS/Rome^H, INFN/Pisa^I; Eri Watanabe, Shuichi Gunji, Masanobu Terashima, Yuma Kan, Yo Saito, Toru Tamagawa^A, Takao Kitaguchi^A, Teruaki Enoto^A, Keisuke Uchiyama^A,B, Tomoshi Takeda^A,B, Ikuyuki Mitsuishi^C, Kazuto Kashiwagura^C, Yuzuru Tawara^C, Yasushi Fukazawa^D, Tsunefumi Mizuno^D, Hiromitsu Takahashi^D, Nagomi Uchida^D, Zhang Sixuan^D, Wataru Iwakiri^E, Kiyoshi Hayashida^F, Kazunori Asakura^F, Martin Weisskopf^G, Brian Ramsey^G, Stephen O’Dell^G, Paolo Soffitta^H, Luca Baldini^I and IXPE Team

1: DIMS Experiment(Dark Matter and Interstellar Meteoroid Study) (5): Present Status and Future; Konan Univ., Osaka Electro-Communication Univ.^A, Turin Univ.^B, NCBJ^C, RIKEN^D,Univ. Warsaw^E, ICRR^F, Univ. Utah^G, INAF^H, Nihon Univ.^I, SKKU^J, NMS^K, Univ. Lodz^L etc.; KAJINO Fumiyoshi, TAMEDA Yuichiro^A, IWAMI Yugo^A, SHINTO Daiki^A, Fujioka Momoka^A, BERTAINA Mario^B, VALENTI Simone^B, BARGHINI Dario^B, SHINOZAKI Kenji^C, KASZTERAN Marcin^C, VRABEL Michal^C, PRZYBYLAK Marika^C, CASOLINO Marco^D, EBISUZAKI Toshikazu^D, TAKIZAWA Yoshiyuki^D, PIOTROWSKI Lech^E, SAGAWA Hiroyuki^F, MATTHEWS John^G, CELLINO Alberto^H, ABE Shinsuke^I, ENDO Mirai, KIKUCHI Keita^I, HASEGAWA Mari^I, PARK Il^J, FUJIWARA Yasunori^K, KOJRO Mateusz^L etc.
2: Development of the operation system for the GAPS heat pipe; ROIS, JAXA^A，Tokai Univ.^B，Kanagawa Univ.^C; M. Kozai，M. Saijo^A，K. Tokunaga^A，S. Okazaki^A，H. Fuke^A，A. Kawachi^B，S. Kobayashi^B, K. Mizuno^B，Y. Shimizu^C, S. Suzuki^C
3: Highlights from the first 6 years of CALET observations on the International Space Station; WISE Waseda Univ., Kanagawa Univ.^A, Ritsumeikan Univ.^B, JAXA/ISAS^C, ICRR Univ. of Tokyo^D, Hirosaki Univ.^E, Shibaura Inst. of Tech.^F, NIPR^G, Yokohama Natl. Univ.^H, Shinshu Univ.^I, LSU^J, Ibaraki College^K, GCSE Waseda Univ.^L, NICT^M, Aoyama Gakuin Univ.^N, Nihon Univ.^O, Osaka City U.^P, Nagoya Univ.^Q, Ibaraki Univ.^R; Shoji Torii, Yosui Akaike, Kazuyoshi Kobayashi, Tadahisa Tamura^A, Masaki Mori^B, Yoichi Asaoka^C, Katsuaki Asano^C, Hideyuki Fuke^D, Kinya Hibino^A, Masakatu Ichimura^E, Katsuaki Kasahara^F, Ryuho Kataoka^G, Yusaku Katayose^H, Chihiro Kato^I, Yuta Kawakubo^J, Shoko Miyake^K, Holger Motz^L, Kazuoki Munakata^I, Satoshi Nakahira^D, Shoji Okuno^A, Shunsuke Ozawa^M, Takanori Sakamoto^N, Yuki Shimizu^A, Shoji Shiomi^O, Yoshiki Tsunesada^P, Kazutaka Yamaoka^Q, Shohei Yanagita^R, Atsumasa Yoshida^N, Kenji Yoshida^F and the CALET collaboration
4: Observation and energy calibration for six years of CALET operation on the International Space Station; WISE Waseda Univ.，Kanagawa Univ.^A，Ritsumeikan Univ.^B，ICRR Univ. of Tokyo^C; Yosui Akaike，Shoji Torii，Kazuyoshi Kobayashi，Tadahisa Tamura^A，Masaki Mori^B，Yoichi Asaoka^C
5: Cosmic-ray proton and helium energy spectra observed by CALET in the energy region of 50GeV-80TeV; WISE Waseda Univ., Siena Univ./INFN Pisa^A, ICRR Univ. of Tokyo^B; Kazuyoshi Kobayashi, Pier S. Marrocchesi, Paolo Brogi, Shoji Torii, Yoichi Asaoka, Yosui Akaike, and the CALET collaboration
