{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2014:2KD4DX7ZT2TDPYZKEOELCORPJ6","short_pith_number":"pith:2KD4DX7Z","schema_version":"1.0","canonical_sha256":"d287c1dff99ea637e32a2388b13a2f4fbe9a551cd665b8088eb63a2d235f37e2","source":{"kind":"arxiv","id":"1401.1386","version":1},"attestation_state":"computed","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$\\alpha$"},"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":"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"},"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"},"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"},"aliases":[{"alias_kind":"arxiv","alias_value":"1401.1386","created_at":"2026-05-18T02:57:07.752754+00:00"},{"alias_kind":"arxiv_version","alias_value":"1401.1386v1","created_at":"2026-05-18T02:57:07.752754+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1401.1386","created_at":"2026-05-18T02:57:07.752754+00:00"},{"alias_kind":"pith_short_12","alias_value":"2KD4DX7ZT2TD","created_at":"2026-05-18T12:28:11.866339+00:00"},{"alias_kind":"pith_short_16","alias_value":"2KD4DX7ZT2TDPYZK","created_at":"2026-05-18T12:28:11.866339+00:00"},{"alias_kind":"pith_short_8","alias_value":"2KD4DX7Z","created_at":"2026-05-18T12:28:11.866339+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":0,"internal_anchor_count":0,"sample":[]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/2KD4DX7ZT2TDPYZKEOELCORPJ6","json":"https://pith.science/pith/2KD4DX7ZT2TDPYZKEOELCORPJ6.json","graph_json":"https://pith.science/api/pith-number/2KD4DX7ZT2TDPYZKEOELCORPJ6/graph.json","events_json":"https://pith.science/api/pith-number/2KD4DX7ZT2TDPYZKEOELCORPJ6/events.json","paper":"https://pith.science/paper/2KD4DX7Z"},"agent_actions":{"view_html":"https://pith.science/pith/2KD4DX7ZT2TDPYZKEOELCORPJ6","download_json":"https://pith.science/pith/2KD4DX7ZT2TDPYZKEOELCORPJ6.json","view_paper":"https://pith.science/paper/2KD4DX7Z","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1401.1386&json=true","fetch_graph":"https://pith.science/api/pith-number/2KD4DX7ZT2TDPYZKEOELCORPJ6/graph.json","fetch_events":"https://pith.science/api/pith-number/2KD4DX7ZT2TDPYZKEOELCORPJ6/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/2KD4DX7ZT2TDPYZKEOELCORPJ6/action/timestamp_anchor","attest_storage":"https://pith.science/pith/2KD4DX7ZT2TDPYZKEOELCORPJ6/action/storage_attestation","attest_author":"https://pith.science/pith/2KD4DX7ZT2TDPYZKEOELCORPJ6/action/author_attestation","sign_citation":"https://pith.science/pith/2KD4DX7ZT2TDPYZKEOELCORPJ6/action/citation_signature","submit_replication":"https://pith.science/pith/2KD4DX7ZT2TDPYZKEOELCORPJ6/action/replication_record"}},"created_at":"2026-05-18T02:57:07.752754+00:00","updated_at":"2026-05-18T02:57:07.752754+00:00"}