Calibration of Scanning Sky Monitor (SSM) onboard AstroSat

2021 ◽  
Vol 42 (2) ◽  
Author(s):  
Abhilash R. Sarwade ◽  
M. C. Ramadevi ◽  
B. T. Ravishankar ◽  
Brajpal Singh ◽  
Blessy Elizabeth Baby ◽  
...  
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1984 ◽  
Author(s):  
A. J. Wardrop
Keyword(s):  

2005 ◽  
Vol 52 (6) ◽  
pp. 2765-2772 ◽  
Author(s):  
K. Yamaoka ◽  
M. Ohno ◽  
Y. Terada ◽  
S. Hong ◽  
J. Kotoku ◽  
...  
Keyword(s):  

1990 ◽  
Vol 10 (2) ◽  
pp. 239-242 ◽  
Author(s):  
S. Brandt ◽  
N. Lund ◽  
A.R. Rao
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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 ◽  

2009 ◽  
Vol 61 (sp1) ◽  
pp. S35-S53 ◽  
Author(s):  
Kazutaka Yamaoka ◽  
Akira Endo ◽  
Teruaki Enoto ◽  
Yasushi Fukazawa ◽  
Ryuji Hara ◽  
...  
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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).


2015 ◽  
Vol 67 (3) ◽  
pp. 41 ◽  
Author(s):  
Tetsuya Yasuda ◽  
Wataru B. Iwakiri ◽  
Makoto S. Tashiro ◽  
Yukikatsu Terada ◽  
Tomomi Kouzu ◽  
...  
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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.


2017 ◽  
Vol 44 (1) ◽  
pp. 11-23 ◽  
Author(s):  
M. C. Ramadevi ◽  
S. Seetha ◽  
Dipankar Bhattacharya ◽  
B. T. Ravishankar ◽  
N. Sitaramamurthy ◽  
...  
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