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Using the onset times of 166 BATSE-detected flares with the GOES peak flux (1 -- 8 \\AA) higher than $1.0 \\times 10^{-5}$ $\\mathrm{Wm^{-2}}$, we prepare for each flare a light curve of the Yangbajing neutron monitor, spanning $\\pm$ 1.5 hours from the BATSE onset time. Based on the light curves, a systematic search for solar neutrons in energies above 100 MeV from the 166 flares was performed. No statistically significant signals d"},"verification_status":{"content_addressed":true,"pith_receipt":true,"author_attested":false,"weak_author_claims":0,"strong_author_claims":0,"externally_anchored":false,"storage_verified":false,"citation_signatures":0,"replication_records":0,"graph_snapshot":true,"references_resolved":false,"formal_links_present":false},"canonical_record":{"source":{"id":"astro-ph/0703428","kind":"arxiv","version":1},"metadata":{"license":"","primary_cat":"astro-ph","submitted_at":"2007-03-16T07:06:11Z","cross_cats_sorted":[],"title_canon_sha256":"a6e7c4778bee5d14a3fdc19ff24804846a4b5ca3d570b305911e1342c97323ce","abstract_canon_sha256":"1dac2d67750c58c2fa62565d1386338e45e64dcde5496618addc4e2ab55151b5"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-04T15:16:37.212626Z","signature_b64":"YvCBaB2KwpehIhYGAZCC9Oaz9piebGc+L89IdpHLqA7eQcvoRBQQoWRPvFOeztyv5+0C9d+1lK+sLeBiGhVvCg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"3a072b24dbb9c8564f873e1dbe3efff797745b5b43cc6b5e2fb0c5e893e9ab12","last_reissued_at":"2026-07-04T15:16:37.212083Z","signature_status":"signed_v1","first_computed_at":"2026-07-04T15:16:37.212083Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Upper limits on the solar-neutron flux at the Yangbajing neutron monitor from BATSE-detected solar flares","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"E. 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