The Formulation of Scaling Expansion in an Euler-Poisson Dark-fluid Model
この論文は、球対称性と多項式状態方程式を仮定した非粘性・非相対論的・回転・自己重力流体としてのダーク流体モデルを提示し、セドフとテイラーの自己相似解を用いてニュートン宇宙論の枠組みに整合する新しい解を導出し、通常の物質からダークエネルギーまでの記述への応用可能性を示したものである。
🔭 Category
astro-ph
900 件の論文
Possible Extragalactic Origins of Five LMC Globular Clusters: Proper Motion Deviations in Gaia DR3
Gaia のデータを用いた大マゼラン雲の球状星団の固有運動解析により、5 つの星団が周囲の恒星と有意に異なる運動を示していることが判明し、これらは北東方向からの矮小銀河との相互作用や合併によって大マゼラン雲に捕獲された可能性、あるいはその合併がタランチュラ星雲の恒星形成を誘発した可能性が示唆されています。
Tamojeet Roychowdhury, Navdha BhallaWed, 11 Ma🔭 astro-ph
Euclid Quick Data Release (Q1) -- Characteristics and limitations of the spectroscopic measurements
本論文は、Euclid 早期データリリース（Q1）の分光処理アルゴリズムの概要と性能を DESI 観測データと比較して検証し、特に赤方偏移 0.9〜1.8 の範囲で厳格な品質基準を適用することで 89% の成功率を達成し、宇宙論解析に向けた有望な結果を示したことを報告しています。
Euclid Collaboration, V. Le Brun, M. Bethermin, M. Moresco, D. Vibert, D. Vergani, C. Surace, G. Zamorani, A. Allaoui, T. Bedrine, P. -Y. Chabaud, G. Daste, F. Dufresne, M. Gray, E. Rossetti, Y. Copin, S. Conseil, E. Maiorano, Z. Mao, E. Palazzi, L. Pozzetti, S. Quai, C. Scarlata, M. Talia, H. M. Courtois, L. Guzzo, B. Kubik, A. M. C. Le Brun, J. A. Peacock, D. Scott, D. Bagot, A. Basset, P. Casenove, R. Gimenez, G. Libet, M. Ruffenach, N. Aghanim, B. Altieri, A. Amara, S. Andreon, N. Auricchio, H. Aussel, C. Baccigalupi, M. Baldi, A. Balestra, S. Bardelli, P. Battaglia, A. Biviano, A. Bonchi, D. Bonino, E. Branchini, M. Brescia, J. Brinchmann, A. Caillat, S. Camera, G. Cañas-Herrera, V. Capobianco, C. Carbone, J. Carretero, S. Casas, F. J. Castander, G. Castignani, S. Cavuoti, K. C. Chambers, A. Cimatti, C. Colodro-Conde, G. Congedo, C. J. Conselice, L. Conversi, A. Costille, F. Courbin, J. -G. Cuby, A. Da Silva, H. Degaudenzi, S. de la Torre, G. De Lucia, A. M. Di Giorgio, H. Dole, M. Douspis, F. Dubath, X. Dupac, S. Dusini, A. Ealet, S. Escoffier, M. Fabricius, M. Farina, R. Farinelli, F. Faustini, S. Ferriol, S. Fotopoulou, N. Fourmanoit, M. Frailis, E. Franceschi, M. Fumana, S. Galeotta, K. George, W. Gillard, B. Gillis, C. Giocoli, J. Gracia-Carpio, B. R. Granett, A. Grazian, F. Grupp, S. V. H. Haugan, J. Hoar, H. Hoekstra, W. Holmes, F. Hormuth, A. Hornstrup, P. Hudelot, K. Jahnke, M. Jhabvala, B. Joachimi, E. Keihänen, S. Kermiche, A. Kiessling, M. Kümmel, M. Kunz, H. Kurki-Suonio, Q. Le Boulc'h, D. Le Mignant, S. Ligori, P. B. Lilje, V. Lindholm, I. Lloro, G. Mainetti, D. Maino, O. Mansutti, S. Marcin, O. Marggraf, M. Martinelli, N. Martinet, F. Marulli, R. Massey, S. Maurogordato, E. Medinaceli, S. Mei, M. Melchior, Y. Mellier, M. Meneghetti, E. Merlin, G. Meylan, A. Mora, L. Moscardini, R. Nakajima, C. Neissner, R. C. Nichol, S. -M. Niemi, J. W. Nightingale, C. Padilla, S. Paltani, F. Pasian, K. Pedersen, W. J. Percival, V. Pettorino, S. Pires, G. Polenta, M. Poncet, L. A. Popa, F. Raison, R. Rebolo, A. Renzi, J. Rhodes, G. Riccio, E. Romelli, M. Roncarelli, R. Saglia, Z. Sakr, D. Sapone, B. Sartoris, M. Sauvage, J. A. Schewtschenko, M. Schirmer, P. Schneider, T. Schrabback, M. Scodeggio, A. Secroun, G. Seidel, M. Seiffert, C. Sirignano, G. Sirri, L. Stanco, J. Steinwagner, P. Tallada-Crespí, A. N. Taylor, H. I. Teplitz, I. Tereno, N. Tessore, S. Toft, R. Toledo-Moreo, F. Torradeflot, I. Tutusaus, L. Valenziano, J. Valiviita, T. Vassallo, G. Verdoes Kleijn, A. Veropalumbo, Y. Wang, J. Weller, A. Zacchei, F. M. Zerbi, I. A. Zinchenko, E. Zucca, V. Allevato, M. Ballardini, M. Bolzonella, E. Bozzo, C. Burigana, R. Cabanac, A. Cappi, D. Di Ferdinando, J. A. Escartin Vigo, G. Fabbian, L. Gabarra, W. G. Hartley, J. Martín-Fleitas, S. Matthew, M. Maturi, N. Mauri, R. B. Metcalf, A. Pezzotta, M. Pöntinen, C. Porciani, I. Risso, V. Scottez, M. Sereno, M. Tenti, M. Viel, M. Wiesmann, Y. Akrami, S. Alvi, I. T. Andika, S. Anselmi, M. Archidiacono, F. Atrio-Barandela, S. Avila, M. Bella, P. Bergamini, D. Bertacca, L. Blot, S. Borgani, M. L. Brown, S. Bruton, A. Calabro, B. Camacho Quevedo, F. Caro, C. S. Carvalho, T. Castro, Y. Charles, R. Chary, F. Cogato, A. R. Cooray, O. Cucciati, S. Davini, F. De Paolis, G. Desprez, A. Díaz-Sánchez, J. J. Diaz, S. Di Domizio, J. M. Diego, P. Dimauro, P. -A. Duc, A. Enia, Y. Fang, A. M. N. Ferguson, A. G. Ferrari, A. Finoguenov, A. Fontana, A. Franco, K. Ganga, J. García-Bellido, T. Gasparetto, V. Gautard, E. Gaztanaga, F. Giacomini, F. Gianotti, G. Gozaliasl, A. Gregorio, M. Guidi, C. M. Gutierrez, A. Hall, C. Hernández-Monteagudo, H. Hildebrandt, J. Hjorth, J. J. E. Kajava, Y. Kang, V. Kansal, D. Karagiannis, K. Kiiveri, C. C. Kirkpatrick, S. Kruk, L. Legrand, M. Lembo, F. Lepori, G. F. Lesci, J. Lesgourgues, L. Leuzzi, T. I. Liaudat, S. J. Liu, A. Loureiro, J. Macias-Perez, M. Magliocchetti, E. A. Magnier, C. Mancini, F. Mannucci, R. Maoli, C. J. A. P. Martins, L. Maurin, M. Miluzio, P. Monaco, A. Montoro, C. Moretti, G. Morgante, S. Nadathur, K. Naidoo, A. Navarro-Alsina, S. Nesseris, F. Passalacqua, K. Paterson, L. Patrizii, A. Pisani, D. Potter, M. Radovich, P. -F. Rocci, S. Sacquegna, M. Sahlén, D. B. Sanders, E. Sarpa, A. Schneider, D. Sciotti, E. Sellentin, F. Shankar, L. C. Smith, K. Tanidis, G. Testera, R. Teyssier, S. Tosi, A. Troja, M. Tucci, C. Valieri, A. Venhola, G. Verza, P. Vielzeuf, N. A. Walton, J. R. Weaver, L. Zalesky, J. G. SorceWed, 11 Ma🔭 astro-ph
Radio Spectral Energy Distribution of Low-z Metal Poor Extreme Starburst Galaxies: Novel insights on the escape of ionizing photons
低赤方偏移の低金属量極端星形成銀河の多周波数電波観測とベイズ的 SED モデリングにより、これらの銀河が高熱分率と自由 - 自由吸収を示すこと、塵の存在が確認されたこと、そしてリーマン連続光の脱出率と電波スペクトル指数の相関が実証されたことが報告されています。
Omkar Bait, Daniel Schaerer, Yuri I. Izotov, Biny SebastianWed, 11 Ma🔭 astro-ph
Meta-learning for cosmological emulation: Rapid adaptation to new lensing kernels
この論文は、メタ学習アルゴリズム（MAML）を用いて、赤方偏移分布の変化に伴う新しい重力レンズカーネルに対して、わずかなサンプル数で迅速に適応し、従来の単一タスク事前学習モデルや事前学習なしのモデルよりも高精度な宇宙論的推論を可能にする宇宙せん断角パワースペクトルのエミュレータを提案・検証したものである。
Charlie MacMahon-Gellér, C. Danielle Leonard, Philip Bull, Markus Michael RauWed, 11 Ma🔭 astro-ph
One-loop renormalization of the effective field theory of inflationary fluctuations from gravitational interactions
この論文は、重力の非線形相互作用に起因するインフレーション中の揺らぎの 1 ループ補正を有効場理論の枠組みで再正化し、超ハルスケールでの原始パワースペクトルの保存とスカラー・テンソル伝播速度の放射補正への不変性を示すとともに、マルチフィールドインフレーションへの応用を論じています。
Matteo Braglia, Lucas PinolWed, 11 Ma🔭 astro-ph
Freezing of the renormalized one-loop primordial scalar power spectrum
この論文は、インフレーション揺らぎの有効場理論を用いて、再正規化された 1 ループの原始スカラーパワースペクトルが音速ハORIZON よりも大きなスケールで完全に凍結することを初めて明示的に証明したものである。
Matteo Braglia, Lucas PinolWed, 11 Ma🔭 astro-ph
