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1. The Far-Infrared Surveyor (FIS) for AKARI

Author

Kawada, Mitsunobu, Baba, Hajime, Barthel, Peter D., Clements, David, Cohen, Martin, Doi, Yasuo, Figueredo, Elysandra, Fujiwara, Mikio, Goto, Tomotsugu, Hasegawa, Sunao, Hibi, Yasunori, Hirao, Takanori, Hiromoto, Norihisa, Jeong, Woong-Seob, Kaneda, Hidehiro, Kawai, Toshihide, Kawamura, Akiko, Kester, Do, Kii, Tsuneo, Kobayashi, Hisato, Kwon, Suk Minn, Lee, Hyung Mok, Makiuti, Sin'itirou, Matsuo, Hiroshi, Matsuura, Shuji, Müller, Thomas G., Murakami, Noriko, Nagata, Hirohisa, Nakagawa, Takao, Narita, Masanao, Noda, Manabu, Oh, Sang Hoon, Okada, Yoko, Okuda, Haruyuki, Oliver, Sebastian, Ootsubo, Takafumi, Pak, Soojong, Park, Yong-Sun, Pearson, Chris P., Rowan-Robinson, Michael, Saito, Toshinobu, Salama, Alberto, Sato, Shinji, Savage, Richard S., Serjeant, Stephen, Shibai, Hiroshi, Shirahata, Mai, Sohn, Jungjoo, Suzuki, Toyoaki, Takagi, Toshinobu, Takahashi, Hidenori, Thomson, Matthew, Usui, Fumihiko, Verdugo, Eva, Watabe, Toyoki, White, Glenn J., Wang, Lingyu, Yamamura, Issei, Yamamuchi, Chisato, and Yasuda, Akiko

Subjects
Astrophysics
Abstract

The Far-Infrared Surveyor (FIS) is one of two focal plane instruments on the AKARI satellite. FIS has four photometric bands at 65, 90, 140, and 160 um, and uses two kinds of array detectors. The FIS arrays and optics are designed to sweep the sky with high spatial resolution and redundancy. The actual scan width is more than eight arcmin, and the pixel pitch is matches the diffraction limit of the telescope. Derived point spread functions (PSFs) from observations of asteroids are similar to the optical model. Significant excesses, however, are clearly seen around tails of the PSFs, whose contributions are about 30% of the total power. All FIS functions are operating well in orbit, and its performance meets the laboratory characterizations, except for the two longer wavelength bands, which are not performing as well as characterized. Furthermore, the FIS has a spectroscopic capability using a Fourier transform spectrometer (FTS). Because the FTS takes advantage of the optics and detectors of the photometer, it can simultaneously make a spectral map. This paper summarizes the in-flight technical and operational performance of the FIS., Comment: 23 pages, 10 figures, and 2 tables. Accepted for publication in the AKARI special issue of the Publications of the Astronomical Society of Japan

Published
2007
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2. Flight Performance of the AKARI Cryogenic System

Author

Nakagawa, Takao, Enya, Keigo, Hirabayashi, Masayuki, Kaneda, Hidehiro, Kii, Tsuneo, Kimura, Yoshiyuki, Matsumoto, Toshio, Murakami, Hiroshi, Murakami, Masahide, Narasaki, Katsuhiro, Narita, Masanao, Ohnishi, Akira, Tsunematsu, Shoji, and Yoshida, Seiji

Subjects
Astrophysics
Abstract

We describe the flight performance of the cryogenic system of the infrared astronomical satellite AKARI, which was successfully launched on 2006 February 21 (UT). AKARI carries a 68.5 cm telescope together with two focal plane instruments, Infrared Cameras (IRC) and Far Infrared Surveyor (FIS), all of which are cooled down to cryogenic temperature to achieve superior sensitivity. The AKARI cryogenic system is a unique hybrid system, which consists of cryogen (liquid helium) and mechanical coolers (2-stage Stirling coolers). With the help of the mechanical coolers, 179 L (26.0 kg) of super-fluid liquid helium can keep the instruments cryogenically cooled for more than 500 days. The on-orbit performance of the AKARI cryogenics is consistent with the design and pre-flight test, and the boil-off gas flow rate is as small as 0.32 mg/s. We observed the increase of the major axis of the AKARI orbit, which can be explained by the thrust due to thermal pressure of vented helium gas., Comment: 19 pages, 10 figures, and 6 tables. Accepted for publication in the AKARI special issue of the Publications of the Astronomical Society of Japan

Published
2007
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3. Optical Identification of the ASCA Lynx Deep Survey: An Association of QSOs and a Supercluster at z=1.3?

Author

Ohta, Kouji, Akiyama, Masayuki, Ueda, Yoshihiro, Yamada, Toru, Nakanishi, Kouichiro, Dalton, Gavin B., Ogasaka, Yasushi, Kii, Tsuneo, and Hayashida, Kiyoshi

Subjects
Astrophysics
Abstract

Results of optical identification of the ASCA Lynx deep survey are presented. Six X-ray sources are detected in the 2-7 keV band using the SIS in a 20'x20' field of view with fluxes larger than ~4x10^{-14} erg s-1 cm-2 in the band. Follow-up optical spectroscopic observations were made, and five out of six sources are identified with AGNs/QSOs at redshifts of 0.5-1.3. We also identify two more additional X-ray sources detected in a soft X-ray band with AGNs/QSOs. It is found that three QSOs identified are located at z~1.3. Two rich clusters and several groups of galaxies are also placed at the same redshift in the surveyed field, and projected separations between the QSOs and the clusters are 3-8 Mpc at the redshift., Comment: 15 pages with 3 figures. Accepted to ApJ

Published
2003
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4. Multiwavelength Monitoring of the BL Lacertae Object PKS 2155-304 in May 1994. II. The IUE Campaign

Author

Pian, Elena, Urry, C. Megan, Treves, Aldo, Maraschi, Laura, Penton, Steve, Shull, J. Michael, Pesce, Joseph E., Grandi, Paola, Kii, Tsuneo, Kollgaard, Ron I., Madejski, Greg, Marshall, Herman, Wamsteker, Willem, Celotti, Annalisa, Courvoisier, Thierry J. -L., Falomo, Renato, Fink, Henner H., George, Ian M., and Ghisellini, Gabriele

Subjects
Astrophysics
Abstract

PKS 2155-304, the brightest BL Lac object in the ultraviolet sky, was monitored with the IUE satellite at ~1 hour time-resolution for ten nearly uninterrupted days in May 1994. The campaign, which was coordinated with EUVE, ROSAT, and ASCA monitoring, along with optical and radio observations from the ground, yielded the largest set of spectra and the richest short time scale variability information ever gathered for a blazar at UV wavelengths. The source flared dramatically during the first day, with an increase by a factor ~2.2 in an hour and a half. In subsequent days, the flux maintained a nearly constant level for ~5 days, then flared with ~35% amplitude for two days. The same variability was seen in both short- and long-wavelength IUE light curves, with zero formal lag (~<2 hr), except during the rapid initial flare, when the variations were not resolved. Spectral index variations were small and not clearly correlated with flux. The flux variability observed in the present monitoring is so rapid that for the first time, based on the UV emission alone, the traditional Delta L/Delta t limit indicating relativistic beaming is exceeded. The most rapid variations, under the likely assumption of synchrotron radiation, lead to a lower limit of 1 G on the magnetic field strength in the UV emitting region. These results are compared with earlier intensive monitoring of PKS 2155-304 with IUE in November 1991, when the UV flux variations had completely different characteristics., Comment: 45 pages, Latex, 11 PostScript figures, to appear in The Astrophysical Journal

Published
1997
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7. Space Vlbi Satellite Halca and its Engineering Accomplishments

Author

Hirosawa, Haruto, Hirabayashi, Hisashi, Kobayashi, Hideyuki, Murata, Yasuhiro, Kii, Tsuneo, Edwards, Philip, Natori, Michihiro, Takano, Tadashi, Yamamoto, Zen-Ichi, Hashimoto, Tatsuaki, Inoue, Kouzaburo, Ohnishi, Akira, Ohshima, Tsutomu, Ichikawa, Tsutomu, Fujisawa, Kenta, Wajima, Kiyoaki, Okayasu, Rikako, Inoue, Makoto, Kawaguchi, Noriyuki, Kameno, Seiji, Shibata, Katsunori, and Asaki, Yoshiaki

Published
2002
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8. The X-ray emission of 3C 273 observed with ASCA

Author

Yaqoob, Tahir, Serlemitsos, Peter, Mushotzky, Richard, Ricker, George, Woo, Jonathan, Weaver, Kim, Kii, Tsuneo, Mitsuda, Kazuhisa, Kotani, Taro, and Hayashida, Kiyoshi

Subjects
Astrophysics
Abstract

We report preliminary results of an Advanced Satellite for Cosmology and Astrophysics (ASCA) observation of 3C 273. There is no spectral variability within the ASCA observation, in contrast to the longer term behavior found with European X-ray Observatory Satellite (EXOSAT) and Ginga which established significant changes in the spectral index of the power-law continuum on timescales of a week or more, uncorrelated with luminosity. Comparison of the ASCA data with a simultaneous Roentgen Satellite (ROSAT) Ginga observation in 1990 December shows that while the shape of the spectrum above approximately 1 keV is essentially the same, the flux in the soft component, below approximately 1 keV, considerably weaker relative to the hard component in the ASCA observation. The 2-10 keV luminosity is at least a factor of approximately 1.5 greater in the ASCA observation than in the ROSAT/Ginga observation while the ratio of 2-10 keV luminosity to 0.4-1.0 keV luminosity increases by a factor of approximately 1.2. Thus the spectral shape of the hard component appears to be independent of the relative magnitude of the soft component and is an important constraint on emission and reprocessing models. We find no significant Fe K line-emission in this observation. The data also highlight very well some of the outstanding problems in the instrumental responses.

