SOME OF MY WORK
A study of the polarization of the Cherenkov Radiation in
Extensive Air Showers of Energy around 1 TeV.
Work developed for the MSC course of the Universidad Complutense de
Madrid.
How to make a reference to this work:
I. de la Calle et
al. 1999, FAMN 3/99, Universidad Complutense de Madrid, Spain.
- Portada.ps (46 Kb.)
- Contents.ps (237 Kb.)
- Introduction
( Introduction.ps (31 Kb.))
- Physical Basis
( Chapter1.ps (11.800 Kb.))
- Cherenkov Radiation
- Extensive Air Showers
- Cherenkov Radiation in EAS
-
- The Imaging Atmospheric Cherenkov Technique
( Chapter2.ps (11.852 Kb.))
- Cherenkov Telescopes
- Gamma/hadron Separation Technique
- Image Parameters
- Image Moment Estimation
- Image Parameters in the context of the Gamma/hadron
Separation Method
- On the Use of Polarization in IACTs
( Chapter3.ps (799 Kb.))
- Basic Physical Ideas
- Implications
- Operational Setup
( Chapter4.ps (772 Kb.))
- Introduction
- Extensive Air Showers Simulation
- CORSIKA Physics
- Cherenkov Radiation in CORSIKA
- CORSIKA parameters and applied modifications
- Detector Simulation
- Ray Tracing
- Light of the Night Sky
- Image Analysis
- Monte Carlo Data Base
- Results
( Chapter5.ps (2.634 Kb.))
- General Characteristics
- Energy Threshold
- Image Parameters
- Conclucions
( Chapter6.ps (242 Kb.))
- Bibliography
( Bibliography.ps (241 Kb.))
- List of Figures
( Figures.ps (265 Kb.))
- List of Tables
( Tables.ps (236 Kb.))
Latest Version: 29 September 1999
Complete Document (compressed file):
tesina.ps.gz (5.421 Kb.)
(
To uncompress the file once you unload it, type: gunzip tesina.ps.gz
)
Publications

A study of the polarization of the Cherenkov Radiation in Extensive Air Showers of Energy around 1 TeV.
Authors: J.L.Contreras, I. de la Calle, J.Cortina
Dpto. de Física Atómica de Ciencias Físicas, Universidad Complutense, E-28040 Madrid. Spain.
The polarization of the emitted Cherenkov Light is one of the less studied features of Extensive Air Showers (EAS), even though it is known to carry important information on topics such as gamma-hadron separation. By means of an Air Shower Monte Carlo simulation we have studied some of the characteristics of the net polarization of Cherenkov Light, for incident particles of energy around 1 TeV. An experimental setup that could be used on Imaging Atmospheric Cherenkov Telescopes, to take advantage of the information contained in the Cherenkov Light polarization, is presented and discussed.
Presented as a Poster in the 16th European Cosmic Ray Simposium in Alcalá de Henares, Madrid, July 20-24, 1998.
Postscript file: Polarization.ps
(384 Kb.)

A study of the effect of polarizing filters in Imaging Cherenkov Telescopes
Authors: I. de la Calle, J.L.Contreras, V.Fonseca
Dpto. de Física Atómica de Ciencias Físicas, Universidad Complutense, E-28040 Madrid. Spain.
In this contribution we study the net polarization of the Cherenkov Light
emitted in Extensive Air Showers of energy around 1 TeV, by means of an Air
Shower Monte Carlo simulation. The study investigates the modification of the
Hillas image parameters and telescope performance due to a particular
arrangement of polarizing filters in front of the camera of a Cherenkov
Telescope.
Presented as a Poster in the TeV Workshop in Snowbird,
Utah 1999.
Postscript file with the poster:
poster.ps (825 Kb.)
Postscript file with the proceedings:
proceed.ps (237 Kb.)

A possible use for polarizers in Imaging Atmospheric Cherenkov
Telescopes.
