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KASCADE-Grande Limits on the Isotropic Diffuse Gamma-Ray Flux between 100 TeV and 1 EeV
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| Zeitschriftentitel: | The Astrophysical Journal |
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| In: | The Astrophysical Journal, 848, 2017, 1, S. 1 |
| Format: | E-Article |
| Sprache: | Unbestimmt |
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American Astronomical Society
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| author_facet |
Apel, W. D. Arteaga-Velázquez, J. C. Bekk, K. Bertaina, M. Blümer, J. Bozdog, H. Brancus, I. M. Cantoni, E. Chiavassa, A. Cossavella, F. Daumiller, K. Souza, V. de Pierro, F. Di Doll, P. Engel, R. Feng, Z. Fuhrmann, D. Gherghel-Lascu, A. Gils, H. J. Glasstetter, R. Grupen, C. Haungs, A. Heck, D. Hörandel, J. R. Huege, T. Kampert, K.-H. Kang, D. Klages, H. O. Link, K. Łuczak, P. Mathes, H. J. Mayer, H. J. Milke, J. Mitrica, B. Morello, C. Oehlschläger, J. Ostapchenko, S. Pierog, T. Rebel, H. Roth, M. Schieler, H. Schoo, S. Schröder, F. G. Sima, O. Toma, G. Trinchero, G. C. Ulrich, H. Weindl, A. Wochele, J. Zabierowski, J. Apel, W. D. Arteaga-Velázquez, J. C. Bekk, K. Bertaina, M. Blümer, J. Bozdog, H. Brancus, I. M. Cantoni, E. Chiavassa, A. Cossavella, F. Daumiller, K. Souza, V. de Pierro, F. Di Doll, P. Engel, R. Feng, Z. Fuhrmann, D. Gherghel-Lascu, A. Gils, H. J. Glasstetter, R. Grupen, C. Haungs, A. Heck, D. Hörandel, J. R. Huege, T. Kampert, K.-H. Kang, D. Klages, H. O. Link, K. Łuczak, P. Mathes, H. J. Mayer, H. J. Milke, J. Mitrica, B. Morello, C. Oehlschläger, J. Ostapchenko, S. Pierog, T. Rebel, H. Roth, M. Schieler, H. Schoo, S. Schröder, F. G. Sima, O. Toma, G. Trinchero, G. C. Ulrich, H. Weindl, A. Wochele, J. Zabierowski, J. |
|---|---|
| author |
Apel, W. D. Arteaga-Velázquez, J. C. Bekk, K. Bertaina, M. Blümer, J. Bozdog, H. Brancus, I. M. Cantoni, E. Chiavassa, A. Cossavella, F. Daumiller, K. Souza, V. de Pierro, F. Di Doll, P. Engel, R. Feng, Z. Fuhrmann, D. Gherghel-Lascu, A. Gils, H. J. Glasstetter, R. Grupen, C. Haungs, A. Heck, D. Hörandel, J. R. Huege, T. Kampert, K.-H. Kang, D. Klages, H. O. Link, K. Łuczak, P. Mathes, H. J. Mayer, H. J. Milke, J. Mitrica, B. Morello, C. Oehlschläger, J. Ostapchenko, S. Pierog, T. Rebel, H. Roth, M. Schieler, H. Schoo, S. Schröder, F. G. Sima, O. Toma, G. Trinchero, G. C. Ulrich, H. Weindl, A. Wochele, J. Zabierowski, J. |
| spellingShingle |
Apel, W. D. Arteaga-Velázquez, J. C. Bekk, K. Bertaina, M. Blümer, J. Bozdog, H. Brancus, I. M. Cantoni, E. Chiavassa, A. Cossavella, F. Daumiller, K. Souza, V. de Pierro, F. Di Doll, P. Engel, R. Feng, Z. Fuhrmann, D. Gherghel-Lascu, A. Gils, H. J. Glasstetter, R. Grupen, C. Haungs, A. Heck, D. Hörandel, J. R. Huege, T. Kampert, K.-H. Kang, D. Klages, H. O. Link, K. Łuczak, P. Mathes, H. J. Mayer, H. J. Milke, J. Mitrica, B. Morello, C. Oehlschläger, J. Ostapchenko, S. Pierog, T. Rebel, H. Roth, M. Schieler, H. Schoo, S. Schröder, F. G. Sima, O. Toma, G. Trinchero, G. C. Ulrich, H. Weindl, A. Wochele, J. Zabierowski, J. The Astrophysical Journal KASCADE-Grande Limits on the Isotropic Diffuse Gamma-Ray Flux between 100 TeV and 1 EeV Space and Planetary Science Astronomy and Astrophysics |
| author_sort |