6: Measurement of iron nuclei below 10GeV/n by means of the geomagnetic effect; Hirosaki Univ.，WISE Waseda Univ.^A，ICRR Univ. of Tokyo^B，Shibaura Inst. of Tech.^C; Masakatsu Ichimura, Yosui Akaike^A, Yoichi Asaoka^B, Katsuaki Kasahara^C, Kazuyoshi Kobayashi^A, Shoji Torii^A for the CALET collaboration

7: Observation of low-energy electrons and protons with CALET around the solar minimum at the solar cycle 24/25; NIT Ibaraki Col.，Shinshu Univ.^A, NIPR^B, JAXA^C, ICRR^D, WISE Waseda Univ.^E, NAOJ^F; Shoko Miyake，Kazuoki Munakata^A，Chihiro Kato^A，Ryuho Kataoka^B, Satoshi Nakahira^C，Yoichi Asaoka^D，Shoji Torii^E，Toshio Terasawa^F，Yosui Akaike^E，Kenkou Kobayashi^E for the CALET Collaboration
^●8: Indirect Search for Heavy Dark Matter with CALET; GCSE Waseda University; Motz Holger
9: MONTE CARLO STUDY OF ELECTRON AND POSITRON COSMIC-RAY PROPAGATION WITH THE CALET SPECTRUM; ICRR, FSCI-Waseda^A, YITP^B, KEK^C; Katsuaki Asano, Yoichi Asaoka, Yosui Akaike^A, Norita Kawanaka^B, Kazunori Kohri^C, Holger M. Motz^A, Toshio Terasawa
10: Radio Constraints on High-energy Multi-messenger Emission from Galaxy Clusters; ICRR, Penn State U.^A, YITP^B; Kosuke Nishiwaki, Katsuaki Asano, Kohta Murase^A,B
11: High energy neutrino emission from general relativistic MHD accretion flow onto supermassive black hole; ICRR, U. of Tokyo; Tomohisa Kawashima, Katsuaki Asano
^●12: Enhancing IceCube's sensitivity to extremely high energy neutrinos: Study on improved rejection of muon bundle background; Chiba University; Maximilian Meier，A. Ishihara，S. Yoshida，C. Hill，N. Shimizu，R. Nagai

^●1: Vibration Analysis of KAGRA Cryostat at Cryogenic Temperature; SOKENDAI^A，KEK^B，ICRR^C，NAOJ^D，University of Toyama^D; Rishabh Bajpai^A，Takayuki Tomaru^D，Honda Tohru^B，Nobuhiro Kimura^C，Toshikazu Suzuki^C，Takafumi Ushiba^C，Kazuhiro Yamamoto^D
2: Dark matter Axion search with riNg Cavity Experiment DANCE (7); Univ. of Tokyo^A, RESCEU^B, Waseda Univ.^C, PRESTO^D, UWM^E, ISAS/JAXA^F, ICRR^G, MPA^H; Hiroki Fujimoto^A, Yuka Oshima^A, Masaki Ando^A,B, Tomohiro Fujita^B,C, Jun’ya Kume^B, Yuta Michimura^A,D, Soichiro Morisaki^E, Koji Nagano^F, Hiromasa Nakatsuka^G, Atsushi Nishizawa^B, Ippei Obata^H
3: Observational constraint to axion dark matters with propagating gravitational waves; UTokyo, U. Tokyo RESCEU^A, UWM^B; Takuya Tsutsui^A, Atsushi Nishizawa^A, Soichiro Morisaki^B
4: Adiabatic evolution of the self-interacting axion cloud; Kyoto U; H. Omiya, T. Takahashi, T. Tanaka
5: LISA-consistency with primordial black holes as dark matter in light of the exponential tail; Nagoya University; R.Inui, Y.Tada, S.Yokoyama, K.T.Abe
6: Development of back-linked Fabry-Perot interferometer for frequency stabilization in space gravitational wave telescope Ⅳ; SOKENDAI^A, JAXA ISAS^B; Ryosuke Sugimoto^A,B, Kiwamu Izumi^B, Koji Nagano^B, Kentaro Komori^B

