A study of the pointed observation methods and sensitivity of HXMT
The Hard X-ray Modulation Telescope (HXMT) is an X-ray astronomy satellite consisting of three slat-collimated instruments, the High Energy X-ray Instrument (HE), the Medium Energy X-ray Instrument (ME), and the Low Energy X-ray Instrument (LE). HXMT will carry out an all sky survey and make pointed...
        Saved in:
      
    
          | Published in | Chinese physics C Vol. 34; no. 1; pp. 66 - 71 | 
|---|---|
| Main Author | |
| Format | Journal Article | 
| Language | English | 
| Published | 
            IOP Publishing
    
        2010
     Department of Engineering Physics, Tsinghua University, Beijing 100084, China Center for Astrophysics, Tsinghua University, Beijing 100084, China%Key Laboratory of Particle Astrophysics, Institute of High Energy Physics,Chinese Academy of Sciences, Beijing 100049, China%Department of Physics, Tsinghua University, Beijing 100084, China Center for Astrophysics, Tsinghua University, Beijing 100084, China Key Laboratory of Particle Astrophysics, Institute of High Energy  | 
| Subjects | |
| Online Access | Get full text | 
| ISSN | 1674-1137 0254-3052 2058-6132  | 
| DOI | 10.1088/1674-1137/34/1/012 | 
Cover
| Abstract | The Hard X-ray Modulation Telescope (HXMT) is an X-ray astronomy satellite consisting of three slat-collimated instruments, the High Energy X-ray Instrument (HE), the Medium Energy X-ray Instrument (ME), and the Low Energy X-ray Instrument (LE). HXMT will carry out an all sky survey and make pointed observations in the 1-250 keV energy band. In order to get the source and background fluxes simultaneously in the pointed observations, two methods, i.e., the combined field of view (FOV) method and the off-axis pointing method are proposed in this paper. Comprehensive analyses of the sensitivities of the three instruments by using these two methods are presented, respectively. It is found that the off-axis pointing method has a higher sensitivity for HE and ME but a lower sensitivity for LE. Since the axes of the three instruments are aligned along the same direction, the off-axis pointing method is recommended as the main method in the pointed observation for HXMT; the combined FOV method can be used when LE is the most relevant instrument in order to satisfy the scientific objective of the observation. | 
    
|---|---|
| AbstractList | O4; The Hard X-ray Modulation Telescope (HXMT) is an X-ray astronomy satellite consisting of three slat-collimated instruments, the High Energy X-ray Instrument (HE), the Medium Energy X-ray Instrument (ME), and the Low Energy X-ray Instrument (LE). HXMT will carry out an all sky survey and make pointed observations in the 1-250 keV energy band. In order to get the source and background fluxes simultaneously in the pointed observations, two methods, i.e., the combined field of view (FOV) method and the off-axis pointing method are proposed in this paper. Comprehensive analyses of the sensitivities of the three instruments by using these two methods are presented, respectively. It is found that the off-axis pointing method has a higher sensitivity for HE and ME but a lower sensitivity for LE. Since the axes of the three instruments are aligned along the same direction, the off-axis pointing method is recommended as the main method in the pointed observation for HXMT; the combined FOV method can be used when LE is the most relevant instrument in order to satisfy the scientific objective of the observation. The Hard X-ray Modulation Telescope (HXMT) is an X-ray astronomy satellite consisting of three slat-collimated instruments, the High Energy X-ray Instrument (HE), the Medium Energy X-ray Instrument (ME), and the Low Energy X-ray Instrument (LE). HXMT will carry out an all sky survey and make pointed observations in the 1-250 keV energy band. In order to get the source and background fluxes simultaneously in the pointed observations, two methods, i.e., the combined field of view (FOV) method and the off-axis pointing method are proposed in this paper. Comprehensive analyses of the sensitivities of the three instruments by using these two methods are presented, respectively. It is found that the off-axis pointing method has a higher sensitivity for HE and ME but a lower sensitivity for LE. Since the axes of the three instruments are aligned along the same direction, the off-axis pointing method is recommended as the main method in the pointed observation for HXMT; the combined FOV method can be used when LE is the most relevant instrument in order to satisfy the scientific objective of the observation.  | 
    
