Zobrazeno 1 - 10
of 515
pro vyhledávání: '"Kazuo MAKISHIMA"'
Publikováno v:
The Astrophysical Journal, Vol 959, Iss 2, p 79 (2023)
The present study aims to reinforce the evidence for the ∼9 s pulsation in the gamma-ray binary LS 5039, derived from a Suzaku observation in 2007 and a NuSTAR observation in 2016. Through a reanalysis of the NuSTAR data incorporating the orbital D
Externí odkaz:
https://doaj.org/article/eb9ed580d95641dfb21e367202da897b
Autor:
Teruaki, Enoto, Kazuhiro, Nakazawa, Kazuo, Makishima, Yujin, Nakagawa E., Takanori, Sakamoto, Masanori, Ohno, Tadayuki, Takahashi, Yukikatsu, Terada, Kazutaka, Yamaoka, Toshio, Murakami, Hiromitsu, Takahashi
The fastest-rotating magnetar 1E 1547.0-5408 was observed in broad-band X-rays with Suzaku for 33 ks on 2009 January 28-29, 7 days after the onset of its latest bursting activity. After removing burst events, the absorption-uncorrected 2-10 keV flux
Externí odkaz:
http://arxiv.org/abs/1002.3668
Autor:
Hidehito Nanto, Harufumi Tsuchiya, Yuna Tsuji, Daisuke Yonetoku, Takahiro Matsumoto, Kazuhiro Nakazawa, Kazuo Makishima, Go Okada, Yoshihiro Furuta, Shohei Hisadomi, Teruaki Enoto, Yuuki Wada, Takayuki Yuasa, Tatsuya Sawano, Gabriel Diniz
Publikováno v:
Physical Review Research. 3
In 2015, the Gamma-Ray Observation of Winter Thunderstorms (GROWTH) collaboration launched a mapping observation campaign for high-energy atmospheric phenomena related to thunderstorms and lightning discharges. This campaign has developed a detection
This paper describes an analysis of the NuSTAR data of the fastest-rotating magnetar 1E 1547$-$5408, acquired in 2016 April for a time lapse of 151 ks. The source was detected with a 1-60 keV flux of $1.7 \times 10^{-11}$ ergs s$^{-1}$ cm$^{-2}$, and
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::ff763f11d55a341e494a2a2bf173695d
http://arxiv.org/abs/2102.00153
http://arxiv.org/abs/2102.00153
Autor:
Teruaki Enoto, Dmitry Khangulyan, Tsunefumi Mizuno, Tadayuki Takahashi, Kairi Mine, Kazuo Makishima, Hiroki Yoneda
We report on detailed analysis of the hard X-ray and GeV gamma-ray spectra of LS 5039, one of the brightest gamma-ray binary system in the Galaxy. The NuSTAR observation covering its entire orbit in 2016 allowed us for the first time to study the orb
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::caa6e2cc964ca7ea43d44a000d132055
IGR J00370+6122 is a high-mass X-ray binary, of which the primary is a B1 Ib star, whereas the companion is suggested to be a neutron star by the detection of 346-s pulsation in one-off 4-ks observation. To better understand the nature of the compact
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d1d2464d4fb73175f4266e45c27b92e1
Autor:
Kazuo Makishima
Publikováno v:
PROCEEDINGS OF THE 14TH ASIA-PACIFIC PHYSICS CONFERENCE.
Through observations with the Suzaku and NuSTAR X-ray observatories, at least three magnetars have been found to show periodic phase modulations in their hard X-ray pulses, with a period T which is ∼104 times longer than their pulse periods. Among
Autor:
Yuuki Wada, H. Odaka, Kazuhiro Nakazawa, Y. Furuta, Takayuki Yuasa, Harufumi Tsuchiya, Teruaki Enoto, Kazuo Makishima
Publikováno v:
Journal of Geophysical Research: Atmospheres. 125
Autor:
Daisuke Yonetoku, Takeshi Morimoto, Tatsuya Sawano, Teruaki Enoto, Mitsuteru Sato, Y. Furuta, Yuuki Wada, Harufumi Tsuchiya, Kazuo Makishima, Masashi Kamogawa, Takayuki Yuasa, Yoshitaka Nakamura, Tomoo Ushio, Kazuhiro Nakazawa, Hideo Sakai
Publikováno v:
Journal of Geophysical Research: Atmospheres. 125
Autor:
Daniel Maier, Tadayuki Takahashi, Greg Madejski, Rie Sato, Masayuki Ohta, Yasunobu Uchiyama, Kunishiro Mori, Takaaki Tanaka, Shin'ichiro Takeda, Madoka Kawaharada, Kouichi Hagino, Kazutaka Yamaoka, Hirokazu Odaka, Shin Watanabe, Makoto Asai, Yoichi Yatsu, Toshio Nakano, Hiromitsu Takahashi, Shinya Saito, Francois Lebrun, Hiromasa Suzuki, Masanori Ohno, D. H. Wright, Hirofumi Noda, Katsuma Miyake, Yukikatsu Terada, Hideki Uchiyama, Motohide Kokubun, Olivier Limousin, Kazuhiro Nakazawa, Tsunefumi Mizuno, Takeshi Nakamori, Kazuo Makishima, Yasushi Fukazawa, Jun Kataoka, Tamotsu Sato, Hiroyasu Tajima, Tatsumi Koi, Shogo B. Kobayashi, Junichiro Katsuta, Teruaki Enoto, Takayuki Yuasa, Philippe Laurent, Hiroaki Murakami, Katsuhiro Hayashi, Goro Sato
Publikováno v:
J.Astron.Telesc.Instrum.Syst.
J.Astron.Telesc.Instrum.Syst., 2020, 6 (4), pp.046003. ⟨10.1117/1.JATIS.6.4.046003⟩
J.Astron.Telesc.Instrum.Syst., 2020, 6 (4), pp.046003. ⟨10.1117/1.JATIS.6.4.046003⟩
Understanding and reducing the in-orbit instrumental backgrounds are essential to achieving high sensitivity in hard X-ray astronomical observations. The observational data of the Hard X-ray Imager (HXI) on board the Hitomi satellite provides useful
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d59d425f7e7ad5a1e5a63c5fa25321e9
https://hal.archives-ouvertes.fr/hal-03129440/file/046003_1.pdf
https://hal.archives-ouvertes.fr/hal-03129440/file/046003_1.pdf