7: On the excitation of higher harmonic quasi-normal modes of spinning black holes; RIKEN iTHEMS; Naritaka Oshita
8: Extraction of parameters for gravitational wave signals using short time Laplace transform; Osaka City University; Satoshi Tsuchida, Nobuyuki Kanda, Yousuke Itoh, Takahiro Sawada, on behalf of the KAGRA Collaboration
9: Usefulness of an ARMA model for noise reduction in gravitational wave detectors; Graduate School of Science, Osaka City University, etc.; Yuya Fujimoto, KAGRA collaboration
10: Impact of correlated magnetic noise on the parameter estimation of stochastic gravitational waves; Nihon Univ., RESCEU^A, YITP^B; Yoshiaki Himemoto, Atsushi Nishizawa^A, Atsushi Taruya^B
11: Demonstration of long signal recycling cavity effect for high-frequency gravitational wave observatory; JAXA/ISAS, Titech^A; Kentaro Komori, Sotatsu Otabe^A, Kentaro Somiya^A
12: Development of displacement-noise-free neutron interferometer for gravitational wave detection(5); Nagoya U., U Tokyo RESCEU^A, Caltech^B, U Tokyo^C; Shoki Iwaguchi, Atsushi Nishizawa^A, Yuki Kawasaki, Yanbei Chen^B, Masaaki Kitaguchi, Taigen Morimoto, Tomohiro Ishikawa, Wu Bin, Izumi Watanabe, Ryuma Shimizu, Hirohiko Shimizu, Yuta Michimura^C, Seiji Kawamura
^●13: Juggled interferometer for gravitational wave detection (2); Nagoya U, U Tokyo^A, Nagoya U. KMI^B; Bin WU, Tomohiro Ishikawa, Shoki Iwaguchi, Ryuma Shimizu, Izumi Watanabe, Yuki Kawasaki, Yuta Michimura^A, Shuichiro Yokoyama^B, Seiji Kawamura

1: Primordial black holes in peak theory with a non-Gaussian tail; ULB, FRIS^A, IAR^B, KMI^C, Nagoya U.^D; Albert Escrivà, Naoya Kitajima^A, ^○Yuichiro Tada^B, Shuichiro Yokoyama^C, Chul-Moon Yoo^D
2: Primordial black hole abundance from two-point correlations between perturbations; Graduate School of Science, the University of Tokyo; Koki Tokeshi, Jun'ichi Yokoyama
3: Simulation of PBH formation from isocurvature perturbations; Nagoya U.，Rikkyo U.^A，WIAS^B，KavliIPMU^C; Chulmoon Yoo，Tomohiro Harada^A，Shin'ichi Hirano，Hirotada Okawa^B，Misao Sasaki^C
^●4: Theoretical bound on primordial non-Gaussianity in single field inflation; RESCEU，The University of Tokyo; Jason Kristiano，Jun'ichi Yokoyama
5: Antipodal correlations of the inflationary primordial gravitational waves; Yamaguchi University; Zhen-Yuan WU, Nobuyuki Sakai, Ryo Saito
6: Angular correlations of the inflationary stochastic gravitational wave background in the perturbed universe; Yamaguchi U; Ryo Saito, Zhen-Yuan Wu, Nobuyuki Sakai

7: Chiral Gravitational Waves at the End of Inflation in Axion-SU(2) Model; WIAS, ICRR^A, RESCEU^B; Tomohiro Fujita^A,B, Kaname Imagawa, Kai Murai
8: SU(N)-natural inflation; WIAS^A, ICRR^B, KEK^C; Tomohiro Fujita^A, Hiromasa Nakatsuka^B, Kyohei Mukaida^C, ^○Kai Murai^B
9: SU(N)-natural inflation in anisotropic background; Dept. of Phys., Rikkyo Univ.^A, WIAS^B; Tomoaki Murata^A, Tomohiro Fujita^B, Tsutomu Kobayashi^A
