Conferencia

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Abstract:

Very high energy (VHE >100 GeV) gamma rays coming from blazars can produce pairs when interacting with the Extragalactic Background Light (EBL) and the Cosmic Microwave Background, generating an electromagnetic cascade. Depending on the Intergalactic Magnetic Field (IGMF) intensity, this cascade may result in an extended isotropic emission of photons around the source (halo), or in a broadening of the emission beam. The detection of these effects might lead to important constrains both on the IGMF intensity and the EBL density, quantities of great relevance in cosmological models. Using a Monte Carlo program, we simulate electromagnetic cascades for different values of the IGMF intensities and coming from a source similar to 1ES0229+200, a blazar with hard intrinsic spectrum at redshift z = 0:14, which is an ideal distance for potentially observing the effect. We study the possible response of a generic future Cherenkov telescope using a simplified model for the sensitivity, effective area and angular resolution. Finally, combining these instrument properties, we calculate the angular distribution of photons and develop a method to test the statistical feasibility of detecting the effect in the near future.

Registro:

Documento: Conferencia
Título:Detecting extended gamma-ray emission with the next generation Cherenkov telescopes
Autor:Alonso, M.F.; Supanitsky, A.D.; Rovero, A.C.
Filiación:Instituto de Astronomía y Física Del Espacio, IAFE, CONICET-UBA, Buenos Aires, Argentina
Año:2015
Volumen:30-July-2015
Título revista:34th International Cosmic Ray Conference, ICRC 2015
Título revista abreviado:Proc. Sci.
ISSN:18248039
Registro:https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_18248039_v30-July-2015_n_p_Alonso

Referencias:

  • Gould, R.J., Schréder, G., Opacity of the universe to high-energy photons (1966) Physical Review Letters, 16, p. 252
  • Gould, R.J., Rephaeli, Y., The effective penetration distance of ultrahigh-energy electrons and photons traversing a cosmic blackbody photon gas (1978) ApJ, 225, p. 318
  • Aharonian, F.A., Coppi, P.S., Voelk, H.J., Very high energy gamma rays from active galactic nuclei: Cascading on the cosmic background radiation fields and the formation of pair halos (1994) ApJ, 423, p. L5
  • Abramowski, A., Search for extended g-ray emission around AGN with H. E. S. S. and Fermi-LAT (2014) A+A, 562, p. 145
  • Aharonian, F.A., Search for a TeV gamma-ray halo of Mkn 501 (2001) A+A, 366, p. 746
  • Aleksíc, J., Search for an extended VHE g-ray emission from Mrk 421 and Mrk 501 with the MAGIC Telescope (2010) A+A, 524, p. 77
  • Fallon, L.J., Searching for extended Pair Halo emission (2010) 25th Texas Symposium on Relativistic Astrophysics, 192
  • Fernandez Alonso, M., (2014) Search for Extended Gamma Ray Emission in Markarian 421 Using VERITAS Observations, , ArXiv e-prints 1406. 4764
  • Acharya, B.S., Introducing the CTA concept (2013) Astroparticle Physics, 43, pp. 3-18
  • Kachelrieß, M., Ostapchenko, S., Tomas, R., ELMAG: A Monte Carlo simulation of electromagnetic cascades on the extragalactic background light and in magnetic fields (2012) Computer Physics Communications, 183, p. 1036
  • Dolag, K., (2010) Lower Limit on the Strength and Filling Factor of Extragalactic Magnetic Fields, , ArXiv e-prints 1009. 1782v2
  • Stecker, F.W., Scully, S.T., The spectrum of 1ES0229+200 and the cosmic infrared background (2008) A+A, 478, pp. L1-L3
  • Dolag, K., Lower limit on the strength and filling factor of extragalactic magnetic fields (2011) ApJ, 727, p. L4
  • Charbonnier, A., Dark matter profiles and annihilation in dwarf spheroidal galaxies: Prospectives for present and future g-ray observatories-I. The classical dwarf spheroidal galaxies (2011) MNRAS, 418, p. 1526
  • Aharonian, F., Akhperjanian, A.G., Observations of the Crab nebula with HESS (2006) A+A, 457, p. 899
  • Taylor, A.M., Vovk, I., Neronov, A., Extragalactic magnetic fields constraints from simultaneous GeV-TeV observations of blazars (2011) A+A, 529, p. 144
  • Daum, A., First results on the performance of the HEGRA IACT array (1997) Astroparticle Physics, 8, pp. 1-11
  • Frodesen, A.G., Skjeggestad, O., (1979) Probability and Statistics in Particle Physics, , Universitetsforlaget, NorwayA4 -

Citas:

---------- APA ----------
Alonso, M.F., Supanitsky, A.D. & Rovero, A.C. (2015) . Detecting extended gamma-ray emission with the next generation Cherenkov telescopes. 34th International Cosmic Ray Conference, ICRC 2015, 30-July-2015.
Recuperado de https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_18248039_v30-July-2015_n_p_Alonso [ ]
---------- CHICAGO ----------
Alonso, M.F., Supanitsky, A.D., Rovero, A.C. "Detecting extended gamma-ray emission with the next generation Cherenkov telescopes" . 34th International Cosmic Ray Conference, ICRC 2015 30-July-2015 (2015).
Recuperado de https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_18248039_v30-July-2015_n_p_Alonso [ ]
---------- MLA ----------
Alonso, M.F., Supanitsky, A.D., Rovero, A.C. "Detecting extended gamma-ray emission with the next generation Cherenkov telescopes" . 34th International Cosmic Ray Conference, ICRC 2015, vol. 30-July-2015, 2015.
Recuperado de https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_18248039_v30-July-2015_n_p_Alonso [ ]
---------- VANCOUVER ----------
Alonso, M.F., Supanitsky, A.D., Rovero, A.C. Detecting extended gamma-ray emission with the next generation Cherenkov telescopes. Proc. Sci. 2015;30-July-2015.
Available from: https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_18248039_v30-July-2015_n_p_Alonso [ ]