no code implementations • 26 Feb 2021 • Tanmoy Chattopadhyay, Soumya Gupta, Vidushi Sharma, Shabnam Iyyani, Ajay Ratheesh, N. P. S. Mithun, E. Aarthy, Sourav Palit, Abhay Kumar, Santosh V Vadawale, A. R. Rao, Varun Bhalerao, Dipankar Bhattacharya
While the 2-pixel Compton scattered events (100 - 300 keV) are used to extract sensitive spectroscopic information, the inclusion of the low-gain pixels (around 20% of the detector plane) after careful calibration extends the energy range of Compton energy spectra to 600 keV.
High Energy Astrophysical Phenomena Instrumentation and Methods for Astrophysics
no code implementations • 26 Feb 2021 • Ajay Ratheesh, A. R. Rao, N. P. S Mithun, Santosh V. Vadawale, Ajay Vibhute, Dipankar Bhattacharya, Priya Pradeep, S. Sreekumar, Varun Bhalerao
As hard X-ray instruments like CZTI are sensitive to cosmic rays in addition to X-rays, it is required to identify and remove particle induced or other noise events and select events for scientific analysis of the data.
High Energy Astrophysical Phenomena Instrumentation and Methods for Astrophysics