| Author | 金晶 陈勇 张双南 张澍 李新乔 李刚 | 
    
| AuthorAffiliation | Department of Engineering Physics, Tsinghua University, Beijing 100084, China Center for Astrophysics, Tsinghua University, Beijing 100084, China Key Laboratory of Particle Astrophysics, Institute of High Energy Physics Chinese Academy of Sciences, Beijing 100049, China Department of Physics, Tsinghua University, Beijing 100084, China | 
    
| AuthorAffiliation_xml | – name: Department of Engineering Physics, Tsinghua University, Beijing 100084, China;Center for Astrophysics, Tsinghua University, Beijing 100084, China%Key Laboratory of Particle Astrophysics, Institute of High Energy Physics,Chinese Academy of Sciences, Beijing 100049, China%Department of Physics, Tsinghua University, Beijing 100084, China;Center for Astrophysics, Tsinghua University, Beijing 100084, China;Key Laboratory of Particle Astrophysics, Institute of High Energy | 
    
| Author_xml | – sequence: 1 fullname: 金晶 陈勇 张双南 张澍 李新乔 李刚  | 
    
| BookMark | eNp9kMtOAjEUhhuDiYC-gKuJG-NinN7mwhKJignGDSbumk4vUIQWpwWCT-_AEE3UkJzkLM73ndP-HdCyzioALhG8RbAoEpTlNEaI5AmhCUogwiegDXFKYwJT3ALtb-AMdLyfQZjR2muDu37kw0puI6ejMFXR0hkblIxc6VW15sE4Gy1UmDrpI25l5JX1Jpi1CXtl-PY8Pgenms-9ujj0Lnh9uB8PhvHo5fFp0B_FguRFiInqaazTXChZ5KkWiCBdIk16mOYixQQqKXAvp1jJFFNRQsF7ivB6kGWplIp0wXWzd8Ot5nbCZm5V2foi-5xs5kxgiGBdCNckbkhROe8rpdmyMgtebRmCbJcX28XBdnEwUnfWSMUvSZiwDyBU3MyPqzeNatzy59Qfji2lrtn4H_bY7qvDs6bOTj5M_e-Si3dt5ooRnNGUUki-AGuhliQ | 
    
| CitedBy_id | crossref_primary_10_1016_j_nima_2019_02_024 crossref_primary_10_1007_s10509_020_03873_8 crossref_primary_10_1088_1674_4527_15_11_012 crossref_primary_10_11728_cjss2016_06_938 crossref_primary_10_1007_s10509_015_2559_1  | 
    
| Cites_doi | 10.1007/BF00462037 10.1086/305377  | 
    
| ClassificationCodes | O4 | 
    
| ContentType | Journal Article | 
    
| Copyright | Copyright © Wanfang Data Co. Ltd. All Rights Reserved. | 
    
| Copyright_xml | – notice: Copyright © Wanfang Data Co. Ltd. All Rights Reserved. | 
    
| DBID | 2RA 92L CQIGP W94 ~WA AAYXX CITATION 2B. 4A8 92I 93N PSX TCJ  | 
    
| DOI | 10.1088/1674-1137/34/1/012 | 
    
| DatabaseName | 中文期刊服务平台 中文科技期刊数据库-CALIS站点 维普中文期刊数据库 中文科技期刊数据库-自然科学 中文科技期刊数据库- 镜像站点 CrossRef Wanfang Data Journals - Hong Kong WANFANG Data Centre Wanfang Data Journals 万方数据期刊 - 香港版 China Online Journals (COJ) China Online Journals (COJ)  | 
    
| DatabaseTitle | CrossRef | 
    
| DatabaseTitleList | |
| DeliveryMethod | fulltext_linktorsrc | 
    
| Discipline | Physics | 
    
| DocumentTitleAlternate | A study of the pointed observation methods and sensitivity of HXMT | 
    
