scholarly journals A Parameterisation ofγ-ray production cross-sections for pp interactions in a broad energy range

2015 ◽  
Vol 105 ◽  
pp. 02002
Author(s):  
Andrew M. Taylor
2015 ◽  
Vol 105 ◽  
pp. 02006
Author(s):  
Andrew M. Taylor ◽  
Ervin Kafexhiu ◽  
Felix Aharonian ◽  
Gabriela Vila

2018 ◽  
Vol 47 (4) ◽  
pp. 043104 ◽  
Author(s):  
R. P. McEachran ◽  
F. Blanco ◽  
G. García ◽  
P. W. Stokes ◽  
R. D. White ◽  
...  

2018 ◽  
Vol 149 (3) ◽  
pp. 034304 ◽  
Author(s):  
Alexandra Loupas ◽  
Ana. I. Lozano ◽  
Francisco Blanco ◽  
Jimena D. Gorfinkiel ◽  
Gustavo García

2014 ◽  
Vol 83 ◽  
pp. 68-76 ◽  
Author(s):  
A.G. Sanz ◽  
M.C. Fuss ◽  
F. Blanco ◽  
F. Carelli ◽  
F. Sebastianelli ◽  
...  

2020 ◽  
Vol 49 (1) ◽  
pp. 013102 ◽  
Author(s):  
R. P. McEachran ◽  
B. P. Marinković ◽  
G. García ◽  
R. D. White ◽  
P. W. Stokes ◽  
...  

2021 ◽  
Vol 922 (2) ◽  
pp. 159
Author(s):  
A. Traina ◽  
S. Marchesi ◽  
C. Vignali ◽  
N. Torres-Albà ◽  
M. Ajello ◽  
...  

Abstract We present the joint Chandra, XMM-Newton, and NuSTAR analysis of two nearby Seyfert galaxies, NGC 3081 and ESO 565-G019. These are the only two having Chandra data in a larger sample of 10 low-redshift (z ≤ 0.05), candidates Compton-thick (CT) Active Galactic Nuclei selected in the 15–150 keV band with Swift-BAT that were still lacking NuSTAR data. Our spectral analysis, performed using physically motivated models, provides an estimate of both the line-of-sight (l.o.s.) and average (N H,S ) column densities of the two torii. NGC 3081 has a Compton-thin l.o.s. column density N H,z = [0.58–0.62] × 1024 cm−2, but the N H,S , beyond the CT threshold (N H,S = [1.41–1.78] × 1024 cm−2), suggests a “patchy” scenario for the distribution of the circumnuclear matter. ESO 565-G019 has both CT l.o.s. and N H,S column densities (N H,z > 2.31 × 1024 cm−2 and N H,S > 2.57 × 1024 cm−2, respectively). The use of physically motivated models, coupled with the broad energy range covered by the data (0.6–70 keV and 0.6–40 keV, for NGC 3081 and ESO 565-G019, respectively) allows us to constrain the covering factor of the obscuring material, which is C TOR = [0.63–0.82] for NGC 3081, and C TOR = [0.39–0.65] for ESO 565-G019.


2015 ◽  
Vol 24 (07) ◽  
pp. 1550055
Author(s):  
Atef Ismail ◽  
Yen Cheong Lee ◽  
M Tammam

Proton elastic scattering at various incident energies is one method to study nuclear density distributions and nuclear radii. Single folding potential describing the p-scattering on 40 Ca over a broad energy range 9–48.4 MeV is constructed. The resulting potential does not need any renormalization to fit the measured elastic scattering angular distributions and total reaction cross-sections. Furthermore, correlation between volume integral and proton incident energy is discussed. Theoretical calculations are in a good agreement with existing experimental data.


Sign in / Sign up

Export Citation Format

Share Document