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Daksha: On Alert for High Energy Transients

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arxiv 2211.12055 v2 pith:3B5YKA5P submitted 2022-11-22 astro-ph.IM astro-ph.HE

Varun Bhalerao , Santosh Vadawale , Shriharsh Tendulkar , Dipankar Bhattacharya , Vikram Rana , Hitesh Kumar L. Adalja , Hrishikesh Belatikar , Mahesh Bhaganagare
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Gulab Dewangan Abhijeet Ghodgaonkar Shiv Kumar Goyal Suresh Gunasekaran P J Guruprasad Jayprakash G. Koyande Salil Kulkarni APK Kutty Tinkal Ladiya Deepak Marla Sujay Mate N.P.S. Mithun Rakesh Mote Sanjoli Narang Ayush Nema Sudhanshu Nimbalkar Archana Pai Sourav Palit Arpit Patel Jinaykumar Patel Priya Pradeep Prabhu Ramachandran B.S. Bharath Saiguhan Divita Saraogi Disha Sawant M. Shanmugam Piyush Sharma Amit Shetye Shreeya Singh Nishant Singh Akshat Singhal S. Sreekumar Srividhya Sridhar Rahul Srinivasan Siddharth Tallur Neeraj K. Tiwari Amrutha Lakshmi Vadladi C. S. Vaishnava Sandeep Vishwakarma Gaurav Waratkar
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keywords dakshawillenergyhightransientscounterpartsearthmonitoring
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We present Daksha, a proposed high energy transients mission for the study of electromagnetic counterparts of gravitational wave sources, and gamma ray bursts. Daksha will comprise of two satellites in low earth equatorial orbits, on opposite sides of earth. Each satellite will carry three types of detectors to cover the entire sky in an energy range from 1 keV to >1 MeV. Any transients detected on-board will be announced publicly within minutes of discovery. All photon data will be downloaded in ground station passes to obtain source positions, spectra, and light curves. In addition, Daksha will address a wide range of science cases including monitoring X-ray pulsars, studies of magnetars, solar flares, searches for fast radio burst counterparts, routine monitoring of bright persistent high energy sources, terrestrial gamma-ray flashes, and probing primordial black hole abundances through lensing. In this paper, we discuss the technical capabilities of Daksha, while the detailed science case is discussed in a separate paper.

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  1. Picolensing as a Probe of Primordial Black Hole Dark Matter

    astro-ph.HE 2024-11 conditional novelty 5.0 of 10

    Asteroid-mass primordial black hole dark matter could be probed by picolensing of gamma-ray bursts, but only with detector separations of at least Earth-L2 distance once realistic GRB size uncertainties are included.

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