Authors: I. de la Calle, J.L.Contreras, J. Cortina,
V.Fonseca
University of Leeds, Department of Physics and Astronomy, LS2 9JT Leeds, UK
Dpto. de Física Atómica de Ciencias Físicas, Universidad Complutense, E-28040 Madrid. Spain.
Cherenkov radiation produced in Extensive Air
Showers shows a net polarization. This article discusses its properties
and physical origin, and proposes an arrangement of polarizers potentially
useful for Imaging Atmospheric Cherenkov Telescopes.
Astorparticle Physics, Vol/Issue 17/2, pp.133-149, 2002.
(astro-ph/0107271)
Other Related C-Polarization References
Authors:
A.K.Tickoo, M.Kothari, H.C.Goyal, V.K.Dhar, R.Koul, S.K.Kaul, R.C.Rannot,
R.K.Kaul, A.Haungs, H.Rebel and C.L.Bhat
Bhabha Atomic Research Centre, Nuclear Research Laboratory,
Trombay, Mumbai-400085, India
Authors:
Bhat, C. L.; Rannot, R. C.; Mahapatra, D. K.; Gandhi, V. N.; Tickoo, A. K.;
Kaul, R.; Kaul, S. K.; Kaul, S. R. Goyal, H. C.; Bhatt, N.
Bhabha Atomic Research Centre, Nuclear Research Laboratory,
Trombay, Mumbai-400085, India
Ref:
Bulletin of the Astronomical Society of India, vol. 27, p.343.
My Current Work
Currently I am working at the Universtity of
Leeds in the Department of physics and
Astronomy inside the Whipple Group
. I joint the gruop in October 1999.
At the moment I am working in the development of the analog transport
of a signal throught a fiber optic system
and its application to the Atmospheric Cherenkov Telescopes.

Design and performance of analog fiber optic links used on the
Whipple 10 metre air Cherenkov telescope.
Authors:I. H. Bond, S. M. Bradbury, I. de la Calle,
P. A. Ogden, H. J. Rose and T. C. Weekes
University of Leeds, Department of Physics and Astronomy, LS2
9JT Leeds, UK
Whipple Observatory, Harvard-Smithsonian Center for
Astrophysics, P.O. Box 97, Amado, AZ 85645-0097, USA
The use of fiber optics instead of coaxial cable for signal transmission can
reduce pulse dispersion and attenuation and so will allow a shorter ADC gate
to be used. Results indicate that the night sky background component could be
reduced by ~25 %. A prototype system of links has been installed on the
Whipple 10 m air Cherenkov telescope and the performance has been assessed
over one year of operation. The bandwidth is 150 MHz and the dynamic range of
the output is from 2 mV to 1 mV. The average gain of the 120 channels is 4.1
and is stable to within a few percent over a typical 3 week observation
period. The baseline noise level is 0.5 mV rms but this can increase to 6
mV amplituede at certain resonance points in the value of the laser bias
current. The deviation from true linearity is typically less than 7% .
To be presented at the 2001 ICRC Hamburg, Germany.

Search for TeV Gamma Ray emission from 4C39.12 with the Whipple
10 metre Cherenkov Telescope
Authors:I. de la Calle and S. M. Bradbury for the VERITAS
collaboration.
University of Leeds, Department of Physics and Astronomy, LS2
9JT Leeds, UK
Among others, the Whipple telescope has been used over the past decade in the
search for VHE emission from BL Lacertae objects applying different target
selection criteria. Here we report on a new candidate, 4C39.12, a radio
selected source in 408 the MHz B2 survey which includes Mrk421 and
Mrk501. Given its low redshift (z=0.02), the close similarities to Mrk421 and
Mrk501 and the recent identification of a relativistic jet at a small angle
with respect to the line of sight (0 < 45 deg) 4C39.12 is a fair
candidate for VHE emission. This object has not been catalogued by EGRET but
it is detected by ROSAT at a level consistent with non-thermal emission from
the core and is classified as an X-ray selected BL Lac in some references.
Over a period of 5 months the Whipple Telescope has been monitoring the object
for evidence of emission above 300 GeV. A 99.99 % confidence upper limit to the
flux is derived from these observations.
