Soft x-ray detection efficiency of large-area avalanche photodiodes

1994 ◽  
Author(s):  
Eric M. Gullikson ◽  
Ernesto V. Gramsch ◽  
Marek Szawlowski
2007 ◽  
Vol 2 (08) ◽  
pp. P08005-P08005 ◽  
Author(s):  
L M P Fernandes ◽  
F D Amaro ◽  
A Antognini ◽  
J M R Cardoso ◽  
C A N Conde ◽  
...  

2003 ◽  
Vol 58 (12) ◽  
pp. 2255-2260 ◽  
Author(s):  
L.M.P. Fernandes ◽  
A. Antognini ◽  
M. Boucher ◽  
C.A.N. Conde ◽  
O. Huot ◽  
...  

2001 ◽  
Vol 30 (3) ◽  
pp. 164-169 ◽  
Author(s):  
L. M. P. Fernandes ◽  
J. A. M. Lopes ◽  
J. M. F. dos Santos ◽  
C. A. N. Conde

1993 ◽  
Author(s):  
Andrzej J. Dabrowski ◽  
Jan S. Iwanczyk ◽  
Yuzhong J. Wang ◽  
Michael C. Madden ◽  
Marek Szawlowski

Author(s):  
Alan Owens ◽  
H Andersson ◽  
M Bavdaz ◽  
L van den Berg ◽  
A Peacock ◽  
...  
Keyword(s):  

2019 ◽  
Vol 489 (3) ◽  
pp. 4300-4310 ◽  
Author(s):  
A Sezer ◽  
T Ergin ◽  
R Yamazaki ◽  
H Sano ◽  
Y Fukui

ABSTRACT We present the results from the Suzaku X-ray Imaging Spectrometer observation of the mixed-morphology supernova remnant (SNR) HB9 (G160.9+2.6). We discovered recombining plasma (RP) in the western Suzaku observation region and the spectra here are well described by a model having collisional ionization equilibrium (CIE) and RP components. On the other hand, the X-ray spectra from the eastern Suzaku observation region are best reproduced by the CIE and non-equilibrium ionization model. We discuss possible scenarios to explain the origin of the RP emission based on the observational properties and concluded that the rarefaction scenario is a possible explanation for the existence of RP. In addition, the gamma-ray emission morphology and spectrum within the energy range of 0.2–300 GeV are investigated using 10 yr of data from the Fermi Large Area Telescope (LAT). The gamma-ray morphology of HB9 is best described by the spatial template of radio continuum emission. The spectrum is well fit to a log-parabola function and its detection significance was found to be 25σ. Moreover, a new gamma-ray point source located just outside the south-east region of the SNR’s shell was detected with a significance of 6σ. We also investigated the archival H i and CO data and detected an expanding shell structure in the velocity range of $-10.5$ and $+1.8$ km s−1 that is coinciding with a region of gamma-ray enhancement at the southern rim of the HB9 shell.


2015 ◽  
Vol 10 (10) ◽  
pp. P10030-P10030 ◽  
Author(s):  
X. Meng ◽  
X. Zhou ◽  
S. Zhang ◽  
J. Lees ◽  
C.H. Tan ◽  
...  
Keyword(s):  

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