{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2013:3YSGMBAIZJL44CLW5PYUK6BSGS","short_pith_number":"pith:3YSGMBAI","schema_version":"1.0","canonical_sha256":"de24660408ca57ce0976ebf1457832349c61687990c2155d9c2a1916e14ccd98","source":{"kind":"arxiv","id":"1303.4186","version":1},"attestation_state":"computed","paper":{"title":"The polarized Gamma-Ray Burst GRB 061122","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"A. Fernandez-Soto, D. Gotz, P. Laurent, S. Covino, Z . Bosnjak","submitted_at":"2013-03-18T08:53:23Z","abstract_excerpt":"We report on the polarization measure, obtained with IBIS on board INTEGRAL, of the prompt emission of GRB 061122. Over an 8 s interval containing the brightest part of the Gamma-Ray Burst we put a lower limit on its polarization fraction of 60% at 68% c.l. and of 33% at 90% c.l. on the 250-800 keV energy range.\n  We performed late time optical and near infra-red imaging observations of the GRB field using the Telescopio Nazionale Galileo (TNG), and the Canada-France-Hawaii Telescope (CFHT). Our multi-band (ugrizYJHK) photometry allowed us to identify the host galaxy of GRB 061122 and to build"},"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":"1303.4186","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2013-03-18T08:53:23Z","cross_cats_sorted":[],"title_canon_sha256":"289f54494abdd50c0674dba769c208f4d1ffc0bae3693b0d56677cdeea1cedbc","abstract_canon_sha256":"5c8c4d9adb29e61e8461bd6cb71b25185a3b1b6e97cc6eed6cee14554fa67e8c"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:51:01.339213Z","signature_b64":"0ewjltj0sEeRRmFujFpOuj5zRVkuBQk/CQO3q9koC/BLbiNZVDmLOfeisudE92zeAofdUDzmXxNxvHWitFPyDw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"de24660408ca57ce0976ebf1457832349c61687990c2155d9c2a1916e14ccd98","last_reissued_at":"2026-05-18T01:51:01.338716Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:51:01.338716Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The polarized Gamma-Ray Burst GRB 061122","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"A. Fernandez-Soto, D. Gotz, P. Laurent, S. Covino, Z . Bosnjak","submitted_at":"2013-03-18T08:53:23Z","abstract_excerpt":"We report on the polarization measure, obtained with IBIS on board INTEGRAL, of the prompt emission of GRB 061122. Over an 8 s interval containing the brightest part of the Gamma-Ray Burst we put a lower limit on its polarization fraction of 60% at 68% c.l. and of 33% at 90% c.l. on the 250-800 keV energy range.\n  We performed late time optical and near infra-red imaging observations of the GRB field using the Telescopio Nazionale Galileo (TNG), and the Canada-France-Hawaii Telescope (CFHT). Our multi-band (ugrizYJHK) photometry allowed us to identify the host galaxy of GRB 061122 and to build"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1303.4186","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":"1303.4186","created_at":"2026-05-18T01:51:01.338787+00:00"},{"alias_kind":"arxiv_version","alias_value":"1303.4186v1","created_at":"2026-05-18T01:51:01.338787+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1303.4186","created_at":"2026-05-18T01:51:01.338787+00:00"},{"alias_kind":"pith_short_12","alias_value":"3YSGMBAIZJL4","created_at":"2026-05-18T12:27:32.513160+00:00"},{"alias_kind":"pith_short_16","alias_value":"3YSGMBAIZJL44CLW","created_at":"2026-05-18T12:27:32.513160+00:00"},{"alias_kind":"pith_short_8","alias_value":"3YSGMBAI","created_at":"2026-05-18T12:27:32.513160+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/3YSGMBAIZJL44CLW5PYUK6BSGS","json":"https://pith.science/pith/3YSGMBAIZJL44CLW5PYUK6BSGS.json","graph_json":"https://pith.science/api/pith-number/3YSGMBAIZJL44CLW5PYUK6BSGS/graph.json","events_json":"https://pith.science/api/pith-number/3YSGMBAIZJL44CLW5PYUK6BSGS/events.json","paper":"https://pith.science/paper/3YSGMBAI"},"agent_actions":{"view_html":"https://pith.science/pith/3YSGMBAIZJL44CLW5PYUK6BSGS","download_json":"https://pith.science/pith/3YSGMBAIZJL44CLW5PYUK6BSGS.json","view_paper":"https://pith.science/paper/3YSGMBAI","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1303.4186&json=true","fetch_graph":"https://pith.science/api/pith-number/3YSGMBAIZJL44CLW5PYUK6BSGS/graph.json","fetch_events":"https://pith.science/api/pith-number/3YSGMBAIZJL44CLW5PYUK6BSGS/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/3YSGMBAIZJL44CLW5PYUK6BSGS/action/timestamp_anchor","attest_storage":"https://pith.science/pith/3YSGMBAIZJL44CLW5PYUK6BSGS/action/storage_attestation","attest_author":"https://pith.science/pith/3YSGMBAIZJL44CLW5PYUK6BSGS/action/author_attestation","sign_citation":"https://pith.science/pith/3YSGMBAIZJL44CLW5PYUK6BSGS/action/citation_signature","submit_replication":"https://pith.science/pith/3YSGMBAIZJL44CLW5PYUK6BSGS/action/replication_record"}},"created_at":"2026-05-18T01:51:01.338787+00:00","updated_at":"2026-05-18T01:51:01.338787+00:00"}