| EISSN | 0254-3052 2058-6132  | 
    
| EndPage | 71 | 
    
| ExternalDocumentID | zgwl_c201001012 10_1088_1674_1137_34_1_012 32645440  | 
    
| GrantInformation_xml | – fundername: Supported by National Basic Research Program of China.973 Program funderid: (2009CB824800)  | 
    
| GroupedDBID | 02O 1JI 1WK 29B 2B. 2C. 2RA 4.4 5B3 5GY 5VR 5VS 7.M 92E 92I 92L 92Q 93N AAGCD AAGID AAJIO AAJKP AALHV AAPBV AATNI ABCXL ABHWH ACAFW ACGFS ACHIP AENEX AFUIB AFYNE AIBLX AKPSB ALMA_UNASSIGNED_HOLDINGS ATQHT BBWZM CCEZO CCVFK CDYEO CEBXE CHBEP CJUJL CQIGP CRLBU CW9 DU5 EBS EDWGO EJD EPQRW EQZZN ER. FA0 FEDTE HVGLF IJHAN IOP IZVLO JCGBZ KNG KOT M45 N5L NT- NT. OK1 PJBAE Q02 RIN RNS RPA RW3 SY9 TCJ TGP W28 W94 ~WA PB6 UNR -SA -SC -S~ AAYXX ABJNI ADEQX AEINN AERVB AOAED CAJEA CAJEC CITATION Q-- ROL U1G U5K U5M 4A8 PSX  | 
    
| ID | FETCH-LOGICAL-c378t-3e9f2f57ced875fc131fb1f39247c5230edc29742ed524cb0ca9e3a230665dde3 | 
    
| IEDL.DBID | IOP | 
    
| ISSN | 1674-1137 | 
    
| IngestDate | Thu May 29 04:07:16 EDT 2025 Wed Oct 01 03:43:12 EDT 2025 Thu Apr 24 23:03:09 EDT 2025 Mon May 13 14:50:16 EDT 2019 Tue Nov 10 14:19:46 EST 2020 Thu Nov 24 20:32:04 EST 2022  | 
    
| IsPeerReviewed | true | 
    
| IsScholarly | true | 
    
| Issue | 1 | 
    
| Keywords | sensitivity off-axis pointed observation HXMT  | 
    
| Language | English | 
    
| LinkModel | DirectLink | 
    
| MergedId | FETCHMERGED-LOGICAL-c378t-3e9f2f57ced875fc131fb1f39247c5230edc29742ed524cb0ca9e3a230665dde3 | 
    
| Notes | 11-5641/O4 P145.3 HXMT, pointed observation, sensitivity, off-axis TH751  | 
    
| PageCount | 6 | 
    
| ParticipantIDs | crossref_primary_10_1088_1674_1137_34_1_012 iop_primary_10_1088_1674_1137_34_1_012 crossref_citationtrail_10_1088_1674_1137_34_1_012 wanfang_journals_zgwl_c201001012 chongqing_backfile_32645440  | 
    
| ProviderPackageCode | CITATION AAYXX  | 
    
| PublicationCentury | 2000 | 
    
| PublicationDate | 2010 20100101 2010-01-00  | 
    
| PublicationDateYYYYMMDD | 2010-01-01 | 
    
| PublicationDate_xml | – year: 2010 text: 2010  | 
    
| PublicationDecade | 2010 | 
    
| PublicationTitle | Chinese physics C | 
    
| PublicationTitleAlternate | Chinese Physica C | 
    
| PublicationTitle_FL | CHINESE PHYSICS C | 
    
| PublicationYear | 2010 | 
    
| Publisher | IOP Publishing Department of Engineering Physics, Tsinghua University, Beijing 100084, China Center for Astrophysics, Tsinghua University, Beijing 100084, China%Key Laboratory of Particle Astrophysics, Institute of High Energy Physics,Chinese Academy of Sciences, Beijing 100049, China%Department of Physics, Tsinghua University, Beijing 100084, China Center for Astrophysics, Tsinghua University, Beijing 100084, China Key Laboratory of Particle Astrophysics, Institute of High Energy  | 
    
