Welcome to HAGAR Group



HAGAR, an array of seven telescopes, is operational at Hanle, Ladakh since 2009. It is operated jointly by Tata Institute of Fundamental Research, Mumbai and Indian Institute of Astrophysics, Bengaluru. It is designed to study very high energy gamma ray emission from celestial objects. Gamma rays are detected indirectly using atmospheric Cherenkov technique. Prime targets include Active Galactic Nuclie (AGNs) and gamma ray pulsars.We aim to study emission regions and processes responsible for gamma ray production in these sources. Study of gamma ray emission is expected to shed some light on long standing puzzle regarding origin of cosmic rays.Also there are possibilities such as study of physics beyond standard model through dark matter searches, tests for Lorentz invariance as well as indirect estimation of extragalactic background light.

 

 

 

 

HAGAR Group: TIFR ,Room No:- C115,D307,C123,C125,D414,Homi Bhabha Road,Colaba,Mumbai, (India)
Phone : 022-22782675 Email : mano.ranjan@tifr.res.in

Developed by : Mano Ranjan,Scientific Assistant(B),DHEP