To be presented at the 2001 ICRC Hamburg, Germany.
Group Publications
HEGRA
The time averaged TeV energy spectrum of Mkn 501 of the extraordinary 1997
outburst as measured with the stereoscopic Cherenkov telescope system of
HEGRA.
F.A. Aharonian, A.G. Akhperjanian, J.A. Barrio, K. Bernlohr, H. Bojahr,
I. Calle, J.L. Contreras, J. Cortina, A. Daum, T. Deckers,
S. Denninghoff, V. Fonseca, J.C. Gonzalez, G. Heinzelmann, M. Hemberger,
G. Hermann, M. Heb, A. Heusler, W. Hofmann, H. Hohl, D. Horns, A. Ibarra,
R. Kankanyan, J. Kettler, C. Kohler, A. Konopelko, H. Kornmeyer, M. Kestel,
D. Kranich, H. Krawczynski, H. Lampeitl, A. Lindner, E. Lorenz, N. Magnussen,
H. Meyer, R. Mirzoyan, A. Moralejo, L. Padilla, M. Panter, D. Petry, R. Plaga,
A. Plyasheshnikov, J. Prahl, G. Puhlhofer, G. Rauterberg, C. Renault,
W. Rhode, A. Rohring, V. Sahakian, M. Samorski, D. Schmele, F. Schroder,
W. Stamm, H.J. Volk, B. Wiebel-Sooth, C. Wiedner, M. Willmer, W. Wittek
Ref:1999A&A...349...11A.
Correlated intense X-Ray and TeV activity of Mkn 501 in 1998 june.
F.A. Aharonian, A.G. Akhperjanian, J.A. Barrio, K. Bernlohr, H. Bojahr,
I. Calle , J.L. Contreras, J. Cortina, A. Daum, T. Deckers,
S. Denninghoff, V. Fonseca, J.C. Gonzalez, G. Heinzelmann, M. Hemberger,
G. Hermann, M. Heb, A. Heusler, W. Hofmann, H. Hohl, D. Horns, A. Ibarra,
R. Kankanyan, J. Kettler, C. Kohler, A. Konopelko, H. Kornmeyer,
M. Kestel, D. Kranich, H. Krawczynski, H. Lampeitl, A. Lindner, E. Lorenz,
N. Magnussen, H. Meyer, R. Mirzoyan, A. Moralejo, L. Padilla, M. Panter,
D. Petry, R. Plaga, A. Plyasheshnikov, J. Prahl, G. Puhlhofer,
G. Rauterberg, C. Renault, W. Rhode, A. Rohring, V. Sahakian, M. Samorski,
D. Schmele, F. Schroder, W. Stamm, H.J. Volk, B. Wiebel-Sooth, C. Wiedner,
M. Willmer, W. Wittek
Ref:2000ApJ...538..127S.
The temporal characteristics of the TeV -emission from Mkn 501 in 1997.
II. Results from HEGRA CT1 and CT2.
F. Aharonian, A.G. Akhperjanian, J.A. Barrio, K. Bernlohr, H. Bojahr,
I. Calle, J.L. Contreras, J. Cortina, A. Daum, T. Deckers,
S. Denninghoff, V. Fonseca, J. Gebauer, J.C. Gonzalez, G. Heinzelmann,
M. Hemberger, G. Hermann, M. Hess, A. Heusler, W. Hofmann, H. Hohl,
D. Horns, A. Ibarra, R. Kankanyan, M. Kestel, O. Kirstein, C. Kohler,
H. Kornmayer, D. Kranich, H. Krawczynski, H. Lampeitl, A. Lindner,
E. Lorenz, N. Magnussen, H. Meyer, R. Mirzoyan, A. Moralejo, L. Padilla,
M. Panter, D. Petry, R. Plaga, A. Plyasheshnikov, J. Prahl, G. Puhlhofer,
G. Rauterberg, C. Renault, W. Rhode, A. Rohring, V. Sahakian, M. Samorski,
D. Schmele, F. Schroder, W. Stamm, B. Wiebel-Sooth, C. Wiedner, M. Willmer,
H. Wirth, W. Wittek
Ref:1999A&A...349...29A.
