X-ray Lobster Eye all-sky monitor for rocket experiment

Author(s):  
V. Dániel ◽  
A. Inneman ◽  
L. Pína ◽  
V. Zadražil ◽  
T. Báča ◽  
...  
2017 ◽  
Author(s):  
Veronika Stehlikova ◽  
Martin Urban ◽  
Ondrej Nentvich ◽  
Adolf Inneman ◽  
Thorsten Döhring ◽  
...  
Keyword(s):  
X Ray ◽  

2016 ◽  
Vol 87 (7) ◽  
pp. 073103 ◽  
Author(s):  
Jie Xu ◽  
Xin Wang ◽  
Qi Zhan ◽  
Shengling Huang ◽  
Yifan Chen ◽  
...  
Keyword(s):  
X Ray ◽  

2021 ◽  
Vol 483 ◽  
pp. 126656
Author(s):  
Longhui Li ◽  
Chen Zhang ◽  
Ge Jin ◽  
Weimin Yuan ◽  
Shuangnan Zhang ◽  
...  

Author(s):  
Ladislav Pína ◽  
René Hudec ◽  
Veronika Maršíková ◽  
Adolf Inneman ◽  
Vladimír Daniel

2011 ◽  
Vol 196 (1) ◽  
pp. 6 ◽  
Author(s):  
Alan M. Levine ◽  
Hale V. Bradt ◽  
Deepto Chakrabarty ◽  
Robin H. D. Corbet ◽  
Robert J. Harris
Keyword(s):  
X Ray ◽  

2005 ◽  
Author(s):  
Michael Gertsenshteyn ◽  
Tomasz Jannson ◽  
Gajendra Savant
Keyword(s):  
X Ray ◽  

1990 ◽  
Vol 123 ◽  
pp. 463-468
Author(s):  
M. Matsuoka ◽  
N. Kawai ◽  
T. Imai ◽  
M. Yamauchi ◽  
A. Yoshida ◽  
...  

AbstractWe propose an X-ray all sky monitor for Japanese Experimental Module (JEM) on the space station. Considering practical circumstances, we show as a case study that the all sky monitor with slit hole cameras is most promising for monitoring the short-term and long-term X-ray transients. We call this all sky monitor as MAXI (Monitor of All-sky X-ray Image). Position determination of gamma-ray bursts could be achieved with accuracy less than one degree observing the X-ray component of the burst. Weak X-ray sources such as active galactic nuclei could be also monitored with time resolution less than one day. The X-ray all sky monitor will work to discover X-ray novae and transient phenomena and give us the alarm for further detailed observations. The obtained data will be also used for archival study.


1990 ◽  
Vol 123 ◽  
pp. 89-110
Author(s):  
H. V. Bradt ◽  
A. M. Levine ◽  
E. H. Morgan ◽  
R. A. Remillard ◽  
J. H. Swank ◽  
...  

AbstractThe capabilities of the X-ray Timing Explorer (XTE) are described with particular attention paid to current scientific problems it will address from galactic neutron star systems to active galactic nuclei. It features a low-background continuous 2-200 keV response with large apertures (a 0.63-m2 proportional counter array and a 0.16-m2 dual rocking NaI/CsI scintillation array). Rapid response (in hours) to temporal phenomena, e.g. transients, is obtained by virtue of a scanning all-sky monitor and rapid maneuverability. XTE will carry out detailed energy-resolved studies of phenomena close to neutron stars (e.g. QPO’s) because of its sub-millisecond timing (to 10 μs), its high telemetry rates (to 256 kb/s), and the high throughput of its data system (to ≳ 2 × 105 c s−1).


1998 ◽  
Vol 164 ◽  
pp. 333-334
Author(s):  
G. G. Pooley ◽  
R. P. Fender

AbstractMonitoring with the Ryle Telescope at 15 GHz of the Galactic X-ray transient source GRS 1915+105 has revealed a remarkable range of rapid and extended flares which appear to be related to the X-ray emission as recorded by the RXTE all-sky monitor. Quasiperiodic oscillations in the range 20–40 min have been found and are probably related to oscillations in the soft X-ray flux.


Author(s):  
Li Jin ◽  
Takanori Sakamoto ◽  
Motoko Serino ◽  
Daisuke Yonetoku ◽  
Tatsuya Sawano ◽  
...  
Keyword(s):  
X Ray ◽  

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