Taking a Break at Cosmic Noon: Continuum-selected Low-mass Galaxies Require Long Burst Cycles
JWST による観測とモデル比較から、宇宙の正午（1<z<3）における低質量銀河の星形成は、分子雲スケールのランダム性ではなく銀河スケールのガス循環によって制御され、1 億年以上の周期で星形成主系列を上下に大きく変動する「バーストサイクル」が支配的であることが示されました。
Abby Mintz, David J. Setton, Jenny E. Greene, Joel Leja, Bingjie Wang, Emilie Burnham, Katherine A. Suess, Hakim Atek, Rachel Bezanson, Gabriel Brammer, Sam E. Cutler, Pratika Dayal, Robert Feldmann, Lukas J. Furtak, Karl Glazebrook, Gourav Khullar, Vasily Kokorev, Ivo Labbé, Jorryt Matthee, Michael V. Maseda, Tim B. Miller, Ikki Mitsuhashi, Themiya Nanayakkara, Richard Pan, Sedona H. Price, John R. Weaver, Katherine E. Whitaker, Belinda WuWed, 11 Ma🔭 astro-ph
Perturbative unitarity bounds on field-space curvature in de Sitter spacetime: purity vs scattering amplitude
この論文は、ド・ジッター時空における場空間の曲率に対する摂動的なユニタリ性の制約を、最近提案された運動量空間エンタングルメント手法を用いて研究し、純度計算を通じてド・ジッター時空の熱的性質を反映したハッブルスケール程度の新たな上限が導かれることを示しています。
Qianhang Cai, Tomoya Inada, Masataka Ishikawa, Kanji Nishii, Toshifumi NoumiWed, 11 Ma🔭 astro-ph
GRB 221009A: Observations with LST-1 of CTAO and Implications for Structured Jets in Long Gamma-Ray Bursts
CTAO の LST-1 による GRB 221009A の観測結果は、バースト発生から約 1.33 日後に 4.1σの有意な過剰を検出したものの、それ以降のデータは背景と一致しており、これにより 1 日後の VHE 放射が$10^{-11}ergcm^{-2}s^{-1}$を大幅に超えるモデルは支持されず、長期 VHE 観測が GRB ジェットの構造解明に寄与することが示されました。
LST Collaboration, K. Abe (Department of Physics, Tokai University, 4-1-1, Kita-Kaname, Hiratsuka, Kanagawa 259-1292, Japan), S. Abe (Institute for Cosmic Ray Research, University of Tokyo, 5-1-5, Kashiwa-no-ha, Kashiwa, Chiba 277-8582, Japan), A. Abhishek (INFN and Università degli Studi di Siena, Dipartimento di Scienze Fisiche, della Terra e dell'Ambiente), F. Acero (Université Paris-Saclay, Université Paris Cité, CEA, CNRS, AIM, F-91191 Gif-sur-Yvette Cedex, France, FSLAC IRL 2009, CNRS/IAC, La Laguna, Tenerife, Spain), A. Aguasca-Cabot (Departament de Física Quàntica i Astrofísica, Institut de Ciències del Cosmos, Universitat de Barcelona, IEEC-UB, Martí i Franquès, 1, 08028, Barcelona, Spain), I. Agudo (Instituto de Astrofísica de Andalucía-CSIC, Glorieta de la Astronomía s/n, 18008, Granada, Spain), C. Alispach (Department of Astronomy, University of Geneva, Chemin d'Ecogia 16, CH-1290 Versoix, Switzerland), D. Ambrosino (INFN Sezione di Napoli, Via Cintia, ed. G, 80126 Napoli, Italy), F. Ambrosino (INAF - Osservatorio Astronomico di Roma, Via di Frascati 33, 00040, Monteporzio Catone, Italy), L. A. Antonelli (INAF - Osservatorio Astronomico di Roma, Via di Frascati 33, 00040, Monteporzio Catone, Italy), C. Aramo (INFN Sezione di Napoli, Via Cintia, ed. G, 80126 Napoli, Italy), A. Arbet-Engels (Max-Planck-Institut für Physik, Boltzmannstraße 8, 85748 Garching bei München), C. Arcaro (INFN Sezione di Padova and Università degli Studi di Padova, Via Marzolo 8, 35131 Padova, Italy), T. T. H. Arnesen (Instituto de Astrofísica de Canarias and Departamento de Astrofísica, Universidad de La Laguna, C. Vía Láctea, s/n, 38205 La Laguna, Santa Cruz de Tenerife, Spain), K. Asano (Institute for Cosmic Ray Research, University of Tokyo, 5-1-5, Kashiwa-no-ha, Kashiwa, Chiba 277-8582, Japan), P. Aubert (Univ. Savoie Mont Blanc, CNRS, Laboratoire d'Annecy de Physique des Particules - IN2P3, 74000 Annecy, France), A. Baktash (Universität Hamburg, Institut für Experimentalphysik, Luruper Chaussee 149, 22761 Hamburg, Germany), M. Balbo (Department of Astronomy, University of Geneva, Chemin d'Ecogia 16, CH-1290 Versoix, Switzerland), A. Bamba (Graduate School of Science, University of Tokyo, 7-3-1 Hongo, Bunkyo-ku, Tokyo 113-0033, Japan), A. Baquero Larriva (IPARCOS-UCM, Instituto de Física de Partículas y del Cosmos, and EMFTEL Department, Universidad Complutense de Madrid, Plaza de Ciencias, 1. Ciudad Universitaria, 28040 Madrid, Spain, Faculty of Science and Technology, Universidad del Azuay, Cuenca, Ecuador), U. Barres de Almeida (Centro Brasileiro de Pesquisas Físicas, Rua Xavier Sigaud 150, RJ 22290-180, Rio de Janeiro, Brazil), J. A. Barrio (IPARCOS-UCM, Instituto de Física de Partículas y del Cosmos, and EMFTEL Department, Universidad Complutense de Madrid, Plaza de Ciencias, 1. Ciudad Universitaria, 28040 Madrid, Spain), L. Barrios Jiménez (Instituto de Astrofísica de Canarias and Departamento de Astrofísica, Universidad de La Laguna, C. Vía Láctea, s/n, 38205 La Laguna, Santa Cruz de Tenerife, Spain), I. Batkovic (INFN Sezione di Padova and Università degli Studi di Padova, Via Marzolo 8, 35131 Padova, Italy), J. Baxter (Institute for Cosmic Ray Research, University of Tokyo, 5-1-5, Kashiwa-no-ha, Kashiwa, Chiba 277-8582, Japan), J. Becerra González (Instituto de Astrofísica de Canarias and Departamento de Astrofísica, Universidad de La Laguna, C. Vía Láctea, s/n, 38205 La Laguna, Santa Cruz de Tenerife, Spain), E. Bernardini (INFN Sezione di Padova and Università degli Studi di Padova, Via Marzolo 8, 35131 Padova, Italy), J. Bernete (CIEMAT, Avda. Complutense 40, 28040 Madrid, Spain), A. Berti (Max-Planck-Institut für Physik, Boltzmannstraße 8, 85748 Garching bei München), I. Bezshyiko (University of Geneva - Département de physique nucléaire et corpusculaire, 24 Quai Ernest Ansernet, 1211 Genève 4, Switzerland), C. Bigongiari (INAF - Osservatorio Astronomico di Roma, Via di Frascati 33, 00040, Monteporzio Catone, Italy), E. Bissaldi (INFN Sezione di Bari and Politecnico di Bari, via Orabona 4, 70124 Bari, Italy), O. Blanch (Institut de Fisica d'Altes Energies), G. Bonnoli (INAF - Osservatorio Astronomico di Brera, Via Brera 28, 20121 Milano, Italy), P. Bordas (Departament de Física Quàntica i Astrofísica, Institut de Ciències del Cosmos, Universitat de Barcelona, IEEC-UB, Martí i Franquès, 1, 08028, Barcelona, Spain), G. Borkowski (Faculty of Physics and Applied Informatics, University of Lodz, ul. Pomorska 149-153, 90-236 Lodz, Poland), G. Brunelli (INAF - Osservatorio di Astrofisica e Scienza dello spazio di Bologna, Via Piero Gobetti 93/3, 40129 Bologna, Italy, Dipartimento di Fisica e Astronomia), A. Bulgarelli (INAF - Osservatorio di Astrofisica e Scienza dello spazio di Bologna, Via Piero Gobetti 93/3, 40129 Bologna, Italy), M. Bunse (Lamarr Institute for Machine Learning and Artificial Intelligence, 44227 Dortmund, Germany), I. Burelli (INFN Sezione di Trieste and Università degli studi di Udine, via delle scienze 206, 33100 Udine, Italy), L. Burmistrov (University of Geneva - Département de physique nucléaire et corpusculaire, 24 Quai Ernest Ansernet, 1211 Genève 4, Switzerland), M. Cardillo (INAF - Istituto di