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| 2026-01 |
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| 2025-11 |
The Altered Chaplygin Model as a Model for Dark Energy |
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| 2025-04 |
Stellar Population and Energy Feedback in the Supergiant Shell LMC 1 |
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| 2015-10 |
First constraints on the ultra-high energy neutrino flux from a prototype station of the Askaryan Radio Array |
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