Hitomi X-ray studies of giant radio pulses from the Crab pulsar. (11th April 2018)
- Record Type:
- Journal Article
- Title:
- Hitomi X-ray studies of giant radio pulses from the Crab pulsar. (11th April 2018)
- Main Title:
- Hitomi X-ray studies of giant radio pulses from the Crab pulsar
- Authors:
- Aharonian, Hitomi Collaboration, Felix
Akamatsu, Hiroki
Akimoto, Fumie
Allen, Steven W
Angelini, Lorella
Audard, Marc
Awaki, Hisamitsu
Axelsson, Magnus
Bamba, Aya
Bautz, Marshall W
Blandford, Roger
Brenneman, Laura W
Brown, Gregory V
Bulbul, Esra
Cackett, Edward M
Chernyakova, Maria
Chiao, Meng P
Coppi, Paolo S
Costantini, Elisa
de Plaa, Jelle
de Vries, Cor P
den Herder, Jan-Willem
Done, Chris
Dotani, Tadayasu
Ebisawa, Ken
Eckart, Megan E
Enoto, Teruaki
Ezoe, Yuichiro
Fabian, Andrew C
Ferrigno, Carlo
Foster, Adam R
Fujimoto, Ryuichi
Fukazawa, Yasushi
Furuzawa, Akihiro
Galeazzi, Massimiliano
Gallo, Luigi C
Gandhi, Poshak
Giustini, Margherita
Goldwurm, Andrea
Gu, Liyi
Guainazzi, Matteo
Haba, Yoshito
Hagino, Kouichi
Hamaguchi, Kenji
Harrus, Ilana M
Hatsukade, Isamu
Hayashi, Katsuhiro
Hayashi, Takayuki
Hayashida, Kiyoshi
Hiraga, Junko S
Hornschemeier, Ann
Hoshino, Akio
Hughes, John P
Ichinohe, Yuto
Iizuka, Ryo
Inoue, Hajime
Inoue, Yoshiyuki
Ishida, Manabu
Ishikawa, Kumi
Ishisaki, Yoshitaka
Iwai, Masachika
Kaastra, Jelle
Kallman, Tim
Kamae, Tsuneyoshi
Kataoka, Jun
Katsuda, Satoru
Kawai, Nobuyuki
Kelley, Richard L
Kilbourne, Caroline A
Kitaguchi, Takao
Kitamoto, Shunji
Kitayama, Tetsu
Kohmura, Takayoshi
Kokubun, Motohide
Koyama, Katsuji
Koyama, Shu
Kretschmar, Peter
Krimm, Hans A
Kubota, Aya
Kunieda, Hideyo
Laurent, Philippe
Lee, Shiu-Hang
Leutenegger, Maurice A
Limousin, Olivier O
Loewenstein, Michael
Long, Knox S
Lumb, David
Madejski, Greg
Maeda, Yoshitomo
Maier, Daniel
Makishima, Kazuo
Markevitch, Maxim
Matsumoto, Hironori
Matsushita, Kyoko
McCammon, Dan
McNamara, Brian R
Mehdipour, Missagh
Miller, Eric D
Miller, Jon M
Mineshige, Shin
Mitsuda, Kazuhisa
Mitsuishi, Ikuyuki
Miyazawa, Takuya
Mizuno, Tsunefumi
Mori, Hideyuki
Mori, Koji
Mukai, Koji
Murakami, Hiroshi
Mushotzky, Richard F
Nakagawa, Takao
Nakajima, Hiroshi
Nakamori, Takeshi
Nakashima, Shinya
Nakazawa, Kazuhiro
Nobukawa, Kumiko K
Nobukawa, Masayoshi
Noda, Hirofumi
Odaka, Hirokazu
Ohashi, Takaya
Ohno, Masanori
Okajima, Takashi
Oshimizu, Kenya
Ota, Naomi
Ozaki, Masanobu
Paerels, Frits
Paltani, Stéphane
Petre, Robert
Pinto, Ciro
Porter, Frederick S
Pottschmidt, Katja
Reynolds, Christopher S
Safi-Harb, Samar
Saito, Shinya
Sakai, Kazuhiro
Sasaki, Toru
Sato, Goro
Sato, Kosuke
Sato, Rie
Sawada, Makoto
Schartel, Norbert
Serlemtsos, Peter J
Seta, Hiromi
Shidatsu, Megumi
Simionescu, Aurora
Smith, Randall K
Soong, Yang
Stawarz, Łukasz
Sugawara, Yasuharu
Sugita, Satoshi
Szymkowiak, Andrew
Tajima, Hiroyasu
Takahashi, Hiromitsu
Takahashi, Tadayuki
Takeda, Shiníchiro
Takei, Yoh
Tamagawa, Toru
Tamura, Takayuki
Tanaka, Takaaki
Tanaka, Yasuo
Tanaka, Yasuyuki T
Tashiro, Makoto S
Tawara, Yuzuru
Terada, Yukikatsu
Terashima, Yuichi
Tombesi, Francesco
Tomida, Hiroshi
Tsuboi, Yohko
Tsujimoto, Masahiro
Tsunemi, Hiroshi
Tsuru, Takeshi Go
Uchida, Hiroyuki
Uchiyama, Hideki
Uchiyama, Yasunobu
Ueda, Shutaro
Ueda, Yoshihiro
Uno, Shiníchiro
Urry, C Megan
Ursino, Eugenio
Watanabe, Shin
Werner, Norbert
Wilkins, Dan R
Williams, Brian J
Yamada, Shinya
Yamaguchi, Hiroya
Yamaoka, Kazutaka
Yamasaki, Noriko Y
Yamauchi, Makoto
Yamauchi, Shigeo
Yaqoob, Tahir
Yatsu, Yoichi
Yonetoku, Daisuke
Zhuravleva, Irina
Zoghbi, Abderahmen
Terasawa, Toshio
Sekido, Mamoru
Takefuji, Kazuhiro
Kawai, Eiji
Misawa, Hiroaki
Tsuchiya, Fuminori
Yamazaki, Ryo
Kobayashi, Eiji
Kisaka, Shota
Aoki, Takahiro
… (more) - Abstract:
