{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2014:2KD4DX7ZT2TDPYZKEOELCORPJ6","short_pith_number":"pith:2KD4DX7Z","canonical_record":{"source":{"id":"1401.1386","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2014-01-07T13:57:45Z","cross_cats_sorted":[],"title_canon_sha256":"fb8cebcd802eed3b8537565f1a80a75450bde21f751e3a73ae2f7d23090da185","abstract_canon_sha256":"e4822d919ddfca047d9fd9273cf150fc6e18dfbab5ffe0e0567de880cb25bc0c"},"schema_version":"1.0"},"canonical_sha256":"d287c1dff99ea637e32a2388b13a2f4fbe9a551cd665b8088eb63a2d235f37e2","source":{"kind":"arxiv","id":"1401.1386","version":1},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1401.1386","created_at":"2026-05-18T02:57:07Z"},{"alias_kind":"arxiv_version","alias_value":"1401.1386v1","created_at":"2026-05-18T02:57:07Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1401.1386","created_at":"2026-05-18T02:57:07Z"},{"alias_kind":"pith_short_12","alias_value":"2KD4DX7ZT2TD","created_at":"2026-05-18T12:28:11Z"},{"alias_kind":"pith_short_16","alias_value":"2KD4DX7ZT2TDPYZK","created_at":"2026-05-18T12:28:11Z"},{"alias_kind":"pith_short_8","alias_value":"2KD4DX7Z","created_at":"2026-05-18T12:28:11Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2014:2KD4DX7ZT2TDPYZKEOELCORPJ6","target":"record","payload":{"canonical_record":{"source":{"id":"1401.1386","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2014-01-07T13:57:45Z","cross_cats_sorted":[],"title_canon_sha256":"fb8cebcd802eed3b8537565f1a80a75450bde21f751e3a73ae2f7d23090da185","abstract_canon_sha256":"e4822d919ddfca047d9fd9273cf150fc6e18dfbab5ffe0e0567de880cb25bc0c"},"schema_version":"1.0"},"canonical_sha256":"d287c1dff99ea637e32a2388b13a2f4fbe9a551cd665b8088eb63a2d235f37e2","receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:57:07.753185Z","signature_b64":"+3cWwfd5m+jIzeYWNlrxZyCx39mmXutK02OhDom4qtxO1xvYvzMybLSFY6IeCQCQM0pv9aaqsodlNVJgMBHmCw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"d287c1dff99ea637e32a2388b13a2f4fbe9a551cd665b8088eb63a2d235f37e2","last_reissued_at":"2026-05-18T02:57:07.752680Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:57:07.752680Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"source_kind":"arxiv","source_id":"1401.1386","source_version":1,"attestation_state":"computed"},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-05-18T02:57:07Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"otlPagSx0r1rYVNLuijZ5FmByhFnvhJ+t/9I/Xg7k47cetQx1xwG2CVQYo5RoJQ554F1JqpQRq0kJe6OCixyDA==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-25T13:01:50.413655Z"},"content_sha256":"12f587cc116ec40b559232ebe4512dcf97eaf011b6aaa0e5871b5be3fc9414ca","schema_version":"1.0","event_id":"sha256:12f587cc116ec40b559232ebe4512dcf97eaf011b6aaa0e5871b5be3fc9414ca"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2014:2KD4DX7ZT2TDPYZKEOELCORPJ6","target":"graph","payload":{"graph_snapshot":{"paper":{"title":"Multi-wavelength observations of the binary system PSR B1259-63/LS 2883 around the 2010-2011 periastron passage","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"A. A. Abdo, A. Coleiro, A. Neronov, D. Malyshev, I. Sushch, Iu. Babyk, J. Mold\\'on, J.M. Paredes, K. Wood, M. Chernyakova, M. de Naurois, M. Rib\\'o, M. V. McSwain, S. Chaty, S. Johnston, U. Schwanke, Y. Uchiyama","submitted_at":"2014-01-07T13:57:45Z","abstract_excerpt":"We report on broad multi-wavelength observations of the 2010-2011 periastron passage of the gamma-ray loud binary system PSR B1259-63. High resolution interferometric radio observations establish extended radio emission trailing the position of the pulsar. Observations with the Fermi Gamma-ray Space Telescope reveal GeV gamma-ray flaring activity of the system, reaching the spin-down luminosity of the pulsar, around 30 days after periastron. There are no clear signatures of variability