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<title>Materiały konferencyjne | Conference Proceedings</title>
<link>http://hdl.handle.net/11089/1106</link>
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<dc:date>2026-04-08T12:53:07Z</dc:date>
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<item rdf:about="http://hdl.handle.net/11089/40125">
<title>Classification of Dermatological Asymmetry of the Skin Lesions using Pretrained Convolutional Neural Networks</title>
<link>http://hdl.handle.net/11089/40125</link>
<description>Classification of Dermatological Asymmetry of the Skin Lesions using Pretrained Convolutional Neural Networks
Beczkowski, Michał; Borowski, Norbert; Milczarski, Piotr
International Conference on Artificial Intelligence and Soft Computing.
</description>
<dc:date>2021-01-01T00:00:00Z</dc:date>
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<item rdf:about="http://hdl.handle.net/11089/38965">
<title>A need for eye lens dosimetry in nuclear medicine</title>
<link>http://hdl.handle.net/11089/38965</link>
<description>A need for eye lens dosimetry in nuclear medicine
Wrzesień, Małgorzata; Albiniak, Łukasz; Królicki, L.; Olszewski, J.
Background: Changing the individual dose limit for the lens of the eye from a value of 150 mSv per year to&#13;
a level of 20 mSv (averaged over defined periods of five years or 50 mSv in a single year) means that issues related to&#13;
routine eye lens dosimetry become interesting from the point of view of radiation protection. This could mean that the&#13;
dosimeter designed to measure the doses at the level of the eye lens may become the next dosimeter routinely worn by&#13;
nuclear medicine workers occupationally exposed to ionising radiation. The dosimeters currently used in nuclear&#13;
medicine are the personal dosimeter and the ring dosimeter. Will this also be the case for nuclear medicine&#13;
employees? In this interdisciplinary branch of medicine, the factors that cause the highest risk of radiation exposure&#13;
of personnel are the process of manual handling, i.e. the process of preparing a radiopharmaceutical called labelling.&#13;
Most of the radiopharmaceuticals used in nuclear medicine are labelled manually. In Poland, the exception from this&#13;
rule is when radiopharmaceuticals are produced for the needs of positron emission tomography (PET), which are&#13;
labelled using automatic processes. Manual procedures also include the process of radiopharmaceutical injection to&#13;
the patients. The aim of the work was to assess the exposure of eye lenses of workers in nuclear medicine, as well as of&#13;
the personnel in centers that produce radiopharmaceuticals for PET diagnostics, from the viewpoint of advisability of&#13;
routine eye lens exposure monitoring, taking into account changes in the dose limit for the lens of the eye. Methods:&#13;
The results of own measurements of the personal dose equivalent Hp(3), carried out in five nuclear medicine&#13;
departments in Poland, as well as in two centers producing radiopharmaceuticals for PET, were subject to analysis.&#13;
The analysis includes two most frequently used radionuclides for diagnostic purposes, namely 99mTc, 18F and the less&#13;
frequently used 68Ga, in addition to 131I, which is used for therapeutic purposes. Dosimetric measurements were made&#13;
using thermoluminescent detectors of domestic manufacture. Results &amp; Conclusions: Estimated analysis of the annual&#13;
exposure makes it possible to indicate cases where the maximum annual value of personal dose equivalent, in terms&#13;
of Hp(3), exceeds threefold the new limit value specified at 20 mSv/year.
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<dc:date>2019-01-01T00:00:00Z</dc:date>
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<item rdf:about="http://hdl.handle.net/11089/22938">
<title>X-ray/γ-ray Correlation in Seyfert 2 Galaxy NGC 4945</title>
<link>http://hdl.handle.net/11089/22938</link>
<description>X-ray/γ-ray Correlation in Seyfert 2 Galaxy NGC 4945
Wojaczyński, Rafał; Niedźwiecki, Andrzej
Aharonian, Felix A.; Hofmann, Werner; Rieger, Frank M.
We report the correlation between the X-ray and γ-ray emission found in our analysis of the Fermi/LAT and Swift/BAT data from 8 years of observations of the nearby Seyfert 2 galaxy NGC 4945. Using the BAT light-curves we determined summed periods of low and high X-ray flux and we found that the average γ-ray spectrum is harder in the latter (higher X-ray flux level), with the difference of the γ-ray spectral index of ~0.4. The correlation indicates that the γ-rays are produced in the active nucleus of this Seyfert galaxy rather than by cosmic rays interacting with the interstellar medium (as assumed in the alternative starburst model). We compare NGC 4945 with two other γ-ray loud galaxies showing both starburst and AGN activities, NGC 1068 and Circinus.
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<dc:date>2017-01-04T00:00:00Z</dc:date>
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