| Publisher_xml | – name: IOP Publishing – name: Department of Engineering Physics, Tsinghua University, Beijing 100084, China – name: Center for Astrophysics, Tsinghua University, Beijing 100084, China%Key Laboratory of Particle Astrophysics, Institute of High Energy Physics,Chinese Academy of Sciences, Beijing 100049, China%Department of Physics, Tsinghua University, Beijing 100084, China – name: Center for Astrophysics, Tsinghua University, Beijing 100084, China – name: Key Laboratory of Particle Astrophysics, Institute of High Energy  | 
    
| References | Li Ti-Pei (1) 2006; 26 4 Li Ti-Pei (2) 1994; 215 Rothschild R E (3) 1998; 496  | 
    
| References_xml | – volume: 215 start-page: 213 issn: 0748-6375 year: 1994 ident: 2 publication-title: ApSS – volume: 26 start-page: 30 issn: 0254-6124 year: 2006 ident: 1 publication-title: Chin. J. Space Sci – ident: 4 doi: 10.1007/BF00462037 – volume: 496 start-page: 538 issn: 0004-637X year: 1998 ident: 3 publication-title: The Astro-physical J. doi: 10.1086/305377  | 
    
| SSID | ssj0064088 | 
    
| Score | 1.7999914 | 
    
| Snippet | The Hard X-ray Modulation Telescope (HXMT) is an X-ray astronomy satellite consisting of three slat-collimated instruments, the High Energy X-ray Instrument... O4; The Hard X-ray Modulation Telescope (HXMT) is an X-ray astronomy satellite consisting of three slat-collimated instruments, the High Energy X-ray...  | 
    
| SourceID | wanfang crossref iop chongqing  | 
    
| SourceType | Aggregation Database Enrichment Source Index Database Publisher  | 
    
| StartPage | 66 | 
    
| SubjectTerms | X射线仪器 X射线天文卫星 低能量 敏感性分析 灵敏度 硬X射线调制望远镜  | 
    
| Title | A study of the pointed observation methods and sensitivity of HXMT | 
    
| URI | http://lib.cqvip.com/qk/92043A/20101/32645440.html http://iopscience.iop.org/1674-1137/34/1/012 https://d.wanfangdata.com.cn/periodical/zgwl-c201001012  | 
    
| Volume | 34 | 
    
| hasFullText | 1 | 
    
| inHoldings | 1 | 
    
| isFullTextHit | |
| isPrint | |
| journalDatabaseRights | – providerCode: PRVIOP databaseName: IOP Science Platform customDbUrl: eissn: 0254-3052 dateEnd: 99991231 omitProxy: false ssIdentifier: ssj0064088 issn: 1674-1137 databaseCode: IOP dateStart: 20080101 isFulltext: true titleUrlDefault: https://iopscience.iop.org/ providerName: IOP Publishing  | 
    
| link | http://utb.summon.serialssolutions.com/2.0.0/link/0/eLvHCXMwjV3fa9swED7SwKAvXdutNEtbRCl9GU4sS_6Rx3QshELWPrSQN2Gfpayk2NmSMshfvzvbCSsdJU825mThk3x3ku6-D-BKY26DwFLkFiXK085KL4ul9bIkDa3LJErkeufJj2j8qG-n4bQFGyq5p3LRWP4e3dYn-VGsPSlV3Fe6L_t-RSnMjp-r9e7uN2Y30n5FMrkVbypk6Ol_XsFICj_LYvaL_MMrj7RH3Vb1O4VLi9k_rmb0ESabgp06w2Tee1llPVy_xW_c6SsO4aCJOcWwniRH0LLFMXyocj9x-QluhqICmRWlExQOikXJGBK5KLPtjq2oiaaXIi1yseSc95p0gpuMp5OHz_A4-v7wbew11AoeqjhZecoOXODCGG1OCxaHUkkaGEfBko6RN4ptjgEtNQKbh4HGzMd0YFXK65UoJIuoTqBdlIU9BeHILMgoyKNB6nSc-Km1jKDjh75EjELsQHeranLNOGfAKUNRow619jsgN8o32KCSMznGs6lOx5PEsOYMa84ouhrSXAe-btssakyOd6WvaRB2Erx8JfhGwCxy1wHRzA3T_OxLs579eTbIaQUM2Bd82bXDLuzXuQi8oXMG7dXvF3tOIc4qu6im9l9K0-w7 | 
    