- Abstract: To search for giant X-ray pulses correlated with the giant radio pulses (GRPs) from the Crab pulsar, we performed a simultaneous observation of the Crab pulsar with the X-ray satellite Hitomi in the 2–300 keV band and the Kashima NICT radio telescope in the 1.4–1.7 GHz band with a net exposure of about 2 ks on 2016 March 25, just before the loss of the Hitomi mission. The timing performance of the Hitomi instruments was confirmed to meet the timing requirement and about 1000 and 100 GRPs were simultaneously observed at the main pulse and inter-pulse phases, respectively, and we found no apparent correlation between the giant radio pulses and the X-ray emission in either the main pulse or inter-pulse phase. All variations are within the 2 σ fluctuations of the X-ray fluxes at the pulse peaks, and the 3 σ upper limits of variations of main pulse or inter-pulse GRPs are 22% or 80% of the peak flux in a 0.20 phase width, respectively, in the 2–300 keV band. The values for main pulse or inter-pulse GRPs become 25% or 110%, respectively, when the phase width is restricted to the 0.03 phase. Among the upper limits from the Hitomi satellite, those in the 4.5–10 keV and 70–300 keV bands are obtained for the first time, and those in other bands are consistent with previous reports. Numerically, the upper limits of the main pulse and inter-pulse GRPs in the 0.20 phase width are about (2.4 and 9.3) × 10 −11 erg cm −2, respectively. No significant variability in pulse profilesAbstract: To search for giant X-ray pulses correlated with the giant radio pulses (GRPs) from the Crab pulsar, we performed a simultaneous observation of the Crab pulsar with the X-ray satellite Hitomi in the 2–300 keV band and the Kashima NICT radio telescope in the 1.4–1.7 GHz band with a net exposure of about 2 ks on 2016 March 25, just before the loss of the Hitomi mission. The timing performance of the Hitomi instruments was confirmed to meet the timing requirement and about 1000 and 100 GRPs were simultaneously observed at the main pulse and inter-pulse phases, respectively, and we found no apparent correlation between the giant radio pulses and the X-ray emission in either the main pulse or inter-pulse phase. All variations are within the 2 σ fluctuations of the X-ray fluxes at the pulse peaks, and the 3 σ upper limits of variations of main pulse or inter-pulse GRPs are 22% or 80% of the peak flux in a 0.20 phase width, respectively, in the 2–300 keV band. The values for main pulse or inter-pulse GRPs become 25% or 110%, respectively, when the phase width is restricted to the 0.03 phase. Among the upper limits from the Hitomi satellite, those in the 4.5–10 keV and 70–300 keV bands are obtained for the first time, and those in other bands are consistent with previous reports. Numerically, the upper limits of the main pulse and inter-pulse GRPs in the 0.20 phase width are about (2.4 and 9.3) × 10 −11 erg cm −2, respectively. No significant variability in pulse profiles implies that the GRPs originated from a local place within the magnetosphere. Although the number of photon-emitting particles should temporarily increase to account for the brightening of the radio emission, the results do not statistically rule out variations correlated with the GRPs, because the possible X-ray enhancement may appear due to a >0.02% brightening of the pulse-peak flux under such conditions. … (more)
- Is Part Of:
- Publications of the Astronomical Society of Japan. Volume 70(2018)Supplement 2
- Journal:
- Publications of the Astronomical Society of Japan
- Issue:
- Volume 70(2018)Supplement 2
- Issue Display:
- Volume 70, Issue 2 (2018)
- Year:
- 2018
- Volume:
- 70
- Issue:
- 2
- Issue Sort Value:
- 2018-0070-0002-0000
- Page Start:
- Page End:
- Publication Date:
- 2018-04-11
- Subjects:
- pulsars: individual (B0531+21) -- radio continuum: stars -- X-rays: stars
Astronomy -- Periodicals
520.5 - Journal URLs:
- http://pasj.asj.or.jp/ ↗
http://pasj.oxfordjournals.org/ ↗
http://www.oxfordjournals.org/ ↗ - DOI:
- 10.1093/pasj/psx083 ↗
- Languages:
- English
- ISSNs:
- 0004-6264
- Deposit Type:
- Legaldeposit
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