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Please use this identifier to cite or link to this item: http://hdl.handle.net/10016/14662

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Title: Validation of NEMA NU4-2008 Scatter Fraction estimation with 18F and 68Ga for the ARGUS smallanimal PET scanner
Author(s): Vicente, Esther
Herraiz, J. L.
Cañadas, Mario
Cal-Gozález, Jacobo
España, Samuel
Desco, Manuel
Vaquero, Juan José
Udías, José Manuel
Publisher: IEEE
Issued date: 2010
Citation: 2010 IEEE Nuclear Science Symposium Conference Record (NSS/MIC), 2010. Pp. 3553 - 3557
URI: http://hdl.handle.net/10016/14662
ISBN: 978-1-4244-9106-3
ISSN: 1095-7863
DOI: 10.1109/NSSMIC.2010.5874470
Description: Proceeding of: 2010 IEEE Nuclear Science Symposium, Medical Imaging Conference, Knoxville, Tennessee, USA, October 30 - November 6, 2010
Abstract: The scatter fraction (SF) in PET data represents the fraction of coincidence events in which at least one of the two emitted photons have been scattered before being detected. It is usually estimated as the ratio of scattered events to total number of coincidences, when the number of random counts is negligible (less than 1% of true rates). SF provides a measurement of the relative sensitivity of the scanner to scattered radiation. It depends on object size, density and location inside the field of view, as well as on detector size, type of detector crystal and energy window. The performance evaluation guideline for smallanimal PET NEMA (National Electrical Manufacturers Association) NU4-2008 proposes the estimation of the SF for three test phantoms made in proportion to the most widely used small animals in the laboratory: mouse, rat and monkey. The method estimates the different coincidence types in sinogram profiles from an off-centered line source inserted in these phantoms. We benchmark the procedure proposed by NEMA to estimate SF with 18F and also with 68Ga, a radionuclide with lager positron range. Real data acquired with the ARGUS smallanimal PET scanner (SEDECAL, Madrid, Spain) as well as simulations of the same scanner with peneloPET are used. The results show that, though SF should be practically the same with both 18F and 68Ga isotopes (and indeed our simulations indicate this) NEMA SF estimations with 68Ga acquisitions are higher. This is due to the fact that 68Ga positron range affects on the width of the line source profiles. Suggestions to modify the protocol to obtain similar SF estimations when using isotopes with larger positron range than 18F are made.
Sponsor: This work has been supported by MEC (FPA2007-62216), UCM (Grupos UCM, 910059), CPAN (Consolider-Ingenio 2010) CSPD-2007-00042, European Regional Funds. AMIT Project funded by CDTI (CENIT Programme), ARTEMIS S2009/DPI-1802, European Regional Development and ENTEPRASE grant, PSE-300000-2009-5, Ministerio de Ciencia e Innovación. Spanish Government.
Publisher version: http://dx.doi.org/10.1109/NSSMIC.2010.5874470
Rights: © IEEE
Appears in Collections:DBIAB - Proceedings

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