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Title: MAGIC upper limits on the GRB 090102 afterglow

Abstract

Indications of a GeV component in the emission from gamma-ray bursts (GRBs) are known since the Energetic Gamma-Ray Experiment Telescope observations during the 1990s and they have been confirmed by the data of the Fermi satellite. Our results have, however, shown that our understanding of GRB physics is still unsatisfactory. The new generation of Cherenkov observatories and in particular the MAGIC telescope, allow for the first time the possibility to extend the measurement of GRBs from several tens up to hundreds of GeV energy range. Both leptonic and hadronic processes have been suggested to explain the possible GeV/TeV counterpart of GRBs. Observations with ground-based telescopes of very high energy (VHE) photons (E > 30 GeV) from these sources are going to play a key role in discriminating among the different proposed emission mechanisms, which are barely distinguishable at lower energies. MAGIC telescope observations of the GRB 090102 (z = 1.547) field and Fermi Large Area Telescope data in the same time interval are analysed to derive upper limits of the GeV/TeV emission. We compare these results to the expected emissions evaluated for different processes in the framework of a relativistic blastwave model for the afterglow. Simultaneous upper limits with Fermimore » and a Cherenkov telescope have been derived for this GRB observation. We obtained results compatible with the expected emission although the difficulties in predicting the HE and VHE emission for the afterglow of this event makes it difficult to draw firmer conclusions. Nonetheless, MAGIC sensitivity in the energy range of overlap with space-based instruments (above about 40 GeV) is about one order of magnitude better with respect to Fermi. This makes evident the constraining power of ground-based observations and shows that the MAGIC telescope has reached the required performance to make possible GRB multiwavelength studies in the VHE range.« less

Authors:
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Publication Date:
Research Org.:
SLAC National Accelerator Laboratory (SLAC), Menlo Park, CA (United States)
Sponsoring Org.:
USDOE
Contributing Org.:
Fermi LAT Collaboration
OSTI Identifier:
1356537
Grant/Contract Number:  
AC02-76SF00515
Resource Type:
Accepted Manuscript
Journal Name:
Monthly Notices of the Royal Astronomical Society
Additional Journal Information:
Journal Volume: 437; Journal Issue: 4; Journal ID: ISSN 0035-8711
Publisher:
Royal Astronomical Society
Country of Publication:
United States
Language:
English
Subject:
79 ASTRONOMY AND ASTROPHYSICS; radiation mechanisms: non-thermal; gamma-ray burst: general