apel, w. d. |
| spelling |
Apel, W. D. Arteaga-Velázquez, J. C. Bekk, K. Bertaina, M. Blümer, J. Bozdog, H. Brancus, I. M. Cantoni, E. Chiavassa, A. Cossavella, F. Daumiller, K. Souza, V. de Pierro, F. Di Doll, P. Engel, R. Feng, Z. Fuhrmann, D. Gherghel-Lascu, A. Gils, H. J. Glasstetter, R. Grupen, C. Haungs, A. Heck, D. Hörandel, J. R. Huege, T. Kampert, K.-H. Kang, D. Klages, H. O. Link, K. Łuczak, P. Mathes, H. J. Mayer, H. J. Milke, J. Mitrica, B. Morello, C. Oehlschläger, J. Ostapchenko, S. Pierog, T. Rebel, H. Roth, M. Schieler, H. Schoo, S. Schröder, F. G. Sima, O. Toma, G. Trinchero, G. C. Ulrich, H. Weindl, A. Wochele, J. Zabierowski, J. 0004-637X 1538-4357 American Astronomical Society Space and Planetary Science Astronomy and Astrophysics http://dx.doi.org/10.3847/1538-4357/aa8bb7 <jats:title>Abstract</jats:title> <jats:p>KASCADE and KASCADE-Grande were multi-detector installations to measure individual air showers of cosmic rays at ultra-high energy. Based on data sets measured by KASCADE and KASCADE-Grande, 90% C.L. upper limits to the flux of gamma<jats:italic>-</jats:italic>rays in the primary cosmic ray flux are determined in an energy range of <jats:inline-formula> <jats:tex-math> <?CDATA ${10}^{14}\mbox{--}{10}^{18}$?> </jats:tex-math> <jats:inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="apjaa8bb7ieqn1.gif" xlink:type="simple" /> </jats:inline-formula> eV. The analysis is performed by selecting air showers with a low muon content as expected for gamma-ray-induced showers compared to air showers induced by energetic nuclei. The best upper limit of the fraction of gamma-rays to the total cosmic ray flux is obtained at <jats:inline-formula> <jats:tex-math> <?CDATA $3.7\times {10}^{15}$?> </jats:tex-math> <jats:inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="apjaa8bb7ieqn2.gif" xlink:type="simple" /> </jats:inline-formula> eV with <jats:inline-formula> <jats:tex-math> <?CDATA $1.1\times {10}^{-5}$?> </jats:tex-math> <jats:inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="apjaa8bb7ieqn3.gif" xlink:type="simple" /> </jats:inline-formula>. Translated to an absolute gamma-ray flux this sets constraints on some fundamental astrophysical models, such as the distance of sources for at least one of the IceCube neutrino excess models.</jats:p> KASCADE-Grande Limits on the Isotropic Diffuse Gamma-Ray Flux between 100 TeV and 1 EeV The Astrophysical Journal |
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American Astronomical Society, 2017 |
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American Astronomical Society, 2017 |
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0004-637X 1538-4357 |
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2017 |
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The Astrophysical Journal |
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| title |
KASCADE-Grande Limits on the Isotropic Diffuse Gamma-Ray Flux between 100 TeV and 1 EeV |
| title_unstemmed |
KASCADE-Grande Limits on the Isotropic Diffuse Gamma-Ray Flux between 100 TeV and 1 EeV |
| title_full |
KASCADE-Grande Limits on the Isotropic Diffuse Gamma-Ray Flux between 100 TeV and 1 EeV |
| title_fullStr |
KASCADE-Grande Limits on the Isotropic Diffuse Gamma-Ray Flux between 100 TeV and 1 EeV |
