Please use this identifier to cite or link to this item:
http://hdl.handle.net/20.500.12386/34706
DC Field | Value | Language |
---|---|---|
dc.contributor.author | SEGRETO, ALBERTO | en_US |
dc.date.accessioned | 2024-02-05T13:38:45Z | - |
dc.date.available | 2024-02-05T13:38:45Z | - |
dc.date.issued | 2004 | en_US |
dc.identifier.issn | 0277-786X | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/34706 | - |
dc.description.abstract | The IBIS instrument launched on board the ESA INTEGRAL observatory on October 2002 is a coded mask telescope composed by two position sensitive detection planes, one with 16384 Cadmium Telluride pixels (ISGRI) and the other with 4096 Caesium Iodide pixels (PICsIT). Events detected in coincidence in the two detector layers are flagged as generated by Compton scattered photons and can be then processed and filtered using the Compton kinematic equations. The analysis of these data is, however, quite complex, mainly due to the presence of a great number of fake events generated by random coincidences between uncorrelated ISGRI and PICsIT events; if this component is not subtracted with great accuracy, false source detections can be produced. In this work, we present the performance (spectral and imaging) obtainable from the IBIS Compton data, by analyzing ground calibration acquisitions. We also analyze the IBIS Compton flight data relative to the Crab observation, to determine its scientific capabilities. | en_US |
dc.language.iso | eng | en_US |
dc.title | Performance of the IBIS Compton mode | en_US |
dc.type | Conference paper | - |
dc.identifier.doi | 10.1117/12.554933 | en_US |
dc.identifier.scopus | 2-s2.0-10044296319 | en_US |
dc.identifier.url | https://api.elsevier.com/content/abstract/scopus_id/10044296319 | en_US |
dc.identifier.url | https://www.spiedigitallibrary.org/conference-proceedings-of-spie/5488/1/Performance-of-the-IBIS-Compton-mode/10.1117/12.554933.short | en_US |
dc.relation.medium | STAMPA | en_US |
dc.relation.volume | 5488 | en_US |
dc.relation.firstpage | 738 | en_US |
dc.relation.lastpage | 749 | en_US |
dc.type.referee | REF_3 | en_US |
dc.description.numberofauthors | 1 | en_US |
dc.description.international | no | en_US |
dc.contributor.country | ITA | en_US |
dc.relation.ispartofbook | UV and Gamma-Ray Space Telescope Systems | en_US |
dc.publisher.name | Bellingham, WA : SPIE, The International Society for Optical Engineering | en_US |
dc.type.invited | no | en_US |
dc.relation.conferencename | UV and Gamma-Ray Space Telescope Systems | en_US |
dc.relation.conferenceplace | Glasgow, Scotland, United Kingdom | en_US |
dc.relation.conferencedate | 21-25 June, 2004 | en_US |
dc.relation.scientificsector | FIS/05 - ASTRONOMIA E ASTROFISICA | en_US |
dc.type.miur | 273 Contributo in Atti di convegno | - |
dc.relation.series | PROCEEDINGS OF SPIE | en_US |
dc.identifier.adsbibcode | 2004SPIE.5488..738S | en_US |
dc.relation.ercsector | ERC sectors::Physical Sciences and Engineering | en_US |
dc.description.apc | no | en_US |
dc.description.oa | 1 – prodotto con file in versione Open Access (allegare il file al passo 5-Carica) | en_US |
item.cerifentitytype | Publications | - |
item.openairecristype | http://purl.org/coar/resource_type/c_18cf | - |
item.fulltext | With Fulltext | - |
item.grantfulltext | open | - |
item.languageiso639-1 | en | - |
item.openairetype | Conference paper | - |
crisitem.journal.journalissn | 0277-786X | - |
crisitem.journal.ance | E136238 | - |
crisitem.author.dept | IASF Palermo | - |
crisitem.author.orcid | 0000-0001-7341-6603 | - |
Appears in Collections: | 3.01 Contributi in Atti di convegno |
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Items in DSpace are published in Open Access, unless otherwise indicated.