{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2015:ITY6PZY2TIQOFHBPE2XCLLZM2L","short_pith_number":"pith:ITY6PZY2","schema_version":"1.0","canonical_sha256":"44f1e7e71a9a20e29c2f26ae25af2cd2f3203a5f75825b2b51654f7781cee4be","source":{"kind":"arxiv","id":"1507.02442","version":1},"attestation_state":"computed","paper":{"title":"Time-Dependent Modeling of Gamma-ray Flares in Blazar PKS1510-089","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Lukasz Stawarz, Marek Sikora, Rafal Moderski, Shinya Saito, Tadayuki Takahashi, Yasuyuki Tanaka","submitted_at":"2015-07-09T10:04:57Z","abstract_excerpt":"Here we present a new approach for constraining luminous blazars, incorporating fully time-dependent and self-consistent modeling of bright gamma-ray flares of PKS1510-089 resolved with Fermi-LAT, in the framework of the internal shock scenario. The results of our modeling imply the location of the gamma-ray flaring zone outside of the broad-line region, namely around 0.3pc from the core for a free-expanding jet with the opening angle Gamma, \\theta_\\mathrm{jet} \\simeq 1 (where Gamma is the jet bulk Lorentz factor), up to \\simeq 3pc for a collimated outflow with Gamma, \\theta_\\mathrm{jet} \\sime"},"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":"1507.02442","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2015-07-09T10:04:57Z","cross_cats_sorted":[],"title_canon_sha256":"894911a2604ecc2022602b13d1d2961c57e46a43aeb7d19fb20d455db97ba8b7","abstract_canon_sha256":"55232f9c9d771f5168c367a02e1b235d277f03476e34dd149f7a9dd0f003cd10"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:33:42.554145Z","signature_b64":"ycV0m+y9/VDhPDmS2b1kGsMc57NhfAdNSl3jsBjBLqWlRaJWbCuIRebGhD8zBi0OFR/pSGBoWx5IQir23vapCA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"44f1e7e71a9a20e29c2f26ae25af2cd2f3203a5f75825b2b51654f7781cee4be","last_reissued_at":"2026-05-18T01:33:42.553800Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:33:42.553800Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Time-Dependent Modeling of Gamma-ray Flares in Blazar PKS1510-089","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Lukasz Stawarz, Marek Sikora, Rafal Moderski, Shinya Saito, Tadayuki Takahashi, Yasuyuki Tanaka","submitted_at":"2015-07-09T10:04:57Z","abstract_excerpt":"Here we present a new approach for constraining luminous blazars, incorporating fully time-dependent and self-consistent modeling of bright gamma-ray flares of PKS1510-089 resolved with Fermi-LAT, in the framework of the internal shock scenario. The results of our modeling imply the location of the gamma-ray flaring zone outside of the broad-line region, namely around 0.3pc from the core for a free-expanding jet with the opening angle Gamma, \\theta_\\mathrm{jet} \\simeq 1 (where Gamma is the jet bulk Lorentz factor), up to \\simeq 3pc for a collimated outflow with Gamma, \\theta_\\mathrm{jet} \\sime"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1507.02442","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":"1507.02442","created_at":"2026-05-18T01:33:42.553852+00:00"},{"alias_kind":"arxiv_version","alias_value":"1507.02442v1","created_at":"2026-05-18T01:33:42.553852+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1507.02442","created_at":"2026-05-18T01:33:42.553852+00:00"},{"alias_kind":"pith_short_12","alias_value":"ITY6PZY2TIQO","created_at":"2026-05-18T12:29:25.134429+00:00"},{"alias_kind":"pith_short_16","alias_value":"ITY6PZY2TIQOFHBP","created_at":"2026-05-18T12:29:25.134429+00:00"},{"alias_kind":"pith_short_8","alias_value":"ITY6PZY2","created_at":"2026-05-18T12:29:25.134429+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/ITY6PZY2TIQOFHBPE2XCLLZM2L","json":"https://pith.science/pith/ITY6PZY2TIQOFHBPE2XCLLZM2L.json","graph_json":"https://pith.science/api/pith-number/ITY6PZY2TIQOFHBPE2XCLLZM2L/graph.json","events_json":"https://pith.science/api/pith-number/ITY6PZY2TIQOFHBPE2XCLLZM2L/events.json","paper":"https://pith.science/paper/ITY6PZY2"},"agent_actions":{"view_html":"https://pith.science/pith/ITY6PZY2TIQOFHBPE2XCLLZM2L","download_json":"https://pith.science/pith/ITY6PZY2TIQOFHBPE2XCLLZM2L.json","view_paper":"https://pith.science/paper/ITY6PZY2","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1507.02442&json=true","fetch_graph":"https://pith.science/api/pith-number/ITY6PZY2TIQOFHBPE2XCLLZM2L/graph.json","fetch_events":"https://pith.science/api/pith-number/ITY6PZY2TIQOFHBPE2XCLLZM2L/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/ITY6PZY2TIQOFHBPE2XCLLZM2L/action/timestamp_anchor","attest_storage":"https://pith.science/pith/ITY6PZY2TIQOFHBPE2XCLLZM2L/action/storage_attestation","attest_author":"https://pith.science/pith/ITY6PZY2TIQOFHBPE2XCLLZM2L/action/author_attestation","sign_citation":"https://pith.science/pith/ITY6PZY2TIQOFHBPE2XCLLZM2L/action/citation_signature","submit_replication":"https://pith.science/pith/ITY6PZY2TIQOFHBPE2XCLLZM2L/action/replication_record"}},"created_at":"2026-05-18T01:33:42.553852+00:00","updated_at":"2026-05-18T01:33:42.553852+00:00"}