Energy Spectrum and Chemical Composition of Cosmic Rays between 0.3 and 10 PeV
determined from the Cherenkov-Light and Charged-Particle distribution in Air Showers.
F. Aharonian, A.G. Akhperjanian, F.Arqueros, J.A. Barrio, K. Bernlohr, H. Bojahr,
I. Calle, J.L. Contreras, J. Cortina, A. Daum, T. Deckers,
S. Denninghoff, V. Fonseca, J. Gebauer, J.C. Gonzalez, G. Heinzelmann,
M. Hemberger, G. Hermann, M. Hess, A. Heusler, W. Hofmann, H. Hohl,
D. Horns, A. Ibarra, R. Kankanyan, M. Kestel, O. Kirstein, C. Kohler,
H. Kornmayer, D. Kranich, H. Krawczynski, H. Lampeitl, A. Lindner,
E. Lorenz, N. Magnussen, H. Meyer, R. Mirzoyan, A. Moralejo, L. Padilla,
M. Panter, D. Petry, R. Plaga, A. Plyasheshnikov, J. Prahl, G. Puhlhofer,
G. Rauterberg, C. Renault, W. Rhode, A. Rohring, V. Sahakian, M. Samorski,
D. Schmele, F. Schroder, W. Stamm, H. Volk, B. Wiebel-Sooth, C. Wiedner, M. Willmer,
H. Wirth, W. Wittek
Ref:2000A&A...359..682H.
Observations of Mkn 421 during 1997 and 1998 in the energy range above 500 GeV
with HEGRA stereoscopic Cherenkov telescope system
F. Aharonian, A.G. Akhperjanian, J.A. Barrio, K. Bernlohr, H. Bojahr,
I. Calle, J.L. Contreras, J. Cortina, A. Daum, T. Deckers,
S. Denninghoff, V. Fonseca, J. Gebauer, J.C. Gonzalez, G. Heinzelmann,
M. Hemberger, G. Hermann, M. Hess, A. Heusler, W. Hofmann, H. Hohl,
D. Horns, A. Ibarra, R. Kankanyan, M. Kestel, O. Kirstein, C. Kohler,
H. Kornmayer, D. Kranich, H. Krawczynski, H. Lampeitl, A. Lindner,
E. Lorenz, N. Magnussen, H. Meyer, R. Mirzoyan, A. Moralejo, L. Padilla,
M. Panter, D. Petry, R. Plaga, A. Plyasheshnikov, J. Prahl, G. Puhlhofer,
G. Rauterberg, C. Renault, W. Rhode, A. Rohring, V. Sahakian, M. Samorski,
D. Schmele, F. Schroder, W. Stamm, H. Volk, B. Wiebel-Sooth, C. Wiedner, M. Willmer,
H. Wirth, W. Wittek
Ref:1999A&A...350..757A.
Constrains on BL Lac objects by the HEGRA-system of Cherenkov telescopes.
F. Aharonian, A.G. Akhperjanian, J.A. Barrio, K. Bernlohr, H. Bojahr,
I. Calle, J.L. Contreras, J. Cortina, A. Daum, T. Deckers,
S. Denninghoff, V. Fonseca, J. Gebauer, J.C. Gonzalez, G. Heinzelmann,
M. Hemberger, G. Hermann, M. Hess, A. Heusler, W. Hofmann, H. Hohl,
D. Horns, A. Ibarra, R. Kankanyan, M. Kestel, O. Kirstein, C. Kohler,
H. Kornmayer, D. Kranich, H. Krawczynski, H. Lampeitl, A. Lindner,
E. Lorenz, N. Magnussen, H. Meyer, R. Mirzoyan, A. Moralejo, L. Padilla,
M. Panter, D. Petry, R. Plaga, A. Plyasheshnikov, J. Prahl, G. Puhlhofer,
G. Rauterberg, C. Renault, W. Rhode, A. Rohring, V. Sahakian, M. Samorski,
D. Schmele, F. Schroder, W. Stamm, H. Volk, B. Wiebel-Sooth, C. Wiedner, M. Willmer,
H. Wirth, W. Wittek
Ref:A&A (?)
