X-ray polarimetry small satellite TSUBAME
'TSUBAME' is a university-built small satellite mission to measure polarization of hard X-ray photons (30-100 keV) from Gamma-ray bursts (GRBs) using azimuthal angle anisotropy of Compton-scattered photons. Polarimetry in the hard X-ray and soft g-ray band plays a crucial role in the under...
Gespeichert in:
| Hauptverfasser: | , , , , , , , , , , , , , , , , , , |
|---|---|
| Format: | Tagungsbericht |
| Sprache: | eng |
| Online-Zugang: | Volltext |
| Tags: |
Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
|
| container_end_page | 610 |
|---|---|
| container_issue | |
| container_start_page | 607 |
| container_title | |
| container_volume | 1000 |
| creator | Arimoto, Makoto Tsubuku, Yoshihiro Toizumi, Takahiro Kobayashi, Mitsuyoshi Yatsu, Yoichi Shimokawabe, Takashi Kataoka, Jun Kawai, Nobuyuki Omagari, Kuniyuki Fujiwara, Ken Konda, Yasumi Tanaka, Yohei Maeno, Masaki Yamanaka, Tomio Ashida, Hiroki Nishida, Junichi Fujihashi, Kouta Ikeda, Takuro Inagawa, Shinichi |
| description | 'TSUBAME' is a university-built small satellite mission to measure polarization of hard X-ray photons (30-100 keV) from Gamma-ray bursts (GRBs) using azimuthal angle anisotropy of Compton-scattered photons. Polarimetry in the hard X-ray and soft g-ray band plays a crucial role in the understanding of high energy emission mechanisms and the distribution of magnetic fields and radiation fields. TSUBAME has two instruments: the Wide-field Bust Monitor (WBM) and the Hard X-ray Compton Polarimeter (HXCP). The WBM determines on board the direction of the burst occurrence with an accuracy of 10 degrees, then using a high speed attitude control device, the HXCP is pointed to the GRB within 10 seconds after the burst occurrence to promptly detect polarized X-ray photons from the GRB.We present a TSUBAME mission overview, results of a Monte Carlo simulation of the X-ray polarization measurement and the plans for the future of this mission. |
| doi_str_mv | 10.1063/1.2943543 |
| format | Conference Proceeding |
| fullrecord | <record><control><sourceid>proquest</sourceid><recordid>TN_cdi_proquest_miscellaneous_33541442</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>33541442</sourcerecordid><originalsourceid>FETCH-LOGICAL-n265t-c817c0bc5215e13a73cfd74e2a019389c3e11f444fac16056580e45965c2e98b3</originalsourceid><addsrcrecordid>eNotj81KAzEURgMqWGsXvsGsBBdT7829mSTLWuoPVFzYQncljXdgJNOpk-mib29BV99ZHc6n1B3CFKGiR5xqz2SYLtTEWwf2zGCI9KUaAXguNdPmWt3k_A2gvbVupB42ZR9OxaFLoW9aGfpTkduQUpHDICk1gxSrz_XT7H1xq67qkLJM_nes1s-L1fy1XH68vM1ny3KvKzOU0aGNsItGoxGkYCnWX5ZFB0BPzkcSxJqZ6xCxAlMZB8LGVyZq8W5HY3X_5z303c9R8rBtmxzPLWEv3TFv6fwKmTX9AiZkQog</addsrcrecordid><sourcetype>Aggregation Database</sourcetype><iscdi>true</iscdi><recordtype>conference_proceeding</recordtype><pqid>33541442</pqid></control><display><type>conference_proceeding</type><title>X-ray polarimetry small satellite TSUBAME</title><source>AIP Journals Complete</source><creator>Arimoto, Makoto ; Tsubuku, Yoshihiro ; Toizumi, Takahiro ; Kobayashi, Mitsuyoshi ; Yatsu, Yoichi ; Shimokawabe, Takashi ; Kataoka, Jun ; Kawai, Nobuyuki ; Omagari, Kuniyuki ; Fujiwara, Ken ; Konda, Yasumi ; Tanaka, Yohei ; Maeno, Masaki ; Yamanaka, Tomio ; Ashida, Hiroki ; Nishida, Junichi ; Fujihashi, Kouta ; Ikeda, Takuro ; Inagawa, Shinichi</creator><creatorcontrib>Arimoto, Makoto ; Tsubuku, Yoshihiro ; Toizumi, Takahiro ; Kobayashi, Mitsuyoshi ; Yatsu, Yoichi ; Shimokawabe, Takashi ; Kataoka, Jun ; Kawai, Nobuyuki ; Omagari, Kuniyuki ; Fujiwara, Ken ; Konda, Yasumi ; Tanaka, Yohei ; Maeno, Masaki ; Yamanaka, Tomio ; Ashida, Hiroki ; Nishida, Junichi ; Fujihashi, Kouta ; Ikeda, Takuro ; Inagawa, Shinichi</creatorcontrib><description>'TSUBAME' is a university-built small satellite mission to measure polarization of hard X-ray photons (30-100 keV) from Gamma-ray bursts (GRBs) using azimuthal angle anisotropy of Compton-scattered photons. Polarimetry in the hard X-ray and soft g-ray band plays a crucial role in the understanding of high energy emission mechanisms and the distribution of magnetic fields and radiation fields. TSUBAME has two instruments: the Wide-field Bust Monitor (WBM) and the Hard X-ray Compton Polarimeter (HXCP). The WBM determines on board the direction of the burst occurrence with an accuracy of 10 degrees, then using a high speed attitude control device, the HXCP is pointed to the GRB within 10 seconds after the burst occurrence to promptly detect polarized X-ray photons from the GRB.We present a TSUBAME mission overview, results of a Monte Carlo simulation of the X-ray polarization measurement and the plans for the future of this mission.</description><identifier>ISSN: 0094-243X</identifier><identifier>ISBN: 9780735405332</identifier><identifier>ISBN: 0735405336</identifier><identifier>DOI: 10.1063/1.2943543</identifier><language>eng</language><ispartof>Gamma-Ray Bursts 2007: Proceedings of the Santa Fe Conference (AIP Conference Proceedings Volume 1000), 2008, Vol.1000, p.607-610</ispartof><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>314,776,780,27901,27902</link.rule.ids></links><search><creatorcontrib>Arimoto, Makoto</creatorcontrib><creatorcontrib>Tsubuku, Yoshihiro</creatorcontrib><creatorcontrib>Toizumi, Takahiro</creatorcontrib><creatorcontrib>Kobayashi, Mitsuyoshi</creatorcontrib><creatorcontrib>Yatsu, Yoichi</creatorcontrib><creatorcontrib>Shimokawabe, Takashi</creatorcontrib><creatorcontrib>Kataoka, Jun</creatorcontrib><creatorcontrib>Kawai, Nobuyuki</creatorcontrib><creatorcontrib>Omagari, Kuniyuki</creatorcontrib><creatorcontrib>Fujiwara, Ken</creatorcontrib><creatorcontrib>Konda, Yasumi</creatorcontrib><creatorcontrib>Tanaka, Yohei</creatorcontrib><creatorcontrib>Maeno, Masaki</creatorcontrib><creatorcontrib>Yamanaka, Tomio</creatorcontrib><creatorcontrib>Ashida, Hiroki</creatorcontrib><creatorcontrib>Nishida, Junichi</creatorcontrib><creatorcontrib>Fujihashi, Kouta</creatorcontrib><creatorcontrib>Ikeda, Takuro</creatorcontrib><creatorcontrib>Inagawa, Shinichi</creatorcontrib><title>X-ray polarimetry small satellite TSUBAME</title><title>Gamma-Ray Bursts 2007: Proceedings of the Santa Fe Conference (AIP Conference Proceedings Volume 1000)</title><description>'TSUBAME' is a university-built small satellite mission to measure polarization of hard X-ray photons (30-100 keV) from Gamma-ray bursts (GRBs) using azimuthal angle anisotropy of Compton-scattered photons. Polarimetry in the hard X-ray and soft g-ray band plays a crucial role in the understanding of high energy emission mechanisms and the distribution of magnetic fields and radiation fields. TSUBAME has two instruments: the Wide-field Bust Monitor (WBM) and the Hard X-ray Compton Polarimeter (HXCP). The WBM determines on board the direction of the burst occurrence with an accuracy of 10 degrees, then using a high speed attitude control device, the HXCP is pointed to the GRB within 10 seconds after the burst occurrence to promptly detect polarized X-ray photons from the GRB.We present a TSUBAME mission overview, results of a Monte Carlo simulation of the X-ray polarization measurement and the plans for the future of this mission.