Zobrazeno 1 - 10
of 63 278
pro vyhledávání: '"A. Yoshinobu"'
Autor:
Zhu, Yongda, Bakx, Tom J. L. C., Ikeda, Ryota, Umehata, Hideki, Becker, George D., Cain, Christopher, Champagne, Jaclyn B., Fan, Xiaohui, Fudamoto, Yoshinobu, Jin, Xiangyu, Ma, Hai-Xia, Sun, Yang, Takeuchi, Tsutomu T., Tee, Wei Leong
We report the discovery of a unique quasar-dusty star-forming galaxy (DSFG) system at $z = 5.63$, consisting of the bright quasar J1133+1603 ($M_{\rm UV} = -27.42$) and its compact, dust-obscured companion, J1133c. ALMA observations reveal a prominen
Externí odkaz:
http://arxiv.org/abs/2411.06698
Autor:
Fujimoto, Tomohiro, Murotani, Yuta, Tamaya, Tomohiro, Kurihara, Takayuki, Kanda, Natsuki, Kim, Changsu, Yoshinobu, Jun, Akiyama, Hidefumi, Kato, Takeo, Matsunaga, Ryusuke
Transverse current generation by circularly polarized light in biased matter has attracted considerable attention for studies of Floquet engineering and inverse spin Hall effect. Field-induced circular photogalvanic effect (FI-CPGE) also contributes
Externí odkaz:
http://arxiv.org/abs/2411.00528
Autor:
Sato, Riku A., Inoue, Akio K., Harikane, Yuichi, Shimakawa, Rhythm, Sugahara, Yuma, Tamura, Yoichi, Hashimoto, Takuya, Ito, Kei, Yamanaka, Satoshi, Mawatari, Ken, Fudamoto, Yoshinobu, Ren, Yi W.
We present the analysis of three intermediate-mass quiescent galaxies (QGs) with stellar masses of $\sim10^{10}M_{\rm \odot}$ at redshifts $z\sim 3 - 4$ using NIRSpec low-resolution spectroscopy. Utilising the SED fitting code BAGPIPES, we confirm th
Externí odkaz:
http://arxiv.org/abs/2410.08745
Autor:
Tanaka, Takumi S., Silverman, John D., Nakazato, Yurina, Onoue, Masafusa, Shimasaku, Kazuhiro, Fudamoto, Yoshinobu, Fujimoto, Seiji, Ding, Xuheng, Faisst, Andreas L., Valentino, Francesco, Jin, Shuowen, Hayward, Christopher C., Kokorev, Vasily, Ceverino, Daniel, Kalita, Boris S., Casey, Caitlin M., Liu, Zhaoxuan, Kaminsky, Aidan, Fei, Qinyue, Andika, Irham T., Lambrides, Erini, Akins, Hollis B., Kartaltepe, Jeyhan S., Koekemoer, Anton M., McCracken, Henry Joy, Rhodes, Jason, Robertson, Brant E., Franco, Maximilien, Liu, Daizhong, Chartab, Nima, Gillman, Steven, Gozaliasl, Ghassem, Hirschmann, Michaela, Huertas-Company, Marc, Massey, Richard, Roy, Namrata, Sattari, Zahra, Shuntov, Marko, Sterling, Joseph, Toft, Sune, Trakhtenbrot, Benny, Yoshida, Naoki, Zavala, Jorge A.