Published
1994

9. The fluorescence-dominated X-ray spectrum of the spiral galaxy NGC 6552

Author

Fukazawa, Yasushi, Makishima, Kazuo, Ebisawa, Ken, Fabian, Andrew C, Gendreau, Keith C, Ikebe, Yasushi, Iwasawa, Kazushi, Kii, Tsuneo, Mushotzky, Richard F, and Ohashi, Takaya

Subjects
Astronomy
Abstract

A hard X-ray source with a 2-10 keV flux of approximately 6 x 10(exp -13) ergs/sec/sq cm was detected with ASCA in the north ecliptic pole region. It is identified with the spiral galaxy NGC 6552 at a redshift of z = 0.026, which is optically classified as a Seyfert 2 galaxy. The X-ray spectrum consists of a series of atomic K-emission lines from (nearly-) neutral species of at least seven abundant elements, and a heavily absorbed (N(sub H) approx. = 6 x 10(exp 23)/sq cm) hard continuum. The iron line has an equivalent width as large as approximately 0.9 keV. Our results show that NGC 6552 is an extreme type 2 Seyfert galaxy, in which the fluorescent lines are produced when hard X-rays from a hidden active nucleus are reflected off thick cool matter into our line of sight. The intrinsic 2-10 keV luminosity of the nucleus is estimated to be at least 6 x 10(exp 42) ergs/s.

Published
1994

10. Discovery of an obscured low luminosity active nucleus in the spiral galaxy NGC 4258

Author

Makishima, Kazuo, Fujimoto, Ryuichi, Ishisaki, Yoshitaka, Kii, Tsuneo, Loewenstein, Michael, Mushotzky, Richard, Serlemitsos, Peter, Sonobe, Takashi, Tashiro, Makoto, and Yaqoob, Tahir

Subjects
Astrophysics
Abstract

The spectra and images of the nearby jet galaxy NGC 4258 (M106) obtained with ASCA indicate presence of several distinct X-ray emission components. The emission above 3 keV is pointlike and coincident in position with the optical nucleus, exhibiting a hard (photon index approximately 1.78) and absorbed N(sub H) approximately 1.5 x 10(exp 23) cm(exp -2) spectrum. This provides clear evidence that NGC 4258 hosts an obscured active nucleus of low luminosity, about 4 x 10(exp 40) ergs s(exp -1) in 2-10 keV after removing the absorption. Iron K-line emission with an equivalent width 0.25 +/- 0.10 keV was detected. The emission below 1 keV is dominated by an extended approximately 4 min thin-thermal component with a temperature approximately 0.5 keV exhibiting atomic emission lines, possibly associated with the jet. There exists a third continuum component with an intermediate spectral hardness, which is brightest at approximately 1 min south-east of the nucleus.

Published
1994

11. Design for LiteBIRD optics

Author

Okada, Nozomi, Kimura, Kimihiro, Inoue, Masanori, Onishi, Toshikazu, Ogawa, Hideo, Sekimoto, Yutaro, Inadani, Jyunji, Kashima, Shingo, Hazumi, Masashi, Ota, Izumi, Matsumura, Tomotake, Murata, Yasuhiro, Nishibori, Toshiyuki, and Kii, Tsuneo

Abstract

第15回宇宙科学シンポジウム (2015年1月6日-7日. 宇宙航空研究開発機構宇宙科学研究所(JAXA)(ISAS)相模原キャンパス), 相模原市, 神奈川県, 15th Space Science Symposium (January 6-7, 2015. Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency(JAXA)(ISAS)Sagamihara Campus), Sagamihara, Kanagawa Japan, 著者人数: 14名, 資料番号: SA6000034079, レポート番号: P-079

Published
2015

12. SPICA system

Author

Saito, Hirobumi, Hashimoto, Tatsuaki, Murakami, Hiroshi, Kii, Tsuneo, Noda, Atsushi, and Ogawa, Akira

Subjects
SPICA, システムエンジニアリング, トップダウンモデル, management method, ウォータフォールモデル, development phase, プロジェクト, top down model, documentation, 管理方法, project management, 文書化, 開発フェーズ, project, progress, work breakdown structure, 作業分割構成, waterfall model, プロジェクト立案, 進捗, プロジェクトマネジメント, system engineering, project planning
Abstract

SPICAは、2012年頃にH2Aロケットでの打上げを目指す次期赤外線天文衛星である。この衛星は、現時点での設計で寸法3.8mΦ×8.6m、総質量2.6トンと極めて大型の衛星であり、また、太陽-地球系のL2軌道に投入し、直径3.5mΦの光学系全体を4Kに冷却するなどミッション的にも野心的な先端性を持つ。このようなSPICAの特徴から考えれば、当然ながら、衛星システムは複雑化し、開発が難航する可能性がある。本文では、システムエンジニアリングの考えを取り入れ、如何に大型で複雑な衛星の開発を行うかについて説明する。, 資料番号: AA0049122033

Published
2005

13. Performance evaluation of an Ultra Fine Sun Sensor onboard Solar-B satellite

Author

Kubo, Masahito, Shimizu, Toshifumi, Hirokawa, Eiji, Kii, Tsuneo, Hashimoto, Tatsuaki, Kosugi, Takeo, Ninomiya, Keiken, Yamamoto, Takahisa, Okumura, Toru, and Tsuno, Katsuhiko

Subjects
NDフィルター, Solar-B衛星, solar spectrometer, reticle, performance evaluation, ultrafine sun sensor, solar simulator, ND filter, 超高精度太陽センサー, 軌道上望遠鏡, レチクル, 性能評価, 太陽分光器, 太陽シミュレーター, Solar-B satellite, spaceborne telescope, CCD
Abstract

Solar-B衛星の重要な特徴の1つは、口径50cmの主鏡の回折限界である0.2秒角の空間分解能で太陽の可視光観測が可能な点である。高分解能の観測の為に厳しい姿勢制御の精度が要求され、高い位置検出精度が太陽センサーに必要となる。Solar-B衛星に搭載される超高精度太陽センサー(Ultra Fine Sun Sensor, UFSS)の角度検出性能をプロトモデル品で検証し、ランダム誤差0.15arcsec(1σ)、視野±0.5度、四方でバイアス誤差約2arcsec(p-p)の実力を実証した。, 資料番号: AA0047899126

Published
2004

15. Space VLBI Satellite HALCA and its Engineering Accomplishments

Author

Edwards, Philip, Hirosawa, Haruto, Hirabayashi, Hisashi, Kobayashi, Hideyuki, Murata, Yasuhiro, Kii, Tsuneo, Natori, Michihiro, Takano, Tadashi, Yamamoto, Zen-Ichi, Hashimoto, Tatsuaki, Inoue, Kouzaburo, Ohnishi, Akira, Ohshima, Tsutomu, Ichikawa, Tsutomu, Fujisawa, Kenta, Wajima, Kiyoaki, Okayasu, Rikako, Inoue, Makoto, Kawaguchi, Noriyuki, Kameno, Seiji, Shibata, Katsunori, and Asaki, Yoshiaki

Subjects
Parabolic antenna, Physics, Astronautics, Spacecraft, business.industry, Aerospace Engineering, law.invention, Telescope, Radio telescope, Attitude control, law, Very-long-baseline interferometry, Satellite, business, Remote sensing
Abstract

著者人数: 22名, 資料番号: SA1003268000

Published
2002

16. FIS: far-infrared surveyor onboard ASTRO-F (IRIS)

Author

Takahashi, Hidenori, Shibai, Hiroshi, Kawada, Mitsunobu, Hirao, Takanori, Watabe, Toyoki, Tsuduku, Yasushi, Nagata, Hirohisa, Utsuno, Hiroshi, Hibi, Yasushi, Hirooka, Shinya, Nakagawa, Takao, Kaneda, Hidehiro, Matsuura, Shuji, Kii, Tsuneo, Makiuti, Shin'ichiro, Okamura, Yoshihiko, Doi, Yasuo, Matsuo, Hiroshi, Hiromoto, Norihisa, Fujiwara, Mikio, and Noda, Manabu

