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Noise subtraction from KAGRA O3GK data using Independent Component Analysis

arXiv 2022年

作者： Abe, H. Akutsu, T. Ando, M. Araya, A. Aritomi, N. Asada, H. Aso, Y. Bae, S. Bae, Y. Bajpai, R. Cannon, K. Cao, Z. Capocasa, E. Chan, M. Chen, C. Chen, D. Chen, K. Chen, Y. Chiang, C.-Y. Chu, Y.-K. Eguchi, S. Eisenmann, M. Enomoto, Y. Flaminio, R. Fong, H.K. Fujii, Y. Fujikawa, Y. Fujimoto, Y. Fukunaga, I. Gao, D. Ge, G.-G. Ha, S. Hadiputrawan, I.P.W. Haino, S. Han, W.-B. Hasegawa, K. Hattori, K. Hayakawa, H. Hayama, K. Himemoto, Y. Hirata, N. Hirose, C. Ho, T.-C. Hsieh, B.-H. Hsieh, H.-F. Hsiung, C. Huang, H.-Y. Huang, P. Huang, Y.-C. Huang, Y.-J. Hui, D.C.Y. Ide, S. Inayoshi, K. Inoue, Y. Ito, K. Itoh, Y. Jeon, C. Jin, H.-B. Jung, K. Jung, P. Kaihotsu, K. Kajita, T. Kakizaki, M. Kamiizumi, M. Kanda, N. Kato, T. Kawaguchi, K. Kim, C. Kim, J. Kim, J.C. Kim, Y.-M. Kimura, N. Kiyota, T. Kobayashi, Y. Kohri, K. Kokeyama, K. Kong, A.K.H. Koyama, N. Kozakai, C. Kume, J. Kuromiya, Y. Kuroyanagi, S. Kwak, K. Lee, E. Lee, H.W. Lee, R. Leonardi, M. Li, K.L. Li, P. Lin, L.C.-C. Lin, C.-Y. Lin, E.T. Lin, F.-K. Lin, F.-L. Lin, H.L. Liu, G.C. Luo, L.-W. Ma'arif, M. Majorana, E. Michimura, Y. Mio, N. Miyakawa, O. Miyo, K. Miyoki, S. Mori, Y. Morisaki, S. Morisue, N. Moriwaki, Y. Nagano, K. Nakamura, K. Nakano, H. Nakano, M. Nakayama, Y. Narikawa, T. Naticchioni, L. Nguyen Quynh, L. Ni, W.-T. Nishimoto, T. Nishizawa, A. Nozaki, S. Obayashi, Y. Ogaki, W. Oh, J.J. Oh, K. Ohashi, M. Ohashi, T. Ohkawa, M. Ohta, H. Okutani, Y. Oohara, K. Oshino, S. Otabe, S. Pan, K.-C. Parisi, A. Park, J. Peña Arellano, F.E. Saha, S. Saito, Y. Sakai, K. Sawada, T. Sekiguchi, Y. Shao, L. Shikano, Y. Shimizu, H. Shimode, K. Shinkai, H. Shishido, T. Shoda, A. Somiya, K. Song, I. Sugimoto, R. Suresh, J. Suzuki, T. Suzuki, T. Suzuki, T. Tagoshi, H. Takahashi, H. Takahashi, R. Takano, S. Takeda, H. Takeda, M. Tanaka, K. Tanaka, T. Tanaka, T. Tanioka, S. Taruya, A. Graduate School of Science Tokyo Institute of Technology Meguro-ku Tokyo152-8551 Japan Mitaka City Tokyo181-8588 Japan Mitaka City Tokyo181-8588 Japan Department of Physics The University of Tokyo Bunkyo-ku Tokyo113-0033 Japan The University of Tokyo Bunkyo-ku Tokyo113-0033 Japan Earthquake Research Institute The University of Tokyo Bunkyo-ku Tokyo113-0032 Japan Department of Mathematics and Physics Gravitational Wave Science Project Hirosaki University Aomori Hirosaki City036-8561 Japan Kamioka-cho Hida City Gifu506-1205 Japan Mitaka City Tokyo181-8588 Japan Yuseong-gu Daejeon34141 Korea Republic of National Institute for Mathematical Sciences Yuseong-gu Daejeon34047 Korea Republic of Ibaraki Tsukuba City305-0801 Japan Department of Astronomy Beijing Normal University Beijing100875 China Department of Applied Physics Fukuoka University Jonan Fukuoka Fukuoka City814-0180 Japan Department of Physics Tamkang University Danshui Dist. New Taipei City25137 Taiwan Department of Physics Institute of Astronomy National Tsing Hua University Hsinchu30013 Taiwan Department of Physics Center for High Energy and High Field Physics National Central University Zhongli District Taoyuan City32001 Taiwan Department of Physics National Tsing Hua University Hsinchu30013 Taiwan Institute of Physics Academia Sinica Nankang Taipei11529 Taiwan Université Savoie Mont Blanc CNRS IN2P3 AnnecyF-74941 France Department of Astronomy The University of Tokyo Mitaka City Tokyo181-8588 Japan Faculty of Engineering Niigata University Nishi-ku Niigata Niigata City950-2181 Japan Department of Physics Graduate School of Science Osaka City University Sumiyoshi-ku Osaka City Osaka558-8585 Japan Chinese Academy of Sciences Xiao Hong Shan Wuhan430071 China Ulju-gun Ulsan44919 Korea Republic of Shanghai Astronomical Observatory Chinese Academy of Sciences Shanghai200030 China KAGRA Observatory The University of Tok