The current paradigm for the co-evolution of galaxies and their supermassive black holes postulates that dust-obscured active galactic nuclei (AGNs) represent a transitional phase towards a more luminous and unobscured state. However, our understandi
Externí odkaz:
http://arxiv.org/abs/2410.00104
Autor:
Schouws, Sander, Bouwens, Rychard J., Ormerod, Katherine, Smit, Renske, Algera, Hiddo, Sommovigo, Laura, Hodge, Jacqueline, Ferrara, Andrea, Oesch, Pascal A., Rowland, Lucie E., van Leeuwen, Ivana, Stefanon, Mauro, Herard-Demanche, Thomas, Fudamoto, Yoshinobu, Röttgering, Huub, van der Werf, Paul
We report the first successful ALMA follow-up observations of a secure $z > 10$ JWST-selected galaxy, by robustly detecting ($6.6\sigma$) the [OIII]$_{88\mu m}\,$ line in JADES-GS-z14-0 (hereafter GS-z14). The ALMA detection yields a spectroscopic re
Externí odkaz:
http://arxiv.org/abs/2409.20549
Autor:
Covelo-Paz, Alba, Giovinazzo, Emma, Oesch, Pascal A., Meyer, Romain A., Weibel, Andrea, Brammer, Gabriel, Fudamoto, Yoshinobu, Kerutt, Josephine, Lin, Jamie, Matharu, Jasleen, Naidu, Rohan P., Velichko, Anna, Bollo, Victoria, Bouwens, Rychard, Chisholm, John, Illingworth, Garth D., Kramarenko, Ivan, Magee, Daniel, Maseda, Michael, Matthee, Jorryt, Nelson, Erica, Reddy, Naveen, Schaerer, Daniel, Stefanon, Mauro, Xiao, Mengyuan
The H{\alpha} nebular emission line is an optimal tracer for recent star formation in galaxies. With the advent of JWST, this line has recently become observable at z>3 for the first time. We present a catalog of 1013 H{\alpha} emitters at 3.7
Externí odkaz:
http://arxiv.org/abs/2409.17241
Autor:
Gu, Yi, Otake, Yoshito, Uemura, Keisuke, Takao, Masaki, Soufi, Mazen, Okada, Seiji, Sugano, Nobuhiko, Talbot, Hugues, Sato, Yoshinobu
Radiography is widely used in orthopedics for its affordability and low radiation exposure. 3D reconstruction from a single radiograph, so-called 2D-3D reconstruction, offers the possibility of various clinical applications, but achieving clinically
Externí odkaz:
http://arxiv.org/abs/2409.16702
Autor:
Soufi, Mazen, Otake, Yoshito, Iwasa, Makoto, Uemura, Keisuke, Hakotani, Tomoki, Hashimoto, Masahiro, Yamada, Yoshitake, Yamada, Minoru, Yokoyama, Yoichi, Jinzaki, Masahiro, Kusano, Suzushi, Takao, Masaki, Okada, Seiji, Sugano, Nobuhiko, Sato, Yoshinobu
Deep learning-based image segmentation has allowed for the fully automated, accurate, and rapid analysis of musculoskeletal (MSK) structures from medical images. However, current approaches were either applied only to 2D cross-sectional images, addre
Externí odkaz:
http://arxiv.org/abs/2409.02770
The determination of material parameters is significantly important in material science, which is often a challenging task. Recently, advancements have shown that magnetic parameters, such as the Dzyaloshinskii-Moriya interaction (DMI), can be estima
Externí odkaz:
http://arxiv.org/abs/2408.12181
Autor:
Ishii, Nozomi, Hashimoto, Takuya, Ferkinhoff, Carl, Rybak, Matus, Inoue, Akio K., Michiyama, Tomonari, Donevski, Darko, Fujimoto, Seiji, Salak, Dragan, Kuno, Nario, Matsuo, Hiroshi, Mawatari, Ken, Tamura, Yoichi, Izumi, Takuma, Nagao, Tohru, Nakazato, Yurina, Osone, Wataru, Sugahara, Yuma, Usui, Mitsutaka, Wakasugi, Koki, Yajima, Hidenobu, Bakx, Tom J. L. C., Fudamoto, Yoshinobu, Meyer, Romain A., Walter, Fabian, Yoshida, Naoki
We report the highest-redshift detection of [O I] 63 $\mu$m from a luminous quasar, J2054-0005, at $z=6.04$ based on the Atacama Large Millimeter/sub-millimeter Array Band 9 observations. The [O I] 63 $\mu$m line luminosity is $(4.5\pm1.5) \times 10^
Externí odkaz:
http://arxiv.org/abs/2408.09944