Abstract

著者人数：21名, 資料番号: SA1001812000

Published
2000

17. 3C279 Results Derived from Two-Frequency VSOP Observations

Author

EDWARDS, P. G., PINER, B. G., WEHRLE, A. E., UNWIN, S. C., LOVELL, J. E. J., HIRABAYASHI, Hisashi, OKAYASU, Rikako, KII, Tsuneo, and MAKINO, Fumiyoshi

Abstract

VSOPシンポジウム(2000年1月19日-21日. 宇宙科学研究所(ISAS)）, 相模原市, 神奈川県, VSOP Symposium (January 19-21, 2000. Institute of Space and Astronautical Science(ISAS)), Sagamihara, Kanagawa Japan, 資料番号: SA6000155007

Published
2000

18. Improvement of the ASCA Position Accuracy

Author

Gotthelf, E. V., Ueda, Yoshihiro, Inoue, Hajime, Ogawara, Yoshiaki, Fujimoto, Ryuichi, Yamaoka, Kazutaka, and Kii, Tsuneo

Abstract

資料番号: SA8000200000

Published
1999

19. Solar-B衛星搭載超高精度太陽センサー(UFSS)の性能検証

Author

Kubo, Masahito, Shimizu, Toshifumi, Hirokawa, Eiji, Kii, Tsuneo, Hashimoto, Tatsuaki, Kosugi, Takeo, Ninomiya, Keiken, Yamamoto, Takahisa, Okumura, Toru, Tsuno, Katsuhiko, 久保 雅仁, 清水 敏文, 広川 英治, 紀伊 恒男, 橋本 樹明, 小杉 健郎, 二宮 敬虔, 山本 貴久, 奥村 徹, 津野 克彦, Kubo, Masahito, Shimizu, Toshifumi, Hirokawa, Eiji, Kii, Tsuneo, Hashimoto, Tatsuaki, Kosugi, Takeo, Ninomiya, Keiken, Yamamoto, Takahisa, Okumura, Toru, Tsuno, Katsuhiko, 久保 雅仁, 清水 敏文, 広川 英治, 紀伊 恒男, 橋本 樹明, 小杉 健郎, 二宮 敬虔, 山本 貴久, 奥村 徹, and 津野 克彦

Abstract

Solar-B衛星の重要な特徴の1つは、口径50cmの主鏡の回折限界である0.2秒角の空間分解能で太陽の可視光観測が可能な点である。高分解能の観測の為に厳しい姿勢制御の精度が要求され、高い位置検出精度が太陽センサーに必要となる。Solar-B衛星に搭載される超高精度太陽センサー(Ultra Fine Sun Sensor, UFSS)の角度検出性能をプロトモデル品で検証し、ランダム誤差0.15arcsec(1σ)、視野±0.5度、四方でバイアス誤差約2arcsec(p-p)の実力を実証した。

Published
2015

20. ASCA Observations of the Composite Warm Absorber in NGC 3516

Author

Kriss, G. A., Krolik, J. H., 大谷, 知行, Espey, B. R., Turner, T. J., 紀伊, 恒男, Tsvetanov, Z., 高橋, 忠幸, Davidsen, A. F., 田代, 信, Zheng, W., Murakami, S., Petre, R., 三原, 建弘, Otani, C., Kii, Tsuneo, Takahashi, Tadayuki, Tashiro, M., Mihara, T., Kriss, G. A., Krolik, J. H., 大谷, 知行, Espey, B. R., Turner, T. J., 紀伊, 恒男, Tsvetanov, Z., 高橋, 忠幸, Davidsen, A. F., 田代, 信, Zheng, W., Murakami, S., Petre, R., 三原, 建弘, Otani, C., Kii, Tsuneo, Takahashi, Tadayuki, Tashiro, M., and Mihara, T.

Abstract

著者人数：14名, Accepted: 1996-03-07

Published
2015

21. X-Ray Spectra of Bright Core-Dominant Quasars: NRAO 140 and 4C 34.47

Author

大橋, 隆哉, 田代, 信, 牧島, 一夫, 紀伊, 恒男, 槙野, 文命, Turner, M. J. L., Williams, O. R., Ohashi, T., Tashiro, Makoto, Makishima, Kazuo, Kii, Tsuneo, Makino, Fumiyoshi, 大橋, 隆哉, 田代, 信, 牧島, 一夫, 紀伊, 恒男, 槙野, 文命, Turner, M. J. L., Williams, O. R., Ohashi, T., Tashiro, Makoto, Makishima, Kazuo, Kii, Tsuneo, and Makino, Fumiyoshi

Abstract

Note: Accepted for publication in The Astrophysical Journal.

Published
2015

22. The Far-Infrared Surveyor (FIS) for AKARI

Author

川田, 光伸, 馬場, 肇, 土井, 靖生, 藤原, 幹生, 後藤, 友嗣, 長谷川, 直, 日比, 康詞, 平尾, 孝憲, 廣本, 宣久, Jeong, Woong-Seob, 金田, 英宏, 河合, 利秀, 河村, 晶子, 紀伊, 恒男, 小林, 久人, 巻内, 慎一郎, 松尾, 宏, 松浦, 周二, 村上, 紀子, 永田, 洋久, 中川, 貴雄, 成田, 正直, 野田, 学, 岡田, 陽子, 奥田, 治之, 大坪, 貴文, 齋藤, 年伸, 佐藤, 紳司, 芝井, 広, 白旗, 麻衣, 鈴木, 仁研, 高木, 俊暢, 高橋, 英則, 臼井, 文彦, 渡部, 豊喜, 山村, 一誠, 山内, 千里, 安田, 晃子, Kawada, Mitsunobu, Baba, Hajime, Barthel, Peter D., Clements, David, Cohen, Martin, Doi, Yasuo, Figueredo, Elysandra, Fujiwara, Mikio, Goto, Tomotsugu, Hasegawa, Sunao, Hibi, Yasunori, Hirao, Takanori, Hiromoto, Norihisa, Kaneda, Hidehiro, Kawai, Toshihide, Kawamura, Akiko, Kester, Do, Kii, Tsuneo, Kobayashi, Hisato, Kwon, Suk Minn, Lee, Hyung Mok, Makiuti, Sin'itirou, Matsuo, Hiroshi, Matsuura, Shuji, Muller, Thomas G., Murakami, Noriko, Nagata, Hirohisa, Nakagawa, Takao, Narita, Masanao, Noda, Manabu, Oh, Sang Hoon, Okada, Yoko, Okuda, Haruyuki, Oliver, Sebastian, Ootsubo, Takafumi, Pak, Soojong, Park, Yong-Sun, Pearson, Chris P., Rowan-Robinson, Michael, Saito, Toshinobu, Salama, Alberto, Sato, Shinji, Savage, Richard S., Serjeant, Stephen, Shibai, Hiroshi, Shirahata, Mai, Sohn, Jungjoo, Suzuki, Toyoaki, Takagi, Toshinobu, Takahashi, Hidenori, Thomson, Matthew, Usui, Fumihiko, Verdugo, Eva, Watabe, Toyoki, White, Glenn J., Wang, Lingyu, Yamamura, Issei, Yamauchi, Chisato, Yasuda, Akiko, 川田, 光伸, 馬場, 肇, 土井, 靖生, 藤原, 幹生, 後藤, 友嗣, 長谷川, 直, 日比, 康詞, 平尾, 孝憲, 廣本, 宣久, Jeong, Woong-Seob, 金田, 英宏, 河合, 利秀, 河村, 晶子, 紀伊, 恒男, 小林, 久人, 巻内, 慎一郎, 松尾, 宏, 松浦, 周二, 村上, 紀子, 永田, 洋久, 中川, 貴雄, 成田, 正直, 野田, 学, 岡田, 陽子, 奥田, 治之, 大坪, 貴文, 齋藤, 年伸, 佐藤, 紳司, 芝井, 広, 白旗, 麻衣, 鈴木, 仁研, 高木, 俊暢, 高橋, 英則, 臼井, 文彦, 渡部, 豊喜, 山村, 一誠, 山内, 千里, 安田, 晃子, Kawada, Mitsunobu, Baba, Hajime, Barthel, Peter D., Clements, David, Cohen, Martin, Doi, Yasuo, Figueredo, Elysandra, Fujiwara, Mikio, Goto, Tomotsugu, Hasegawa, Sunao, Hibi, Yasunori, Hirao, Takanori, Hiromoto, Norihisa, Kaneda, Hidehiro, Kawai, Toshihide, Kawamura, Akiko, Kester, Do, Kii, Tsuneo, Kobayashi, Hisato, Kwon, Suk Minn, Lee, Hyung Mok, Makiuti, Sin'itirou, Matsuo, Hiroshi, Matsuura, Shuji, Muller, Thomas G., Murakami, Noriko, Nagata, Hirohisa, Nakagawa, Takao, Narita, Masanao, Noda, Manabu, Oh, Sang Hoon, Okada, Yoko, Okuda, Haruyuki, Oliver, Sebastian, Ootsubo, Takafumi, Pak, Soojong, Park, Yong-Sun, Pearson, Chris P., Rowan-Robinson, Michael, Saito, Toshinobu, Salama, Alberto, Sato, Shinji, Savage, Richard S., Serjeant, Stephen, Shibai, Hiroshi, Shirahata, Mai, Sohn, Jungjoo, Suzuki, Toyoaki, Takagi, Toshinobu, Takahashi, Hidenori, Thomson, Matthew, Usui, Fumihiko, Verdugo, Eva, Watabe, Toyoki, White, Glenn J., Wang, Lingyu, Yamamura, Issei, Yamauchi, Chisato, and Yasuda, Akiko