| title_full_unstemmed |
KASCADE-Grande Limits on the Isotropic Diffuse Gamma-Ray Flux between 100 TeV and 1 EeV |
| title_short |
KASCADE-Grande Limits on the Isotropic Diffuse Gamma-Ray Flux between 100 TeV and 1 EeV |
| title_sort |
kascade-grande limits on the isotropic diffuse gamma-ray flux between 100 tev and 1 eev |
| topic |
Space and Planetary Science Astronomy and Astrophysics |
| url |
http://dx.doi.org/10.3847/1538-4357/aa8bb7 |
| publishDate |
2017 |
| physical |
1 |
| description |
<jats:title>Abstract</jats:title>
<jats:p>KASCADE and KASCADE-Grande were multi-detector installations to measure individual air showers of cosmic rays at ultra-high energy. Based on data sets measured by KASCADE and KASCADE-Grande, 90% C.L. upper limits to the flux of gamma<jats:italic>-</jats:italic>rays in the primary cosmic ray flux are determined in an energy range of <jats:inline-formula>
<jats:tex-math>
<?CDATA ${10}^{14}\mbox{--}{10}^{18}$?>
</jats:tex-math>
<jats:inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="apjaa8bb7ieqn1.gif" xlink:type="simple" />
</jats:inline-formula> eV. The analysis is performed by selecting air showers with a low muon content as expected for gamma-ray-induced showers compared to air showers induced by energetic nuclei. The best upper limit of the fraction of gamma-rays to the total cosmic ray flux is obtained at <jats:inline-formula>
<jats:tex-math>
<?CDATA $3.7\times {10}^{15}$?>
</jats:tex-math>
<jats:inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="apjaa8bb7ieqn2.gif" xlink:type="simple" />
</jats:inline-formula> eV with <jats:inline-formula>
<jats:tex-math>
<?CDATA $1.1\times {10}^{-5}$?>
</jats:tex-math>
<jats:inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="apjaa8bb7ieqn3.gif" xlink:type="simple" />
</jats:inline-formula>. Translated to an absolute gamma-ray flux this sets constraints on some fundamental astrophysical models, such as the distance of sources for at least one of the IceCube neutrino excess models.</jats:p> |
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| author | Apel, W. D., Arteaga-Velázquez, J. C., Bekk, K., Bertaina, M., Blümer, J., Bozdog, H., Brancus, I. M., Cantoni, E., Chiavassa, A., Cossavella, F., Daumiller, K., Souza, V. de, Pierro, F. Di, Doll, P., Engel, R., Feng, Z., Fuhrmann, D., Gherghel-Lascu, A., Gils, H. J., Glasstetter, R., Grupen, C., Haungs, A., Heck, D., Hörandel, J. R., Huege, T., Kampert, K.-H., Kang, D., Klages, H. O., Link, K., Łuczak, P., Mathes, H. J., Mayer, H. J., Milke, J., Mitrica, B., Morello, C., Oehlschläger, J., Ostapchenko, S., Pierog, T., Rebel, H., Roth, M., Schieler, H., Schoo, S., Schröder, F. G., Sima, O., Toma, G., Trinchero, G. C., Ulrich, H., Weindl, A., Wochele, J., Zabierowski, J. |
| author_facet | Apel, W. D., Arteaga-Velázquez, J. C., Bekk, K., Bertaina, M., Blümer, J., Bozdog, H., Brancus, I. M., Cantoni, E., Chiavassa, A., Cossavella, F., Daumiller, K., Souza, V. de, Pierro, F. Di, Doll, P., Engel, R., Feng, Z., Fuhrmann, D., Gherghel-Lascu, A., Gils, H. J., Glasstetter, R., Grupen, C., Haungs, A., Heck, D., Hörandel, J. R., Huege, T., Kampert, K.