Large-Area X-Ray Micro-Fluorescence Imaging of Heterogeneous Materials

1992 ◽  
pp. 1255-1264 ◽  
Author(s):  
B. J. Cross ◽  
R. D. Lamb ◽  
S. Ma ◽  
J. M. Paque
Keyword(s):  
Fluorescence Imaging ◽  
Heterogeneous Materials ◽  
Large Area ◽  
X Ray ◽  
Area X

Characteristics of a robust and portable large area X-ray fluorescence imaging system

2013 ◽  
Vol 43 (2) ◽  
pp. 126-130 ◽  
Author(s):  
R. G. Figueroa ◽  
E. Lozano ◽  
F. Belmar ◽  
D. Alcaman ◽  
A. von Bohlen ◽  
...  
Keyword(s):  
Fluorescence Imaging ◽  
Imaging System ◽  
Large Area ◽  
X Ray ◽  
Fluorescence Imaging System ◽  
Area X

A large area X-ray imager with online linearization and noise suppression

2011 ◽  
Author(s):  
T. He ◽  
R. Durst ◽  
B. L. Becker ◽  
J. Kaercher ◽  
G. Wachter
Keyword(s):  
Noise Suppression ◽  
Large Area ◽  
X Ray ◽  
Area X

Balloon Observations of Several Southern X-Ray Sources

1979 ◽  
Vol 3 (5) ◽  
pp. 349-350 ◽  
Author(s):  
J. G. Greenhill ◽  
M. L Duldig ◽  
M. W. Emery ◽  
A. G. Fenton ◽  
K. B. Fenton ◽  
...  
Keyword(s):  
Gamma Ray ◽  
Transient Increase ◽  
Large Area ◽  
Gamma Ray Burst ◽  
X Ray ◽  
The University ◽  
Area X

The University of Tasmania balloon-borne large area X-ray telescope was flown from Alice Springs on 20 November 1978. A number of known X-ray sources were observed and a transient increase believed to be a gamma ray burst was detected.

New large-area x-ray image sensor

1998 ◽  
Author(s):  
Donald R. Ouimette ◽  
Sol Nudelman ◽  
Richard S. Aikens
Keyword(s):  
Image Sensor ◽  
Large Area ◽  
X Ray ◽  
Area X

scholarly journals High Speed, High Resolution and Large Area X-ray Imaging Using Silicon Drift Detectors

2011 ◽  
Vol 17 (S2) ◽  
pp. 892-893 ◽  
Author(s):  
R Terborg ◽  
J Berlin ◽  
T Salge
Keyword(s):  
High Resolution ◽  
High Speed ◽  
Large Area ◽  
X Ray ◽  
X Ray Imaging ◽  
Silicon Drift Detectors ◽  
Area X

Extended abstract of a paper presented at Microscopy and Microanalysis 2011 in Nashville, Tennessee, USA, August 7–August 11, 2011.

scholarly journals Study of recent outburst in the Be/X-ray binary RX J0209.6−7427 with AstroSat: a new ultraluminous X-ray pulsar in the Magellanic Bridge?

2020 ◽  
Vol 495 (3) ◽  
pp. 2664-2672 ◽  
Author(s):  
Amar Deo Chandra ◽  
Jayashree Roy ◽  
P C Agrawal ◽  
Manojendu Choudhury
Keyword(s):  
Energy Band ◽  
Spectral Characteristics ◽  
Spectral Studies ◽  
X Rays ◽  
Energy Bands ◽  
Large Area ◽  
Pulse Profile ◽  
X Ray ◽  
Outburst Energy ◽  
Area X

ABSTRACT We present the timing and spectral studies of RX J0209.6–7427 during its rare 2019 outburst using observations with the Soft X-ray Telescope (SXT) and Large Area X-ray Proportional Counter (LAXPC) instruments on the AstroSat satellite. Pulsations having a periodicity of 9.29 s were detected for the first time by the NICER mission in the 0.2–10 keV energy band and, as reported here, by AstroSat over a broad energy band covering 0.3–80 keV. The pulsar exhibits a rapid spin-up during the outburst. Energy resolved folded pulse profiles are generated in several energy bands in 3–80 keV. To the best of our knowledge this is the first report of the timing and spectral characteristics of this Be binary pulsar in hard X-rays. There is suggestion of evolution of the pulse profile with energy. The energy spectrum of the pulsar is determined and from the best-fitting spectral values, the X-ray luminosity of RX J0209.6−7427 is inferred to be 1.6 × 1039 erg s−1. Our timing and spectral studies suggest that this source has features of an ultraluminous X-ray pulsar in the Magellanic Bridge. Details of the results are presented and discussed in terms of the current ideas.

scholarly journals Small-Scale Structure Deduced from X- and γ-ray Timing Measurements

2001 ◽  
Vol 205 ◽  
pp. 244-251
Author(s):  
M. Coleman Miller
Keyword(s):  
Black Holes ◽  
Neutron Stars ◽  
Small Scale ◽  
Large Area ◽  
X Ray ◽  
Strong Gravity ◽  
Thermonuclear Burning ◽  
General Relativistic ◽  
Γ Ray ◽  
Area X

X-ray timing observations of neutron stars and black holes are among the few available probes of ultrastrong magnetic fields, strong gravity, high densities, and the propagation of thermonuclear burning. Here we review the evidence for these effects revealed with data from the Rossi Explorer in the last five years. We also discuss the exciting prospects for making the first quantitative tests of strong-gravity general relativistic predictions with a large-area X-ray timing mission.

T1601-2-4 Fabrication of Large Area X-ray Mask Using Carbon Wafer

2010 ◽  
Vol 2010.8 (0) ◽  
pp. 203-204
Author(s):  
Daiji NODA ◽  
Atsushi TOKUOKA ◽  
Tadashi HATTORI
Keyword(s):  
Large Area ◽  
X Ray ◽  
Area X

Large-Area X-ray Lithography System for LIGA Process Operating in Wide Energy Range of Synchrotron Radiation

2005 ◽  
Vol 44 (7B) ◽  
pp. 5500-5504 ◽  
Author(s):  
Yuichi Utsumi ◽  
Takefumi Kishimoto ◽  
Tadashi Hattori ◽  
Hirotsugu Hara
Keyword(s):  
Synchrotron Radiation ◽  
Energy Range ◽  
Wide Energy Range ◽  
Large Area ◽  
X Ray ◽  
Wide Energy ◽  
Area X ◽  
Lithography System
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