Astrofisica e Planetologia Spaziali), S. Caroff (Univ. Savoie Mont Blanc, CNRS, Laboratoire d'Annecy de Physique des Particules - IN2P3, 74000 Annecy, France), A. Carosi (INAF - Osservatorio Astronomico di Roma, Via di Frascati 33, 00040, Monteporzio Catone, Italy), R. Carraro (INAF - Osservatorio Astronomico di Roma, Via di Frascati 33, 00040, Monteporzio Catone, Italy), M. S. Carrasco (Aix Marseille Univ, CNRS/IN2P3, CPPM, Marseille, France), F. Cassol (Aix Marseille Univ, CNRS/IN2P3, CPPM, Marseille, France), D. Cerasole (INFN Sezione di Bari and Università di Bari, via Orabona 4, 70126 Bari, Italy), G. Ceribella (Max-Planck-Institut für Physik, Boltzmannstraße 8, 85748 Garching bei München), A. Cerviño Cortínez (IPARCOS-UCM, Instituto de Física de Partículas y del Cosmos, and EMFTEL Department, Universidad Complutense de Madrid, Plaza de Ciencias, 1. Ciudad Universitaria, 28040 Madrid, Spain), Y. Chai (Max-Planck-Institut für Physik, Boltzmannstraße 8, 85748 Garching bei München), K. Cheng (Institute for Cosmic Ray Research, University of Tokyo, 5-1-5, Kashiwa-no-ha, Kashiwa, Chiba 277-8582, Japan), A. Chiavassa (INFN Sezione di Torino, Via P. Giuria 1, 10125 Torino, Italy, Dipartimento di Fisica - Universitá degli Studi di Torino, Via Pietro Giuria 1 - 10125 Torino, Italy), M. Chikawa (Institute for Cosmic Ray Research, University of Tokyo, 5-1-5, Kashiwa-no-ha, Kashiwa, Chiba 277-8582, Japan), G. Chon (Max-Planck-Institut für Physik, Boltzmannstraße 8, 85748 Garching bei München), L. Chytka (Palacky University Olomouc, Faculty of Science, 17. listopadu 1192/12, 771 46 Olomouc, Czech Republic), G. M. Cicciari (Dipartimento di Fisica e Chimica 'E. Segrè' Università degli Studi di Palermo, via delle Scienze, 90128 Palermo, INFN Sezione di Catania, Via S. Sofia 64, 95123 Catania, Italy), A. Cifuentes (CIEMAT, Avda. Complutense 40, 28040 Madrid, Spain), J. L. Contreras (IPARCOS-UCM, Instituto de Física de Partículas y del Cosmos, and EMFTEL Department, Universidad Complutense de Madrid, Plaza de Ciencias, 1. Ciudad Universitaria, 28040 Madrid, Spain), J. Cortina (CIEMAT, Avda. Complutense 40, 28040 Madrid, Spain), H. Costantini (Aix Marseille Univ, CNRS/IN2P3, CPPM, Marseille, France), M. Dalchenko (University of Geneva - Département de physique nucléaire et corpusculaire, 24 Quai Ernest Ansernet, 1211 Genève 4, Switzerland), P. Da Vela (INAF - Osservatorio di Astrofisica e Scienza dello spazio di Bologna, Via Piero Gobetti 93/3, 40129 Bologna, Italy), F. Dazzi (INAF - Osservatorio Astronomico di Roma, Via di Frascati 33, 00040, Monteporzio Catone, Italy), A. De Angelis (INFN Sezione di Padova and Università degli Studi di Padova, Via Marzolo 8, 35131 Padova, Italy), M. de Bony de Lavergne (IRFU, CEA, Université Paris-Saclay, Bât 141, 91191 Gif-sur-Yvette, France), R. Del Burgo (INFN Sezione di Napoli, Via Cintia, ed. G, 80126 Napoli, Italy), C. Delgado (CIEMAT, Avda. Complutense 40, 28040 Madrid, Spain), J. Delgado Mengual (Port d'Informació Científica, Edifici D, Carrer de l'Albareda, 08193 Bellaterrra), M. Dellaiera (Univ. Savoie Mont Blanc, CNRS, Laboratoire d'Annecy de Physique des Particules - IN2P3, 74000 Annecy, France), D. della Volpe (University of Geneva - Département de physique nucléaire et corpusculaire, 24 Quai Ernest Ansernet, 1211 Genève 4, Switzerland), B. De Lotto (INFN Sezione di Trieste and Università degli studi di Udine, via delle scienze 206, 33100 Udine, Italy), L. Del Peral (University of Alcalá UAH, Departamento de Physics and Mathematics, Pza. San Diego, 28801, Alcalá de Henares, Madrid, Spain), R. de Menezes (INFN Sezione di Torino, Via P. Giuria 1, 10125 Torino, Italy), G. De Palma (INFN Sezione di Bari and Politecnico di Bari, via Orabona 4, 70124 Bari, Italy), C. Díaz (CIEMAT, Avda. Complutense 40, 28040 Madrid, Spain), A. Di Piano (INAF - Osservatorio di Astrofisica e Scienza dello spazio di Bologna, Via Piero Gobetti 93/3, 40129 Bologna, Italy), F. Di Pierro (INFN Sezione di Torino, Via P. Giuria 1, 10125 Torino, Italy), R. Di Tria (INFN Sezione di Bari and Università di Bari, via Orabona 4, 70126 Bari, Italy), L. Di Venere (INFN Sezione di Bari, via Orabona 4, 70125, Bari, Italy), R. M. Dominik (Department of Physics, TU Dortmund University, Otto-Hahn-Str. 4, 44227 Dortmund, Germany), D. Dominis Prester (University of Rijeka, Department of Physics, Radmile Matejcic 2, 51000 Rijeka, Croatia), A. Donini (INAF - Osservatorio Astronomico di Roma, Via di Frascati 33, 00040, Monteporzio Catone, Italy), D. Dorner (Institute for Theoretical Physics and Astrophysics, Universität Würzburg, Campus Hubland Nord, Emil-Fischer-Str. 31, 97074 Würzburg, Germany), M. Doro (INFN Sezione di Padova and Università degli Studi di Padova, Via Marzolo 8, 35131 Padova, Italy), L. Eisenberger (Institute for Theoretical Physics and Astrophysics, Universität Würzburg, Campus Hubland Nord, Emil-Fischer-Str. 31, 97074 Würzburg, Germany), D. Elsässer (Department of Physics, TU Dortmund University, Otto-Hahn-Str. 4, 44227 Dortmund, Germany), G. Emery (Aix Marseille Univ, CNRS/IN2P3, CPPM, Marseille, France), J. Escudero (Instituto de Astrofísica de Andalucía-CSIC, Glorieta de la Astronomía s/n, 18008, Granada, Spain), V. Fallah Ramazani (Department of Physics and Astronomy, University of Turku, Finland, FI-20014 University of Turku, Finland, Department of Physics, TU Dortmund University, Otto-Hahn-Str. 4, 44227 Dortmund, Germany), F. Ferrarotto (INFN Sezione di Roma La Sapienza, P.le Aldo Moro, 2 - 00185 Rome, Italy), A. Fiasson (Univ. Savoie Mont Blanc, CNRS, Laboratoire d'Annecy de Physique des Particules - IN2P3, 74000 Annecy, France, ILANCE, CNRS - University of Tokyo International Research Laboratory, University of Tokyo, 5-1-5 Kashiwa-no-Ha Kashiwa City, Chiba 277-8582, Japan), L. Foffano (INAF - Istituto di Astrofisica e Planetologia Spaziali), F. Frías García-Lago (Instituto de Astrofísica de Canarias and Departamento de Astrofísica, Universidad de La Laguna, C. Vía Láctea, s/n, 38205 La Laguna, Santa Cruz de Tenerife, Spain), S. Fröse (Department of Physics, TU Dortmund University, Otto-Hahn-Str. 4, 44227 Dortmund, Germany), Y. Fukazawa (Physics Program, Graduate School of Advanced Science and Engineering, Hiroshima University, 1-3-1 Kagamiyama, Higashi-Hiroshima City, Hiroshima, 739-8526, Japan), S. Gallozzi (INAF - Osservatorio Astronomico di Roma, Via di Frascati 33, 00040, Monteporzio Catone, Italy), R. Garcia López (Instituto de Astrofísica de Canarias and Departamento de