Abstract

著者人数: 60名

Published
2015

23. Improvement of the ASCA Position Accuracy

Author

上田, 佳宏, 井上, 一, 小川原, 嘉明, 藤本, 龍一, 山岡, 和貴, 紀伊, 恒男, Gotthelf, E. V., Ueda, Yoshihiro, Inoue, Hajime, Ogawara, Yoshiaki, Fujimoto, Ryuichi, Yamaoka, Kazutaka, Kii, Tsuneo, 上田, 佳宏, 井上, 一, 小川原, 嘉明, 藤本, 龍一, 山岡, 和貴, 紀伊, 恒男, Gotthelf, E. V., Ueda, Yoshihiro, Inoue, Hajime, Ogawara, Yoshiaki, Fujimoto, Ryuichi, Yamaoka, Kazutaka, and Kii, Tsuneo

Published
2015

24. Discovery of a Prominent Cyclotron Absorption Feature from the Transient X-Ray Pulsar X 0331+53

Author

牧島, 一夫, 三原, 建弘, 石田, 学, 大橋, 隆哉, 坂尾, 太郎, 田代, 信, 鶴, 剛, 紀伊, 恒男, 槙野, 文命, 村上, 敏夫, 長瀬, 文昭, 田中, 靖郎, 國枝, 秀世, 田原, 譲, 北本, 俊二, 宮本, 重徳, 吉田, 篤正, Turner, M. J. L., Makishima, Kazuo, Mihara, Tatehiro, Ishida, Manabu, Ohashi, Takaya, Sakao, Taro, Tashiro, Makoto, Tsuru, Takeshi, Kii, Tsuneo, Makino, Fumiyoshi, Murakami, Toshio, Nagase, Fumiaki, Tanaka, Yasuo, Kunieda, Hideyo, Tawara, Yuzuru, Kitamoto, Shunji, Miyamoto, Sigenori, Yoshida, Atsumasa, 牧島, 一夫, 三原, 建弘, 石田, 学, 大橋, 隆哉, 坂尾, 太郎, 田代, 信, 鶴, 剛, 紀伊, 恒男, 槙野, 文命, 村上, 敏夫, 長瀬, 文昭, 田中, 靖郎, 國枝, 秀世, 田原, 譲, 北本, 俊二, 宮本, 重徳, 吉田, 篤正, Turner, M. J. L., Makishima, Kazuo, Mihara, Tatehiro, Ishida, Manabu, Ohashi, Takaya, Sakao, Taro, Tashiro, Makoto, Tsuru, Takeshi, Kii, Tsuneo, Makino, Fumiyoshi, Murakami, Toshio, Nagase, Fumiaki, Tanaka, Yasuo, Kunieda, Hideyo, Tawara, Yuzuru, Kitamoto, Shunji, Miyamoto, Sigenori, and Yoshida, Atsumasa

Abstract

著者人数: 18名, Note: Accepted for publication in The Astrophysical Journal (Letters)

Published
2015

25. X-Ray Continuum and Evidence for an Iron Emission Line from the Quasar E 1821+643

Author

紀伊, 恒男, Williams, O. R., 大橋, 隆哉, 粟木, 久光, 林田, 清, 井上, 一, 近藤, 秀治, 小山, 勝二, 槙野, 文命, 牧島, 一夫, Saxton, R. D., Stewart, G. C., 高野, 史郎, 田中, 靖郎, Turner, M. J. L., Kii, Tsuneo, Ohashi, Takaya, Awaki, Hisamitsu, Hayashida, Kiyoshi, Inoue, Hajime, Kondo, Hideji, Koyama, Katsuji, Makino, Fumiyoshi, Makishima, Kazuo, Takano, Shirou, Tanaka, Yasuo, 紀伊, 恒男, Williams, O. R., 大橋, 隆哉, 粟木, 久光, 林田, 清, 井上, 一, 近藤, 秀治, 小山, 勝二, 槙野, 文命, 牧島, 一夫, Saxton, R. D., Stewart, G. C., 高野, 史郎, 田中, 靖郎, Turner, M. J. L., Kii, Tsuneo, Ohashi, Takaya, Awaki, Hisamitsu, Hayashida, Kiyoshi, Inoue, Hajime, Kondo, Hideji, Koyama, Katsuji, Makino, Fumiyoshi, Makishima, Kazuo, Takano, Shirou, and Tanaka, Yasuo

Abstract

著者人数: 15名, Note: Accepted for publication in The Astrophysical Journal on July 24, 1990. To appear in the February 1, 1991 issue.

Published
2015

26. Spin-Down of the X-ray Pulsar GX 1+4 During an Extended Low State

Author

牧島, 一夫, 大橋, 隆哉, 坂尾, 太郎, 堂谷, 忠靖, 井上, 一, 小山, 勝二, 槙野, 文命, 満田, 和久, 長瀬, 文昭, Thomas, H. D., Turner, M. J. L., 紀伊, 恒男, 田原, 譲, Makishima, Kazuo, Ohashi, Takaya, Sakao, Taro, Dotani, Tadayasu, Inoue, Hajime, Koyama, Katsuji, Makino, Fumiyoshi, Mitsuda, Kazuhisa, Nagase, Fumiaki, Kii, Tsuneo, Tawara, Yuzuru, 牧島, 一夫, 大橋, 隆哉, 坂尾, 太郎, 堂谷, 忠靖, 井上, 一, 小山, 勝二, 槙野, 文命, 満田, 和久, 長瀬, 文昭, Thomas, H. D., Turner, M. J. L., 紀伊, 恒男, 田原, 譲, Makishima, Kazuo, Ohashi, Takaya, Sakao, Taro, Dotani, Tadayasu, Inoue, Hajime, Koyama, Katsuji, Makino, Fumiyoshi, Mitsuda, Kazuhisa, Nagase, Fumiaki, Kii, Tsuneo, and Tawara, Yuzuru

Abstract

著者人数: 13名, Note: submitted to Nature on 23 Dec. 1987.

Published
2015

27. Antenna Deploy Experiment of Scientific Satellite HALCA

Author

HIROSAWA, Haruto, NATORI, Michihiro, KII, Tsuneo, TAKANO, Tadashi, HASHIMOTO, Tatsuaki, OHNISHI, Akira, INOUE, Kouzaburo, MURATA, Yasuhiro, MIYOSHI, Kazuo, INOUE, Toshio, NODA, Takahiko, KURIBAYASHI, Yutaka, TAJIMA, Takanori, KONDOH, Kumiko, SASAKI, Takashi, YANAI, Hideo, HAGINO, Shinji, OGURA, Naoto, OKAMOTO, Akira, SUGIYAMA, Shohtaro, and NAKAGAWA, Eiji

Subjects
軌道上実験, 展開型アンテナ, 電波天文衛星, アンテナ展開, 科学衛星
Abstract

科学衛星「はるか」は, スポース VLBI に必要な工学諸技術の実験ならびにスペース VLBI による電波天文観測を行うことを目的として, 1997年2月12日, 宇宙科学研究所の新型ロケット M-V の初号機により打ち上げられた。「はるか」では数々の工学的課題への取り組みがなされたが, それらの中で, ケーブルとメッシュからなる, 有効開口径8cmのパラボラアンテナの軌道上での展開が, 最大の工学的課題であった。打ち上げ約2週間後の2月24日から28日にかけてアンテナ展開実験を行い, 展開に成功した。本稿は「はるか」のアンテナ展開実験を, 衛星システム全体としてのオペレーションの観点から詳述するものである。, The paper describes details of the antenna deploy experiment of the scientific satellite HALCA conducted on 24 to 28,February 1997. HALCA was launched on 12 February 1997 by the ISAS's new rocket M-V for the purpose of engineering experiments on the technologies necessary for space VLBI and radio astronomical observations by space VLBI. HALCA has been designed as an orbiting radio telescope, and deployment of a parabolic antenna with an effective aperture diameter of 8 meters, the aperture of which is made of molybdenum mesh and a tremendous number of cables, was the largest engineering challenge in the HALCA's engineering experiments. The deploy of the antenna was successfully conducted following an operational sequence carefully of the antenna was successfully conducted following an operational sequence carefully designed and prepared. The success of the antenna deployment has opened a way towards the successful space VLBI experiments that HALCA has conducted since the first reception of a signal from a celestial radio source on 24 March 1997., 資料番号: SA0165948000

Published
1998

28. Sky surveys withASCA — Deep Sky Survey

Author

Miyaji, T., Hasinger, G., Ogasaka, Y., Kii, Tsuneo, Ueda, Yoshihiro, Takahashi, Tadayuki, Inoue, Hajime, Ishisaki, Y., Ohta, K., Yamada, T., and Makishima, K.

