Large Area X-ray Proportional Counter (LAXPC) Instrument on AstroSat and Some Preliminary Results from its performance in the orbit

Abstract

Large Area X-ray Propositional Counter (LAXPC) instrument on AstroSat is aimed at providing high time resolution X-ray observations in 3 to 80 keV energy band with moderate energy resolution. To achieve large collecting area, a cluster of three co-aligned identical LAXPC detectors, is used to realize an effective area in access of about 6000 cm2 at 15 keV. The large detection volume of the LAXPC detectors, filled with xenon gas at about 2 atmosphere pressure, results in detection efficiency greater than 50%, above 30 keV. In this article, we present salient features of the LAXPC detectors, their testing and characterization in the laboratory prior to launch and calibration in the orbit. Some preliminary results on timing and spectral characteristics of a few X-ray binaries and other type of sources, are briefly discussed to demonstrate that the LAXPC instrument is performing as planned in the orbit.

11 pages, 15 Figures, Accepted for publication in Journal of Astronomy and Astrophysics

References in corpus (6)

• X-ray Properties of Black-Hole Binaries
• Modeling the Emission Processes in Blazars
• AstroSat/LAXPC reveals the high energy variability of GRS 1915+105 in the chi class
• Repetitive Patterns in Rapid Optical Variations in the Nearby Black-hole Binary V404 Cygni
• AstroSat/LAXPC observation of Cygnus X-1 in the hard state
• Performance of Large Area X-ray Proportional Counters in a Balloon Experiment

Cited by in corpus (1)

• Broadband reflection spectroscopy of MAXI J1535-571 using AstroSat: Estimation of black hole mass and spin