Developing a Way of Processing Complex X-Ray and Gamma Spectra in the Range of Low Energies

2021 ◽  
Vol 85 (10) ◽  
pp. 1122-1127
Author(s):  
M. V. Zheltonozhskaya ◽  
V. A. Zheltonozhsky ◽  
D. E. Myznikov ◽  
A. N. Nikitin ◽  
N. V. Strilchuk ◽  
...  
Keyword(s):  
X Ray ◽  
Low Energies ◽  
Gamma Spectra

THE INTERPLAY OF PROMPT AND AFTERGLOW EMISSION IN GRB 060418

2008 ◽  
Vol 17 (09) ◽  
pp. 1343-1349 ◽  
Author(s):  
S. D. VERGANI ◽  
D. MALESANI ◽  
E. MOLINARI
Keyword(s):  
Gamma Rays ◽  
Spectral Properties ◽  
Gamma Ray ◽  
Early Time ◽  
Lorentz Factor ◽  
X Ray ◽  
Central Engine ◽  
Low Energies ◽  
Prompt Emission

We present observations of the early afterglow emission of GRB 060418. Thanks to the simultaneous coverage at optical, X-ray and gamma-ray wavelengths, we can detect and separate the external shock emission (visible in the optical and late X-ray data) and the central engine activity (early X and gamma rays). The two components are clearly distinguished based on temporal and spectral properties. The detection of the afterglow onset (in the optical) allows the determination of the fundamental fireball properties, namely its bulk Lorentz factor and total energy. The early time X-ray flare closely resembles the prompt emission gamma-ray pulses in its temporal profile, being wider at low energies and showing lags between the hard and soft bands. This provides a strong suggestion that X-ray flares are a continuation of the prompt emission.

Exosat Observations of H2252−035: Pulse Phase and Orbital Phase Dependent Low Energy Absorption and Iron Line Emission

1987 ◽  
Vol 93 ◽  
pp. 281-292
Author(s):  
W. Pietsch ◽  
W. Voges ◽  
E. Kendziorra ◽  
M. Pakull
Keyword(s):  
Energy Absorption ◽  
Line Emission ◽  
Low Energy ◽  
Gas Absorption ◽  
X Rays ◽  
Medium Energy ◽  
Iron Line ◽  
X Ray ◽  
Low Energies ◽  
Optical Light Curve

AbstractThe 805 sec pulsing X-ray source H2252−035 has been observed for 7 h on September 14/15 and on September 17, 1983 in X-rays with the low energy telescope and the medium energy detectors of EXOSAT. While below 2 keV the semiamplitude of the 805 s pulses is ~ 100% in the 2.3–7.9 keV band it is only ~ 40%. X-ray dips that are more pronounced in low energies occur simultaneously with the orbital minimum of the optical light curve. The medium energy spectra during dips with respect to the non dip spectrum can be explained by just enhanced cold gas absorption of an additional absorbing column of 2 1022 cm−2. Model spectra for the 805 s minimum have to include a strong iron emission line at 6.55 keV with an equivalent width of 3 keV in addition to a reduced continuum intensity (radiating area) and enhanced low energy absorption.

First TDCR measurements at low energies using a miniature x-ray tube

2014 ◽  
Vol 93 ◽  
pp. 7-12 ◽  
Author(s):  
E. Halter ◽  
C. Thiam ◽  
C. Bobin ◽  
J. Bouchard ◽  
D. Chambellan ◽  
...  
Keyword(s):  
X Ray ◽  
Low Energies

Quantitative analysis with a two-detector measuring system in in-air PIXE-design to improve detection sensitivity at low energies

2013 ◽  
Vol 23 (01n02) ◽  
pp. 55-67 ◽  
Author(s):  
K. Sera ◽  
S. Goto ◽  
C. Takahashi ◽  
Y. Saitoh
Keyword(s):  
Quantitative Analysis ◽  
Production Cross ◽  
Detection Sensitivity ◽  
Measuring System ◽  
X Rays ◽  
Standard Material ◽  
X Ray ◽  
New Device ◽  
Low Energies ◽  
Improve Detection Sensitivity

In this paper, a two-detector measuring system in in-air PIXE system composed of two Si(Li) detectors has been developed for simultaneous measurement of low- and high-Z elements. In order to improve detection sensitivity of the detector for low energy region, a new device which is attached at the tip of the detector has been designed. It is made of acryl and has a thin end on which a 1.5 μm-thick Mylar film is stuck. As a result, it exhibited a miraculous effect in improving detection sensitivity at low energies and it became possible to detect K X-rays of aluminium. In order to perform quantitative analysis in in-air system, we have measured detection efficiencies for the two Si(Li) detectors including the effect of X-ray absorption in air on the basis of the method that we developed. Concerning the beam energy at the target and corresponding X-ray production cross-sections, the same values as were reported in the previous paper were applicable since conditions of irradiating system were unchanged. It was confirmed that the new method allows us to quantitatively analyze all the elements heavier than aluminum and to obtain mostly the same results as those by in-vacuum PIXE for various kinds of samples. Accuracy of analysis was also confirmed by using a standard material.

