Erratum: Study of gamma-ray emission by proton beam interaction with injected Boron atoms for future medical imaging applications

2017 ◽  
Vol 12 (04) ◽  
pp. E04001-E04001
Author(s):  
G Petringa ◽  
G.A.P Cirrone ◽  
C Caliri ◽  
G Cuttone ◽  
L Giuffrida ◽  
...  
2017 ◽  
Vol 12 (03) ◽  
pp. C03049-C03049 ◽  
Author(s):  
G. Petringa ◽  
G.A.P. Cirrone ◽  
C. Caliri ◽  
G. Cuttone ◽  
L. Giuffrida ◽  
...  

2021 ◽  
pp. 191-196
Author(s):  
V.V. Levenets ◽  
A.Yu. Lonin ◽  
O.P. Omelnik ◽  
A.O. Shchur

The low values of isotope effects in the sorption/decontamination processes make it possible to investigate the properties of the sorbing and decontaminating agents with the use of stable isotope simulators. In the work present-ed here the element content was determined from the characteristic X-ray emission induced by the proton beam (PIXE), by gamma-ray emission from the radioactive source, and by emission from the X-ray tube. Based on the results of efficiency determination for different kinds of sorbents and decontaminants, recommendations have been given for the choice of materials having the wanted performance characteristics.


2017 ◽  
Vol 33 ◽  
pp. 197-206 ◽  
Author(s):  
Melek Zarifi ◽  
Susanna Guatelli ◽  
David Bolst ◽  
Brian Hutton ◽  
Anatoly Rosenfeld ◽  
...  

1998 ◽  
Vol 502 (1) ◽  
pp. 428-436 ◽  
Author(s):  
Igor V. Moskalenko ◽  
Werner Collmar ◽  
Volker Schonfelder

2021 ◽  
pp. 109559
Author(s):  
R.F.P. Simões ◽  
C.J. da Silva ◽  
R.L. da Silva ◽  
L.V. de Sá ◽  
R. Poledna ◽  
...  

2018 ◽  
Vol 614 ◽  
pp. L1 ◽  
Author(s):  
A. Lähteenmäki ◽  
E. Järvelä ◽  
V. Ramakrishnan ◽  
M. Tornikoski ◽  
J. Tammi ◽  
...  

We have detected six narrow-line Seyfert 1 (NLS1) galaxies at 37 GHz that were previously classified as radio silent and two that were classified as radio quiet. These detections reveal the presumption that NLS1 galaxies labelled radio quiet or radio silent and hosted by spiral galaxies are unable to launch jets to be incorrect. The detections are a plausible indicator of the presence of a powerful, most likely relativistic jet because this intensity of emission at 37 GHz cannot be explained by, for example, radiation from supernova remnants. Additionally, one of the detected NLS1 galaxies is a newly discovered source of gamma rays and three others are candidates for future detections.


2017 ◽  
Author(s):  
S. V. Bogovalov ◽  
F. Aharonian ◽  
D. Khangulyan

2010 ◽  
Vol 712 (1) ◽  
pp. L10-L15 ◽  
Author(s):  
S. Sabatini ◽  
M. Tavani ◽  
E. Striani ◽  
A. Bulgarelli ◽  
V. Vittorini ◽  
...  
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