HEGRA search for TeV emission from BL Lac objects.
F. Aharonian, A.G. Akhperjanian, J.A. Barrio, K. Bernlohr, H. Bojahr,
I. Calle, J.L. Contreras, J. Cortina, A. Daum, T. Deckers,
S. Denninghoff, V. Fonseca, J.C. Gonzalez, G. Heinzelmann,
M. Hemberger, G. Hermann, M. Heb, A. Heusler, W. Hofmann, H. Hohl,
D. Horns, A. Ibarra, R. Kankanyan, J. Kettler, C. Kohler, A. Konopelko,
H. Kornmayer, D. Kranich, H. Krawczynski, H. Lampeitl, A. Lindner,
E. Lorenz, N. Magnussen, H. Meyer, R. Mirzoyan, A. Moralejo, L. Padilla,
M. Panter, D. Petry, R. Plaga, A. Plyasheshnikov, J. Prahl, G. Puhlhofer,
G. Rauterberg, C. Renault, W. Rhode, A. Rohring, V. Sahakian, M. Samorski,
D. Schmele, F. Schroder, W. Stamm, H. Volk, B. Wiebel-Sooth, C. Wiedner,
M. Willmer, W. Wittek
Ref:2000A&A...353..847A
The Energy of TeV Gamma-Rays from the Crab Nebula as measured by the HEGRA
system of imaging air Cherenkov telescopes.
F. Aharonian, A.G. Akhperjanian, J.A. Barrio, K. Bernlohr, H. Bojahr,
I. Calle, J.L. Contreras, J. Cortina, A. Daum, T. Deckers,
S. Denninghoff, V. Fonseca, J. Gebauer, J.C. Gonzalez, G. Heinzelmann,
M. Hemberger, G. Hermann, M. Hess, A. Heusler, W. Hofmann, H. Hohl, D. Horns,
A. Ibarra, R. Kankanyan, M. Kestel, O. Kirstein, C. Kohler, H. Kornmayer,
D. Kranich, H. Krawczynski, H. Lampeitl, A. Lindner, E. Lorenz, N. Magnussen,
H. Meyer, R. Mirzoyan, A. Moralejo, L. Padilla, M. Panter, D. Petry, R. Plaga,
A. Plyasheshnikov, J. Prahl, G. Puhlhofer, G. Rauterberg, C. Renault,
W. Rhode, A. Rohring, V. Sahakian, M. Samorski, D. Schmele, F. Schroder,
W. Stamm, H. Volk, B. Wiebel-Sooth, C. Wiedner, M. Willmer, W. Wittek
Ref:2000ApJ...539..317A
An experimental limit on the size of the emission region for VHE gamma rays in
the Crab Nebula.
F. Aharonian, A.G. Akhperjanian, J.A. Barrio, K. Bernlohr, H. Bojahr,
I. Calle, J.L. Contreras, J. Cortina, A. Daum, T. Deckers,
S. Denninghoff, V. Fonseca, J.C. Gonzalez, N. Gotting, G. Heinzelmann,
M. Hemberger, G. Hermann, M. Hess, A. Heusler, W. Hofmann, H. Hohl, D. Horns,
A. Ibarra, R. Kankanyan, J. Kettle, C. Kohler, A. Konpelko, H. Kornmayer,
M. Kestel, D. Kranich, H. Krawczynski, H. Lampeitl, A. Lindner, E. Lorenz,
N. Magnussen, O. Mang, H. Meyer, R. Mirzoyan, A. Moralejo, L. Padilla,
M. Panter, D. Petry, R. Plaga, A. Plyasheshnikov, J. Prahl, G. Puhlhofer,
G. Rauterberg, C. Renault, W. Rhode, A. Rohring, V. Sahakian, M. Samorski,
M. Schilling, F. Schroder, W. Stamm, M. Tluczykont, H. Volk, B. Wiebel-Sooth,
C. Wiedner, M. Willmer, W. Wittek
Ref: A&A (?)
