{"created":"2023-06-20T14:38:42.999381+00:00","id":5307,"links":{},"metadata":{"_buckets":{"deposit":"48e1a04d-8d8e-41c3-a1bf-248499ba30ce"},"_deposit":{"created_by":1,"id":"5307","owners":[1],"pid":{"revision_id":0,"type":"depid","value":"5307"},"status":"published"},"_oai":{"id":"oai:jaxa.repo.nii.ac.jp:00005307","sets":["1887:1891","9:789:956:959"]},"author_link":["25685","25724","25699","25716","25717","25709","25683","25712","25686","25727","25703","25680","25698","25700","25715","25693","25713","25710","25714","25691","25675","25702","25682","25706","25723","25705","25722","25708","25695","25725","25681","25677","25674","25687","25679","25696","25694","25688","25707","25721","25692","25676","25678","25726","25718","25684","25704","25697","25690","25711","25720","25701","25719","25689"],"item_5_biblio_info_10":{"attribute_name":"書誌情報","attribute_value_mlt":[{"bibliographicIssueDates":{"bibliographicIssueDate":"2009-02-27","bibliographicIssueDateType":"Issued"},"bibliographicPageEnd":"361","bibliographicPageStart":"356","bibliographicVolumeNumber":"JAXA-SP-08-014E","bibliographic_titles":[{"bibliographic_title":"宇宙航空研究開発機構特別資料"},{"bibliographic_title":"JAXA Special Publication: Astrophysics with All-Sky X-Ray observations: 3rd International MAXI Workshop","bibliographic_titleLang":"en"}]}]},"item_5_description_15":{"attribute_name":"会議概要(会議名, 開催地, 会期, 主催者等)(英)","attribute_value_mlt":[{"subitem_description":"Astrophysics with All-Sky X-Ray observations: 3rd International MAXI Workshop (RIKEN, 10-12 June 2008)","subitem_description_type":"Other"}]},"item_5_description_17":{"attribute_name":"抄録(英)","attribute_value_mlt":[{"subitem_description":"ASTRO-H, the new Japanese X-ray Astronomy Satellite following Suzaku, is an international X-ray mission which is currently planed for launch in 2013. ASTRO-H is a combination of wide band X-ray spectroscopy (3 - 80 keV) provided by multi-layer coating, focusing hard X-ray mirrors and hard X-ray imaging detectors, and high energy-resolution soft X-ray spectroscopy (0.3 - 10 keV) provided by thin-foil X-ray optics and a micro-calorimeter array. The mission will also carry an X-ray CCD camera as a focal plane detector for a soft X-ray telescope and a non-focusing soft gamma-ray detector. With these instruments, ASTRO-H covers very wide energy range from 0.3 keV to 600 keV. The micro-calorimeter system will be developed by international collaboration lead by lSAS/JAXA and NASA. The simultaneous broad bandpass, coupled with high spectral resolution of delta.E ca. 7 eV by the micro-calorimeter will enable a wide variety of important science themes to be pursued.","subitem_description_type":"Other"}]},"item_5_description_32":{"attribute_name":"資料番号","attribute_value_mlt":[{"subitem_description":"資料番号: AA0064306068","subitem_description_type":"Other"}]},"item_5_description_33":{"attribute_name":"レポート番号","attribute_value_mlt":[{"subitem_description":"レポート番号: JAXA-SP-08-014E","subitem_description_type":"Other"}]},"item_5_publisher_8":{"attribute_name":"出版者","attribute_value_mlt":[{"subitem_publisher":"宇宙航空研究開発機構"}]},"item_5_publisher_9":{"attribute_name":"出版者(英)","attribute_value_mlt":[{"subitem_publisher":"Japan Aerospace Exploration Agency 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