| linkProvider | IOP Publishing | 
    
| linkToPdf | http://utb.summon.serialssolutions.com/2.0.0/link/0/eLvHCXMwpV3dT9swED8NJqa9sDGGVtiHNU17QWni2E7SR_ZRlTEYDyDxZiUXu0igpNBWk_rX7y5JqzGmCWlPyYMvce6su7Pzu98BfNBYujh2lLklmQq0dzIoUumCIsuN84VEiVzvfHySjM71twuzRBM2tTD1pHP9fbptiYJbFXaAuCxk3HwgpUpDpUMZkocNJ6Vfg8dGmQE3MTj8cbp0xomOmtaTK5mububvz2F-hcu6Gt9Q1LgTp9ZoLk1VT-XzavxbABo-g2I59RZ3ctWfz4o-Lv5gdfyvb3sOm116Kg5agS145KoXsNHARHG6DZ8ORMNHK2ovKHMUk5rpJkpRF6vDXdH2pJ6KvCrFlOHxbX8KFhldHJ-9hPPh17PPo6DrwhCgSrNZoNzAx96k6Era23iUSpINPeVVOkU-U3YlxrQriV1pYo1FhPnAqZy3Nokh56l2YL2qK_cKhCcPIpO4TAa512kW5c4x2U5kIomYGOzB3kr_FMXxirmpLCWY2mgd9UAuLWKxIzDnPhrXtvmRnmWWtWdZe1bR1ZL2erC_kpm09B3_HP2RDPOgge_vDLw3wJLVeiC6BWM7vzC1i_HPa4uMQGBuv3j3oS98B09Ovwzt98OToz142iIY-BjoNazPbufuDSVGs-Jts_R_AfBt_Ck | 
    
| openUrl | ctx_ver=Z39.88-2004&ctx_enc=info%3Aofi%2Fenc%3AUTF-8&rfr_id=info%3Asid%2Fsummon.serialssolutions.com&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Ajournal&rft.genre=article&rft.atitle=A+study+of+the+pointed+observation+methods+and+sensitivity+of+HXMT&rft.jtitle=%E4%B8%AD%E5%9B%BD%E7%89%A9%E7%90%86C%EF%BC%88%E8%8B%B1%E6%96%87%E7%89%88%EF%BC%89&rft.au=JIN+Jing&rft.au=CHEN+Yong&rft.au=ZHANG+Shuang-Nan&rft.au=ZHANG+Shu&rft.date=2010&rft.pub=Department+of+Engineering+Physics%2C+Tsinghua+University%2C+Beijing+100084%2C+China&rft.issn=1674-1137&rft.volume=34&rft.issue=1&rft.spage=66&rft.epage=71&rft_id=info:doi/10.1088%2F1674-1137%2F34%2F1%2F012&rft.externalDocID=zgwl_c201001012 | 
    
| thumbnail_s | http://utb.summon.serialssolutions.com/2.0.0/image/custom?url=http%3A%2F%2Fimage.cqvip.com%2Fvip1000%2Fqk%2F92043A%2F92043A.jpg http://utb.summon.serialssolutions.com/2.0.0/image/custom?url=http%3A%2F%2Fwww.wanfangdata.com.cn%2Fimages%2FPeriodicalImages%2Fzgwl-c%2Fzgwl-c.jpg  |