Gamma Ray Astronomy Initiatives in India V C

Gamma Ray Astronomy Initiatives in India V. C. Sahni Bhabha Atomic Research Centre Mumbai, India

Gamma Ray Astronomy – Relatively young field # Direct detection upto ~10 Ge. V outside atmosphere # Ground based detection uses atmosphere as transducer * Atmospheric Cerenkov Technique *Atmospheric Scintillation Technique Multiple Probes are needed for getting a more accurate perspective of the multi-colour universe around us.

#Various available windows Radio, IR, Visible, X-Rays, Gamma Rays – HE 30 Me. V-30 Ge. V VHE 30 Ge. V- 100 Te. V UHE >100 Te. V #Why Gamma Ray Astronomy ? *Possible sites of cosmic ray production *Excellent probes of very energetic phenomena Charge neutrality *Understand new phenomena not seen at other energies *Probes of intergalactic radiation fields

VHE gamma ray astronomy programmes in India * NRL-HARL Division of BARC Imaging Technique (TACTIC telescope at Mt. Abu(1400 m amsl), Rajasthan) (ACT – first generation gamma ray telescope set up at Gulmarg(2700 m amsl) in 1985) * HEG of TIFR Wavefront sampling Technique (PACT telescope at Pachmari, MP) * BARC, TIFR & IIA at Hanle. (4200 m amsl) - proposed 21 m diameter MACE and 7 detector array HAGAR

BARC VHE Gamma Ray Astronomy Programme Set up high sensitivity telescope systems at Mt. Abu & Hanle for probing the sky in the Ge. V –Te. V energy range. Most recent window to the universe (First detection of CRAB nebula in Te. V energy range in 1989 by the Whipple group) §TACTIC (1. 0 Te. V-50 Te. V) §MYSTIQUE (10 Te. V-500 Te. V) (wide angle survey instrument) §MACE (30 Ge. V-30 Te. V) (at 4200 m altitude at Hanle, Ladakh)

CRAB Nebula – Cosmic Laboratory .

Gamma Ray Sky as seen by EGRET (1991 -2000) Earlier Satellite Experiments OSO 1967, SAS 2 1972, COSB 1975

Challenges in Ground based VHE gamma-ray Astronomy §Extremely weak flux (1 photon/sq. m/week in space) §Large CR background (>500: 1) §Large LONS background §Low duty cycle (<15%) §Variability of the transducer (atmosphere) Advantages of Atmospheric Cerenkov Technique §Large effective area (~10**4 sq. m) §Good angular resolution (2 nd gen. Systems) §Calorimetric component

Sensitivity enhancement §CRAB Nebula Flux [F(0. 5 Te. V) ~4. 5 X 10**-11/sqcm/s] §ON/OFF monitoring [10 hr observation ~0. 7 sigma] §Imaging [10 hr observation ~8. 1 sigma] Fg~70% acceptance Fp~99. 7% rejection §Stereo imaging §Spectral content §Temporal characteristics §Polarization index

Atmospheric Cerenkov Technique --

Physics behind Cerenkov Imaging Technique

Comparison of actual recorded images

TACTIC Telescope Te. V Atmospheric Cerenkov Telescope with Imaging Camera 349 -pixel camera 0. 3 deg resolution 9. 5 sq. m light collector Energy threshold ~1 Te. V

Point Spread Function of the TIE Light Collector

TIE Drive Control System (Alt. -Az. Mounting)

Block Diagram of the TIE DAS

TACTIC Data Acquisition System

TACTIC Control Console .

Sensitivity estimate of TACTIC

Mkn-501 Observations with prototype 81 -pixel camera

Crab Nebula Observations

Crab Nebula Observations

Mkn 421 Observations

Mkn 421 Observations

Simulation results

Simulation results

TACTIC results

TACTIC Vertex Elements Additional discrimination parameters §Polarization §Spectral content §Temporal characteristics Duplex camera design §Beam splitters §Dichroic filters §Polarizers §High speed digitizers

4 -element TACTIC array .

