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
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