10: We show that a recent constraint on the cosmic birefringence effect due to dark energy can be related to the constraints on the coupling of axion dark matter to photon, by relying on a simple model of two-axion alignment mechanism with periodic potentials. Owing to the alignment of the potentials, one linear combination of two fields provides a nearly flat direction and acts as dark energy, whereas the other combination provides a steep direction and acts as dark matter. This scenario solves the known conceptual issues of one-field model for dark energy and predicts the connection between seemingly disparate constraints on the dark sectors of our universe.; MPA; Ippei Obata
11: Helical magnetic fields from inflation and the generation of the cosmic baryon number; Fukushima U.，IEEC-CSIC^A，Chandernagore Coll.^B，IIT Guwahati^C; Kazuharu Bamba，Sergei D. Odintsov^A，Tanmoy Paul^B，Debaprasad Maity^C
^●12: Wash-in leptogenesis and its realization; University of Tokyo, CERN^A, KEK^B, Tohoku University^C; Kohei Kamada, Valerie Domcke^A, Kyohei Mukaida^B, Kai Schmitz^A, Masaki Yamada^C

1: SMILE61: Backgrounds in the SMILE2+ experiment; Kyoto University, JAXA^A, Kobe University^B, Tohoku University^C, Kanazawa University^D, University of Maryland, Baltimore County^E; T. Ikeda, T. Tanimori, A. Takada, T. Takemura, K, Yoshikawa, Y. Nakamura, M. Abe, S. Ogio, M. Tsuda, Y. Yoshida, K. Kobayashi, K. Tahara, H. Kubo, Y. Mizumura^A, K. Miuchi^B, S. Kurosawa^C, T. Sawano^D, K. Hamaguchi^E
2: SMILE62: Current status of high-energy event analysis for the MeV gamma-ray observation balloon experiment SMILE-2+; Kyoto University, JAXA^A, Kobe University^B, Tohoku University^C, Kanazawa University^D, University of Maryland, Baltimore County^E; S. Ogio, T. Tanimori, A. Takada, T. Ikeda, T. Takemura, K, Yoshikawa, Y. Nakamura, M. Abe, M. Tsuda, Y. Yoshida, K. Kobayashi, K. Tahara, H. Kubo, Y. Mizumura^A, K. Miuchi^B, S. Kurosawa^C, T. Sawano^D, K. Hamaguchi^E
3: SMILE63: Development of the trigger circuit for SMILE-3, the loaded-on-balloon experiment of the sky survey in MeV gamma-ray; Kyoto University, JAXA^A, Kobe University^B, Tohoku University^C, Kanazawa University^D, University of Maryland, Baltimore County^E; K. Tahara, T. Tanimori, A. Takada, T. IkedaT. Takemura, K, Yoshikawa, Y. Nakamura, M. Abe, S. Ogio, M. Tsuda, Y. Yoshida, K. Kobayashi, Y. Mizumura^A, K. Miuchi^B, S. Kurosawa^C, T. Sawano^D, K. Hamaguchi^E
4: Status of Hard X-ray Focusing Polarimeter, X-Calibur Balloon-Borne Experiment, for 2022 Flight; Hiroshima U., WUSTL^A, Osaka U.^B, Ehime U.^C, Rice U.^D, DG CIRCUITS^E, NASA WFF^F, RIKEN^G, Fujita Health U.^H, Guarino Engineering Services^I, Yamagata U.^J, Nagoya U.