Subjects
Physics, Astrophysics::High Energy Astrophysical Phenomena, media_common.quotation_subject, Astrophysics::Instrumentation and Methods for Astrophysics, Cosmic background radiation, Astronomy, Astronomy and Astrophysics, Astrophysics::Cosmology and Extragalactic Astrophysics, Astrophysics, Space and Planetary Science, Sky, medicine, medicine.symptom, Astrophysics::Galaxy Astrophysics, Confusion, media_common
Abstract

著者人数：11名, 資料番号: SA1002268000

Published
1998

30. Evidence of Ionized Iron Emission Line from the Radio Quiet Quasar E 1821+643 by ASCA

Author

Yamashita, Akiko, Matsumoto, Chiho, Ishida, Manabu, Inoue, Hajime, Kii, Tsuneo, Makishima, Kazuo, Takahashi, Tadayuki, and Tashiro, Makoto

Subjects
Astrophysics::Instrumentation and Methods for Astrophysics, Computer Science::Digital Libraries
Abstract

Note: To appear in the Astrophysical Journal, vol. 486, 資料番号: SA8000272000

Published
1997

31. スロースピン衛星に作用する重力傾斜トルクと、その「あかり」衛星の姿勢復旧運用への適用

Author

Sakai, Shinichiro, Kawakatsu, Yasuhiro, Hashimoto, Tatsuaki, Yamamura, Issei, Kii, Tsuneo, and Murakami, Hiroshi

Abstract

第23回アストロダイナミクスシンポジウム (2013年7月29-45日. 宇宙航空研究開発機構宇宙科学研究所(JAXA)(ISAS)), 相模原市, 神奈川県, The 23rd Workshop on JAXA Astrodynamics and Flight Mechanics 2013 (July 29-30, 2013. Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency (JAXA)(ISAS)), Sagamihara, Kanagawa Japan, 資料番号: SA6000040015, レポート番号: A-15

Published
2013

33. ASCA Observation of X-ray/TeV Flare from the BL Lac Object Mkn 421

Author

Madejski, G., Takahashi, Tadayuki, Tashiro, Makoto, Kubo, Hidetoshi, Kamae, T., Kataoka, Jun, Kii, Tsuneo, Makino, Fumiyoshi, Makishima, Kazuo, and Yamasaki, Noriko

Subjects
Astrophysics::Instrumentation and Methods for Astrophysics, Computer Science::Digital Libraries
Abstract

Note: to be published in Astrophysical Journal Letter, 1996, 資料番号: SA8000299000

Published
1996

34. ASCA Observation of X-ray/TeV Flare from Mkn 421

Author

Madejski, G., Takahashi, Tadayuki, Kataoka, Jun, Kii, Tsuneo, Kubo, Hidetoshi, Makino, Fumiyoshi, Makishima, Kazuo, Tashiro, Makoto, and Yamasaki, Noriko

Abstract

Note: to be published in Proceedings of "Multifrequency Behaviour of High Energy Cosmic Sources", 1995, May 22-27, Vulcano, Italy (Mem. Soc. Astron. Ital.), 資料番号: SA8000306000

Published
1996

35. 高精度大型宇宙構造システムの開発研究:高精度を指向した材料開発の取り組み

Author

Goto, Ken, Kobayashi, Satoshi, Ueda, Masahito, Iwata, Minoru, Yokozeki, Tomohiro, Naito, Kimiyoshi, Kogo, Yasuo, Koyama, Masashi, Kii, Tsuneo, Yoshihara, Keisuke, Koyanagi, Jun, Ogasawara, Toshio, Ishizawa, Junichiro, and Kamiya, Tomohiro

Abstract

第12回宇宙科学シンポジウム (2012年1月5日-6日. 宇宙航空研究開発機構宇宙科学研究所(JAXA)(ISAS)相模原キャンパス), 相模原市, 神奈川県, 12th Space Science Symposium (January 5-6, 2012. Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency(JAXA)(ISAS)Sagamihara Campus), Sagamihara, Kanagawa Japan, 著者人数: 14名, 資料番号: SA6000064303, レポート番号: P5-042

Published
2012

36. Feasibility study on ASTRO-G observation signal system

Author

Kono, Yusuke, Suzuki, Shunsaku, Bushimata, Takeshi, Kawaguchi, Noriyuki, Yoshihara, Keisuke, Ogushi, Yoshio, Takashima, Takeshi, Hirose, Kazuyuki, Ikeda, Masahiko, Mizuta, Eiichi, Murata, Yasuhiro, Nishibori, Toshiyuki, Asaki, Yoshiharu, and Kii, Tsuneo

Abstract

第11回宇宙科学シンポジウム (2011年1月5日-7日. 宇宙航空研究開発機構宇宙科学研究所相模原キャンパス), 相模原市, 神奈川県, 11th Space Science Symposium (January 5-7, 2011. Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency), Sagamihara, Kanagawa Japan, 形態: カラー図版あり, 形態: CD-ROM1枚, 著者人数: 14人, Physical characteristics: Original contains color illustrations, Note: One CD-ROM, Number of authors: 14, 資料番号: AA0065426113

Published
2011

37. ASTRO-G: Comprehensive evaluation of LDR

Author

Ishimura, Kosei, Kii, Tsuneo, Komatsu, Keiji, Goto, Ken, Murata, Yasuhiro, Iwata, Takahiro, Asaki, Yoshiharu, Doi, Akihiro, Higuchi, Ken, and Hagino, Shinji

Abstract

第11回宇宙科学シンポジウム (2011年1月5日-7日. 宇宙航空研究開発機構宇宙科学研究所相模原キャンパス), 相模原市, 神奈川県, 11th Space Science Symposium (January 5-7, 2011. Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency), Sagamihara, Kanagawa Japan, 形態: カラー図版あり, 形態: CD-ROM1枚, 著者人数: 14人, Physical characteristics: Original contains color illustrations, Note: One CD-ROM, Number of authors: 14, 資料番号: AA0065426110

Published
2011

38. ASTRO-G: EM tests of LDR

Author

ASTRO-G技術研究チーム, Komatsu, Keiji, Kii, Tsuneo, Goto, Ken, Ishimura, Kosei, Higuchi, Ken, Yoshihara, Makoto, Iikura, Shoichi, Matsumoto, Kazuro, and ASTRO-G research team

Abstract

第11回宇宙科学シンポジウム (2011年1月5日-7日. 宇宙航空研究開発機構宇宙科学研究所相模原キャンパス), 相模原市, 神奈川県, 11th Space Science Symposium (January 5-7, 2011. Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency), Sagamihara, Kanagawa Japan, 形態: カラー図版あり, 形態: CD-ROM1枚, Physical characteristics: Original contains color illustrations, Note: One CD-ROM, 資料番号: AA0065426111

Published
2011

39. Technology demonstration for ASTRO-G

Author

Mitsuda, Kazuhisa, Kii, Tsuneo, Yoshihara, Keisuke, Murata, Yasuhiro, Saito, Hirobumi, Komatsu, Keiji, Tsuboi, Masato, Sakai, Shinichiro, Takeuchi, Hiroshi, and Mochizuki, Nanako

Abstract

第11回宇宙科学シンポジウム (2011年1月5日-7日. 宇宙航空研究開発機構宇宙科学研究所相模原キャンパス), 相模原市, 神奈川県, 11th Space Science Symposium (January 5-7, 2011. Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency), Sagamihara, Kanagawa Japan, 形態: カラー図版あり, 形態: CD-ROM1枚, 著者人数: 11人, Physical characteristics: Original contains color illustrations, Note: One CD-ROM, Number of authors: 11, 資料番号: AA0065426108

Published
2011

40. Summary and present status of ASTRO-G project

Author

ASTROG プロジェクトチーム, Saito, Hirobumi, Tsuboi, Masato, Mitsuda, Kazuhisa, Kii, Tsuneo, Yoshihara, Keisuke, Murata, Yasuhiro, and ASTRO-G project team

Abstract

第10回宇宙科学シンポジウム (2010年1月7日-8日. 宇宙航空研究開発機構宇宙科学研究本部), 10th Space Science Symposium (January 7-8, 2010. Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency (JAXA)), Sagamihara, Kanagawa Japan, 形態: カラー図版あり, 形態: CD-ROM1枚, 著者名の誤記: 紀伊, 恒夫, Physical characteristics: Original contains color illustrations, Note: One CD-ROM, 資料番号: AA0064742049

Published
2010

41. X-Ray Spectra of Bright Core-Dominant Quasars: NRAO 140 and 4C 34.47

Author

Turner, M. J. L., Williams, O. R., Ohashi, T., Tashiro, Makoto, Makishima, Kazuo, Kii, Tsuneo, and Makino, Fumiyoshi

Subjects
Astrophysics::Instrumentation and Methods for Astrophysics, Computer Science::Digital Libraries
Abstract

