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
1 code implementation • 7 Jan 2021 • Biswajit Mondal, Santosh V. Vadawale, N. P. S. Mithun, C. S. Vaishnava, Neeraj K. Tiwari, S. K. Goyal, Singam S. Panini, Vinita Navalkar, Chiranjit Karmakar, Mansukhlal R. Patel, R. B. Upadhyay
We have initiated the development of hard X-ray optics for future Indian X-ray astronomical missions, and in this context, we have developed a program, DarpanX, to calculate X-ray reflectivity for single and multilayer mirrors.
Instrumentation and Methods for Astrophysics