Astrofísica, Universidad de La Laguna, C. Vía Láctea, s/n, 38205 La Laguna, Santa Cruz de Tenerife, Spain), S. Garcia Soto (CIEMAT, Avda. Complutense 40, 28040 Madrid, Spain), C. Gasbarra (INFN Sezione di Roma Tor Vergata, Via della Ricerca Scientifica 1, 00133 Rome, Italy), D. Gasparrini (INFN Sezione di Roma Tor Vergata, Via della Ricerca Scientifica 1, 00133 Rome, Italy), D. Geyer (Department of Physics, TU Dortmund University, Otto-Hahn-Str. 4, 44227 Dortmund, Germany), J. Giesbrecht Paiva (Centro Brasileiro de Pesquisas Físicas, Rua Xavier Sigaud 150, RJ 22290-180, Rio de Janeiro, Brazil), N. Giglietto (INFN Sezione di Bari and Politecnico di Bari, via Orabona 4, 70124 Bari, Italy), F. Giordano (INFN Sezione di Bari and Università di Bari, via Orabona 4, 70126 Bari, Italy), N. Godinovic (University of Split, FESB, R. Boškovica 32, 21000 Split, Croatia), T. Gradetzke (Department of Physics, TU Dortmund University, Otto-Hahn-Str. 4, 44227 Dortmund, Germany), R. Grau (Institut de Fisica d'Altes Energies), D. Green (Max-Planck-Institut für Physik, Boltzmannstraße 8, 85748 Garching bei München), J. Green (Max-Planck-Institut für Physik, Boltzmannstraße 8, 85748 Garching bei München), S. Gunji (Department of Physics, Yamagata University, 1-4-12 Kojirakawa-machi, Yamagata-shi, 990-8560, Japan), P. Günther (Institute for Theoretical Physics and Astrophysics, Universität Würzburg, Campus Hubland Nord, Emil-Fischer-Str. 31, 97074 Würzburg, Germany), J. Hackfeld (Institut für Theoretische Physik, Lehrstuhl IV: Plasma-Astroteilchenphysik, Ruhr-Universität Bochum, Universitätsstraße 150, 44801 Bochum, Germany), D. Hadasch (Institute for Cosmic Ray Research, University of Tokyo, 5-1-5, Kashiwa-no-ha, Kashiwa, Chiba 277-8582, Japan), A. Hahn (Max-Planck-Institut für Physik, Boltzmannstraße 8, 85748 Garching bei München), M. Hashizume (Physics Program, Graduate School of Advanced Science and Engineering, Hiroshima University, 1-3-1 Kagamiyama, Higashi-Hiroshima City, Hiroshima, 739-8526, Japan), T. Hassan (CIEMAT, Avda. Complutense 40, 28040 Madrid, Spain), K. Hayashi (Institute for Cosmic Ray Research, University of Tokyo, 5-1-5, Kashiwa-no-ha, Kashiwa, Chiba 277-8582, Japan, Sendai College, National Institute of Technology, 4-16-1 Ayashi-Chuo, Aoba-ku, Sendai city, Miyagi 989-3128, Japan), L. Heckmann (Max-Planck-Institut für Physik, Boltzmannstraße 8, 85748 Garching bei München, Université Paris Cité, CNRS, Astroparticule et Cosmologie, F-75013 Paris, France), M. Heller (University of Geneva - Département de physique nucléaire et corpusculaire, 24 Quai Ernest Ansernet, 1211 Genève 4, Switzerland), J. Herrera Llorente (Instituto de Astrofísica de Canarias and Departamento de Astrofísica, Universidad de La Laguna, C. Vía Láctea, s/n, 38205 La Laguna, Santa Cruz de Tenerife, Spain), K. Hirotani (Institute for Cosmic Ray Research, University of Tokyo, 5-1-5, Kashiwa-no-ha, Kashiwa, Chiba 277-8582, Japan), D. Hoffmann (Aix Marseille Univ, CNRS/IN2P3, CPPM, Marseille, France), D. Horns (Universität Hamburg, Institut für Experimentalphysik, Luruper Chaussee 149, 22761 Hamburg, Germany), J. Houles (Aix Marseille Univ, CNRS/IN2P3, CPPM, Marseille, France), M. Hrabovsky (Palacky University Olomouc, Faculty of Science, 17. listopadu 1192/12, 771 46 Olomouc, Czech Republic), D. Hrupec (Josip Juraj Strossmayer University of Osijek, Department of Physics, Trg Ljudevita Gaja 6, 31000 Osijek, Croatia), D. Hui (Institute for Cosmic Ray Research, University of Tokyo, 5-1-5, Kashiwa-no-ha, Kashiwa, Chiba 277-8582, Japan, Department of Astronomy and Space Science, Chungnam National University, Daejeon 34134, Republic of Korea), M. Iarlori (INFN Dipartimento di Scienze Fisiche e Chimiche - Università degli Studi dell'Aquila and Gran Sasso Science Institute, Via Vetoio 1, Viale Crispi 7, 67100 L'Aquila, Italy), R. Imazawa (Physics Program, Graduate School of Advanced Science and Engineering, Hiroshima University, 1-3-1 Kagamiyama, Higashi-Hiroshima City, Hiroshima, 739-8526, Japan), T. Inada (Institute for Cosmic Ray Research, University of Tokyo, 5-1-5, Kashiwa-no-ha, Kashiwa, Chiba 277-8582, Japan), Y. Inome (Institute for Cosmic Ray Research, University of Tokyo, 5-1-5, Kashiwa-no-ha, Kashiwa, Chiba 277-8582, Japan), S. Inoue (Institute for Cosmic Ray Research, University of Tokyo, 5-1-5, Kashiwa-no-ha, Kashiwa, Chiba 277-8582, Japan, Chiba University, 1-33, Yayoicho, Inage-ku, Chiba-shi, Chiba, 263-8522 Japan), K. Ioka (Kitashirakawa Oiwakecho, Sakyo Ward, Kyoto, 606-8502, Japan), M. Iori (INFN Sezione di Roma La Sapienza, P.le Aldo Moro, 2 - 00185 Rome, Italy), T. Itokawa (Institute for Cosmic Ray Research, University of Tokyo, 5-1-5, Kashiwa-no-ha, Kashiwa, Chiba 277-8582, Japan), A. Iuliano (INFN Sezione di Napoli, Via Cintia, ed. G, 80126 Napoli, Italy), J. Jahanvi (INFN Sezione di Trieste and Università degli studi di Udine, via delle scienze 206, 33100 Udine, Italy), I. Jimenez Martinez (Max-Planck-Institut für Physik, Boltzmannstraße 8, 85748 Garching bei München), J. Jimenez Quiles (Institut de Fisica d'Altes Energies), I. Jorge Rodrigo (CIEMAT, Avda. Complutense 40, 28040 Madrid, Spain), J. Jurysek (FZU - Institute of Physics of the Czech Academy of Sciences, Na Slovance 1999/2, 182 21 Praha 8, Czech Republic), M. Kagaya (Institute for Cosmic Ray Research, University of Tokyo, 5-1-5, Kashiwa-no-ha, Kashiwa, Chiba 277-8582, Japan, Sendai College, National Institute of Technology, 4-16-1 Ayashi-Chuo, Aoba-ku, Sendai city, Miyagi 989-3128, Japan), O. Kalashev (Laboratory for High Energy Physics, École Polytechnique Fédérale, CH-1015 Lausanne, Switzerland), V. Karas (Astronomical Institute of the Czech Academy of Sciences, Bocni II 1401 - 14100 Prague, Czech Republic), H. Katagiri (Faculty of Science, Ibaraki University, 2 Chome-1-1 Bunkyo, Mito, Ibaraki 310-0056, Japan), D. Kerszberg (Institut de Fisica d'Altes Energies, Sorbonne Université, CNRS/IN2P3, Laboratoire de Physique Nucléaire et de Hautes Energies, LPNHE, 4 place Jussieu, 75005 Paris, France), T. Kiyomot (Graduate School of Science and Engineering, Saitama University, 255 Simo-Ohkubo, Sakura-ku, Saitama city, Saitama 338-8570, Japan), Y. Kobayashi (Institute for Cosmic Ray Research, University of Tokyo, 5-1-5, Kashiwa-no-ha, Kashiwa, Chiba 277-8582, Japan), K. Kohri (Institute of Particle and Nuclear Studies, KEK), A. Kong (Institute for Cosmic Ray Research, University of Tokyo, 5-1-5, Kashiwa-no-ha, Kashiwa, Chiba 277-8582, Japan), P. Kornecki (Instituto de Astrofísica