Note: Accepted for publication in The Astrophysical Journal., 資料番号: SA8000384000

Published
1992

42. The space infrared telescope for cosmology and astrophysics: SPICA A joint mission between JAXA and ESA

Author

SWINYARD, Bruce, NAKAGAWA, Takao, MERKEN, Patrick, ROYER, Pierre, SOUVERIJNS, Tim, VANDENBUSSCHE, Bart, WAELKENS, Christoffel, DAVIS, Peter, DI FRANCESCO, James, HALPERN, Mark, HOUDE, Martin, JOHNSTONE, Doug, JONCAS, Gilles, NAYLOR, David, PLUME, Rene, SCOTT, Douglas, ABERGEL, A., BENSAMMAR, S., BRAINE, J., BUAT, V., BURGARELLA, D., CAIS, Ph., DOLE, H., DUBAND, L., ELBAZ, D., GERIN, M., GIARD, M., GOICOECHEA, J., JOBLIN, C., JONES, A., KNEIB, J. P., LAGACHE, Guilaine, MADDEN, S., PONS, R., PAJOT, F., RAMBAUD, D., RAVERA, L., RISTORCELLI, I., RODRIGUEZ, L., VIVES, S., ZAVAGNO, Annie, GEIS, Norbert, KRAUSE, Oliver, LUTZ, Dieter, POGLITSCH, Albrecht, RAAB, Walfried, STEGMAIER, Jutta, STURM, Eckhard, TUFFS, Richard, LEE, Hyung Mok, KOO, Bon-Chul, IM, Myungshin, PAK, Soojong, HAN, Wonyong, PARK, Jang-Hyun, NAM, Uk-Won, JIN, Ho, LEE, Dae-Hee, YUK, In-Soo, LEE, Sungho, AIKAWA, Yuri, ARIMOTO, Nobuo, DOI, Yasuo, ENYA, Keigo, FUKAGAWA, Misato, FURUSHO, Reiko, HASEGAWA, Sunao, HAYASHI, Masahiko, HONDA KANAGAWA, Mitsuhiko, IDA, Shigeru, IMANISHI, MASATOSHI, INUTSUKA, Shu-Ichiro, IZUMIURA, Hideyuki, KAMAYA, Hideyuki, KANEDA, Hidehiro, KASUGA, Toshihiro, KATAZA, Hirokazu, KAWABATA, Koji, KAWADA, Mitsunobu, KAWAKITA, Hideyo, KII, Tsuneo, KODA, Jin, KODAMA, Tadayuki, KOKUBO, Eiichiro, KOMATSU, Keiji, MATSUHARA, Hideo, MATSUMOTO, Toshio, MATSUURA, Shuji, MIYATA, Takashi, MIYATA, Murakam, NAGATA, Hirohisa, NAGATA, Tetsuya, NAKAJIMA, Tadashi, NAOTO, Kobayashi, NISHI, Ryoichi, NODA, Atsushi, OKAMOTO, Atsushi, OKAMOTO, Yoshiko K., OMUKAI, Kazuyuki, ONAKA, Takashi, OOTSUBO, Takafumi, OUCHI, Masami, SAITO, Hirobumi, SATO, Yoichi, SAKO, Shigeyuki, SEKIGUCHI, Tomohiko, SHIBAI, Hiroshi, SUGITA, Hiroyuki, SUGITANI, Koji, SUSA, Hajime, PYO, Tae-Soo, TAMURA, Motohide, UEDA, Yoshihiro, UENO, Munetaka, WADA, Takehiko, WATANABE, Jun'Ichi, YAMADA, Toru, YAMAMURA, Issei, YOSHIDA, Naoki, YOSHIMI, Kitamura, YUI, Yukari, BENEDETTINI, Milena, CERULLI, Riccardo, DI GIORGIO, Anna, MOLINARI, Sergio, ORFEI, Renato, PEZZUTO, Stefano, PIAZZO, Lorenzo, SARACENO, Paolo, SPINOGLIO, Luigi, DE GRAAUW, Thijs, DE KORTE, Piet, HELMICH, Frank, HOEVERS, Henk, HUISMAN, Robert, SHIPMAN, Russell, VAN DER TAK, Floris, VAN DER WERF, Paul, WILD, Wolfgang, ACOSTA-PULIDO, Jose, CERNICHARO, Jose, HERREROS, Jose, MARTIN-PINTADO, Jesus, NAJARRO, Francisco, PEREZ-FOURMON, Ismael, RAMON PARDO, Juan, GOMEZ, Francisca, CASTRO RODRIGUEZ, Nieves, ADE, Peter, BARLOW, Mike, CLEMENTS, David, FERLET, Marc, FRASER, Helen, GRIFFIN, Douglas, GRIFFIN, Matthew, HARGRAVE, Peter, ISAAK, Kate, IVISON, Robert, MANSOUR, Malik, LANIESSE, Jonathan, MAUSKOPF, Phillip, MOROZOV, Dmitry, OLIVER, Seb, ORLANDO, Angiola, PAGE, Mathew, POPESCU, Cristina, SERJEANT, Stephen, SUDIWALA, Rashmi, RIGOPOULOU, Dimitra, WALKER, Ian, WHITE, Glenn, VITI, Serena, WINTER, Berend, BOCK, Jamie, BRADFORD, Matt, HARWIT, Martin, HOLMES, Warren, Institut Méditerranéen d'Ecologie et de Paléoécologie (IMEP), Université Paul Cézanne - Aix-Marseille 3-Centre National de la Recherche Scientifique (CNRS)-Avignon Université (AU)-Université de Provence - Aix-Marseille 1, Institute of Atomic Physics, Université de Roumanie, Groundwater Tracing Unit, Department of Geological Sciences, School of Environmental Sciences [Norwich], University of East Anglia [Norwich] (UEA), Institut de Recherche en Immunologie et en Cancérologie [UdeM-Montréal] (IRIC), Université de Montréal (UdeM), Department of Zoology, University of Otago [Dunedin, Nouvelle-Zélande], Transplantation Biology Group, Imperial College London, Institut d'astrophysique spatiale (IAS), Université Paris-Sud - Paris 11 (UP11)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), Observatoire de Paris - Site de Paris (OP), Centre National de la Recherche Scientifique (CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Institut national des sciences de l'Univers (INSU - CNRS), FORMATION STELLAIRE 2009, Laboratoire d'astrodynamique, d'astrophysique et d'aéronomie de bordeaux (L3AB), Université Sciences et Technologies - Bordeaux 1-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Université Sciences et Technologies - Bordeaux 1-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Observatoire aquitain des sciences de l'univers (OASU), Université Sciences et Technologies - Bordeaux 1-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Centre National de la Recherche Scientifique (CNRS)-Laboratoire d'Astrophysique de Bordeaux [Pessac] (LAB), Université de Bordeaux (UB)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Université de Bordeaux (UB), Laboratoire d'Astrophysique de Marseille (LAM), Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Aix Marseille Université (AMU)-Centre National d'Études Spatiales [Toulouse] (CNES), Laboratoire d'Etude du Rayonnement et de la Matière en Astrophysique (LERMA), École normale supérieure - Paris (ENS Paris), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université de Cergy Pontoise (UCP), Université Paris-Seine-Université Paris-Seine-Centre National de la Recherche Scientifique (CNRS), Laboratoire de Radioastronomie (LRA), Fédération de recherche du Département de physique de l'Ecole Normale Supérieure - ENS Paris (FRDPENS), Centre National de la Recherche Scientifique (CNRS)-École normale supérieure - Paris (ENS Paris), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-École normale supérieure - Paris (ENS Paris), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL), Processus mentaux et activation cérébrale, Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-IFR19-Institut National de la Santé et de la Recherche Médicale (INSERM), IFR des neurosciences de Lyon (IFNL), Centre National de la Recherche Scientifique (CNRS)-Institut National de la Santé et de la Recherche Médicale (INSERM)-Centre Hospitalier le Vinatier [Bron]-Hospices Civils de Lyon (HCL)-Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon, Centre d'étude spatiale des rayonnements (CESR), Observatoire Midi-Pyrénées (OMP), Météo France-Centre National d'Études Spatiales [Toulouse] (CNES)-Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Météo France-Centre National d'Études Spatiales [Toulouse] (CNES)-Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Toulouse III - Paul Sabatier (UT3), Université Fédérale Toulouse Midi-Pyrénées, British Antarctic Survey (BAS), Natural Environment Research Council (NERC), Department of Radio and Space Science [Göteborg], Chalmers University of Technology [Göteborg], Laboratoire Astrophysique de Toulouse-Tarbes (LATT), Centre National de la Recherche Scientifique (CNRS)-Observatoire Midi-Pyrénées (OMP), Météo France-Centre National d'Études Spatiales [Toulouse] (CNES)-Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Météo France-Centre National d'Études Spatiales [Toulouse] (CNES)-Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Toulouse III - Paul Sabatier (UT3), Services communs OMP (UMS 831), Université Toulouse III - Paul Sabatier (UT3), Université Fédérale Toulouse Midi-Pyrénées-Université Fédérale Toulouse Midi-Pyrénées-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire Midi-Pyrénées (OMP), Météo France-Centre National d'Études Spatiales [Toulouse] (CNES)-Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Météo France-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Centre National de la Recherche Scientifique (CNRS), Département d'Astrophysique, de physique des Particules, de physique Nucléaire et de l'Instrumentation Associée (DAPNIA), Commissariat à l'énergie atomique et aux énergies alternatives (CEA), Solar Influences Data Analysis Center [Brussels] (SIDC), Royal Observatory of Belgium [Brussels] (ROB), Propriétés Optiques des Matériaux et Applications (POMA), Centre National de la Recherche Scientifique (CNRS)-Université d'Angers (UA), Franche-Comté Électronique Mécanique, Thermique et Optique - Sciences et Technologies (UMR 6174) (FEMTO-ST), Université de Technologie de Belfort-Montbeliard (UTBM)-Ecole Nationale Supérieure de Mécanique et des Microtechniques (ENSMM)-Université de Franche-Comté (UFC), Université Bourgogne Franche-Comté [COMUE] (UBFC)-Université Bourgogne Franche-Comté [COMUE] (UBFC)-Centre National de la Recherche Scientifique (CNRS), Observatoire Astronomique de Marseille Provence (OAMP), Université de Provence - Aix-Marseille 1-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), Department of Physiology, The University of Hong Kong (HKU), School of Environmental Systems Engineering (SESE), The University of Western Australia (UWA), Centre for Water Research (CWR), Macaulay Institute, Centre Science des Matériaux et des Structures (SMS-ENSMSE), École des Mines de Saint-Étienne (Mines Saint-Étienne MSE), Institut Mines-Télécom [Paris] (IMT)-Institut Mines-Télécom [Paris] (IMT), Département Mécanique et Procédés d'Elaboration (MPE-ENSMSE), Institut Mines-Télécom [Paris] (IMT)-Institut Mines-Télécom [Paris] (IMT)-SMS, Department of Obstetrics and Gynecology [Stanford], Stanford Medicine, Stanford University-Stanford University, Korea Astronomy and Space Science Institute (KASI), Okayama University, Jack Baskin School of Engineering (UCSC), University of California [Santa Cruz] (UCSC), University of California-University of California, Adobe Systems