Science with the Daksha High Energy Transients Mission

Autor: Bhalerao, Varun, Sawant, Disha, Pai, Archana, Tendulkar, Shriharsh, Vadawale, Santosh, Bhattacharya, Dipankar, Rana, Vikram, Adalja, Hitesh Kumar L., Anupama, G C, Bala, Suman, Banerjee, Smaranika, Basu, Judhajeet, Belatikar, Hrishikesh, Beniamini, Paz, Bhaganagare, Mahesh, Bhaskar, Ankush, Bhattacharjee, Soumyadeep, Bose, Sukanta, Cenko, Brad, Chanda, Mehul Vijay, Dewangan, Gulab, Dixit, Vishal, Dutta, Anirban, Gawade, Priyanka, Ghodgaonkar, Abhijeet, Goyal, Shiv Kumar, Gunasekaran, Suresh, Guruprasad, P J, Hemanth, Manikantan, Hotokezaka, Kenta, Iyyani, Shabnam, Kasliwal, Mansi, Koyande, Jayprakash G., Kulkarni, Salil, Kutty, APK, Ladiya, Tinkal, Marla, Deepak, Mate, Sujay, Mehla, Advait, Mithun, N. P. S., More, Surhud, Mote, Rakesh, Mukherjee, Dipanjan, Narang, Sanjoli, Narendranath, Shyama, Nema, Ayush, Nimbalkar, Sudhanshu, Nissanke, Samaya, Palit, Sourav, Patel, Jinaykumar, Patel, Arpit, Paul, Biswajit, Pradeep, Priya, Ramachandran, Prabhu, Roy, Kinjal, Saiguhan, B. S. Bharath, Saji, Joseph, Saleem, M., Saraogi, Divita, Sastry, Parth, Shanmugam, M., Sharma, Piyush, Shetye, Amit, Singh, Nishant, Singh, Shreeya, Singhal, Akshat, Sreekumar, S., Sridhar, Srividhya, Srinivasan, Rahul, Tallur, Siddharth, Tiwari, Neeraj K., Vadladi, Amrutha Lakshmi, Vaishnava, C. S., Vishwakarma, Sandeep, Waratkar, Gaurav

We present the science case for the proposed Daksha high energy transients mission. Daksha will comprise of two satellites covering the entire sky from 1~keV to $>1$~MeV. The primary objectives of the mission are to discover and characterize electrom

Externí odkaz: http://arxiv.org/abs/2211.12052

Hard X-ray polarisation measurement capability of proposed Indian high-energy transient mission – Daksha

Autor: Mate, Sujay, Bala, Suman, Sastry, Parth, Mehla, Advait, Saraogi, Divita, NPS, Mithun, Palit, Sourav, Waratkar, Gaurav, Bhalerao, Varun, Tendulkar, Shriharsh, Vadawale, Santosh

Daksha, a proposed Indian mission, will be the most sensitive all-sky high-energy time domain telescope in the world. Daksha will detect and characterise about ten electromagnetic counterparts of the gravitational wave (EMGW) events per year and abou

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::5c14c3ba9156d54f05555a48e1115b2c

Prospects of measuring gamma-ray burst polarization with the Dakshamission

Autor: Bala, Suman, Mate, Sujay, Mehla, Advait, Sastry, Parth, Mithun, N. P. S., Palit, Sourav, Chanda, Mehul Vijay, Saraogi, Divita, Vaishnava, C. S., Waratkar, Gaurav, Bhalerao, Varun, Bhattacharya, Dipankar, Tendulkar, Shriharsh, Vadawale, Santosh

Publikováno v: Journal of Astronomical Telescopes, Instruments, and Systems; December 2023, Vol. 9 Issue: 4 p048002-048002, 1p