</description><issn>0094-243X</issn><isbn>9780735405332</isbn><isbn>0735405336</isbn><fulltext>true</fulltext><rsrctype>conference_proceeding</rsrctype><creationdate>2008</creationdate><recordtype>conference_proceeding</recordtype><recordid>eNotj81KAzEURgMqWGsXvsGsBBdT7829mSTLWuoPVFzYQncljXdgJNOpk-mib29BV99ZHc6n1B3CFKGiR5xqz2SYLtTEWwf2zGCI9KUaAXguNdPmWt3k_A2gvbVupB42ZR9OxaFLoW9aGfpTkduQUpHDICk1gxSrz_XT7H1xq67qkLJM_nes1s-L1fy1XH68vM1ny3KvKzOU0aGNsItGoxGkYCnWX5ZFB0BPzkcSxJqZ6xCxAlMZB8LGVyZq8W5HY3X_5z303c9R8rBtmxzPLWEv3TFv6fwKmTX9AiZkQog</recordid><startdate>20080101</startdate><enddate>20080101</enddate><creator>Arimoto, Makoto</creator><creator>Tsubuku, Yoshihiro</creator><creator>Toizumi, Takahiro</creator><creator>Kobayashi, Mitsuyoshi</creator><creator>Yatsu, Yoichi</creator><creator>Shimokawabe, Takashi</creator><creator>Kataoka, Jun</creator><creator>Kawai, Nobuyuki</creator><creator>Omagari, Kuniyuki</creator><creator>Fujiwara, Ken</creator><creator>Konda, Yasumi</creator><creator>Tanaka, Yohei</creator><creator>Maeno, Masaki</creator><creator>Yamanaka, Tomio</creator><creator>Ashida, Hiroki</creator><creator>Nishida, Junichi</creator><creator>Fujihashi, Kouta</creator><creator>Ikeda, Takuro</creator><creator>Inagawa, Shinichi</creator><scope>7U5</scope><scope>8FD</scope><scope>L7M</scope></search><sort><creationdate>20080101</creationdate><title>X-ray polarimetry small satellite TSUBAME</title><author>Arimoto, Makoto ; Tsubuku, Yoshihiro ; Toizumi, Takahiro ; Kobayashi, Mitsuyoshi ; Yatsu, Yoichi ; Shimokawabe, Takashi ; Kataoka, Jun ; Kawai, Nobuyuki ; Omagari, Kuniyuki ; Fujiwara, Ken ; Konda, Yasumi ; Tanaka, Yohei ; Maeno, Masaki ; Yamanaka, Tomio ; Ashida, Hiroki ; Nishida, Junichi ; Fujihashi, Kouta ; Ikeda, Takuro ; Inagawa, Shinichi</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-n265t-c817c0bc5215e13a73cfd74e2a019389c3e11f444fac16056580e45965c2e98b3</frbrgroupid><rsrctype>conference_proceedings</rsrctype><prefilter>conference_proceedings</prefilter><language>eng</language><creationdate>2008</creationdate><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Arimoto, Makoto</creatorcontrib><creatorcontrib>Tsubuku, Yoshihiro</creatorcontrib><creatorcontrib>Toizumi, Takahiro</creatorcontrib><creatorcontrib>Kobayashi, Mitsuyoshi</creatorcontrib><creatorcontrib>Yatsu, Yoichi</creatorcontrib><creatorcontrib>Shimokawabe, Takashi</creatorcontrib><creatorcontrib>Kataoka, Jun</creatorcontrib><creatorcontrib>Kawai, Nobuyuki</creatorcontrib><creatorcontrib>Omagari, Kuniyuki</creatorcontrib><creatorcontrib>Fujiwara, Ken</creatorcontrib><creatorcontrib>Konda, Yasumi</creatorcontrib><creatorcontrib>Tanaka, Yohei</creatorcontrib><creatorcontrib>Maeno, Masaki</creatorcontrib><creatorcontrib>Yamanaka, Tomio</creatorcontrib><creatorcontrib>Ashida, Hiroki</creatorcontrib><creatorcontrib>Nishida, Junichi</creatorcontrib><creatorcontrib>Fujihashi, Kouta</creatorcontrib><creatorcontrib>Ikeda, Takuro</creatorcontrib><creatorcontrib>Inagawa, Shinichi</creatorcontrib><collection>Solid