-H., Kang, D., Klages, H. O., Link, K., Łuczak, P., Mathes, H. J., Mayer, H. J., Milke, J., Mitrica, B., Morello, C., Oehlschläger, J., Ostapchenko, S., Pierog, T., Rebel, H., Roth, M., Schieler, H., Schoo, S., Schröder, F. G., Sima, O., Toma, G., Trinchero, G. C., Ulrich, H., Weindl, A., Wochele, J., Zabierowski, J., Apel, W. D., Arteaga-Velázquez, J. C., Bekk, K., Bertaina, M., Blümer, J., Bozdog, H., Brancus, I. M., Cantoni, E., Chiavassa, A., Cossavella, F., Daumiller, K., Souza, V. de, Pierro, F. Di, Doll, P., Engel, R., Feng, Z., Fuhrmann, D., Gherghel-Lascu, A., Gils, H. J., Glasstetter, R., Grupen, C., Haungs, A., Heck, D., Hörandel, J. R., Huege, T., Kampert, K.-H., Kang, D., Klages, H. O., Link, K., Łuczak, P., Mathes, H. J., Mayer, H. J., Milke, J., Mitrica, B., Morello, C., Oehlschläger, J., Ostapchenko, S., Pierog, T., Rebel, H., Roth, M., Schieler, H., Schoo, S., Schröder, F. G., Sima, O., Toma, G., Trinchero, G. C., Ulrich, H., Weindl, A., Wochele, J., Zabierowski, J. |
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| description | <jats:title>Abstract</jats:title> <jats:p>KASCADE and KASCADE-Grande were multi-detector installations to measure individual air showers of cosmic rays at ultra-high energy. Based on data sets measured by KASCADE and KASCADE-Grande, 90% C.L. upper limits to the flux of gamma<jats:italic>-</jats:italic>rays in the primary cosmic ray flux are determined in an energy range of <jats:inline-formula> <jats:tex-math> <?CDATA ${10}^{14}\mbox{--}{10}^{18}$?> </jats:tex-math> <jats:inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="apjaa8bb7ieqn1.gif" xlink:type="simple" /> </jats:inline-formula> eV. The analysis is performed by selecting air showers with a low muon content as expected for gamma-ray-induced showers compared to air showers induced by energetic nuclei. The best upper limit of the fraction of gamma-rays to the total cosmic ray flux is obtained at <jats:inline-formula> <jats:tex-math> <?CDATA $3.7\times {10}^{15}$?> </jats:tex-math> <jats:inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="apjaa8bb7ieqn2.gif" xlink:type="simple" /> </jats:inline-formula> eV with <jats:inline-formula> <jats:tex-math> <?CDATA $1.1\times {10}^{-5}$?> </jats:tex-math> <jats:inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="apjaa8bb7ieqn3.gif" xlink:type="simple" /> </jats:inline-formula>. Translated to an absolute gamma-ray flux this sets constraints on some fundamental astrophysical models, such as the distance of sources for at least one of the IceCube neutrino excess models.</jats:p> |
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| spelling | Apel, W. D. Arteaga-Velázquez, J. C. Bekk, K. Bertaina, M. Blümer, J. Bozdog, H. Brancus, I. M. Cantoni, E. Chiavassa, A. Cossavella, F. Daumiller, K. Souza, V. de Pierro, F. Di Doll, P. Engel, R. Feng, Z. Fuhrmann, D. Gherghel-Lascu, A. Gils, H. J. Glasstetter, R. Grupen, C. Haungs, A. Heck, D. Hörandel, J. R. Huege, T. Kampert, K.-H. Kang, D. Klages, H. O. Link, K. Łuczak, P. Mathes, H. J. Mayer, H. J. Milke, J. Mitrica, B. Morello, C. Oehlschläger, J. Ostapchenko, S. Pierog, T. Rebel, H. Roth, M. Schieler, H. Schoo, S. Schröder, F. G. Sima, O. Toma, G. Trinchero, G. C. Ulrich, H. Weindl, A. Wochele, J. Zabierowski, J. 0004-637X 1538-4357 American Astronomical Society Space and Planetary Science Astronomy and Astrophysics http://dx.doi.org/10.3847/1538-4357/aa8bb7 <jats:title>Abstract</jats:title> <jats:p>KASCADE and KASCADE-Grande were multi-detector installations to measure individual air showers of cosmic rays at ultra-high energy. Based on data sets measured by KASCADE and KASCADE-Grande, 90% C.L. upper limits to the flux of gamma<jats:italic>-</jats:italic>rays in the primary cosmic ray flux are determined in an energy range of <jats:inline-formula> <jats:tex-math> <?CDATA ${10}^{14}\mbox{--}{10}^{18}$?