Cosmic Ray Proton Spectrum determined with the Imaging Atmospheric Cherenkov
Technique.
F. Aharonian, A. G. Akhperjanian, J. A. Barrio, A. S. Belgarian,
K. Bernlohr, J. J. G. Beteta, H. Bojahr, S. Bradbury, I. Calle,
J. L. Contreras, J. Cortina, A. Daum, T. Deckers, S. Denninghoff,
V. Fonseca, J. C. Gonzalez, G. Heinzelmann, M. Hemberger, G. Hermann,
M. Hess, A. Heusler, W. Hofmann, H. Hohl, I. Holl, D. Horns, A. Ibarra,
R. Kankanyan, M. Kestel, O. Kirstein, C. Kohler, A. Konopelko,
H. Kornmeyer, D. Kranich, H. Krawczynski, H. Lampeitl, A. Lindner,
E. Lorenz, N. Magnussen, H. Meyer, R. Mirzoyan, A. Moralejo, L. Padilla,
M. Panter, D. Petry, R. Plaga, A. Plyasheshnikov, J. Prahl, C. Prosch,
G. Puhlhofer, G. Rauterberg, C. Renault, W. Rhode, A. Rohring,
V. Sahakian, M. Samorski, D. Schmele, F. Schroder, W. Stamm, H. J. Volk,
B. Wiebel-Sooth, C. A. Wiedner, M. Willmer, and H. Wirth
Ref: Phys. Rev. D 59, 092003 (1999)
WHIPPLE
[6~
Cutoff in the TeV Energy Spectrum of Markarian 421 During Strong Flares in 2001
F. Krennrich, H.M. Badran, I.H. Bond, S.M. Bradbury, J.H. Buckley,
D.A. Carter-Lewis, M. Catanese, W. Cui, S. Dunlea, D. Das, I. de la Calle
Perez, D.J. Fegan, S.J. Fegan, J.P. Finley, J.A. Gaidos, K. Gibbs,
G.H. Gillanders, T.A. Hall, A.M. Hillas, J. Holder, D. Horan, M. Jordan, M.
Kertzman, D. Kieda, J. Kildea, J. Knapp, K. Kosack, M.J. Lang, S. LeBohec,
B. McKernan, P. Moriarty, D. Müller, R. Ong, R. Pallassini, D. Petry, J.
Quinn, N.W. Reay, P.T. Reynolds, H.J. Rose, G.H. Sembroski, R. Sidwell,
N. Stanton, S.P. Swordy, V.V. Vassiliev, S.P. Wakely, T.C. Weekes
Ref: Accepted in ApJL (2001)
Detection of the BL Lac Object 1H1426+428 at TeV Gamma Ray Energies.
D. Horan, H.M. Badran, I.H. Bond, S.M. Bradbury, J.H. Buckley,
D.A. Carter-Lewis, M. Catanese, W. Cui, S. Dunlea, D. Das, I. de la
Calle Perez, D.J. Fegan, S.J. Fegan, J.P. Finley, J.A. Gaidos, K. Gibbs,
G.H. Gillanders, T.A. Hall, A.M. Hillas, J. Holder, D. Horan, M. Jordan,
M. Kertzman, D. Kieda, J. Kildea, J. Knapp, K. Kosack, M.J. Lang,
S. LeBohec, B. McKernan, P. Moriarty, D. M|ller, R. Ong, R. Pallassini,
D. Petry, J. Quinn, N.W. Reay, P.T. Reynolds, H.J. Rose, G.H. Sembroski,
R. Sidwell, N. Stanton, S.P. Swordy, V.V. Vassiliev, S.P. Wakely, T.C. Weekes
Ref: Accepted in ApJ (2002)
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