de Andalucía-CSIC, Glorieta de la Astronomía s/n, 18008, Granada, Spain), H. Kubo (Institute for Cosmic Ray Research, University of Tokyo, 5-1-5, Kashiwa-no-ha, Kashiwa, Chiba 277-8582, Japan), J. Kushida (Department of Physics, Tokai University, 4-1-1, Kita-Kaname, Hiratsuka, Kanagawa 259-1292, Japan), B. Lacave (University of Geneva - Département de physique nucléaire et corpusculaire, 24 Quai Ernest Ansernet, 1211 Genève 4, Switzerland), M. Lainez (IPARCOS-UCM, Instituto de Física de Partículas y del Cosmos, and EMFTEL Department, Universidad Complutense de Madrid, Plaza de Ciencias, 1. Ciudad Universitaria, 28040 Madrid, Spain), G. Lamanna (Univ. Savoie Mont Blanc, CNRS, Laboratoire d'Annecy de Physique des Particules - IN2P3, 74000 Annecy, France), A. Lamastra (INAF - Osservatorio Astronomico di Roma, Via di Frascati 33, 00040, Monteporzio Catone, Italy), L. Lemoigne (Univ. Savoie Mont Blanc, CNRS, Laboratoire d'Annecy de Physique des Particules - IN2P3, 74000 Annecy, France), M. Linhoff (Department of Physics, TU Dortmund University, Otto-Hahn-Str. 4, 44227 Dortmund, Germany), S. Lombardi (INAF - Osservatorio Astronomico di Roma, Via di Frascati 33, 00040, Monteporzio Catone, Italy), F. Longo (INFN Sezione di Trieste and Università degli Studi di Trieste, Via Valerio 2 I, 34127 Trieste, Italy), R. López-Coto (Instituto de Astrofísica de Andalucía-CSIC, Glorieta de la Astronomía s/n, 18008, Granada, Spain), M. López-Moya (IPARCOS-UCM, Instituto de Física de Partículas y del Cosmos, and EMFTEL Department, Universidad Complutense de Madrid, Plaza de Ciencias, 1. Ciudad Universitaria, 28040 Madrid, Spain), A. López-Oramas (Instituto de Astrofísica de Canarias and Departamento de Astrofísica, Universidad de La Laguna, C. Vía Láctea, s/n, 38205 La Laguna, Santa Cruz de Tenerife, Spain), S. Loporchio (INFN Sezione di Bari and Università di Bari, via Orabona 4, 70126 Bari, Italy), A. Lorini (INFN and Università degli Studi di Siena, Dipartimento di Scienze Fisiche, della Terra e dell'Ambiente), J. Lozano Bahilo (University of Alcalá UAH, Departamento de Physics and Mathematics, Pza. San Diego, 28801, Alcalá de Henares, Madrid, Spain), F. Lucarelli (INAF - Osservatorio Astronomico di Roma, Via di Frascati 33, 00040, Monteporzio Catone, Italy), H. Luciani (INFN Sezione di Trieste and Università degli Studi di Trieste, Via Valerio 2 I, 34127 Trieste, Italy), P. L. Luque-Escamilla (Escuela Politécnica Superior de Jaén, Universidad de Jaén, Campus Las Lagunillas s/n, Edif. A3, 23071 Jaén, Spain), P. Majumdar (Institute for Cosmic Ray Research, University of Tokyo, 5-1-5, Kashiwa-no-ha, Kashiwa, Chiba 277-8582, Japan, Saha Institute of Nuclear Physics, Sector 1, AF Block, Bidhan Nagar, Bidhannagar, Kolkata, West Bengal 700064, India), M. Makariev (Institute for Nuclear Research and Nuclear Energy, Bulgarian Academy of Sciences, 72 boul. Tsarigradsko chaussee, 1784 Sofia, Bulgaria), M. Mallamaci (Dipartimento di Fisica e Chimica 'E. Segrè' Università degli Studi di Palermo, via delle Scienze, 90128 Palermo, INFN Sezione di Catania, Via S. Sofia 64, 95123 Catania, Italy), D. Mandat (FZU - Institute of Physics of the Czech Academy of Sciences, Na Slovance 1999/2, 182 21 Praha 8, Czech Republic), M. Manganaro (University of Rijeka, Department of Physics, Radmile Matejcic 2, 51000 Rijeka, Croatia), D. K. Maniadakis (INAF - Osservatorio Astronomico di Roma, Via di Frascati 33, 00040, Monteporzio Catone, Italy), G. Manicò (INFN Sezione di Catania, Via S. Sofia 64, 95123 Catania, Italy), K. Mannheim (Institute for Theoretical Physics and Astrophysics, Universität Würzburg, Campus Hubland Nord, Emil-Fischer-Str. 31, 97074 Würzburg, Germany), S. Marchesi (INAF - Osservatorio di Astrofisica e Scienza dello spazio di Bologna, Via Piero Gobetti 93/3, 40129 Bologna, Italy, Dipartimento di Fisica e Astronomia, Department of Physics and Astronomy, Clemson University, Kinard Lab of Physics, Clemson, SC 29634, USA), F. Marini (INFN Sezione di Padova and Università degli Studi di Padova, Via Marzolo 8, 35131 Padova, Italy), M. Mariotti (INFN Sezione di Padova and Università degli Studi di Padova, Via Marzolo 8, 35131 Padova, Italy), P. Marquez (Institut de Fisica d'Altes Energies), G. Marsella (Dipartimento di Fisica e Chimica 'E. Segrè' Università degli Studi di Palermo, via delle Scienze, 90128 Palermo, INFN Sezione di Catania, Via S. Sofia 64, 95123 Catania, Italy), J. Martí (Escuela Politécnica Superior de Jaén, Universidad de Jaén, Campus Las Lagunillas s/n, Edif. A3, 23071 Jaén, Spain), O. Martinez (Grupo de Electronica, Universidad Complutense de Madrid, Av. Complutense s/n, 28040 Madrid, Spain), G. Martínez (CIEMAT, Avda. Complutense 40, 28040 Madrid, Spain), M. Martínez (Institut de Fisica d'Altes Energies), A. Mas-Aguilar (IPARCOS-UCM, Instituto de Física de Partículas y del Cosmos, and EMFTEL Department, Universidad Complutense de Madrid, Plaza de Ciencias, 1. Ciudad Universitaria, 28040 Madrid, Spain), M. Massa (INFN and Università degli Studi di Siena, Dipartimento di Scienze Fisiche, della Terra e dell'Ambiente), G. Maurin (Univ. Savoie Mont Blanc, CNRS, Laboratoire d'Annecy de Physique des Particules - IN2P3, 74000 Annecy, France), D. Mazin (Institute for Cosmic Ray Research, University of Tokyo, 5-1-5, Kashiwa-no-ha, Kashiwa, Chiba 277-8582, Japan, Max-Planck-Institut für Physik, Boltzmannstraße 8, 85748 Garching bei München), J. Méndez-Gallego (Instituto de Astrofísica de Andalucía-CSIC, Glorieta de la Astronomía s/n, 18008, Granada, Spain), S. Menon (INAF - Osservatorio Astronomico di Roma, Via di Frascati 33, 00040, Monteporzio Catone, Italy), E. Mestre Guillen (Institute of Space Sciences), D. Miceli (INFN Sezione di Padova and Università degli Studi di Padova, Via Marzolo 8, 35131 Padova, Italy), T. Miener (IPARCOS-UCM, Instituto de Física de Partículas y del Cosmos, and EMFTEL Department, Universidad Complutense de Madrid, Plaza de Ciencias, 1. Ciudad Universitaria, 28040 Madrid, Spain), J. M. Miranda (Grupo de Electronica, Universidad Complutense de Madrid, Av. Complutense s/n, 28040 Madrid, Spain), R. Mirzoyan (Max-Planck-Institut für Physik, Boltzmannstraße 8, 85748 Garching bei München), M. Mizote (Department of Physics, Konan University, 8-9-1 Okamoto, Higashinada-ku Kobe 658-8501, Japan), T. Mizuno (Physics Program, Graduate School of Advanced Science and Engineering, Hiroshima University, 1-3-1 Kagamiyama, Higashi-Hiroshima City, Hiroshima, 739-8526, Japan), M. Molero Gonzalez (Instituto de