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Videla, M |
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dc.contributor.author |
Villaseñor, L |
en |
dc.contributor.author |
Van, T |
en |
dc.contributor.author |
Vorobiov, S |
en |
dc.contributor.author |
Voyvodic, L |
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dc.contributor.author |
Wahlberg, H |
en |
dc.contributor.author |
Wainberg, O |
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dc.contributor.author |
Waldenmaier, T |
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dc.contributor.author |
Walker, P |
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dc.contributor.author |
Warner, D |
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dc.contributor.author |
Watson, A |
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dc.contributor.author |
Westerhoff, S |
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dc.contributor.author |
Wiebusch, C |
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dc.contributor.author |
Wieczorek, G |
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dc.contributor.author |
Wiencke, L |
en |
dc.contributor.author |
Wilczyńska, B |
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dc.contributor.author |
Wilczyński, H |
en |
dc.contributor.author |
Wileman, C |
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dc.contributor.author |
Winnick, M |
en |
dc.contributor.author |
Xu, J |
en |
dc.contributor.author |
Yamamoto, T |
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dc.contributor.author |
Younk, P |
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dc.contributor.author |
Zas, E |
en |
dc.contributor.author |
Zavrtanik, D |
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dc.contributor.author |
Zavrtanik, M |
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dc.contributor.author |
Zech, A |
en |
dc.contributor.author |
Zepeda, A |
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dc.contributor.author |
Zha, M |
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dc.contributor.author |
Ziolkowski, M |
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dc.date.accessioned |
2014-03-01T01:55:47Z |
|
dc.date.available |
2014-03-01T01:55:47Z |
|
dc.date.issued |
2007 |
en |
dc.identifier.uri |
https://dspace.lib.ntua.gr/xmlui/handle/123456789/27850 |
|
dc.subject |
Cosmic Ray |
en |
dc.subject |
Event Detection |
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dc.subject |
Upper Bound |
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dc.subject |
Fluorescence Detector |
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dc.subject |
Galactic Centre |
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dc.title |
Anisotropy studies around the galactic centre at EeV energies with the Auger Observatory |
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heal.type |
journalArticle |
en |
heal.identifier.primary |
10.1016/j.astropartphys.2006.11.002 |
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heal.identifier.secondary |
http://dx.doi.org/10.1016/j.astropartphys.2006.11.002 |
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heal.publicationDate |
2007 |
en |
heal.abstract |
Data from the Pierre Auger Observatory are analyzed to search for anisotropies near the direction of the Galactic Centre at EeV energies. The exposure of the surface array in this part of the sky is already significantly larger than that of the fore-runner experiments. Our results do not support previous findings of localized excesses in the AGASA and SUGAR data. |
en |
heal.journalName |
Astroparticle Physics |
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dc.identifier.doi |
10.1016/j.astropartphys.2006.11.002 |
en |