Zobrazeno 1 - 10
of 186
pro vyhledávání: '"Yoshitake, Hiroshi"'
Autor:
Yoshitake, Hiroshi, Abbeel, Pieter
In this study, we propose a novel approach for investigating optimization performance by flexible robot coordination in automated warehouses with multi-agent reinforcement learning (MARL)-based control. Automated systems using robots are expected to
Externí odkaz:
http://arxiv.org/abs/2308.06036
Publikováno v:
In Transportation Research Part F: Psychology and Behaviour August 2021 81:608-621
Publikováno v:
Journal of Robotics & Mechatronics; Aug2024, Vol. 36 Issue 4, p918-927, 10p
Autor:
Yoshitake, Hiroshi, Sakai, Kazuhiro, Mitsuda, Kazuhisa, Yamasaki, Noriko Y., Takei, Yoh, Yamamoto, Ryo
Long-term time variabilities of the OVII (0.57 keV) emission in the soft X-ray diffuse background were studied using six Suzaku annual observations of blank sky towards the Lockman Hole made from 2006 to 2011. After time intervals in which the emissi
Externí odkaz:
http://arxiv.org/abs/1301.5174
Autor:
Ezoe, Yuichiro, Miyoshi, Yoshizumi, Yoshitake, Hiroshi, Mitsuda, Kazuhisa, Terada, Naoki, Oishi, Shihoko, Ohashi, Takaya
We present an analysis of a Suzaku observation taken during the geomagnetic storm of 2005 August 23-24. We found time variation of diffuse soft X-ray emission when a coronal mass ejection hit Earth and caused a geomagnetic storm. The diffuse emission
Externí odkaz:
http://arxiv.org/abs/1105.5984
Publikováno v:
ApJ,727,L38 (2011)
We report on a new merging group of galaxies, Suzaku J1552+2739 at z ~ 0.08 revealed by a SUZAKU observation. The group was found by observing a junction of galaxy filaments optically identified in the Sloan Digital Sky Survey spectroscopic data. Suz
Externí odkaz:
http://arxiv.org/abs/1101.0614
Autor:
Ezoe, Yuichiro, Ebisawa, Ken, Yamasaki, Noriko Y., Mitsuda, Kazuhisa, Yoshitake, Hiroshi, Terada, Naoki, Miyoshi, Yoshizumi, Fujimoto, Ryuichi
We report the detection of a time variable OVII line emission in a deep 100 ks Suzaku X-ray Imaging Spectrometer spectrum of the Galactic Ridge X-ray emission. The observed line intensity is too strong (11+/-2 line unit or photon cm^-2 s^-1 str^-1) t
Externí odkaz:
http://arxiv.org/abs/1006.5253
Autor:
Yoshitake, Hiroshi, Shino, Motoki
Publikováno v:
In IATSS Research December 2018 42(4):240-247
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Akademický článek
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