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Autor:
Katoh, Ryuzi, Seki, Kazuhiko
Publikováno v:
J. Chem. Phys. 161, 124706 (2024)
We recently presented a quantitative model to explain the particle-size dependence of photoluminescence (PL) quantum yields and revealed that exciton quenching is not diffusion controlled, but limited by surface reactions. However, the exciton decay
Externí odkaz:
http://arxiv.org/abs/2408.08692
Autor:
Katoh, Masuko1 (AUTHOR), Nakayama, Izuma2 (AUTHOR), Wainberg, Zev A3 (AUTHOR), Shitara, Kohei2 (AUTHOR), Katoh, Masaru1,4 (AUTHOR) mkatoh-kkr@umin.ac.jp
Publikováno v:
Clinical & Translational Medicine. Jun2024, Vol. 14 Issue 6, p1-5. 5p.
Autor:
Katoh, Yuki1,2 kato.yuki@nihon-u.ac.jp, Kubo, Akiko3, Hayashi, Nobuki4, Sugi, Toshihiro4, Katoh, Kanoko4, Udagawa, Seiichi5, Ogawa, Tadashi6, Iwata, Takashi2, Nishio, Hiroshi2, Sugawara, Masaki2, Hirai, Shuichi1, Kawana, Kei4
Publikováno v:
Scientific Reports. 9/6/2024, Vol. 14 Issue 1, p1-11. 11p.
Autor:
Katoh, Haruki, Yasui, Chikako, Ikeda, Yuji, Kobayashi, Naoto, Matsunaga, Noriyuki, Kondo, Sohei, Sameshima, Hiroaki, Hamano, Satoshi, Mizumoto, Misaki, Kawakita, Hideyo, Fukue, Kei, Otsubo, Shogo, Takenaka, Keiichi
In this study, we performed high-resolution near-infrared (NIR) spectroscopy (R = 28,000; ${\lambda} = 0.90$-1.35 ${\mu}$m) with a high signal-to-noise ratio on HD 200775, a very young (${\sim}$0.1 Myr old) and massive intermediate-mass star (a binar
Externí odkaz:
http://arxiv.org/abs/2403.09774
Autor:
Vissapragada, Shreyas, McCreery, Patrick, Santos, Leonardo A. Dos, Espinoza, Néstor, McWilliam, Andrew, Matsunaga, Noriyuki, Redai, Jéa Adams, Behr, Patrick, France, Kevin, Hamano, Satoshi, Hull, Charlie, Ikeda, Yuji, Katoh, Haruki, Kawakita, Hideyo, López-Morales, Mercedes, Ceballos, Kevin N. Ortiz, Otsubo, Shogo, Sarugaku, Yuki, Takeuchi, Tomomi
The recent discovery of ``ultra-hot'' ($P < 1$ day) Neptunes has come as a surprise: some of these planets have managed to retain gaseous envelopes despite being close enough to their host stars to trigger strong photoevaporation and/or Roche lobe ov
Externí odkaz:
http://arxiv.org/abs/2401.16474
Autor:
Hamano, Satoshi, Ikeda, Yuji, Otsubo, Shogo, Katoh, Haruki, Fukue, Kei, Matsunaga, Noriyuki, Taniguchi, Daisuke, Kawakita, Hideyo, Takenaka, Keiichi, Kondo, Sohei, Sameshima, Hiroaki
We present a data reduction pipeline written in Python for data obtained with the near-infrared cross-dispersed echelle spectrograph, WINERED, which yields a 0.91$-$1.35 $\mu$m spectrum with the resolving power of $R_{\text{max}} \equiv \lambda / \De
Externí odkaz:
http://arxiv.org/abs/2401.04876
Publikováno v:
Music Trades. Jul2018, Vol. 166 Issue 6, p100-104. 4p.
Autor:
Minniti, D., Matsunaga, N., Fernandez-Trincado, J. G., Otsubo, S., Sarugaku, Y., Takeuchi, T., Katoh, H., Hamano, S., Ikeda, Y., Kawakita, H., Lucas, P. W., Smith, L. C., Petralia, I., Garro, E. R., Saito, R. K., Alonso-Garcia, J., Gomez, M., Navarro, M. G.
Context. The Galactic centre is hazardous for stellar clusters because of the strong tidal force. Supposedly, many clusters were destroyed and contributed stars to the crowded stellar field of the bulge and the nuclear stellar cluster. However, it is
Externí odkaz:
http://arxiv.org/abs/2312.16028
Autor:
Katoh, Takanobu A., Hinde, Elizabeth
Publikováno v:
Biophysical Reviews; Oct2024, Vol. 16 Issue 5, p547-550, 4p