Implications to sources of ultra-high-energy cosmic rays from their arrival distribution

H Takami, K Sato - Astroparticle Physics, 2009 - Elsevier
We estimate the local number density of sources of ultra-high-energy cosmic rays (UHECRs)
based on the statistical features of their arrival direction distribution. We calculate the arrival …
被引用次数：34 相关文章

Implications to Sources of Ultra-high-energy Cosmic Rays from their Arrival Distribution

H Takami, K Sato - Astropart. Phys., 2009 - inspirehep.net
We estimate the local number density of sources of ultra-high-energy cosmic rays (UHECRs)
based on the statistical features of their arrival direction distribution. We calculate the arrival …

Implications to sources of ultra-high-energy cosmic rays from their arrival distribution

H Takami, K Sato - Astroparticle Physics, 2009 - infona.pl
We estimate the local number density of sources of ultra-high-energy cosmic rays (UHECRs)
based on the statistical features of their arrival direction distribution. We calculate the arrival …

[引用][C] Implications to Sources of Ultra-high-energy Cosmic Rays from their Arrival Distribution

高見一 - Astroparticle Physics 40, 2009 - cir.nii.ac.jp
Implications to Sources of Ultra-high-energy Cosmic Rays from their Arrival Distribution | CiNii
Research CiNii 国立情報学研究所 学術情報ナビゲータ[サイニィ] 詳細へ移動 検索フォームへ移動 …
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[PDF][PDF] Implications to Sources of Ultra-high-energy Cosmic Rays from their Arrival Distribution

H Takamia, K Satoa - arXiv preprint arXiv:0807.3442, 2008 - Citeseer
We estimate the local number density of sources of ultra-high-energy cosmic rays (UHECRs)
based on the statistical features of their arrival direction distribution. We calculate the arrival …

Implications to sources of ultra-high-energy cosmic rays from their arrival distribution

H Takami, K Sato - Astroparticle Physics, 2009 - ui.adsabs.harvard.edu
We estimate the local number density of sources of ultra-high-energy cosmic rays (UHECRs)
based on the statistical features of their arrival direction distribution. We calculate the arrival …

Implications to Sources of Ultra-high-energy Cosmic Rays from their Arrival Distribution

H Takami, K Sato - arXiv preprint arXiv:0807.3442, 2008 - arxiv.org
We estimate the local number density of sources of ultra-high-energy cosmic rays (UHECRs)
based on the statistical features of their arrival direction distribution. We calculate the arrival …

[引用][C] Implications to sources of ultra-high-energy cosmic rays from their arrival distribution

H Takami, K Sato - Astroparticle Physics, 2009 - cir.nii.ac.jp
Implications to sources of ultra-high-energy cosmic rays from their arrival distribution | CiNii
Research CiNii 国立情報学研究所 学術情報ナビゲータ[サイニィ] 詳細へ移動 検索フォームへ …