at radio, X-ray and TeV energies at the time of the GeV flare. Variability around periastron in the H$\\alpha$"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1401.1386","kind":"arxiv","version":1},"verdict":{"id":null,"model_set":{},"created_at":null,"strongest_claim":"","one_line_summary":"","pipeline_version":null,"weakest_assumption":"","pith_extraction_headline":""},"references":{"count":0,"sample":[],"resolved_work":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","internal_anchors":0},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"author_claims":{"count":0,"strong_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"builder_version":"pith-number-builder-2026-05-17-v1"},"verdict_id":null},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-05-18T02:57:07Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"lfd/swQ59py0vv2CHCUhh/KOZYVIUZpTWSwFClfCGI1VcGKzR3pBgUYtyufY2NQp9+2pXX7k4R5KJkbspjK1CA==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-25T13:01:50.414357Z"},"content_sha256":"c2e0c0109bd7201227d3298b7a0f6ed13f8ab369392d8a6291d119968aab1c5c","schema_version":"1.0","event_id":"sha256:c2e0c0109bd7201227d3298b7a0f6ed13f8ab369392d8a6291d119968aab1c5c"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/2KD4DX7ZT2TDPYZKEOELCORPJ6/bundle.json","state_url":"https://pith.science/pith/2KD4DX7ZT2TDPYZKEOELCORPJ6/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/2KD4DX7ZT2TDPYZKEOELCORPJ6/bundle.json","status":"primary"}],"public_keys":[{"key_id":"pith-v1-2026-05","algorithm":"ed25519","format":"raw","public_key_b64":"stVStoiQhXFxp4s2pdzPNoqVNBMojDU/fJ2db5S3CbM=","public_key_hex":"b2d552b68890857171a78b36a5dccf368a953413288c353f7c9d9d6f94b709b3","fingerprint_sha256_b32_first128bits":"RVFV5Z2OI2J3ZUO7ERDEBCYNKS","fingerprint_sha256_hex":"8d4b5ee74e4693bcd1df2446408b0d54","rotates_at":null,"url":"https://pith.science/pith-signing-key.json","notes":"Pith uses this Ed25519 key to sign canonical record SHA-256 digests. Verify with: ed25519_verify(public_key, message=canonical_sha256_bytes, signature=base64decode(signature_b64))."}],"merge_version":"pith-open-graph-merge-v1","built_at":"2026-05-25T13:01:50Z","links":{"resolver":"https://pith.science/pith/2KD4DX7ZT2TDPYZKEOELCORPJ6","bundle":"https://pith.science/pith/2KD4DX7ZT2TDPYZKEOELCORPJ6/bundle.json","state":"https://pith.science/pith/2KD4DX7ZT2TDPYZKEOELCORPJ6/state.json","well_known_bundle":"https://pith.science/.well-known/pith/2KD4DX7ZT2TDPYZKEOELCORPJ6/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2014:2KD4DX7ZT2TDPYZKEOELCORPJ6","merge_version":"pith-open-graph-merge-v1","event_count":2,"valid_event_count":2,"invalid_event_count":0,"equivocation_count":0,"current":{"canonical_record":{"metadata":{"abstract_canon_sha256":"e4822d919ddfca047d9fd9273cf150fc6e18dfbab5ffe0e0567de880cb25bc0c","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2014-01-07T13:57:45Z","title_canon_sha256":"fb8cebcd802eed3b8537565f1a80a75450bde21f751e3a73ae2f7d23090da185"},"schema_version":"1.0","source":{"id":"1401.1386","kind":"arxiv","version":1}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1401.1386","created_at":"2026-05-18T02:57:07Z"},{"alias_kind":"arxiv_version","alias_value":"1401.1386v1","created_at":"2026-05-18T02:57:07Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1401.1386","created_at":"2026-05-18T02:57:07Z"},{"alias_kind":"pith_short_12","alias_value":"2KD4DX7ZT2TD","created_at":"2026-05-18T12:28:11Z"},{"alias_kind":"pith_short_16","alias_value":"2KD4DX7ZT2TDPYZK","created_at":"2026-05-18T12:28:11Z"},{"alias_kind":"pith_short_8","alias_value":"2KD4DX7Z","created_at":"2026-05-18T12:28:11Z"}],"graph_snapshots":[{"event_id":"sha256:c2e0c0109bd7201227d3298b7a0f6ed13f8ab369392d8a6291d119968aab1c5c","target":"graph","created_at":"2026-05-18T02:57:07Z","signer":{"key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signer_id":"pith.science","signer_type":"pith_registry"},"payload":{"graph_snapshot":{"author_claims":{"count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","strong_count":0},"builder_version":"pith-number-builder-2026-05-17-v1","claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"paper":{"abstract_excerpt":"We