Citation Formats

Aleksic, J., Ansoldi, S., Antonelli, L. A., Antoranz, P., Babic, A., de Almeida, U. B., Barrio, J. A., Gonzalez, J. B., Bednarek, W., Berger, K., Bernardini, E., Biland, A., Blanch, O., Bock, R. K., Boller, A., Bonnefoy, S., Bonnoli, G., Borracci, F., Bretz, T., Carmona, E., Carosi, A., Fidalgo, D. C., Colin, P., Colombo, E., Contreras, J. L., Cortina, J., Cossio, L., Covino, S., Da Vela, P., Dazzi, F., De Angelis, A., De Caneva, G., De Lotto, B., Mendez, C. D., Doert, M., Dominguez, A., Prester, D. D., Dorner, D., Doro, M., Eisenacher, D., Elsaesser, D., Farina, E., Ferenc, D., Fonseca, M. V., Font, L., Frantzen, K., Fruck, C., Lopez, R. J. G., Garczarczyk, M., Terrats, D. G., Gaug, M., Giavitto, G., Godinovic, N., Munoz, A. G., Gozzini, S. R., Hadamek, A., Hadasch, D., Herrero, A., Hose, J., Hrupec, D., Idec, W., Kadenius, V., Knoetig, M. L., Krahenbuhl, T., Krause, J., Kushida, J., Barbera, A. L., Lelas, D., Lewandowska, N., Lindfors, E., Lombardi, S., Lopez-Coto, R., Lopez, M., Lopez-Oramas, A., Lorenz, E., Lozano, I., Makariev, M., Mallot, K., Maneva, G., Mankuzhiyil, N., Mannheim, K., Maraschi, L., Marcote, B., Mariotti, M., Martinez, M., Masbou, J., Mazin, D., Menzel, U., Meucci, M., Miranda, J. M., Mirzoyan, R., Moldon, J., Moralejo, A., Munar-Adrover, P., Nakajima, D., Niedzwiecki, A., Nilsson, K., Nowak, N., Orito, R., Overkemping, A., Paiano, S., Palatiello, M., Paneque, D., Paoletti, R., Paredes, J. M., Partini, S., Persic, M., Prada, F., Moroni, P. G. P., Prandini, E., Preziuso, S., Puljak, I., Reichardt, I., Reinthal, R., Rhode, W., Ribo, M., Rico, J., Garcia, J. R., Rugamer, S., Saggion, A., Saito, K., Saito, T., Salvati, M., Satalecka, K., Scalzotto, V., Scapin, V., Schultz, C., Schweizer, T., Shore, S. N., Sillanpaa, A., Sitarek, J., Snidaric, I., Sobczynska, D., Spanier, F., Stamatescu, V., Stamerra, A., Storz, J., Sun, S., Suric, T., Takalo, L., Tavecchio, F., Temnikov, P., Terzic, T., Tescaro, D., Teshima, M., Thaele, J., Tibolla, O., Torres, D. F., Toyama, T., Treves, A., Uellenbeck, M., Vogler, P., Wagner, R. M., Weitzel, Q., Zandanel, F., Zanin, R., Bouvier, A., Hayashida, M., Tajima, H., and Longo, F. MAGIC upper limits on the GRB 090102 afterglow. United States: N. p., 2013. Web. doi:10.1093/mnras/stt2041.
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Aleksic, J., Ansoldi, S., Antonelli, L. A., Antoranz, P., Babic, A., de Almeida, U. B., Barrio, J. A., Gonzalez, J. B., Bednarek, W., Berger, K., Bernardini, E., Biland, A., Blanch, O., Bock, R. K., Boller, A., Bonnefoy, S., Bonnoli, G., Borracci, F., Bretz, T., Carmona, E., Carosi, A., Fidalgo, D. C., Colin, P., Colombo, E., Contreras, J. L., Cortina, J., Cossio, L., Covino, S., Da Vela, P., Dazzi, F., De Angelis, A., De Caneva, G., De Lotto, B., Mendez, C. D., Doert, M., Dominguez, A., Prester, D. D., Dorner, D., Doro, M., Eisenacher, D., Elsaesser, D., Farina, E., Ferenc, D., Fonseca, M. V., Font, L., Frantzen, K., Fruck, C., Lopez, R. J. G., Garczarczyk, M., Terrats, D. G., Gaug, M., Giavitto, G., Godinovic, N., Munoz, A. G., Gozzini, S. R., Hadamek, A., Hadasch, D., Herrero, A., Hose, J., Hrupec, D., Idec, W., Kadenius, V., Knoetig, M. L., Krahenbuhl, T., Krause, J., Kushida, J., Barbera, A. L., Lelas, D., Lewandowska, N., Lindfors, E., Lombardi, S., Lopez-Coto, R., Lopez, M., Lopez-Oramas, A., Lorenz, E., Lozano, I., Makariev, M., Mallot, K., Maneva, G., Mankuzhiyil, N., Mannheim, K., Maraschi, L., Marcote, B., Mariotti, M., Martinez, M., Masbou, J., Mazin, D., Menzel, U., Meucci, M., Miranda, J. M., Mirzoyan, R., Moldon, J., Moralejo, A., Munar-Adrover, P., Nakajima, D., Niedzwiecki, A., Nilsson, K., Nowak, N., Orito, R., Overkemping, A., Paiano, S., Palatiello, M., Paneque, D., Paoletti, R., Paredes, J. M., Partini, S., Persic, M., Prada, F., Moroni, P. G. P., Prandini, E., Preziuso, S., Puljak, I., Reichardt, I., Reinthal, R., Rhode, W., Ribo, M., Rico, J., Garcia, J. R., Rugamer, S., Saggion, A., Saito, K., Saito, T., Salvati, M., Satalecka, K., Scalzotto, V., Scapin, V., Schultz, C., Schweizer, T., Shore, S. N., Sillanpaa, A., Sitarek, J., Snidaric, I., Sobczynska, D., Spanier, F., Stamatescu, V., Stamerra, A., Storz, J., Sun, S., Suric, T., Takalo, L., Tavecchio, F., Temnikov, P., Terzic, T., Tescaro, D., Teshima, M., Thaele, J., Tibolla, O., Torres, D. F., Toyama, T., Treves, A., Uellenbeck, M., Vogler, P., Wagner, R. M., Weitzel, Q., Zandanel, F., Zanin, R., Bouvier, A., Hayashida, M., Tajima, H., & Longo, F. MAGIC upper limits on the GRB 090102 afterglow. United States. https://doi.org/10.1093/mnras/stt2041