> </jats:tex-math> <jats:inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="apjaa8bb7ieqn1.gif" xlink:type="simple" /> </jats:inline-formula> eV. The analysis is performed by selecting air showers with a low muon content as expected for gamma-ray-induced showers compared to air showers induced by energetic nuclei. The best upper limit of the fraction of gamma-rays to the total cosmic ray flux is obtained at <jats:inline-formula> <jats:tex-math> <?CDATA $3.7\times {10}^{15}$?> </jats:tex-math> <jats:inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="apjaa8bb7ieqn2.gif" xlink:type="simple" /> </jats:inline-formula> eV with <jats:inline-formula> <jats:tex-math> <?CDATA $1.1\times {10}^{-5}$?> </jats:tex-math> <jats:inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="apjaa8bb7ieqn3.gif" xlink:type="simple" /> </jats:inline-formula>. Translated to an absolute gamma-ray flux this sets constraints on some fundamental astrophysical models, such as the distance of sources for at least one of the IceCube neutrino excess models.</jats:p> KASCADE-Grande Limits on the Isotropic Diffuse Gamma-Ray Flux between 100 TeV and 1 EeV The Astrophysical Journal |
| spellingShingle | Apel, W. D., Arteaga-Velázquez, J. C., Bekk, K., Bertaina, M., Blümer, J., Bozdog, H., Brancus, I. M., Cantoni, E., Chiavassa, A., Cossavella, F., Daumiller, K., Souza, V. de, Pierro, F. Di, Doll, P., Engel, R., Feng, Z., Fuhrmann, D., Gherghel-Lascu, A., Gils, H. J., Glasstetter, R., Grupen, C., Haungs, A., Heck, D., Hörandel, J. R., Huege, T., Kampert, K.-H., Kang, D., Klages, H. O., Link, K., Łuczak, P., Mathes, H. J., Mayer, H. J., Milke, J., Mitrica, B., Morello, C., Oehlschläger, J., Ostapchenko, S., Pierog, T., Rebel, H., Roth, M., Schieler, H., Schoo, S., Schröder, F. G., Sima, O., Toma, G., Trinchero, G. C., Ulrich, H., Weindl, A., Wochele, J., Zabierowski, J., The Astrophysical Journal, KASCADE-Grande Limits on the Isotropic Diffuse Gamma-Ray Flux between 100 TeV and 1 EeV, Space and Planetary Science, Astronomy and Astrophysics |
| title | KASCADE-Grande Limits on the Isotropic Diffuse Gamma-Ray Flux between 100 TeV and 1 EeV |
| title_full | KASCADE-Grande Limits on the Isotropic Diffuse Gamma-Ray Flux between 100 TeV and 1 EeV |
| title_fullStr | KASCADE-Grande Limits on the Isotropic Diffuse Gamma-Ray Flux between 100 TeV and 1 EeV |
| title_full_unstemmed | KASCADE-Grande Limits on the Isotropic Diffuse Gamma-Ray Flux between 100 TeV and 1 EeV |
| title_short | KASCADE-Grande Limits on the Isotropic Diffuse Gamma-Ray Flux between 100 TeV and 1 EeV |
| title_sort | kascade-grande limits on the isotropic diffuse gamma-ray flux between 100 tev and 1 eev |
| title_unstemmed | KASCADE-Grande Limits on the Isotropic Diffuse Gamma-Ray Flux between 100 TeV and 1 EeV |
| topic | Space and Planetary Science, Astronomy and Astrophysics |
| url | http://dx.doi.org/10.3847/1538-4357/aa8bb7 |