In April 2020, KAGRA conducted its first science observation in combination with the GEO 600 detector (O3GK) for two weeks. According to the noise budget estimation, suspension control noise in the low frequency band ... 详细信息

来源：评论

CO Multi-line Imaging of Nearby Galaxies (COMING). XII. CO-to-H2 Conversion Factor and Dust-to-Gas Ratio

arXiv

引用

arXiv 2023年

作者： Yasuda, Atsushi Kuno, Nario Sorai, Kazuo Muraoka, Kazuyuki Miyamoto, Yusuke Kaneko, Hiroyuki Yajima, Yoshiyuki Tanaka, Takahiro Morokuma-Matsui, Kana Takeuchi, Tsutomu T. Kobayashi, Masato I.N. Graduate School of Pure and Applied Sciences University of Tsukuba 1-1-1 Tennodai Ibaraki Tsukuba305-8571 Japan Tomonaga Center for the History of the Universe University of Tsukuba 1-1-1 Tennodai Ibaraki Tsukuba305-8571 Japan Department of Physics School of Science and Technology Kwansei Gakuin University 2-1 Gakuen Hyogo Sanda669-1337 Japan Department of Physics Faculty of Science Hokkaido University Kita 10 Nishi 8 Kita-ku Sapporo Hokkaido060-0810 Japan Department of Cosmosciences Graduate School of Science Hokkaido University Kita 10 Nishi 8 Kita-ku Sapporo Hokkaido060-0810 Japan Department of Physics Graduate School of Science Osaka Metropolitan University 1-1 Gakuen-cho Naka-ku Sakai Osaka599-8531 Japan Department of Electrical Electronic and Computer Engineering Faculty of Engineering Fukui University of Technology 3-6-1 Gakuen Fukui Fukui910-8505 Japan Graduate School of Education Joetsu University of Education 1 Yamayashiki-machi Joetsu Niigata943-8512 Japan Center for Astronomy Ibaraki University 2-1-1 Bunkyo Ibaraki Mito310-8512 Japan Institute of Astronomy Graduate School of Science The University of Tokyo 2-21-1 Osawa Mitaka Tokyo181-0015 Japan Division of Particle and Astrophysical Science Nagoya University Furo-cho Chikusa-ku Aichi Nagoya464-8602 Japan Division of Science National Astronomical Observatory of Japan Osawa 2-21-1 Mitaka Tokyo181-8588 Japan I. Physikalisches Institut Universität zu Köln Zülpicher Str 77 KölnD-50937 Germany

We simultaneously measured the spatially-resolved CO-to-H2 conversion factor (αCO) and dust-to-gas ratio (DGR) in nearby galaxies on a kiloparsec scale. In this study, we used 12CO(J = 1 − 0) data obtained by the Nob... 详细信息

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The cross-section measurement for the 3H(e,e'K+)nnΛ reaction