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Aleksic, J., Ansoldi, S., Antonelli, L. A., Antoranz, P., Babic, A., de Almeida, U. B., Barrio, J. A., Gonzalez, J. B., Bednarek, W., Berger, K., Bernardini, E., Biland, A., Blanch, O., Bock, R. K., Boller, A., Bonnefoy, S., Bonnoli, G., Borracci, F., Bretz, T., Carmona, E., Carosi, A., Fidalgo, D. C., Colin, P., Colombo, E., Contreras, J. L., Cortina, J., Cossio, L., Covino, S., Da Vela, P., Dazzi, F., De Angelis, A., De Caneva, G., De Lotto, B., Mendez, C. D., Doert, M., Dominguez, A., Prester, D. D., Dorner, D., Doro, M., Eisenacher, D., Elsaesser, D., Farina, E., Ferenc, D., Fonseca, M. V., Font, L., Frantzen, K., Fruck, C., Lopez, R. J. G., Garczarczyk, M., Terrats, D. G., Gaug, M., Giavitto, G., Godinovic, N., Munoz, A. G., Gozzini, S. R., Hadamek, A., Hadasch, D., Herrero, A., Hose, J., Hrupec, D., Idec, W., Kadenius, V., Knoetig, M. L., Krahenbuhl, T., Krause, J., Kushida, J., Barbera, A. L., Lelas, D., Lewandowska, N., Lindfors, E., Lombardi, S., Lopez-Coto, R., Lopez, M., Lopez-Oramas, A., Lorenz, E., Lozano, I., Makariev, M., Mallot, K., Maneva, G., Mankuzhiyil, N., Mannheim, K., Maraschi, L., Marcote, B., Mariotti, M., Martinez, M., Masbou, J., Mazin, D., Menzel, U., Meucci, M., Miranda, J. M., Mirzoyan, R., Moldon, J., Moralejo, A., Munar-Adrover, P., Nakajima, D., Niedzwiecki, A., Nilsson, K., Nowak, N., Orito, R., Overkemping, A., Paiano, S., Palatiello, M., Paneque, D., Paoletti, R., Paredes, J. M., Partini, S., Persic, M., Prada, F., Moroni, P. G. P., Prandini, E., Preziuso, S., Puljak, I., Reichardt, I., Reinthal, R., Rhode, W., Ribo, M., Rico, J., Garcia, J. R., Rugamer, S., Saggion, A., Saito, K., Saito, T., Salvati, M., Satalecka, K., Scalzotto, V., Scapin, V., Schultz, C., Schweizer, T., Shore, S. N., Sillanpaa, A., Sitarek, J., Snidaric, I., Sobczynska, D., Spanier, F., Stamatescu, V., Stamerra, A., Storz, J., Sun, S., Suric, T., Takalo, L., Tavecchio, F., Temnikov, P., Terzic, T., Tescaro, D., Teshima, M., Thaele, J., Tibolla, O., Torres, D. F., Toyama, T., Treves, A., Uellenbeck, M., Vogler, P., Wagner, R. M., Weitzel, Q., Zandanel, F., Zanin, R., Bouvier, A., Hayashida, M., Tajima, H., and Longo, F. Mon . "MAGIC upper limits on the GRB 090102 afterglow". United States. https://doi.org/10.1093/mnras/stt2041. https://www.osti.gov/servlets/purl/1356537.
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@article{osti_1356537,
title = {MAGIC upper limits on the GRB 090102 afterglow},
author = {Aleksic, J. and Ansoldi, S. and Antonelli, L. A. and Antoranz, P. and Babic, A. and de Almeida, U. B. and Barrio, J. A. and Gonzalez, J. B. and Bednarek, W. and Berger, K. and Bernardini, E. and Biland, A. and Blanch, O. and Bock, R. K. and Boller, A. and Bonnefoy, S. and Bonnoli, G. and Borracci, F. and Bretz, T. and Carmona, E. and Carosi, A. and Fidalgo, D. C. and Colin, P. and Colombo, E. and Contreras, J. L. and Cortina, J. and Cossio, L. and Covino, S. and Da Vela, P. and Dazzi, F. and De Angelis, A. and De Caneva, G. and De Lotto, B. and Mendez, C. D. and Doert, M. and Dominguez, A. and Prester, D. D. and Dorner, D. and Doro, M. and Eisenacher, D. and Elsaesser, D. and Farina, E. and Ferenc, D. and Fonseca, M. V. and Font, L. and Frantzen, K. and Fruck, C. and Lopez, R. J. G. and Garczarczyk, M. and Terrats, D. G. and Gaug, M. and Giavitto, G. and Godinovic, N. and Munoz, A. G. and Gozzini, S. R. and Hadamek, A. and