TACTIC Important Publications 1. Semi-intelligent trigger-generation scheme for Cerenkov light Imaging cameras. C. L. Bhat, A. K. Tickoo, R. Koul and I. K. Kaul Nucl. Inst. & Methods A, 340 (1994) 413. 2. A computer-programmable delay-generator scheme for TACTIC gamma-ray telescope. A. K. Tickoo, C. L. Bhat, R. Koul, I. K. Kaul, S. K. Kaul and S. R. Kaul Nucl. Instr. & Methods A, 349 (1994) 600. 1. Hybrid Zener based VDN – a better choice for Cerenkov light imaging camera. C. L. Bhat, R. Koul, S. R. Kaul, S. K. Kaul, I. K. Kaul & H. Goyal Meas. Sci. Technol. 7 1996 706. 2. Use of ‘look-up’ table improves the accuracy of a low-cost resolver-based absolute shaft encoder. S. K. Kaul, R. Koul, C. L. Bhat, I. K. Kaul and A. K. Tickoo Meas. Sci. Technol. , 8 1997 329 1. Potential of TACTIC for cosmic ray mass composition investigations. R. C. Rannot, C. L. Bhat, M. L. Sapru, A. K. Razdan, V. N. Gandhi, T. Thouw, H. Rebel and D. Heck. Nucl. Phys. B (Proc. Suppl. ) 52 B (1997) 269. 2. Very high Energy gamma-rays from Markarian 501. R. J. Protheroe, C. L. Bhat, P. Fleury, E. Lorentz, M. Teshima & T. C. Weekes. Proc. 25 th ICRC, 8, 1997, 317. 3. 4. 1. 2. 2. 3. 1. 2. 3. 2. AGN detection ranges of MACE and TACTIC Imaging gamma-ray telescopes. C. L. Kaul, K. Shanthi, C. L. Bhat, A. K. Tickoo & R. K. Kaul Experimental Astronomy, 9, 1999, 81. Drive control system for the TACTIC gamma-ray telescope A. K. Tickoo, R. Koul, S. K. Kaul, I. K. Kaul, C. L. Bhat, N. G. Bhatt, M. Kothari, H. C. Goyal, N. K. Agarwal & S. R. Kaul Experimental Astronomy, 9, 1999, 81. First results on characterization of Cerenkov images through combined use of Hillas fractal and wavelet parameters. A. Haungs, A. K. Razdan, C. L. Bhat, R. C. Rannot and H. Rebel Astropart. Phys. 12, 1999, 145. Artificial Neural Network approach for reconstruction of event arrival direction in wide-angle atmospheric Cerenkov detector arrays : A feasibility study. V. K. Dhar, A. K. Tickoo, R. Koul and C. L. Bhat. Experimental Astronomy, 10, 2000, 487

TACTIC Important Publications 11. On single counts rate stabilization scheme employed in Imaging camera of TACTIC gamma-ray telescope. N. Bhatt, K. K. Yadav, A. Kanda, R. Koul, S. R. Kaul, H. C. Goyal, V. K. Dhar, S. K. Kaul, K. Venugopal, A. K. Tickoo, I. K. Kaul, M. Kothari and C. L. Bhat Meas. Sci. Technol. , 12, 2001, 167. 12. TACTIC Imaging gamma-ray telescope : A simulation study of the effect of switched of pixels on its quality factor. S. K. Charagi, M. K. Koul, M. L. Sapru, R. C. Rannot & C. L. Bhat Experimental Astronomy, 11, 2001, 71. 13. Examining feasibility of air shower core-location from polarization state of associated Cerenkov light. V. J. Gokhale, R. C. Rannot, A. K. Tickoo, S. Bhattacharyya and C. L. Bhat Experimental Astronomy, 12, 2001, 195. 14. Image and non-image parameters of atmospheric Cherenkov events : a comparative study of their ray/hadron classification potential in ultrahigh energy regime. A. Razdan, A. Haungs, H. Rebel and C. L. Bhat Astroparticle Physics 17 (2002) 497 -508. • Programmable topological trigger generator for the 349 -pixel imaging camera of the TACTIC telescope. S. R. Kaul, R. Koul, I. K. Kaul, A. K. Tickoo, K. K. Yadav and C. L. Bhat Nucl. Instr. & Methods A, 496, 2003, 400. • Real time data acquisition and control system for the 349 -pixel TACTIC atmospheric Cerenkov imaging telescope; K. K. Yadav, R. Koul, A. Kanda, S. R. Kaul, A. K. Tickoo, R. C. Rannot, P. Chandra, N. Bhatt, N. Chouhan, K. Venugopal, M. Kothari, H. C. Goyal, V. K. Dhar and S. K. Kaul; Nucl. Instr & Methods A 527, 2004, 411 -422.

PACT (Pachmari Array of Cerenkov Telescopes) *Temporal and spatial distribution of Cerenkov photons for g/p segregation. *Arrival time recorded .

PACT Layout • Each telescope 7 mirrors of 0. 9 m dia • 25 telescopes deployed • Fo. V ~ 3 deg • 4 sectors • 4 -fold coincidence • Timing and pulse height data recorded

PACT Results # Pulsed emission from Te. V sources detected from CRAB Pulsar and Geminga (not confirmed yet by other telescopes) Once confirmed this result will have far reaching consequences in Astrophysics

Concurrent observation campaigns (PACT, TACTIC & Optical telescopes in India) * Mkn 421, Mkn 501, H 1426 * Concurrent detection of short duration flares with telescopes using different techniques for g/p segregation.

Why Ge. V Astronomy ? # Only a handful of Te. V sources detected # EGRET detected 270 sources in Me. V-Ge. V range # >100 sources expected in the 10 -100 Ge. V range

Ge. V Astronomy - Need for a large light collector .

Increase in Cerenkov photon flux at high altitude

MACE telescope .

MACE sensitivity

Mkn 421 Energy Spectrum .

Thank you