State and Superconductivity Abstracts</collection><collection>Technology Research Database</collection><collection>Advanced Technologies Database with Aerospace</collection></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Arimoto, Makoto</au><au>Tsubuku, Yoshihiro</au><au>Toizumi, Takahiro</au><au>Kobayashi, Mitsuyoshi</au><au>Yatsu, Yoichi</au><au>Shimokawabe, Takashi</au><au>Kataoka, Jun</au><au>Kawai, Nobuyuki</au><au>Omagari, Kuniyuki</au><au>Fujiwara, Ken</au><au>Konda, Yasumi</au><au>Tanaka, Yohei</au><au>Maeno, Masaki</au><au>Yamanaka, Tomio</au><au>Ashida, Hiroki</au><au>Nishida, Junichi</au><au>Fujihashi, Kouta</au><au>Ikeda, Takuro</au><au>Inagawa, Shinichi</au><format>book</format><genre>proceeding</genre><ristype>CONF</ristype><atitle>X-ray polarimetry small satellite TSUBAME</atitle><btitle>Gamma-Ray Bursts 2007: Proceedings of the Santa Fe Conference (AIP Conference Proceedings Volume 1000)</btitle><date>2008-01-01</date><risdate>2008</risdate><volume>1000</volume><spage>607</spage><epage>610</epage><pages>607-610</pages><issn>0094-243X</issn><isbn>9780735405332</isbn><isbn>0735405336</isbn><abstract>'TSUBAME' is a university-built small satellite mission to measure polarization of hard X-ray photons (30-100 keV) from Gamma-ray bursts (GRBs) using azimuthal angle anisotropy of Compton-scattered photons. Polarimetry in the hard X-ray and soft g-ray band plays a crucial role in the understanding of high energy emission mechanisms and the distribution of magnetic fields and radiation fields. TSUBAME has two instruments: the Wide-field Bust Monitor (WBM) and the Hard X-ray Compton Polarimeter (HXCP). The WBM determines on board the direction of the burst occurrence with an accuracy of 10 degrees, then using a high speed attitude control device, the HXCP is pointed to the GRB within 10 seconds after the burst occurrence to promptly detect polarized X-ray photons from the GRB.We present a TSUBAME mission overview, results of a Monte Carlo simulation of the X-ray polarization measurement and the plans for the future of this mission.</abstract><doi>10.1063/1.2943543</doi><tpages>4</tpages><oa>free_for_read</oa></addata></record> |
| fulltext | fulltext |
| identifier | ISSN: 0094-243X |
| ispartof | Gamma-Ray Bursts 2007: Proceedings of the Santa Fe Conference (AIP Conference Proceedings Volume 1000), 2008, Vol.1000, p.607-610 |
| issn | 0094-243X |
| language | eng |
| recordid | cdi_proquest_miscellaneous_33541442 |
| source | AIP Journals Complete |
| title | X-ray polarimetry small satellite TSUBAME |
| url | https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-02-10T01%3A35%3A58IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-proquest&rft_val_fmt=info:ofi/fmt:kev:mtx:book&rft.genre=proceeding&rft.atitle=X-ray%20polarimetry%20small%20satellite%20TSUBAME&rft.btitle=Gamma-Ray%20Bursts%202007:%20Proceedings%20of%20the%20Santa%20Fe%20Conference%20(AIP%20Conference%20Proceedings%20Volume%201000)&rft.au=Arimoto,%20Makoto&rft.date=2008-01-01&rft.volume=1000&rft.spage=607&rft.epage=610&rft.pages=607-610&rft.issn=0094-243X&rft.isbn=9780735405332&rft.isbn_list=0735405336&rft_id=info:doi/10.1063/1.2943543&rft_dat=%3Cproquest%3E33541442%3C/proquest%3E%3Curl%3E%3C/url%3E&disable_directlink=true&sfx.directlink=off&sfx.report_link=0&rft_id=info:oai/&rft_pqid=33541442&rft_id=info:pmid/&rfr_iscdi=true |