Hadasch, D. and Herrero, A. and Hose, J. and Hrupec, D. and Idec, W. and Kadenius, V. and Knoetig, M. L. and Krahenbuhl, T. and Krause, J. and Kushida, J. and Barbera, A. L. and Lelas, D. and Lewandowska, N. and Lindfors, E. and Lombardi, S. and Lopez-Coto, R. and Lopez, M. and Lopez-Oramas, A. and Lorenz, E. and Lozano, I. and Makariev, M. and Mallot, K. and Maneva, G. and Mankuzhiyil, N. and Mannheim, K. and Maraschi, L. and Marcote, B. and Mariotti, M. and Martinez, M. and Masbou, J. and Mazin, D. and Menzel, U. and Meucci, M. and Miranda, J. M. and Mirzoyan, R. and Moldon, J. and Moralejo, A. and Munar-Adrover, P. and Nakajima, D. and Niedzwiecki, A. and Nilsson, K. and Nowak, N. and Orito, R. and Overkemping, A. and Paiano, S. and Palatiello, M. and Paneque, D. and Paoletti, R. and Paredes, J. M. and Partini, S. and Persic, M. and Prada, F. and Moroni, P. G. P. and Prandini, E. and Preziuso, S. and Puljak, I. and Reichardt, I. and Reinthal, R. and Rhode, W. and Ribo, M. and Rico, J. and Garcia, J. R. and Rugamer, S. and Saggion, A. and Saito, K. and Saito, T. and Salvati, M. and Satalecka, K. and Scalzotto, V. and Scapin, V. and Schultz, C. and Schweizer, T. and Shore, S. N. and Sillanpaa, A. and Sitarek, J. and Snidaric, I. and Sobczynska, D. and Spanier, F. and Stamatescu, V. and Stamerra, A. and Storz, J. and Sun, S. and Suric, T. and Takalo, L. and Tavecchio, F. and Temnikov, P. and Terzic, T. and Tescaro, D. and Teshima, M. and Thaele, J. and Tibolla, O. and Torres, D. F. and Toyama, T. and Treves, A. and Uellenbeck, M. and Vogler, P. and Wagner, R. M. and Weitzel, Q. and Zandanel, F. and Zanin, R. and Bouvier, A. and Hayashida, M. and Tajima, H. and Longo, F.},
abstractNote = {Indications of a GeV component in the emission from gamma-ray bursts (GRBs) are known since the Energetic Gamma-Ray Experiment Telescope observations during the 1990s and they have been confirmed by the data of the Fermi satellite. Our results have, however, shown that our understanding of GRB physics is still unsatisfactory. The new generation of Cherenkov observatories and in particular the MAGIC telescope, allow for the first time the possibility to extend the measurement of GRBs from several tens up to hundreds of GeV energy range. Both leptonic and hadronic processes have been suggested to explain the possible GeV/TeV counterpart of GRBs. Observations with ground-based telescopes of very high energy (VHE) photons (E > 30 GeV) from these sources are going to play a key role in discriminating among the different proposed emission mechanisms, which are barely distinguishable at lower energies. MAGIC telescope observations of the GRB 090102 (z = 1.547) field and Fermi Large Area Telescope data in the same time interval are analysed to derive upper limits of the GeV/TeV emission. We compare these results to the expected emissions evaluated for different processes in the framework of a relativistic blastwave model for the afterglow. Simultaneous upper limits with Fermi and a Cherenkov telescope have been derived for this GRB observation. We obtained results compatible with the expected emission although the difficulties in predicting the HE and VHE emission for the afterglow of this event makes it difficult to draw firmer conclusions. Nonetheless, MAGIC sensitivity in the energy range of overlap with space-based instruments (above about 40 GeV) is about one order of magnitude better with respect to Fermi. This makes evident the constraining power of ground-based observations and shows that the MAGIC telescope has reached the required performance to make possible GRB multiwavelength studies in the VHE range.},
doi = {10.1093/mnras/stt2041},
journal = {Monthly Notices of the Royal Astronomical Society},
number = 4,
volume = 437,
place = {United States},
year = {Mon Dec 09 00:00:00 EST 2013},
month = {Mon Dec 09 00:00:00 EST 2013}
}
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Performance of the MAGIC stereo system obtained with Crab Nebula data
journal, February 2012

