Zobrazeno 1 - 10
of 19 395
pro vyhledávání: '"Oguri"'
Autor:
Tajiri T, Suzuki M, Kutsuna T, Nishiyama H, Ito K, Takeda N, Fukumitsu K, Kanemitsu Y, Fukuda S, Umemura T, Ohkubo H, Maeno K, Ito Y, Oguri T, Takemura M, Yoshikawa K, Niimi A
Publikováno v:
Journal of Asthma and Allergy, Vol Volume 16, Pp 149-157 (2023)
Tomoko Tajiri,1 Motohiko Suzuki,2,3 Takeo Kutsuna,4 Hirono Nishiyama,1 Keima Ito,1 Norihisa Takeda,1 Kensuke Fukumitsu,1 Yoshihiro Kanemitsu,1 Satoshi Fukuda,1 Takehiro Umemura,1 Hirotsugu Ohkubo,1 Ken Maeno,1 Yutaka Ito,1 Tetsuya Oguri,1 Masaya Take
Externí odkaz:
https://doaj.org/article/347e7635eab74af0b8935f5c06b4a20f
Autor:
Ito K, Tajiri T, Nishiyama H, Kurokawa R, Yap JMG, Takeda N, Fukumitsu K, Kanemitsu Y, Fukuda S, Uemura T, Ohkubo H, Maeno K, Ito Y, Oguri T, Takemura M, Niimi A
Publikováno v:
Journal of Asthma and Allergy, Vol Volume 15, Pp 1561-1568 (2022)
Keima Ito,1 Tomoko Tajiri,1 Hirono Nishiyama,1 Ryota Kurokawa,1 Jenifer Maries Go Yap,1 Norihisa Takeda,1 Kensuke Fukumitsu,1 Yoshihiro Kanemitsu,1 Satoshi Fukuda,1 Takehiro Uemura,1 Hirotsugu Ohkubo,1 Ken Maeno,1 Yutaka Ito,1 Tetsuya Oguri,1,2 Masay
Externí odkaz:
https://doaj.org/article/f684cc52f0a74626868bee48502bdc97
Autor:
Abe, Katsuya T., Oguri, Masamune, Birrer, Simon, Khadka, Narayan, Marshall, Philip J., Lemon, Cameron, More, Anupreeta, Collaboration, the LSST Dark Energy Science
Time delays in both galaxy- and cluster-scale strong gravitational lenses have recently attracted a lot of attention in the context of the Hubble tension. Future wide-field cadenced surveys, such as the LSST, are anticipated to discover strong lenses
Externí odkaz:
http://arxiv.org/abs/2411.07509
Autor:
Kagaya, Tomoyuki, Lou, Yuxuan, Yuan, Thong Jing, Lakshmi, Subramanian, Karlekar, Jayashree, Pranata, Sugiri, Murakami, Natsuki, Kinose, Akira, Oguri, Koki, Wick, Felix, You, Yang
In recent years, Large Language Models (LLMs) have demonstrated high reasoning capabilities, drawing attention for their applications as agents in various decision-making processes. One notably promising application of LLM agents is robotic manipulat
Externí odkaz:
http://arxiv.org/abs/2410.16919
Autor:
Gross, Arran C., Chen, Yu-Ching, Oguri, Masamune, Nolan, Liam, Liu, Xin, Shen, Yue, Zhuang, Ming-Yang, Li, Junyao, Zakamska, Nadia L., Hwang, Hsiang-Chih, Ishikawa, Yuzo
Dual Active Galactic Nuclei (dual AGNs), a phase in some galaxy mergers during which both central supermassive black holes (SMBHs) are active, are expected to be a key observable stage leading up to SMBH mergers. Constraining the population of dual A
Externí odkaz:
http://arxiv.org/abs/2409.16363
Autor:
Oguri, Masamune, Miyazaki, Satoshi
Clusters of galaxies can be identified from peaks in weak lensing aperture mass maps constructed from weak lensing shear catalogs. Such purely gravitational cluster selection considerably differs from traditional cluster selections based on baryonic
Externí odkaz:
http://arxiv.org/abs/2409.12361
Autor:
Shrivastava, Shaurya, Oguri, Kenshiro
In this work, we propose novel LMI-based controller synthesis frameworks for periodically time-varying Markov-jump linear systems. We first discuss the necessary conditions for mean square stability and derive Lyapunov-like conditions for stability a
Externí odkaz:
http://arxiv.org/abs/2409.11537
Autor:
Euclid Collaboration, McPartland, C. J. R., Zalesky, L., Weaver, J. R., Toft, S., Sanders, D. B., Mobasher, B., Suzuki, N., Szapudi, I., Valdes, I., Murphree, G., Chartab, N., Allen, N., Taamoli, S., Eisenhardt, P. R. M., Arnouts, S., Atek, H., Brinchmann, J., Castellano, M., Chary, R., Ortiz, O. Chávez, Cuby, J. -G., Finkelstein, S. L., Goto, T., Gwyn, S., Harikane, Y., Inoue, A. K., McCracken, H. J., Mohr, J. J., Oesch, P. A., Ouchi, M., Oguri, M., Rhodes, J., Rottgering, H. J. A., Sawicki, M., Scaramella, R., Scarlata, C., Silverman, J. D., Stern, D., Teplitz, H. I., Shuntov, M., Altieri, B., Amara, A., Andreon, S., Auricchio, N., Aussel, H., Baccigalupi, C., Baldi, M., Bardelli, S., Bender, R., Bonino, D., Branchini, E., Brescia, M., Camera, S., Capobianco, V., Carbone, C., Carretero, J., Casas, S., Castander, F. J., Castignani, G., Cavuoti, S., Cimatti, A., Colodro-Conde, C., Congedo, G., Conselice, C. J., Conversi, L., Copin, Y., Courbin, F., Courtois, H. M., Da Silva, A., Degaudenzi, H., De Lucia, G., Di Giorgio, A. M., Dinis, J., Douspis, M., Dubath, F., Dupac, X., Dusini, S., Fabricius, M., Farina, M., Farrens, S., Ferriol, S., Fotopoulou, S., Frailis, M., Franceschi, E., Fumana, M., Galeotta, S., Garilli, B., George, K., Gillis, B., Giocoli, C., Grazian, A., Grupp, F., Guzzo, L., Hoekstra, H., Holmes, W., Hook, I., Hormuth, F., Hornstrup, A., Hudelot, P., Jahnke, K., Keihänen, E., Kermiche, S., Kiessling, A., Kilbinger, M., Kitching, T., Kubik, B., Kunz, M., Kurki-Suonio, H., Lilje, P. B., Lindholm, V., Lloro, I., Mainetti, G., Maiorano, E., Mansutti, O., Marggraf, O., Markovic, K., Martinelli, M., Martinet, N., Marulli, F., Massey, R., Maurogordato, S., Medinaceli, E., Mei, S., Melchior, M., Mellier, Y., Meneghetti, M., Merlin, E., Meylan, G., Moresco, M., Moscardini, L., Munari, E., Nakajima, R., Neissner, C., Niemi, S. -M., Nightingale, J. W., Padilla, C., Paltani, S., Pasian, F., Pedersen, K., Percival, W. J., Pettorino, V., Polenta, G., Poncet, M., Popa, L. A., Pozzetti, L., Raison, F., Rebolo, R., Renzi, A., Riccio, G., Romelli, E., Roncarelli, M., Rossetti, E., Saglia, R., Sakr, Z., Sánchez, A. G., Sapone, D., Sartoris, B., Schirmer, M., Schneider, P., Schrabback, T., Secroun, A., Seidel, G., Serrano, S., Sirignano, C., Sirri, G., Stanco, L., Steinwagner, J., Surace, C., Tallada-Crespi, P., Tavagnacco, D., Tereno, I., Toledo-Moreo, R., Torradeflot, F., Tutusaus, I., Valentijn, E. A., Valenziano, L., Vassallo, T., Veropalumbo, A., Wang, Y., Weller, J., Zamorani, G., Zoubian, J., Zucca, E., Biviano, A., Bolzonella, M., Boucaud, A., Bozzo, E., Burigana, C., Di Ferdinando, D., Farinelli, R., Gracia-Carpio, J., Mauri, N., Scottez, V., Tenti, M., Viel, M., Wiesmann, M., Akrami, Y., Allevato, V., Anselmi, S., Ballardini, M., Bethermin, M., Borgani, S., Borlaff, A. S., Bruton, S., Cabanac, R., Calabro, A., Cañas-Herrera, G., Cappi, A., Carvalho, C. S., Castro, T., Chambers, K. C., Contarini, S., Cooray, A. R., Coupon, J., Davini, S., de la Torre, S., Desprez, G., Díaz-Sánchez, A., Di Domizio, S., Dole, H., Vigo, J. A. Escartin, Escoffier, S., Ferrari, A. G., Ferreira, P. G., Ferrero, I., Finelli, F., Fornari, F., Gabarra, L., Ganga, K., García-Bellido, J., Gautard, V., Gaztanaga, E., Giacomini, F., Gozaliasl, G., Gregorio, A., Hall, A., Hartley, W. G., Hildebrandt, H., Hjorth, J., Huertas-Company, M., Ilbert, O., Kajava, J. J. E., Kansal, V., Karagiannis, D., Kirkpatrick, C. C., Legrand, L., Libet, G., Loureiro, A., Macias-Perez, J., Maggio, G., Magliocchetti, M., Mancini, C., Mannucci, F., Maoli, R., Martins, C. J. A. P., Matthew, S., Maturi, M., Maurin, L., Metcalf, R. B., Monaco, P., Moretti, C., Morgante, G., Musi, P., Walton, Nicholas A., Odier, J., Patrizii, L., Pöntinen, M., Popa, V., Porciani, C., Potter, D., Reimberg, P., Risso, I., Rocci, P. -F., Sahlén, M., Schneider, A., Sereno, M., Simon, P., Mancini, A. Spurio, Stanford, S. A., Tao, C., Testera, G., Teyssier, R., Tosi, S., Troja, A., Tucci, M., Valieri, C., Valiviita, J., Vergani, D., Verza, G., Shankar, F.