^K, ISAS^L, KTH^M, OKC^N, UNH^O, OIST^P, NASA GSFC^Q, TMU^R, TUS^S, UMD^T, NRL^U; Hiromitsu Takahashi, Quin Abarr^A, Mio Aoyagi^B, Kazunori Asakura^B, Hisamitsu Awaki^C, Matthew G. Baring^D, Richard Bose^A, Dana Braun^A, Gianluigi de Geronimo^E, Paul Dowkontt^A, John Elliot^F, Teruaki Enoto^G, Manel Errando^A, Yasushi Fukazawa, Akihiro Furuzawa^H, Thomas Gadson^F, Epharaim Gau^A, Victor Guarino^I, Shuichi Gunji^J, Kazuhiro Hakamada^B, Ryota Hagiwara^B, Kenny Hall^F, Maho Hanaoka^B, Keon Harmon^F, Kengo Hattori^B, Kiyoshi Hayashida^B,L, Scott Heatwole^F, Arman Hossen^A, Shuntaro Ide^B, Ryuta Imamura^B, Fumiya Imazato, Ryo Imazawa, Kazunori Ishibashi^K, Manabu Ishida^L, Asami Ishikura^B, Kota Ishiwatari^B, Nirmal Kumar Iyer^M,N, Fabian Kislat^O, Mozsi Kiss^M,N, Norika Kameya^C, Wataru Kamogawa^B, Takao Kitaguchi^G, David Kotsifakis^F, Henric Krawczynski^A, James Lanzi^F, Lindsey Lisalda^A, Yoshitomo Maeda^L, Yusuke Matsushita^B, Hiroto Matake, Hironori Matsumoto^B, Taisei Mineta^B, Asuka Miyamoto^R, Takuya Miyazawa^P, Tsunefumi Mizuno, Nozomi Nakaniwa^R, Hirofumi Noda^B, Yuuichi Ode^B, Takashi Okajima^Q, Takaki Okazaki^B, Izabella Pastrani^A, Mark Pearce^M,N, Zachary Peterson^F, Helen Poon, Chris Purdy^F, Brian Rauch^A, Felix Ryde^M,N, Yoshitaka Saito^L, Shotaro Sakuma^B, Atsuya Sato^B, Kenmei Sawagami^B, Chris Shreeves^F, Garry Simburger^A, Carl Snow^F, Sean Spooner^O, Theodor-Adrian Stana^M,N, David Stuchlik^F, Hitomi Suzuki^R, Tomoshi Takeda^S, Mai Takeo^R, Toru Tamagawa^G, Keisuke Tamura^Q, Hiroshi Tsunemi^B, Nagomi Uchida, Yuusuke Uchida, Keisuke Uchiyama^T, Brett Vincent^F, Andrew West^A, Eric Wulf^U, Ryuya Yamamoto, Chong Yang, Tomokage Yoneyama^B, Yuto Yoshida^S, Marina Yoshimoto^B, XL-Calibur team
5: Development of the X-ray Polarimeter Using CMOS Imager X: Beam Test for Imaging Polarimetry; Univ. of Tokyo, ICEPP^A, Kavli IPMU^B, JAXA^C, NAOJ^D; T. Iwata, H. Odaka, T. Tamba, T. Watanabe, T. Kasuga, S. Takashima, S. Nammoku, M. Ichihashi, A. Tanimoto, A. Bamba, Y. Kamiya^A, T. Takahashi^B, S. Nagasawa^B, T. Minami^B, S. Watanabe^C, N. Narukage^D
6: GRAMS 8: Project Status; Univ. of Tokyo, Waseda Univ.^A, Rikkyo Univ.^B, Osaka Univ.^C, Hiroshima Univ.^D, Eotvos Lorand Univ.^E, RIKEN^F, Toyama Univ.^G, Northeastern Univ.^H, Columbia Univ.^I, Barnard College^J; H. Odaka, S. Takashima, T. Tamba, S. Nammoku, A. Bamba, K. Yawata, K. Aoyama^A, K. Iwasawa^A, M. Sakurai^A, M. Tanaka^A, T. Nakasone^A, Yorita^A, Y. Ichinohe^B, D. Khangulyan^B, Y. Inoue^C, Y. Uchida^D, U. Suda^D, H. Takahashi^D, Y. Fukazawa^D, M. Ohno^E, N. Tsuji^F, Yoneda^F, N. Hiroshima^G, T. Aramaki^H, G. Karagiorgi^I, R. Mukherjee^J, GRAMS Collaboration

7: Status of GEM-based X-ray detector onboard 6U Cube NinjaSat; Tokyo Univ. of Sci., RIKEN^A, Chuo Univ.^B, Tokyo Metropolitan Univ.^C, Shibaura Inst. of Tech.^D, Nat'l Changhua Univ. of Edu.^E, Hiroshima Univ.^F, Univ. of Tokyo^G, Waseda Univ.^H; T. Takeda, T. Tamagawa^A, T. Enoto^A, T. Kitaguchi^A, Y. Kato^A, T. Mihara^A, W. Iwakiri^B, M. Numazawa^C, K. Uchiyama, Y. Yoshida, N. Ota, S. Hayashi, H. Sato^D, H. Chin-Ping^E, H. Takahashi^F, H. Odaka^G, T. Tamba^G, K. Taniguchi^H