arXiv

引用

arXiv 2021年

作者： Suzuki, Kazuki N. Gogami, T. Pandey, B. Itabashi, K. Nagao, S. Okuyama, K. Nakamura, S.N. Tang, L. Abrams, D. Akiyama, T. Androic, D. Aniol, K. Gayoso, C. Ayerbe Bane, J. Barcus, S. Barrow, J. Bellini, V. Bhatt, H. Bhetuwal, D. Biswas, D. Camsonne, A. Castellanos, J. Chen, J.-P. Chen, J. Covrig, S. Chrisman, D. Cruz-Torres, R. Das, R. Fuchey, E. Gnanvo, K. Garibaldi, F. Gautam, T. Gomez, J. Gueye, P. Hague, T.J. Hansen, O. Henry, W. Hauenstein, F. Higinbotham, D.W. Hyde, C.E. Kaneta, M. Keppel, C. Kutz, T. Lashley-Colthirst, N. Li, S. Liu, H. Mammei, J. Markowitz, P. McClellan, R.E. Meddi, F. Meekins, D. Michaels, R. Mihovilovič, M. Moyer, A. Nguyen, D. Nycz, M. Owen, V. Palatchi, C. Park, S. Petkovic, T. Premathilake, S. Reimer, P.E. Reinhold, J. Riordan, S. Rodriguez, V. Samanta, C. Santiesteban, S.N. Sawatzky, B. Širca, S. Slifer, K. Su, T. Tian, Y. Toyama, Y. Uehara, K. Urciuoli, G.M. Votaw, D. Williamson, J. Wojtsekhowski, B. Wood, S.A. Yale, B. Ye, Z. Zhang, J. Zheng, X. Graduate School of Science Kyoto University Kyoto606-8502 Japan Graduate School of Science Tohoku University Miyagi Sendai980-8578 Japan Department of Physics Hampton University VA23668 United States Thomas Jefferson National Accelerator Facility Newport NewsVA23606 United States Department of Physics University of Virginia CharlottesvilleVA22904 United States Department of Physics Department of Applied Physics University of Zagreb ZagrebHR-10000 Croatia Physics and Astronomy Department California State University Los AngelesCA90032 United States Department of Physics The College of William and Mary VA23185 United States Department of Physics University of Tennessee KnoxvilleTN37996 United States INFN Sezione di Roma Rome00185 Italy Department of Physics Mississippi State University Mississippi State MS39762 United States Department of Physics Florida International University MiamiFL33199 United States Department of Physics and Astronomy Michigan State University East LansingMI48824 United States National Superconducting Cyclotron Laboratory Michigan State University East LansingMI48824 United States Department of Physics Massachusetts Institute of Technology CambridgeMA02139 United States Department of Physics State University of New York Stony BrookNY11794 United States Department of Physics University of Connecticut StorrsCT06269 United States Istituto Superiore di Sanità Rome00161 Italy Department of Physics Kent State University KentOH44242 United States Department of Physics Old Dominion University NorfolkVA23529 United States Department of Physics University of New Hampshire DurhamNH03824 United States Nuclear Science Division Lawrence Berkeley National Laboratory BerkeleyCA94720 United States Department of Physics Columbia University New YorkNY10027 United States Department of Physics and Astronomy University of Manitoba WinnipegMBR3T 2N2 Canada Sapienza University of Rome RomeI-00185 Italy

The small binding energy of hypertrition leads to predictions of non-existence of bound hypernuclei for the isotriplet three-body system such as nnΛ. However, invariant mass spectroscopy at GSI reported events that m... 详细信息

来源：评论

Spectroscopically resolved partial phase curve of the rapid heating and cooling of the highly-eccentric Hot Jupiter HAT-P-2b with WFC3

arXiv

引用

arXiv 2024年

作者： Jacobs, Bob Désert, Jean-Michel Lewis, Nikole Challener, Ryan C. Mayorga, L.C. de Beurs, Zoë L. Parmentier, Vivien Stevenson, Kevin B. de Wit, Julien Barat, Saugata Fortney, Jonathan Kataria, Tiffany Line, Michael Anton Pannekoek Institute for Astronomy University of Amsterdam Science Park 904 Amsterdam1098 XH Netherlands Department of Astrophysics IMAPP Radboud University PO Box 9010 Nijmegen6500 GL Netherlands Department of Astronomy Carl Sagan Institute Cornell University 122 Sciences Drive IthacaNY14853 United States Johns Hopkins University Applied Physics Laboratory 11100 Johns Hopkins Rd LaurelMD20723 United States Department of Earth Atmospheric and Planetary Sciences Massachusetts Institute of Technology CambridgeMA02139 United States NSF Graduate Research Fellow MIT Presidential Fellow MIT Collamore-Rogers Fellow United States Laboratoire Lagrange Observatoire de la Côte d’Azur Université Côte d’Azur Nice France Department of Astronomy and Astrophysics University of California Santa CruzCA95064 United States NASA Jet Propulsion Laboratory California Institute of Technology PasadenaCA91109 United States School of Earth and Space Exploration Arizona State University TempeAZ85287 United States

The extreme environments of transiting close-in exoplanets in highly-eccentric orbits are ideal for testing exo-climate physics. Spectroscopically resolved phase curves not only allow for the characterization of their... 详细信息

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