Inc. (Adobe Advanced Technology Labs), Adobe Systems Inc., Defence Evaluation and Research Agency (DERA), Ministry of Defence (UK) (MOD)-Propulsion and Performance Department, Centre for Air Transport and the Environment (CATE), Manchester Metropolitan University (MMU), Department of Chemistry, Williams Hall-Kent State University, School of Earth and Atmospheric Sciences [Atlanta], Georgia Institute of Technology [Atlanta], Department of Earth and Planetary Sciences [Kobe], Kobe University, National Institute of Agro-Environmental Sciences (NIAES), Department of Earth System Science and Technology [Fukuoka] (ESST), Kyushu University [Fukuoka], Tokyo Institute of Technology [Tokyo] (TITECH), Department of Information and Communication Engineering, Graduate School of Information Science and Technology-The University of Tokyo (UTokyo), Department of Physics and Earth Sciences, University of the Ryukyus [Okinawa], Japan Agency for Marine-Earth Science and Technology (JAMSTEC), Center for Climate System Research [Kashiwa] (CCSR), The University of Tokyo (UTokyo), School of Humanities [Univ of Toyama], University of Toyama, Department of Mechanical System (Hiroshima University), Hiroshima University, High Temperature Plasma Center [Tokyo], Discrete Optimization Laboratory, Toyohashi University of Technology, Hatakeyama Laboratory, University of Electro-Communications [Tokyo] (UEC)-Tohoku University [Sendai], Institute of Industrial Science (IIS), Institut de génétique et biologie moléculaire et cellulaire (IGBMC), Université Louis Pasteur - Strasbourg I-Institut National de la Santé et de la Recherche Médicale (INSERM)-Centre National de la Recherche Scientifique (CNRS), Science and Technology Research Center (MCC), Mitsubishi Chemical Corporation, Institute for Solid State Physics [Tokyo] (ISSP), University of Electro-Communications [Tokyo] (UEC), Faculty of Science and Engineering [Waseda], Waseda University, Department of Civil Engineering, Chuo University (Chuo University), Frontier Collaborative Research Center (FCRC), Istituto di Fisica dello Spazio Interplanetario (IFSI), Consiglio Nazionale delle Ricerche (CNR), Antarctic Research a European Network for Astrophysics (ARENA), Institut de biologie et chimie des protéines [Lyon] (IBCP), Université de Lyon-Université de Lyon-Centre National de la Recherche Scientifique (CNRS), SRON Netherlands Institute for Space Research (SRON), Max-Planck-Institut für Radioastronomie (MPIFR), Departamento de Astrofísica Molecular e Infrarroja (DAMIR), Instituto de Estructura de la Materia (IEM), Consejo Superior de Investigaciones Científicas [Madrid] (CSIC)-Consejo Superior de Investigaciones Científicas [Madrid] (CSIC), Centro de Investigaciones Biológicas (CSIC), Consejo Superior de Investigaciones Científicas [Madrid] (CSIC), Laboratoire d'océanographie et de biogéochimie (LOB), Université de la Méditerranée - Aix-Marseille 2-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), Ecosystèmes Littoraux et Cotiers, Université de Lille, Sciences et Technologies-Centre National de la Recherche Scientifique (CNRS), Royal Observatory Edinburgh (ROE), University of Edinburgh, Processus d'Activation Sélective par Transfert d'Energie Uni-électronique ou Radiatif (UMR 8640) (PASTEUR), Université Pierre et Marie Curie - Paris 6 (UPMC)-Département de Chimie - ENS Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-École normale supérieure - Paris (ENS Paris), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Institut de Chimie du CNRS (INC)-Centre National de la Recherche Scientifique (CNRS), Ecole Supérieure des Affaires (ESA), Université Pierre Mendès France - Grenoble 2 (UPMF), Service de Neurologie [CHU Pitié-Salpêtrière], IFR70-CHU Pitié-Salpêtrière [AP-HP], Sorbonne Université (SU)-Assistance publique - Hôpitaux de Paris (AP-HP) (AP-HP)-Sorbonne Université (SU)-Assistance publique - Hôpitaux de Paris (AP-HP) (AP-HP), Neurologie et thérapeutique expérimentale, Institut National de la Santé et de la Recherche Médicale (INSERM)-IFR70-Université Pierre et Marie Curie - Paris 6 (UPMC), Department of Physics, University of Wales, Engineering Department, University of Cambridge [UK] (CAM), SLAC National Accelerator Laboratory (SLAC), Stanford University, Université Paul Cézanne - Aix-Marseille 3-Université de Provence - Aix-Marseille 1-Avignon Université (AU)-Centre National de la Recherche Scientifique (CNRS), Université Paris-Sud - Paris 11 (UP11)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Centre National d’Études Spatiales [Paris] (CNES), Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS), Université Sciences et Technologies - Bordeaux 1 (UB)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Université Sciences et Technologies - Bordeaux 1 (UB)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Observatoire aquitain des sciences de l'univers (OASU), Université Sciences et Technologies - Bordeaux 1 (UB)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Centre National de la Recherche Scientifique (CNRS)-Laboratoire d'Astrophysique de Bordeaux [Pessac] (LAB), Aix Marseille Université (AMU)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS), École normale supérieure - Paris (ENS-PSL), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-École normale supérieure - Paris (ENS-PSL), Université de Lyon-Université de Lyon-Hospices Civils de Lyon (HCL)-Centre Hospitalier le Vinatier [Bron]-Institut National de la Santé et de la Recherche Médicale (INSERM)-Centre National de la Recherche Scientifique (CNRS), Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire Midi-Pyrénées (OMP), Institut de Recherche pour le Développement (IRD)-Université Toulouse III - Paul Sabatier (UT3), Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France -Institut de Recherche pour le Développement (IRD)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France -Centre National de la Recherche Scientifique (CNRS), Université d'Angers (UA)-Centre National de la Recherche Scientifique (CNRS), Université de Technologie de Belfort-Montbeliard (UTBM)-Ecole Nationale Supérieure de Mécanique et des Microtechniques (ENSMM)-Centre National de la Recherche Scientifique (CNRS)-Université de Franche-Comté (UFC), Université Bourgogne Franche-Comté [COMUE] (UBFC)-Université Bourgogne Franche-Comté [COMUE] (UBFC), University of California [Santa Cruz] (UC Santa Cruz), University of California (UC)-University of California (UC), Kyushu University, Waseda University [Tokyo, Japan], National Research Council of Italy | Consiglio Nazionale delle Ricerche (CNR), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-École normale supérieure - Paris (ENS-PSL), CHU Pitié-Salpêtrière [AP-HP], Assistance publique - Hôpitaux de Paris (AP-HP) (AP-HP)-Sorbonne Université (SU), Université Pierre et Marie Curie - Paris 6 (UPMC)-IFR70-Institut National de la Santé et de la Recherche Médicale (INSERM), Institut de Recherche en Immunologie et en Cancérologie (IRIC), Université de Montréal [Montréal], PSL Research University (PSL)-PSL Research University (PSL)-Institut national des sciences de l'Univers (INSU - CNRS), École normale supérieure - Paris (ENS Paris)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université de Cergy Pontoise (UCP), Centre National de la Recherche Scientifique (CNRS)-École normale supérieure - Paris (ENS Paris)-Centre National de la Recherche Scientifique (CNRS)-École normale supérieure - Paris (ENS Paris), Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS), Services communs OMP - UMS 831 (UMS 831), Université Fédérale Toulouse Midi-Pyrénées-Université Fédérale Toulouse Midi-Pyrénées-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Université Toulouse III - Paul Sabatier (UT3), Royal Observatory of Belgium [Brussels], Université de Franche-Comté (UFC)-Centre National de la Recherche Scientifique (CNRS)-Ecole Nationale Supérieure de Mécanique et des Microtechniques (ENSMM)-Université de Technologie de Belfort-Montbeliard (UTBM), Division of Reproductive Biology, Stanford University [Stanford], Okayama University [Okayama], Graduate School of Information Science and Technology-The University of Tokyo, The University of Tokyo, Department of linguistic [Toyama], Consejo Superior de Investigaciones Científicas [Spain] (CSIC)-Consejo Superior de Investigaciones Científicas [Spain] (CSIC), Consejo Superior de Investigaciones Científicas [Spain] (CSIC), École normale supérieure - Paris (ENS Paris)-École normale supérieure - Paris (ENS Paris)-Centre National de la Recherche Scientifique (CNRS), Service de neurologie 1 [CHU Pitié-Salpétrière], Assistance publique - Hôpitaux de Paris (AP-HP) (APHP)-CHU Pitié-Salpêtrière [APHP], Stanford Linear Accelerator Center (SLAC), Astronomy, Institut de Recherche pour le Développement (IRD)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Université Fédérale Toulouse Midi-Pyrénées-Météo-France -Institut de Recherche pour le Développement (IRD)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France -Centre National de la Recherche Scientifique (CNRS), Assistance publique - Hôpitaux de Paris (AP-HP) (AP-HP)-Assistance publique - Hôpitaux de Paris (AP-HP) (AP-HP), The University of Tokyo (UTokyo)-Graduate School of Information Science and Technology, Assistance publique - Hôpitaux de Paris (AP-HP) (AP-HP)-CHU Pitié-Salpêtrière [AP-HP], and Assistance publique - Hôpitaux de Paris (AP-HP) (AP-HP)-Sorbonne Université (SU)-Sorbonne Université (SU)