8: Development of pulse shape discrimination method between X-ray and cosmic ray in NinjaSat; Tokyo Univ. of Sci., RIKEN^A, Chuo Univ.^B, Tokyo Metropolitan Univ.^C, Shibaura Inst. of Tech.^D, Nat'l Changhua Univ. of Edu.^E, Hiroshima Univ.^F, Univ. of Tokyo^G, Waseda Univ.^H; Y.Yoshida, T. Tamagawa^A, T. Enoto^A, T. Kitaguchi^A, Y. Kato^A, T. Mihara^A, W. Iwakiri^B, M. Numazawa^C, K. Uchiyama, T. Takeda, N. Ota, S. Hayashi, H. Sato^D, H. Chin-Ping^E, H. Takahashi^F, H. Odaka^G, T. Tamba^G, K. Taniguchi^H
9: Development of Data Acquisition System onboad 6U Cube NinjaSat; RIKEN, Chuo Univ.^A, Tokyo Metropolitan Univ.^B, Tokyo Univ. of Sci.^C, Shibaura Inst. of Tech.^D, Nat'l Changhua Univ. of Edu.^E, Hiroshima Univ.^F, Univ. of Tokyo^G, Waseda Univ.^H; T. Kitaguchi, T. Tamagawa, T. Enoto, Y. Kato, T. Mihara, W. Iwakiri^A, M. Numazawa^B, K. Uchiyama^C, T. Takeda^C, Y.Yoshida^C, N. Ota^C, S. Hayashi^C, H. Sato^D, H. Chin-Ping^E, H. Takahashi^F, H. Odaka^G, T. Tamba^G, K. Taniguchi^H
10: Development of a mini-semiconductor Compton telescope with Si/CdTe double-sided strip detector and BGO active shield for ballooning experiments; Nagoya U., Kavli IPMU. U.Tokyo^A, JAXA^B, Technical Center of Nagoya U.^C; Yuna Tsuji, Kazuhiro Nakazawa, Shin'ichiro Takeda^A, Keigo Okuma, Mii Ando, Shin Watanabe^B, Tadayuki Takahashi^A, Masahiko Kobayashi, Naoki Ishida^C, Takahiro Minami^A
11: Development of BGO active shield for mini-semiconductor Compton telescope for balloon experiment; Nagoya U., Kavli IPMU. U.Tokyo^A, JAXA^B, Technical Center of Nagoya U.^C; Mii Ando, Kazuhiro Nakazawa, Yuna Tsuji, Keigo Okuma, Shin'ichiro Takeda^A, Shin Watanabe^B, Tadayuki Takahashi^A, Masahiko Kobayashi, Naoki Ishida^C
12: Detection of sub-MeV gamma-ray with an advanced Compton camera using SOIPIX; NIT Sendai College, Ibaraki Univ.^A, Univ. of Miyazaki^B, Univ. of Tokyo^C, Kyoto Univ.^D, Konan Univ.^E, Riken^F; Mika Kagaya, Hideaki Katagiri^A, Ryo Kato^A, Naomi Tojo^A, Ayaki Takeda^B, Kenji Shimazoe^C, Takeshi Go Tsuru^D, Takaaki Tanaka^E, Mizuki Uenomachi^F, Lan Zhang^C
13: Study of performance and response of thick CdTe double-sided strip detectors for space gamma-ray observation; Univ. of Tokyo, Kavli IPMU^A, ISAS/JAXA^B; Takahiro Minami^A, Miho Katsuragawa^A, Shunsaku Nagasawa^A, Tadayuki Takahashi^A, Shin’ichiro Takeda^A, Yutaka Tsuzuki^A, Shin Watanabe^B
14: Focusing Performance of Lobster Eye Optics with a Soft X-ray Beamline; School of Mathematics and Physics, Kanazawa University; Hatsune Goto

1: Observation of solar neutrons by SciCRT XXI － Observational report; ISEE, Nagoya Univ.，ICRR, Univ. of Tokyo^A，Faculty of Science, Shinshu Univ.^B，College of Engineering, Chubu Univ.^C，Astronomical Observatory^D，JFEA^E，National Defence Academy^F，JAXA^G，IHEP, CAS^H; Y. Matsubara，Y. Itow，T. Kawabata，T. Sako^A，K. Munakata^B，C. Kato^B，S. Asakno^B，H. Takamaru^C，A. Oshima^C，T. Koi^C，S. Shibata^D，H. Kojima^D，H. Tsuchiya^E，K. Watanabe^F，M. Kozai^G，Y. Nakamura^H