Euclid will provide deep NIR imaging to $\sim$26.5 AB magnitude over $\sim$59 deg$^2$ in its deep and auxiliary fields. The Cosmic DAWN survey complements the deep Euclid data with matched depth multiwavelength imaging and spectroscopy in the UV--IR
Externí odkaz:
http://arxiv.org/abs/2408.05275
Autor:
Takase, Y., Vacher, L., Ishino, H., Patanchon, G., Montier, L., Stever, S. L., Ishizaka, K., Nagano, Y., Wang, W., Aumont, J., Aizawa, K., Anand, A., Baccigalupi, C., Ballardini, M., Banday, A. J., Barreiro, R. B., Bartolo, N., Basak, S., Bersanelli, M., Bortolami, M., Brinckmann, T., Calabrese, E., Campeti, P., Carinos, E., Carones, A., Casas, F. J., Cheung, K., Clermont, L., Columbro, F., Coppolecchia, A., Cuttaia, F., de Bernardis, P., de Haan, T., de la Hoz, E., Della Torre, S., Diego-Palazuelos, P., D'Alessandro, G., Eriksen, H. K., Errard, J., Finelli, F., Fuskeland, U., Galloni, G., Galloway, M., Gervasi, M., Ghigna, T., Giardiello, S., Gimeno-Amo, C., Gjerløw, E., González, R. González, Gruppuso, A., Hazumi, M., Henrot-Versillé, S., Hergt, L. T., Ikuma, K., Kohri, K., Lamagna, L., Lattanzi, M., Leloup, C., Lembo, M., Levrier, F., Lonappan, A. I., López-Caniego, M., Luzzi, G., Maffei, B., Martínez-González, E., Masi, S., Matarrese, S., Matsuda, F. T., Matsumura, T., Micheli, S., Migliaccio, M., Monelli, M., Morgante, G., Mot, B., Nagata, R., Namikawa, T., Novelli, A., Odagiri, K., Oguri, S., Omae, R., Pagano, L., Paoletti, D., Piacentini, F., Pinchera, M., Polenta, G., Porcelli, L., Raffuzzi, N., Remazeilles, M., Ritacco, A., Ruiz-Granda, M., Sakurai, Y., Scott, D., Sekimoto, Y., Shiraishi, M., Signorelli, G., Sullivan, R. M., Takakura, H., Terenzi, L., Tomasi, M., Tristram, M., van Tent, B., Vielva, P., Wehus, I. K., Westbrook, B., Weymann-Despres, G., Wollack, E. J., Zannoni, M., Zhou, Y.
Large angular scale surveys in the absence of atmosphere are essential for measuring the primordial $B$-mode power spectrum of the Cosmic Microwave Background (CMB). Since this proposed measurement is about three to four orders of magnitude fainter t
Externí odkaz:
http://arxiv.org/abs/2408.03040
Autor:
Tsujii, Miku, Baselmans, Jochem J. A., Choi, Jihoon, Coppens, Antonio H. M., Fasano, Alessandro, Génova-Santos, Ricardo Tanausú, Hattori, Makoto, Hazumi, Masashi, Honda, Shunsuke, Ikemitsu, Takuji, Ishida, Hidesato, Ishitsuka, Hikaru, Jeong, Hoyong, Jo, Yonggil, Karatsu, Kenichi, Kataoka, Keisuke, Kiuchi, Kenji, Komine, Junta, Koyano, Ryo, Kutsuma, Hiroki, Lee, Kyungmin, Mima, Satoru, Nagai, Makoto, Nagasaki, Taketo, Naruse, Masato, Oguri, Shugo, Otani, Chiko, Peel, Michael W., Rebolo, Rafael, Rubiño-Martín, José Alberto, Sekimoto, Yutaro, Sueno, Yoshinori, Suzuki, Junya, Taino, Tohru, Tajima, Osamu, Tanaka, Tomonaga, Thoen, David J., Tomita, Nozomu, Tsuji, Yuta, Uchida, Tomohisa, Won, Eunil, Yoshida, Mitsuhiro
GroundBIRD is a ground-based cosmic microwave background (CMB) experiment for observing the polarization pattern imprinted on large angular scales ($\ell > 6$ ) from the Teide Observatory in Tenerife, Spain. Our primary scientific objective is a prec
Externí odkaz:
http://arxiv.org/abs/2407.17019