report on broad multi-wavelength observations of the 2010-2011 periastron passage of the gamma-ray loud binary system PSR B1259-63. High resolution interferometric radio observations establish extended radio emission trailing the position of the pulsar. Observations with the Fermi Gamma-ray Space Telescope reveal GeV gamma-ray flaring activity of the system, reaching the spin-down luminosity of the pulsar, around 30 days after periastron. There are no clear signatures of variability at radio, X-ray and TeV energies at the time of the GeV flare. Variability around periastron in the H$\\alpha$","authors_text":"A. A. Abdo, A. Coleiro, A. Neronov, D. Malyshev, I. Sushch, Iu. Babyk, J. Mold\\'on, J.M. Paredes, K. Wood, M. Chernyakova, M. de Naurois, M. Rib\\'o, M. V. McSwain, S. Chaty, S. Johnston, U. Schwanke, Y. Uchiyama","cross_cats":[],"headline":"","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2014-01-07T13:57:45Z","title":"Multi-wavelength observations of the binary system PSR B1259-63/LS 2883 around the 2010-2011 periastron passage"},"references":{"count":0,"internal_anchors":0,"resolved_work":0,"sample":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1401.1386","kind":"arxiv","version":1},"verdict":{"created_at":null,"id":null,"model_set":{},"one_line_summary":"","pipeline_version":null,"pith_extraction_headline":"","strongest_claim":"","weakest_assumption":""}},"verdict_id":null}}],"author_attestations":[],"timestamp_anchors":[],"storage_attestations":[],"citation_signatures":[],"replication_records":[],"corrections":[],"mirror_hints":[],"record_created":{"event_id":"sha256:12f587cc116ec40b559232ebe4512dcf97eaf011b6aaa0e5871b5be3fc9414ca","target":"record","created_at":"2026-05-18T02:57:07Z","signer":{"key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signer_id":"pith.science","signer_type":"pith_registry"},"payload":{"attestation_state":"computed","canonical_record":{"metadata":{"abstract_canon_sha256":"e4822d919ddfca047d9fd9273cf150fc6e18dfbab5ffe0e0567de880cb25bc0c","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2014-01-07T13:57:45Z","title_canon_sha256":"fb8cebcd802eed3b8537565f1a80a75450bde21f751e3a73ae2f7d23090da185"},"schema_version":"1.0","source":{"id":"1401.1386","kind":"arxiv","version":1}},"canonical_sha256":"d287c1dff99ea637e32a2388b13a2f4fbe9a551cd665b8088eb63a2d235f37e2","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"d287c1dff99ea637e32a2388b13a2f4fbe9a551cd665b8088eb63a2d235f37e2","first_computed_at":"2026-05-18T02:57:07.752680Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-05-18T02:57:07.752680Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"+3cWwfd5m+jIzeYWNlrxZyCx39mmXutK02OhDom4qtxO1xvYvzMybLSFY6IeCQCQM0pv9aaqsodlNVJgMBHmCw==","signature_status":"signed_v1","signed_at":"2026-05-18T02:57:07.753185Z","signed_message":"canonical_sha256_bytes"},"source_id":"1401.1386","source_kind":"arxiv","source_version":1}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:12f587cc116ec40b559232ebe4512dcf97eaf011b6aaa0e5871b5be3fc9414ca","sha256:c2e0c0109bd7201227d3298b7a0f6ed13f8ab369392d8a6291d119968aab1c5c"],"state_sha256":"360c464672e57d77be2825461810c6adb1a1fb0bf2fd93031285437521730b44"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"7lJqaug2Vg+PGdfA+g7AJ6ITUJPWQ9nUYoI9S5Ya7PxLSE+eFEPCVpn9DD0I1qnkixQSnTNhYKWd7iEXZv8JCQ==","signed_message":"bundle_sha256_bytes","signed_at":"2026-05-25T13:01:50.416688Z","bundle_sha256":"e0304b6bbd397d905867f550b0d3c0033b58f1773a1f30fc3ca7154a180c2106"}}