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This emission is consistent with being produced by synchrotron emission of electrons accelerated to high energy by the relativistic collisionless shock propagating into the weakly magnetized medium. Here we show that this high-energy afterglow emission constrains the preshock magnetic field to satisfy 1(n/1cc)^{9/8} mG<B<10^2(n/1cc)^{3/8}mG, where n is the preshock density, more stringent than the"},"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":"1004.0791","kind":"arxiv","version":3},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2010-04-06T07:55:53Z","cross_cats_sorted":[],"title_canon_sha256":"7e7b4ee537bcc4c425cd34aae706cde65ea6684aeb02c67973dc7375c9becbee","abstract_canon_sha256":"09ea2e5ab5074a4528f768173318aad59b564990e3e5c39edcb0d9e2d1f341a0"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T04:22:29.805032Z","signature_b64":"BF4VIA7OV4uKBj/u0x5l0f3Ls+26hE599GP2J31cd5tU/MXn5vwzI1IpQ+FCCrwK2Cl/7Alxv4HCJhejOj3BBQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"29ae4d94d95c88a629e9f2e3293f7f12de504288e6647f45f6c439e0d218a74c","last_reissued_at":"2026-05-18T04:22:29.804410Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T04:22:29.804410Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The upstream magnetic field of collisionless GRB shocks: constraint by Fermi-LAT observations","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Xiao-Hong Zhao (YNO/NAOC), Zhuo Li (PKU)","submitted_at":"2010-04-06T07:55:53Z","abstract_excerpt":"Long-lived >100 MeV emission has been a common feature of most Fermi-LAT detected gamma-ray bursts (GRBs), e.g., detected up to ~10^3s in long GRBs 080916C and 090902B and ~10^2s in short GRB 090510. 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