1 code implementation • 24 Dec 2020 • Anirban Chakraborty, Manjari Bagchi
By comparing the distributions of various parameters of synthetic pulsars detectable by the Parkes Multibeam Pulsar Survey, the Pulsar Arecibo L-band Feed Array Survey, and two Swinburne Multibeam surveys with those of the real pulsars detected by the same surveys, we find that a good and physically realistic model can be obtained by using a uniform distribution of the braking index in the range of 2. 5 to 3. 0, a uniform distribution of the cosine of the angle between the spin and the magnetic axis in the range of 0 to 1, a log-normal birth distribution of the surface magnetic field with the mean and the standard deviation as 12. 85 and 0. 55 respectively while keeping the distributions of other parameters unchanged from the ones most commonly used in the literature.
High Energy Astrophysical Phenomena Solar and Stellar Astrophysics
no code implementations • 6 Jul 2020 • Abhimanyu Susobhanan, Yogesh Maan, Bhal Chandra Joshi, T. Prabu, Shantanu Desai, Yashwant Gupta, A. Gopakumar, Neelam Dhanda Batra, Arpita Choudhary, Mayuresh P. Surnis, Lankeswar Dey, Jaikhomba Singha, K. Nobleson, Manjari Bagchi, Avishek Basu, Suryarao Bethapudi, Kishalay De, Raghav Girgaonkar, M. A. Krishnakumar, P. K. Manoharan, Arun Kumar Naidu, Dhruv Pathak, Sai Chaitanya Susarla
We introduce pinta, a pipeline for reducing the upgraded Giant Metre-wave Radio Telescope (uGMRT) raw pulsar timing data, developed for the Indian Pulsar Timing Array experiment.
Instrumentation and Methods for Astrophysics High Energy Astrophysical Phenomena