Astrofísica de Canarias and Departamento de Astrofísica, Universidad de La Laguna, C. Vía Láctea, s/n, 38205 La Laguna, Santa Cruz de Tenerife, Spain), E. Molina (Instituto de Astrofísica de Canarias and Departamento de Astrofísica, Universidad de La Laguna, C. Vía Láctea, s/n, 38205 La Laguna, Santa Cruz de Tenerife, Spain), T. Montaruli (University of Geneva - Département de physique nucléaire et corpusculaire, 24 Quai Ernest Ansernet, 1211 Genève 4, Switzerland), A. Moralejo (Institut de Fisica d'Altes Energies), D. Morcuende (Instituto de Astrofísica de Andalucía-CSIC, Glorieta de la Astronomía s/n, 18008, Granada, Spain), A. Moreno Ramos (Grupo de Electronica, Universidad Complutense de Madrid, Av. Complutense s/n, 28040 Madrid, Spain), A. Morselli (INFN Sezione di Roma Tor Vergata, Via della Ricerca Scientifica 1, 00133 Rome, Italy), V. Moya (IPARCOS-UCM, Instituto de Física de Partículas y del Cosmos, and EMFTEL Department, Universidad Complutense de Madrid, Plaza de Ciencias, 1. Ciudad Universitaria, 28040 Madrid, Spain), H. Muraishi (School of Allied Health Sciences, Kitasato University, Sagamihara, Kanagawa 228-8555, Japan), S. Nagataki (RIKEN, Institute of Physical and Chemical Research, 2-1 Hirosawa, Wako, Saitama, 351-0198, Japan), T. Nakamori (Department of Physics, Yamagata University, 1-4-12 Kojirakawa-machi, Yamagata-shi, 990-8560, Japan), A. Neronov (Laboratory for High Energy Physics, École Polytechnique Fédérale, CH-1015 Lausanne, Switzerland), D. Nieto Castaño (IPARCOS-UCM, Instituto de Física de Partículas y del Cosmos, and EMFTEL Department, Universidad Complutense de Madrid, Plaza de Ciencias, 1. Ciudad Universitaria, 28040 Madrid, Spain), M. Nievas Rosillo (Instituto de Astrofísica de Canarias and Departamento de Astrofísica, Universidad de La Laguna, C. Vía Láctea, s/n, 38205 La Laguna, Santa Cruz de Tenerife, Spain), L. Nikolic (INFN and Università degli Studi di Siena, Dipartimento di Scienze Fisiche, della Terra e dell'Ambiente), K. Nishijima (Department of Physics, Tokai University, 4-1-1, Kita-Kaname, Hiratsuka, Kanagawa 259-1292, Japan), K. Noda (Institute for Cosmic Ray Research, University of Tokyo, 5-1-5, Kashiwa-no-ha, Kashiwa, Chiba 277-8582, Japan, Chiba University, 1-33, Yayoicho, Inage-ku, Chiba-shi, Chiba, 263-8522 Japan), D. Nosek (Charles University, Institute of Particle and Nuclear Physics, V Holešovičkách 2, 180 00 Prague 8, Czech Republic), V. Novotny (Charles University, Institute of Particle and Nuclear Physics, V Holešovičkách 2, 180 00 Prague 8, Czech Republic), S. Nozaki (Max-Planck-Institut für Physik, Boltzmannstraße 8, 85748 Garching bei München), M. Ohishi (Institute for Cosmic Ray Research, University of Tokyo, 5-1-5, Kashiwa-no-ha, Kashiwa, Chiba 277-8582, Japan), Y. Ohtani (Institute for Cosmic Ray Research, University of Tokyo, 5-1-5, Kashiwa-no-ha, Kashiwa, Chiba 277-8582, Japan), T. Oka (Division of Physics and Astronomy, Graduate School of Science, Kyoto University, Sakyo-ku, Kyoto, 606-8502, Japan), A. Okumura (Institute for Space-Earth Environmental Research, Nagoya University, Chikusa-ku, Nagoya 464-8601, Japan, Kobayashi-Maskawa Institute), R. Orito (Graduate School of Technology, Industrial and Social Sciences, Tokushima University, 2-1 Minamijosanjima, Tokushima, 770-8506, Japan), L. Orsini (INFN and Università degli Studi di Siena, Dipartimento di Scienze Fisiche, della Terra e dell'Ambiente), J. Otero-Santos (Instituto de Astrofísica de Andalucía-CSIC, Glorieta de la Astronomía s/n, 18008, Granada, Spain), P. Ottanelli (INFN Sezione di Pisa, Edificio C - Polo Fibonacci, Largo Bruno Pontecorvo 3, 56127 Pisa, Italy), M. Palatiello (INAF - Osservatorio Astronomico di Roma, Via di Frascati 33, 00040, Monteporzio Catone, Italy), G. Panebianco (INAF - Osservatorio di Astrofisica e Scienza dello spazio di Bologna, Via Piero Gobetti 93/3, 40129 Bologna, Italy), D. Paneque (Max-Planck-Institut für Physik, Boltzmannstraße 8, 85748 Garching bei München), F. R. Pantaleo (INFN Sezione di Bari and Politecnico di Bari, via Orabona 4, 70124 Bari, Italy), R. Paoletti (INFN and Università degli Studi di Siena, Dipartimento di Scienze Fisiche, della Terra e dell'Ambiente), J. M. Paredes (Departament de Física Quàntica i Astrofísica, Institut de Ciències del Cosmos, Universitat de Barcelona, IEEC-UB, Martí i Franquès, 1, 08028, Barcelona, Spain), M. Pech (Palacky University Olomouc, Faculty of Science, 17. listopadu 1192/12, 771 46 Olomouc, Czech Republic, FZU - Institute of Physics of the Czech Academy of Sciences, Na Slovance 1999/2, 182 21 Praha 8, Czech Republic), M. Pecimotika (Institut de Fisica d'Altes Energies), M. Peresano (Max-Planck-Institut für Physik, Boltzmannstraße 8, 85748 Garching bei München), F. Pfeifle (Institute for Theoretical Physics and Astrophysics, Universität Würzburg, Campus Hubland Nord, Emil-Fischer-Str. 31, 97074 Würzburg, Germany), E. Pietropaolo (INFN Dipartimento di Scienze Fisiche e Chimiche - Università degli Studi dell'Aquila and Gran Sasso Science Institute, Via Vetoio 1, Viale Crispi 7, 67100 L'Aquila, Italy), M. Pihet (Departament de Física Quàntica i Astrofísica, Institut de Ciències del Cosmos, Universitat de Barcelona, IEEC-UB, Martí i Franquès, 1, 08028, Barcelona, Spain), G. Pirola (Max-Planck-Institut für Physik, Boltzmannstraße 8, 85748 Garching bei München), C. Plard (Univ. Savoie Mont Blanc, CNRS, Laboratoire d'Annecy de Physique des Particules - IN2P3, 74000 Annecy, France), F. Podobnik (INFN and Università degli Studi di Siena, Dipartimento di Scienze Fisiche, della Terra e dell'Ambiente), M. Polo (CIEMAT, Avda. Complutense 40, 28040 Madrid, Spain), E. Prandini (INFN Sezione di Padova and Università degli Studi di Padova, Via Marzolo 8, 35131 Padova, Italy), M. Prouza (FZU - Institute of Physics of the Czech Academy of Sciences, Na Slovance 1999/2, 182 21 Praha 8, Czech Republic), S. Rainò (INFN Sezione di Bari and Università di Bari, via Orabona 4, 70126 Bari, Italy), R. Rando (INFN Sezione di Padova and Università degli Studi di Padova, Via Marzolo 8, 35131 Padova, Italy), W. Rhode (Department of Physics, TU Dortmund University, Otto-Hahn-Str. 4, 44227 Dortmund, Germany), M. Ribó (Departament de Física Quàntica i Astrofísica, Institut de Ciències del Cosmos, Universitat de Barcelona, IEEC-UB, Martí i Franquès, 1, 08028, Barcelona, Spain), V. Rizi (INFN Dipartimento di Scienze Fisiche e Chimiche - Università degli Studi dell'Aquila and Gran Sasso Science Institute, Via Vetoio 1, Viale Crispi 7, 67100 