Subjects
[SDU.ASTR.CO]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO], Infrared telescope, UNIVERSE, Astrophysics, Spica, Astrophysics::Cosmology and Extragalactic Astrophysics, POLYCYCLIC AROMATIC-HYDROCARBON, 7. Clean energy, 01 natural sciences, Space missions, Cosmology, Space exploration, law.invention, STAR-FORMATION, 010309 optics, Telescope, [PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO], Spitzer Space Telescope, law, 0103 physical sciences, 010303 astronomy & astrophysics, Astrophysics::Galaxy Astrophysics, Physics, Infrared astronomy, SPECTRUM, Spacecraft, [SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph], SUBMILLIMETER GALAXIES, business.industry, Astrophysics::Instrumentation and Methods for Astrophysics, Astronomy, Astronomy and Astrophysics, MODEL, SPITZER, PAHS, Space and Planetary Science, Infrared, Physics::Space Physics, IR, Astrophysics::Earth and Planetary Astrophysics, business, EMISSION
Abstract

International audience; The Space Infrared telescope for Cosmology and Astrophysics (SPICA) is planned to be the next space astronomy mission observing in the infrared. The mission is planned to be launched in 2017 and will feature a 3.5 m telescope cooled to 30 microns wavelength). We describe the scientific advances that will be made possible by this large increase in sensitivity and give details of the mission, spacecraft and focal plane conceptual design.

Published
2009

43. Discovery of a Prominent Cyclotron Absorption Feature from the Transient X-Ray Pulsar X 0331+53

Author

Turner, M. J. L., Makishima, Kazuo, Mihara, Tatehiro, Ishida, Manabu, Ohashi, Takaya, Sakao, Taro, Tashiro, Makoto, Tsuru, Takeshi, Kii, Tsuneo, Makino, Fumiyoshi, Murakami, Toshio, Nagase, Fumiaki, Tanaka, Yasuo, Kunieda, Hideyo, Tawara, Yuzuru, Kitamoto, Shunji, Miyamoto, Sigenori, and Yoshida, Atsumasa

Abstract

著者人数: 18名, Note: Accepted for publication in The Astrophysical Journal (Letters), 資料番号: SA8000434000

Published
1990

45. Multi-frequency Observation of Quasar 3C279 in the Outburst

Author

Turner, M. J. L., Sadun, A. C., Urry, C. M., Neugebauer, G., Matthews, K., Terasranta, H., Aller, M. F., Makino, Fumiyoshi, Kii, Tsuneo, Hayashida, Kiyoshi, and Ohashi, Takaya

Abstract

著者人数: 11名, Note: Presented at Georgia State University Conference on "Variability of Active Galactic Nuclei", May 2-4, 1990. Georgia State University in Atlanta., 資料番号: SA8000441000

Published
1990

47. Observations of the peculiar hard X-ray transient X0331 + 53 (V0332 + 53)

Author

Corbet, Robin H. D., Makishima, Kazuo, Ohashi, Takaya, Kawai, Nobuyuki, Matsuoka, Masaru, Koyama, Katsuji, Kunieda, Hideyo, Tawara, Yuzuru, Ushimaru, Naoko, Inoue, Hajime, Kii, Tsuneo, Makino, Fumiyoshi, Mitsuda, Kazuhisa, Murakami, Toshio, Nagase, Fumiak, Ogawara, Yoshiaki, Tanaka, Yasuo, Kitamoto, Shunji, Miyamoto, Shigenori, Tsunemi, Hiroshi, and Yamashita, Koujun

Abstract

著者人数：21名, Accepted: 1989-10-04, 資料番号: SA1001405000

Published
1990

48. X-Ray Continuum and Evidence for an Iron Emission Line from the Quasar E 1821+643

Author

Williams, O. R., Saxton, R. D., Stewart, G. C., Turner, M. J. L., Kii, Tsuneo, Ohashi, Takaya, Awaki, Hisamitsu, Hayashida, Kiyoshi, Inoue, Hajime, Kondo, Hideji, Koyama, Katsuji, Makino, Fumiyoshi, Makishima, Kazuo, Takano, Shirou, and Tanaka, Yasuo

Abstract

著者人数: 15名, Note: Accepted for publication in The Astrophysical Journal on July 24, 1990. To appear in the February 1, 1991 issue., 資料番号: SA8000443000

Published
1990

49. ASTRO-F - Super IRAS - The All Sky Infra-Red Survey

Author

Pearson, Chris P., Shibai, Hiroshi, Matsumoto, Toshio, Murakami, Hiroshi, Nakagawa, Takao, Kawada, Mitsunobu, Onaka, Takashi, Matsuhara, Hideo, Kii, Tsuneo, Yamamura, Issei, and Takagi, Toshinobu

Subjects
Physics, Infrared, media_common.quotation_subject, Astrophysics (astro-ph), FOS: Physical sciences, Astronomy and Astrophysics, Astrophysics, Redshift, Galaxy, Wavelength, Space and Planetary Science, Sky, Scale structure, Satellite, Photometric redshift, media_common
Abstract

著者人数：11名, Accepted: 2003-10-10, 資料番号: SA1001330000

Published
2002
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50. Multiwavelength Monitoring of the BL Lacertae Object PKS 2155-304 in May 1994. III. Probing the Inner Jet through Multiwavelength Correlations

Author

Urry, C. Megan, Treves, Aldo, Maraschi, Laura, Marshall, Herman L., Madejski, Greg, Penton, Steve, Pesce, Joseph E., Pian, Elena, Celotti, Annalisa, Sambruna, R. M., Shull, J. M., Smith, Paul S., Kii, Tsuneo, Fujimoto, Ryuichi, Makino, Fumiyoshi, Otani, Chiko, Sasaki, Koichi, Takahashi, Tadayuki, and Tashiro, M.

Subjects
PKS 2155-304, Physics, Astrophysics::High Energy Astrophysical Phenomena, Astrophysics (astro-ph), FOS: Physical sciences, Astronomy and Astrophysics, Astrophysics, Light curve, law.invention, Wavelength, Amplitude, Space and Planetary Science, law, ROSAT, Astrophysics::Solar and Stellar Astrophysics, Blazar, BL Lac object, Flare
Abstract

著者人数：19名, Accepted: 1997-04-21, 資料番号: SA1002215000

Published
1997

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