scholarly journals 4U 1909+07: a Hidden Pearl

10.14311/1326 ◽  
2011 ◽  
Vol 51 (1) ◽  
Author(s):  
I. Kreykenbohm ◽  
F. Fürst ◽  
L. Barrágan ◽  
J. Wilms ◽  
R. E. Rothschild ◽  
...  
Keyword(s):  
Timing Analysis ◽  
High Mass ◽  
Folding Energy ◽  
Pulse Profile ◽  
Spectral Parameters ◽  
Phase Dependence ◽  
X Ray ◽  
Low Energies ◽  
Fluorescence Line ◽  
Energy Dependent

We present a detailed spectral and timing analysis of the High Mass X-ray Binary (HMXB) 4U 1909+07 with INTEGRAL and RXTE. 4U1909+07 is a persistent accreting X-ray pulsar with a period of approximately 605 s. The period changes erratically consistent with a random walk expected for a wind accreting system. INTEGRAL detects the source with an average of 2.4 cps (corresponding to 15mCrab), but sometimes exhibits flaring activity up to 50 cps (i.e. 300mCrab). The strongly energy dependent pulse profile shows a double peaked structure at low energies and only a single narrow peak at energies above 20 keV. The phase averaged spectrum is well described by a powerlaw modified at higher energies by an exponential cutoff and photoelectric absorption at low energies. In addition at 6.4 keV a strong iron fluorescence line and at lower energies a blackbody component are present. We performed phase resolved spectroscopy to study the pulse phase dependence of the spectral parameters: while most spectral parameters are constant within uncertainties, the blackbody normalization and the cutoff folding energy vary strongly with phase.

SI(LI) and Hpg Detectors: Recent Measurements

1998 ◽  
Vol 4 (S2) ◽  
pp. 166-167
Author(s):  
R A Sareen ◽  
T Nashashibi
Keyword(s):  
Activation Energy ◽  
Electron Microscope ◽  
Band Gap ◽  
Spectral Characteristics ◽  
Energy Dispersive ◽  
X Rays ◽  
X Ray ◽  
Synchrotron Beam ◽  
Energy Dispersive Microanalysis ◽  
Low Energies

Small Si (Si(Li), Intrinsic Si, PEN diodes) and Ge (HPG) planar detectors are used for measuring the energy and intensity of X-rays at low energies (below 100 keV). Applications include energy dispersive microanalysis in the electron microscope and x-ray fluorescence in tube excited systems. They are also finding increasing use on synchrotron beam lines. Both types of detector have unique and special properties and there is a wealth of information in the literature1 describing their principles of operation including their spectral characteristics.For example, the superior resolution (110 eV compared to 130 eV (FWHM) at 5.9 keV) obtained with 10 mm2 HPG detectors is a consequence of Ge's smaller band gap (0.7 eV compared to 1.1 eV eV for Si). This leads directly to a lower value for the activation energy (2.9 eV compared to 3.81 eV at 77K). Both materials have very similar Fano factors (approximately 0.11).

scholarly journals Micromegas for dark matter searches: CAST/IAXO & TREX-DM experiments

2018 ◽  
Vol 174 ◽  
pp. 01008 ◽  
Author(s):  
J. G. Garza ◽  
S. Aune ◽  
F. Aznar ◽  
J. F. Castel ◽  
S. Cebrián ◽  
...  
Keyword(s):  
Dark Matter ◽  
Light Nuclei ◽  
Solar Telescope ◽  
Particle Detectors ◽  
X Ray ◽  
Time Projection Chambers ◽  
Low Energies ◽  
Low Mass ◽  
Time Projection ◽  
Low Mass Wimp

The most compelling candidates for Dark Matter to day are WIMPs and axions. The applicability of gasesous Time Projection Chambers (TPCs) with Micromesh Gas Structures (Micromegas) to the search of these particles is explored within this work. Both particles would produce an extremely low rate at very low energies in particle detectors. Micromegas detectors can provide both low background rates and low energy threshold, due to the high granularity, radiopurity and uniformity of the readout. Small (few cm wide) Micromegas detectors are used to image the axion-induced x-ray signal expected in the CERN Axion Solar Telescope (CAST) experiment. We show the background levels obtained in CAST and the prospects to further reduce them to the values required by the Internation Axion Observatory (IAXO). We also present TREX-DM, a scaled-up version of the Micromegas used in axion research, but this time dedicated to the low-mass WIMP detection. TREX-DM is a high-pressure Micromegas-based TPC designed to host a few hundreds of grams of light nuclei (argon or neon) with energy thresholds potentially at the level of 100 eV. The detector is described in detail, as well as the results of the commissioning and characterization phase on surface. Besides, the background model of TREX-DM is presented, along with the anticipated sensitivity of this search, which could go beyond current experimental limits.

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