L'Aquila, Italy), G. Rodriguez Fernandez (INFN Sezione di Roma Tor Vergata, Via della Ricerca Scientifica 1, 00133 Rome, Italy), M. D. Rodríguez Frías (University of Alcalá UAH, Departamento de Physics and Mathematics, Pza. San Diego, 28801, Alcalá de Henares, Madrid, Spain), P. Romano (INAF - Osservatorio Astronomico di Brera, Via Brera 28, 20121 Milano, Italy), A. Roy (Physics Program, Graduate School of Advanced Science and Engineering, Hiroshima University, 1-3-1 Kagamiyama, Higashi-Hiroshima City, Hiroshima, 739-8526, Japan), A. Ruina (INFN Sezione di Padova and Università degli Studi di Padova, Via Marzolo 8, 35131 Padova, Italy), E. Ruiz-Velasco (Univ. Savoie Mont Blanc, CNRS, Laboratoire d'Annecy de Physique des Particules - IN2P3, 74000 Annecy, France), T. Saito (Institute for Cosmic Ray Research, University of Tokyo, 5-1-5, Kashiwa-no-ha, Kashiwa, Chiba 277-8582, Japan), S. Sakurai (Institute for Cosmic Ray Research, University of Tokyo, 5-1-5, Kashiwa-no-ha, Kashiwa, Chiba 277-8582, Japan), D. A. Sanchez (Univ. Savoie Mont Blanc, CNRS, Laboratoire d'Annecy de Physique des Particules - IN2P3, 74000 Annecy, France), H. Sano (Institute for Cosmic Ray Research, University of Tokyo, 5-1-5, Kashiwa-no-ha, Kashiwa, Chiba 277-8582, Japan, Gifu University, Faculty of Engineering, 1-1 Yanagido, Gifu 501-1193, Japan), T. Šaric (University of Split, FESB, R. Boškovica 32, 21000 Split, Croatia), Y. Sato (Department of Physical Sciences, Aoyama Gakuin University, Fuchinobe, Sagamihara, Kanagawa, 252-5258, Japan), F. G. Saturni (INAF - Osservatorio Astronomico di Roma, Via di Frascati 33, 00040, Monteporzio Catone, Italy), V. Savchenko (Laboratory for High Energy Physics, École Polytechnique Fédérale, CH-1015 Lausanne, Switzerland), F. Schiavone (INFN Sezione di Bari and Università di Bari, via Orabona 4, 70126 Bari, Italy), B. Schleicher (Institute for Theoretical Physics and Astrophysics, Universität Würzburg, Campus Hubland Nord, Emil-Fischer-Str. 31, 97074 Würzburg, Germany), F. Schmuckermaier (Max-Planck-Institut für Physik, Boltzmannstraße 8, 85748 Garching bei München), J. L. Schubert (Department of Physics, TU Dortmund University, Otto-Hahn-Str. 4, 44227 Dortmund, Germany), F. Schussler (IRFU, CEA, Université Paris-Saclay, Bât 141, 91191 Gif-sur-Yvette, France), T. Schweizer (Max-Planck-Institut für Physik, Boltzmannstraße 8, 85748 Garching bei München), M. Seglar Arroyo (Institut de Fisica d'Altes Energies), T. Siegert (Institute for Theoretical Physics and Astrophysics, Universität Würzburg, Campus Hubland Nord, Emil-Fischer-Str. 31, 97074 Würzburg, Germany), G. Silvestri (INFN Sezione di Padova and Università degli Studi di Padova, Via Marzolo 8, 35131 Padova, Italy), A. Simongini (INAF - Osservatorio Astronomico di Roma, Via di Frascati 33, 00040, Monteporzio Catone, Italy, Macroarea di Scienze MMFFNN, Università di Roma Tor Vergata, Via della Ricerca Scientifica 1, 00133 Rome, Italy), J. Sitarek (Faculty of Physics and Applied Informatics, University of Lodz, ul. Pomorska 149-153, 90-236 Lodz, Poland), V. Sliusar (Department of Astronomy, University of Geneva, Chemin d'Ecogia 16, CH-1290 Versoix, Switzerland), A. Stamerra (INAF - Osservatorio Astronomico di Roma, Via di Frascati 33, 00040, Monteporzio Catone, Italy), J. Striškovic (Josip Juraj Strossmayer University of Osijek, Department of Physics, Trg Ljudevita Gaja 6, 31000 Osijek, Croatia), M. Strzys (Institute for Cosmic Ray Research, University of Tokyo, 5-1-5, Kashiwa-no-ha, Kashiwa, Chiba 277-8582, Japan), Y. Suda (Physics Program, Graduate School of Advanced Science and Engineering, Hiroshima University, 1-3-1 Kagamiyama, Higashi-Hiroshima City, Hiroshima, 739-8526, Japan), A. Sunny (INAF - Osservatorio Astronomico di Roma, Via di Frascati 33, 00040, Monteporzio Catone, Italy, Macroarea di Scienze MMFFNN, Università di Roma Tor Vergata, Via della Ricerca Scientifica 1, 00133 Rome, Italy), H. Tajima (Institute for Space-Earth Environmental Research, Nagoya University, Chikusa-ku, Nagoya 464-8601, Japan), M. Takahashi (Institute for Space-Earth Environmental Research, Nagoya University, Chikusa-ku, Nagoya 464-8601, Japan), J. Takata (Institute for Cosmic Ray Research, University of Tokyo, 5-1-5, Kashiwa-no-ha, Kashiwa, Chiba 277-8582, Japan), R. Takeishi (Institute for Cosmic Ray Research, University of Tokyo, 5-1-5, Kashiwa-no-ha, Kashiwa, Chiba 277-8582, Japan), P. H. T. Tam (Institute for Cosmic Ray Research, University of Tokyo, 5-1-5, Kashiwa-no-ha, Kashiwa, Chiba 277-8582, Japan), S. J. Tanaka (Department of Physical Sciences, Aoyama Gakuin University, Fuchinobe, Sagamihara, Kanagawa, 252-5258, Japan), D. Tateishi (Graduate School of Science and Engineering, Saitama University, 255 Simo-Ohkubo, Sakura-ku, Saitama city, Saitama 338-8570, Japan), T. Tavernier (FZU - Institute of Physics of the Czech Academy of Sciences, Na Slovance 1999/2, 182 21 Praha 8, Czech Republic), P. Temnikov (Institute for Nuclear Research and Nuclear Energy, Bulgarian Academy of Sciences, 72 boul. Tsarigradsko chaussee, 1784 Sofia, Bulgaria), Y. Terada (Graduate School of Science and Engineering, Saitama University, 255 Simo-Ohkubo, Sakura-ku, Saitama city, Saitama 338-8570, Japan), K. Terauchi (Division of Physics and Astronomy, Graduate School of Science, Kyoto University, Sakyo-ku, Kyoto, 606-8502, Japan), T. Terzic (University of Rijeka, Department of Physics, Radmile Matejcic 2, 51000 Rijeka, Croatia), M. Teshima (Institute for Cosmic Ray Research, University of Tokyo, 5-1-5, Kashiwa-no-ha, Kashiwa, Chiba 277-8582, Japan, Max-Planck-Institut für Physik, Boltzmannstraße 8, 85748 Garching bei München), M. Tluczykont (Universität Hamburg, Institut für Experimentalphysik, Luruper Chaussee 149, 22761 Hamburg, Germany), F. Tokanai (Department of Physics, Yamagata University, 1-4-12 Kojirakawa-machi, Yamagata-shi, 990-8560, Japan), T. Tomura (Institute for Cosmic Ray Research, University of Tokyo, 5-1-5, Kashiwa-no-ha, Kashiwa, Chiba 277-8582, Japan), D. F. Torres (Institute of Space Sciences), F. Tramonti (INFN and Università degli Studi di Siena, Dipartimento di Scienze Fisiche, della Terra e dell'Ambiente), P. Travnicek (FZU - Institute of Physics of the Czech Academy of Sciences, Na Slovance 1999/2, 182 21 Praha 8, Czech Republic), G. Tripodo (INFN Sezione di Catania, Via S. Sofia 64, 95123 Catania, Italy), A. Tutone (INAF - Osservatorio Astronomico di Roma, Via di Frascati 33, 00040, Monteporzio Catone, Italy), M. Vacula (Palacky University Olomouc, Faculty