Position resolution limits in pure noble gaseous detectors for X-ray energies from 1 to 60 keV
dc.contributor.author | Azevedo, C. D. R | |
dc.contributor.author | Correia, P. M. | |
dc.contributor.author | Silva, A. L. M | |
dc.contributor.author | Carramate, L. F. N. D. | |
dc.contributor.author | Veloso, J. F. C. A. | |
dc.contributor.buuauthor | Biagi, S. | |
dc.contributor.buuauthor | Veenhof, R. | |
dc.contributor.department | Uludağ Üniversitesi/Fen-Edebiyat Fakültesi/Fizik Bölümü. | tr_TR |
dc.contributor.orcid | 0000-0002-7085-7275 | tr_TR |
dc.contributor.scopusid | 57193398882 | tr_TR |
dc.contributor.scopusid | 6603742499 | tr_TR |
dc.date.accessioned | 2022-08-12T13:14:41Z | |
dc.date.available | 2022-08-12T13:14:41Z | |
dc.date.issued | 2015-02-04 | |
dc.description.abstract | The calculated position resolutions for X-ray photons (1-60 keV) in pure noble gases at atmospheric pressure are presented. In this work we show the influence of the atomic shells and the detector dimensions on the intrinsic position resolution of the used noble gas. The calculated results were obtained by using a new software tool, Degrad, and compared to the available experimental data. | en_US |
dc.description.sponsorship | European Commission (CERN/FP/123604/2011) | en_US |
dc.description.sponsorship | European Commission (PTDC/FIS/110925/2009) | en_US |
dc.description.sponsorship | COMPETE (CENTRO-07-ST24-FEDER-002030) | en_US |
dc.description.sponsorship | Portuguese Foundation for Science and Technology (SFRH/BPD/79163/2011) | en_US |
dc.description.sponsorship | Portuguese Foundation for Science and Technology (BD/52330/2013) | en_US |
dc.description.sponsorship | Portuguese Foundation for Science and Technology (SFRH/BD/71429/2010) | en_US |
dc.identifier.citation | Azevedo, C. D. R. vd. (2015). "Position resolution limits in pure noble gaseous detectors for X-ray energies from 1 to 60 keV". Physics Letters B, 714, 272-275. | en_US |
dc.identifier.endpage | 275 | tr_TR |
dc.identifier.issn | 0370-2693 | |
dc.identifier.issn | 1873-2445 | |
dc.identifier.scopus | 2-s2.0-84921369554 | tr_TR |
dc.identifier.startpage | 272 | tr_TR |
dc.identifier.uri | https://doi.org/10.1016/j.physletb.2014.12.054 | |
dc.identifier.uri | https://www.sciencedirect.com/science/article/pii/S0370269314009356 | |
dc.identifier.uri | http://hdl.handle.net/11452/28190 | |
dc.identifier.volume | 741 | tr_TR |
dc.identifier.wos | 000348290800043 | tr_TR |
dc.indexed.scopus | Scopus | en_US |
dc.indexed.wos | SCIE | en_US |
dc.language.iso | en | en_US |
dc.publisher | Elsevier | en_US |
dc.relation.collaboration | Yurt dışı | tr_TR |
dc.relation.journal | Physics Letters B | en_US |
dc.relation.publicationcategory | Makale - Uluslararası Hakemli Dergi | tr_TR |
dc.rights | info:eu-repo/semantics/openAccess | en_US |
dc.subject | Gaseous detectors | en_US |
dc.subject | Intrinsic position resolution | en_US |
dc.subject | X-rays | en_US |
dc.subject | Noble gas | en_US |
dc.subject | Astronomy & astrophysics | en_US |
dc.subject | Physics | en_US |
dc.subject.scopus | Gaseous Detectors; Photomultipliers; Detector | en_US |
dc.subject.wos | Astronomy & astrophysics | en_US |
dc.subject.wos | Physics, nuclear | en_US |
dc.subject.wos | Physics, particles & fields | en_US |
dc.title | Position resolution limits in pure noble gaseous detectors for X-ray energies from 1 to 60 keV | en_US |
dc.type | Article | |
dc.wos.quartile | Q1 | en_US |