2: Study on Intensity Variation of Cosmic Rays in Various Directions Observed by A Large Area High Precision Muon Tracking Detector(28); Chub Innovation Astronomical Observatory^A, Department of Engineering, Chubu University^B, Faculty of Sciencs, Osaka City University^C, Tata Institute of Fundamental Research^D, Institute for Cosmic Ray Research, University of Tokyo^E, School of Helth Science, Asahi University^F, Faculty of Sciencs, Kochi University^G, Faculty of Information, Hiroshima City University^H; H.Kojima^A, A.Ohsima^B, S.Ogio^C, S.Kawakami^C, T.Nonaka^E, Y.Hayashi^C, T.Matsuyama^C, K.Yamazaki^B, S.Shibata^A, I.Morishita^F, H.Takamaru^B, T.Koi^B, T.Nakamura^G, K.Tanaka^H, K.Suzuki^B, S.K.Gupta^D, P.K.Mohanty^D, S.R.Dugad^D, B.Hariharan^D
3: Heliospheric modulation of the cosmic-ray anisotropy observed by the Tibet ASgamma experiment (3); ICRR, Univ. of Tokyo, Dept. of Phys., Hirosaki Univ.^A, Dept. of Phys., Shinshu Univ.^B, Fac. of Engn., Yokohama Natl. Univ.^C, Fac. of Engn., Kanagawa Univ.^D,Utsunomiya Univ.^E, Shibaura Inst. of Tech.^F, ROIS^H, Coll. of Ind. Tech., Nihon Univ.^I, NII^J, NICT^K, Tokyo Metro. Coll. of Ind. Tech.^L, Dept. of Phys., Konan Univ.^M, Shonan Inst. of Tech.^N, Res. Inst. for Sci. and Engn., Waseda^O, JAEA^P; T. K. Sako, M. Amenomori^A, S. Asano^B, A. Gomi^C, K. Hibino^D, N. Hotta^E, K. Kasahara^F, Y. Katayose^C, C. Kato^B, S. Kato, T. Kawashima, K. Kawata, M. Kozai^H, D. Kurashige^C, K. Munakata^B, K. Nagaya^C, Y. Nakamura, Y. Nakazawa^I, H. Nanjo^A, M. Nishizawa^J, M. Ohnishi, S. Okukawa^C, S. Ozawa^K, T. Saito^L, Y. Sakakibara^C, M. Sakata^M, T. Sako, M. Shibata^C, A. Shiomi^I, H. Sugimoto^N, W. Takano^D, M. Takita, N. Tateyama^D, S. Torii^O, H. Tsuchiya^P, S. Udo^D, Y. Yokoe et al. (The Tibet ASgamma Collaboration)
4: Space Weather Study by Large Muon Telescope; Coll. of Engn. Chubu Univ., Grad. Sch. of Sci. Osaka City Univ.^A, Tata Inst. India^B, ICRR. Univ. of Tokyo^C, Grad. Sch. of Inf. Hiroshima City Univ.^D, Fac. of Sci. Kochi Univ.^E, IPMU^F, Fac. Econ. Asahi Univ.^G; A. Oshima, N. Ito^A, S. Ogio^A, S. Kawakami^A, H. Kojima, S. Shibata, H. Takamaru, K. Tanaka^D, H. Tanaka^F, T. Nakamura^E, T. Nonaka^C, Y. Hayashi^A, T. Matsuyama^A, I. Morishita^G, K. Yamazaki, P.K. Mohanty^B, S.K. Gupta^B, S.R. Dugad^B, B. Hariharan^B
5: CR observation of the space weather event on Nov. 2021.; Shinshu Univ., NIPR^A, NIT Ibaraki Col.^B, Res. Org. of Inf. & Systems^C, Sokendai^D; Chihiro Kato, Shunta Asano, ^○Kazuoki Munakta, Ryuho Kataoka^A, Akira Kadokura^A, Shoko Miyake^B, Masayoshi Kozai^C, Herbert Akihito Uchida^A, Kiyoka Murase^D for the GMDN collaboration
6: Correction of the atmospheric temperature effect on ground-level cosmic ray muon intensity variation; Shinshu Univ., NIPR^A, NIT Ibaraki Col.^B, Res. Org. of Inf. & Systems^C; Shunta Asano, Chihiro Kato, Ryuho Kataoka^A, ^○Kazuoki Munakta, Akira Kadokura^A, Shoko Miyake^B, Masayoshi Kozai^C

Program

Cosmic Rays/Astrophysics