of Science, 17. listopadu 1192/12, 771 46 Olomouc, Czech Republic), J. van Scherpenberg (Max-Planck-Institut für Physik, Boltzmannstraße 8, 85748 Garching bei München), M. Vázquez Acosta (Instituto de Astrofísica de Canarias and Departamento de Astrofísica, Universidad de La Laguna, C. Vía Láctea, s/n, 38205 La Laguna, Santa Cruz de Tenerife, Spain), S. Ventura (INFN and Università degli Studi di Siena, Dipartimento di Scienze Fisiche, della Terra e dell'Ambiente), S. Vercellone (INAF - Osservatorio Astronomico di Brera, Via Brera 28, 20121 Milano, Italy), G. Verna (INFN and Università degli Studi di Siena, Dipartimento di Scienze Fisiche, della Terra e dell'Ambiente), I. Viale (INFN Sezione di Padova and Università degli Studi di Padova, Via Marzolo 8, 35131 Padova, Italy), A. Vigliano (INFN Sezione di Trieste and Università degli studi di Udine, via delle scienze 206, 33100 Udine, Italy), C. F. Vigorito (INFN Sezione di Torino, Via P. Giuria 1, 10125 Torino, Italy, Dipartimento di Fisica - Universitá degli Studi di Torino, Via Pietro Giuria 1 - 10125 Torino, Italy), E. Visentin (INFN Sezione di Torino, Via P. Giuria 1, 10125 Torino, Italy, Dipartimento di Fisica - Universitá degli Studi di Torino, Via Pietro Giuria 1 - 10125 Torino, Italy), V. Vitale (INFN Sezione di Roma Tor Vergata, Via della Ricerca Scientifica 1, 00133 Rome, Italy), V. Voitsekhovskyi (University of Geneva - Département de physique nucléaire et corpusculaire, 24 Quai Ernest Ansernet, 1211 Genève 4, Switzerland), G. Voutsinas (University of Geneva - Département de physique nucléaire et corpusculaire, 24 Quai Ernest Ansernet, 1211 Genève 4, Switzerland), I. Vovk (Institute for Cosmic Ray Research, University of Tokyo, 5-1-5, Kashiwa-no-ha, Kashiwa, Chiba 277-8582, Japan), T. Vuillaume (Univ. Savoie Mont Blanc, CNRS, Laboratoire d'Annecy de Physique des Particules - IN2P3, 74000 Annecy, France), R. Walter (Department of Astronomy, University of Geneva, Chemin d'Ecogia 16, CH-1290 Versoix, Switzerland), L. Wan (Institute for Cosmic Ray Research, University of Tokyo, 5-1-5, Kashiwa-no-ha, Kashiwa, Chiba 277-8582, Japan), M. Will (Max-Planck-Institut für Physik, Boltzmannstraße 8, 85748 Garching bei München), J. Wójtowicz (Faculty of Physics and Applied Informatics, University of Lodz, ul. Pomorska 149-153, 90-236 Lodz, Poland), T. Yamamoto (Department of Physics, Konan University, 8-9-1 Okamoto, Higashinada-ku Kobe 658-8501, Japan), R. Yamazaki (Department of Physical Sciences, Aoyama Gakuin University, Fuchinobe, Sagamihara, Kanagawa, 252-5258, Japan), Y. Yao (Department of Physics, Tokai University, 4-1-1, Kita-Kaname, Hiratsuka, Kanagawa 259-1292, Japan), P. K. H. Yeung (Institute for Cosmic Ray Research, University of Tokyo, 5-1-5, Kashiwa-no-ha, Kashiwa, Chiba 277-8582, Japan), T. Yoshida (Faculty of Science, Ibaraki University, 2 Chome-1-1 Bunkyo, Mito, Ibaraki 310-0056, Japan), T. Yoshikoshi (Institute for Cosmic Ray Research, University of Tokyo, 5-1-5, Kashiwa-no-ha, Kashiwa, Chiba 277-8582, Japan), W. Zhang (Institute of Space Sciences)Wed, 11 Ma🔭 astro-ph
Stochastic modelling of cosmic-ray sources for Galactic diffuse emissions
この論文は、モンテカルロシミュレーションを用いて、超新星残骸を代表的な宇宙線源とし、その離散性がガンマ線やニュートリノによる銀河拡散放射に与える影響を確率的に解析し、特に時間依存拡散シナリオにおいて源の確率性がモデル不確実性を増大させ、LHAASO などの観測データとの整合性を高める可能性を示したものである。
Anton Stall, Philipp MertschWed, 11 Ma🔭 astro-ph
Numerical effects on the stripping of dark matter and stars in IllustrisTNG galaxy groups and clusters
IllustrisTNG シミュレーションを用いた解析により、ダークマターのストリッピングは数値分解能に依存しないが、恒星質量のストリッピングは分解能に強く依存し、分解能の向上が衛星銀河のコンパクト化や恒星ハローの過大評価につながることが示されました。
Mark R. Lovell (ICC Durham, Durham Physics, University of Iceland), Annalisa Pillepich (MPIA), Christoph Engler (MPIA), Dylan Nelson (Heidelberg), Rahul Ramesh (Heidelberg), Volker Springel (MPA), Lars Hernquist (ITP Harvard)Wed, 11 Ma🔭 astro-ph
Lyman-α Escape through Anisotropic Media
本論文は、モンテカルロ放射輸送シミュレーションを用いて、リマンα光子が中性ガス中の不均質な経路を通過する際、最低の光学的深さを持つ経路ではなく実質的な光学的深さを持つ経路を通過し、流出や塵、柱密度分布がスペクトル形状や中心フラックスに与える影響を定量的に解明し、イオン化光子の脱出予測への示唆を提示するものである。
Silvia Almada Monter, Max Gronke, Seok-Jun ChangWed, 11 Ma🔭 astro-ph
The detection of high X-ray polarization from an accretion disc corona source and its modelling via Monte Carlo radiation transfer simulation
IXPE による中性子星連星 2S 0921-630 の観測で高 X 線偏光度が検出され、その特徴は外縁円盤からの熱放射風による散乱を考慮したモンテカルロシミュレーションモデルで説明可能であるが、エネルギーに伴う偏光角の変化についてはより複雑な非対称な散乱幾何学が必要である可能性が示唆された。
Ryota Tomaru, Chris Done, Hirokazu OdakaWed, 11 Ma🔭 astro-ph
Stellar halos of bright central galaxies II: Scaling relations, colors and metallicity evolution with redshift
本論文は、半解析モデルを用いて bright central galaxies（BCG）を取り巻く恒星ハロの形成と進化を研究し、その質量・色・金属量に関するスケーリング関係を赤方偏移とともに解明するとともに、VST や Fornax 深宇宙サーベイなどの観測データと比較し、恒星ハロが BCG と銀河団内光（ICL）の間の遷移領域として機能し、その性質がハロの集中度や ICL 形成効率、および降着する矮小銀河の質量分布に依存することを示しています。
Emanuele Contini, Marilena Spavone, Rossella Ragusa, Enrica Iodice, Sukyoung K YiWed, 11 Ma🔭 astro-ph
XSNAP: An X-ray Supernova Analysis Pipeline with Application to the Type II Supernova 2024ggi
この論文では、Swift、Chandra、XMM による超新星 2024ggi の X 線観測データを処理・解析するための新しいオープンソース Python パッケージ「XSNAP」を開発し、これを用いて爆発前の 117 年間にわたる progenitor 星の質量損失率を定量化しました。
Ferdinand, W. V. Jacobson-Galán, M. M. Kasliwal, Erez A. ZimmermanWed, 11 Ma🔭 astro-ph
Scalar field dark matter and stepped dark radiation in an extended Wess-Zumino dark radiation model
この論文は、超対称性に基づく Wess-Zumino ダーク放射モデルを拡張し、スカラー場ダークマターとステップ状ダーク放射を純運動量結合で相互作用させる新たなモデルを構築・検証した結果、Hubble 定数やS8の緊張をわずかに緩和するものの、完全な解決には至らずさらなる研究が必要であることを示しました。
Gang LiuWed, 11 Ma🔭 astro-ph
The Response of Planetary Atmospheres to the Impact of Icy Comets III: Impact Driven Atmospheric Escape
この論文は、潮汐ロックされた惑星の地球型大気と対比させ、彗星衝突による水蒸気輸送が大気循環によってどのように高高度へ運ばれ水素の脱出を促進するかをシミュレーションし、特に衝突位置（昼側か夜側か）が脱出率に決定的な影響を与えることを明らかにしたものである。
Felix Sainsbury-Martinez, Greg Cooke, Catherine WalshWed, 11 Ma🔭 astro-ph
Simulation-Based Prediction of Black Hole Spectra: From $10M_\odotto10^8 M_\odot$
この論文は、一般相対性磁気流体力学シミュレーションデータに標準的な放射物理を適用する新しいポスト処理手法を開発し、太陽質量の 10 倍から 1 億倍までのブラックホールにおける降着スペクトルを初めて予測・解析することで、観測されるブラックホールの多様な特性を再現できることを示しています。
Chris Nagele, Julian H. Krolik, Rongrong Liu, Brooks E. Kinch, Jeremy D. SchnittmanWed, 11 Ma🔭 astro-ph
Reconstructing Gamma Ray Burst Energy Relations with Observational H(z) data in Neural Network Framework
この論文は、観測ハッブルパラメータデータを用いたニューラルネットワーク（特にベイズニューラルネットワーク）によるモデル非依存のガンマ線バースト較正法を提案し、アマトリ関係の傾きを以前の方法と整合性のある形で導出するとともに、不確実性の伝播をより頑健に行う手法を実証しています。
Nilanjana Bagchi Aurpa, Abha Dev Habib, Nisha RaniWed, 11 Ma🔭 astro-ph
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