Flux Upper Limit on Gamma-Ray Emission by GRB 050713a from MAGIC Telescope Observations
journal, March 2006

  • Albert, J.; Aliu, E.; Anderhub, H.
  • The Astrophysical Journal, Vol. 641, Issue 1
  • DOI: 10.1086/503767

MAGIC observation of the GRB 080430 afterglow
journal, July 2010

Random Forests
journal, January 2001

Limits and confidence intervals in the presence of nuisance parameters
journal, October 2005

  • Rolke, Wolfgang A.; López, Angel M.; Conrad, Jan
  • Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment, Vol. 551, Issue 2-3
  • DOI: 10.1016/j.nima.2005.05.068

miRNALoc: predicting miRNA subcellular localizations based on principal component scores of physico-chemical properties and pseudo compositions of di-nucleotides
journal, September 2020

  • Meher, Prabina Kumar; Satpathy, Subhrajit; Rao, Atmakuri Ramakrishna
  • Scientific Reports, Vol. 10, Issue 1
  • DOI: 10.1038/s41598-020-71381-4

Gamma-ray bursts in the Swift era
journal, February 2007

Observations of Gamma-Ray Bursts of Cosmic Origin
conference, January 2004

  • Klebesadel, Ray W.
  • GAMMA-RAY BURSTS: 30 YEARS OF DISCOVERY: Gamma-Ray Burst Symposium, AIP Conference Proceedings
  • DOI: 10.1063/1.1810791

The extragalactic optical-infrared background radiations, their time evolution and the cosmic photon-photon opacity
text, January 2008

H.E.S.S. Observations of the Prompt and Afterglow Phases of GRB 060602B
text, January 2008

Observation of Pulsed Gamma-rays Above 25 GeV from the Crab Pulsar with MAGIC
text, January 2008

Prospects for GRB Science with the Fermi Large Area Telescope
text, January 2009

MAGIC observation of the GRB080430 afterglow
text, January 2010

Ten per cent polarized optical emission from GRB 090102
text, January 2010

Performance of the MAGIC stereo system obtained with Crab Nebula data
text, January 2011

High Energy Spectral Components in Gamma-Ray Burst Afterglows
text, January 2001

Particle acceleration by ultra-relativistic shocks: theory and simulations
text, January 2001

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    Works referencing / citing this record:

    Search for TeV Gamma-ray Emission from GRB 100621A, an extremely bright GRB in X-rays, with H.E.S.S.
    journal, April 2014

    High-Energy Emission from Gamma-Ray Bursts
    journal, January 2012

    Physics of Gamma-Ray Bursts Prompt Emission
    journal, January 2015

    Teraelectronvolt emission from the γ-ray burst GRB 190114C
    text, January 2019

    • Bernardini, Elisa; Bhattacharya, Biswajit; Garczarczyk, Markus
    • Deutsches Elektronen-Synchrotron, DESY, Hamburg
    • DOI: 10.3204/pubdb-2019-04673

    Search for Gamma-Ray Bursts with the ARGO-YBJ Detector in Shower Mode
    journal, June 2017

    Synchrotron Self-Compton as a Likely Mechanism of Photons beyond the Synchrotron Limit in GRB 190114C
    journal, October 2019

    • Fraija, N.; Duran, R. Barniol; Dichiara, S.
    • The Astrophysical Journal, Vol. 883, Issue 2
    • DOI: 10.3847/1538-4357/ab3ec4

    Teraelectronvolt emission from the γ-ray burst GRB 190114C
    journal, November 2019

    Physics of Gamma-Ray Bursts Prompt Emission
    text, January 2015

    Search for Gamma Ray Bursts with the ARGO-YBJ Detector in Shower Mode
    text, January 2017

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