{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2011:RXEWA6X7NW33SWROW6LMGOVIZS","short_pith_number":"pith:RXEWA6X7","schema_version":"1.0","canonical_sha256":"8dc9607aff6db7b95a2eb796c33aa8ccad1f51e5360ed547588f2d02cc0647cb","source":{"kind":"arxiv","id":"1111.0325","version":1},"attestation_state":"computed","paper":{"title":"Pulsar Emission Geometry and Accelerating Field Strength","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Alice K. Harding, Constantinos Kalapotharakos, Damien Parent, Ioannis Contopoulos, M. Coleman Miller, Megan E. DeCesar","submitted_at":"2011-11-01T21:38:09Z","abstract_excerpt":"The high-quality Fermi LAT observations of gamma-ray pulsars have opened a new window to understanding the generation mechanisms of high-energy emission from these systems. The high statistics allow for careful modeling of the light curve features as well as for phase resolved spectral modeling. We modeled the LAT light curves of the Vela and CTA 1 pulsars with simulated high-energy light curves generated from geometrical representations of the outer gap and slot gap emission models, within the vacuum retarded dipole and force-free fields. A Markov Chain Monte Carlo maximum likelihood method w"},"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":"1111.0325","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2011-11-01T21:38:09Z","cross_cats_sorted":[],"title_canon_sha256":"21b4703314947f23c29c9ee6a438bd42e3fe3b12702d26d8d277c9b3da46b07c","abstract_canon_sha256":"378af5f82f9a507d10ad26c214844ef2a1d5f28cd15287c285a19b31975e4cf5"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T04:09:45.258851Z","signature_b64":"k3urrK9vBvDk2t3fafDIIvdRqTACfmhJlM6lQt3f9a/IOl9jPV1CMn5/Rjy0yK4neUgBm8qGXJvIWBkLnH06Cw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"8dc9607aff6db7b95a2eb796c33aa8ccad1f51e5360ed547588f2d02cc0647cb","last_reissued_at":"2026-05-18T04:09:45.258096Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T04:09:45.258096Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Pulsar Emission Geometry and Accelerating Field Strength","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Alice K. Harding, Constantinos Kalapotharakos, Damien Parent, Ioannis Contopoulos, M. Coleman Miller, Megan E. DeCesar","submitted_at":"2011-11-01T21:38:09Z","abstract_excerpt":"The high-quality Fermi LAT observations of gamma-ray pulsars have opened a new window to understanding the generation mechanisms of high-energy emission from these systems. The high statistics allow for careful modeling of the light curve features as well as for phase resolved spectral modeling. We modeled the LAT light curves of the Vela and CTA 1 pulsars with simulated high-energy light curves generated from geometrical representations of the outer gap and slot gap emission models, within the vacuum retarded dipole and force-free fields. A Markov Chain Monte Carlo maximum likelihood method w"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1111.0325","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":"1111.0325","created_at":"2026-05-18T04:09:45.258155+00:00"},{"alias_kind":"arxiv_version","alias_value":"1111.0325v1","created_at":"2026-05-18T04:09:45.258155+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1111.0325","created_at":"2026-05-18T04:09:45.258155+00:00"},{"alias_kind":"pith_short_12","alias_value":"RXEWA6X7NW33","created_at":"2026-05-18T12:26:41.206345+00:00"},{"alias_kind":"pith_short_16","alias_value":"RXEWA6X7NW33SWRO","created_at":"2026-05-18T12:26:41.206345+00:00"},{"alias_kind":"pith_short_8","alias_value":"RXEWA6X7","created_at":"2026-05-18T12:26:41.206345+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/RXEWA6X7NW33SWROW6LMGOVIZS","json":"https://pith.science/pith/RXEWA6X7NW33SWROW6LMGOVIZS.json","graph_json":"https://pith.science/api/pith-number/RXEWA6X7NW33SWROW6LMGOVIZS/graph.json","events_json":"https://pith.science/api/pith-number/RXEWA6X7NW33SWROW6LMGOVIZS/events.json","paper":"https://pith.science/paper/RXEWA6X7"},"agent_actions":{"view_html":"https://pith.science/pith/RXEWA6X7NW33SWROW6LMGOVIZS","download_json":"https://pith.science/pith/RXEWA6X7NW33SWROW6LMGOVIZS.json","view_paper":"https://pith.science/paper/RXEWA6X7","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1111.0325&json=true","fetch_graph":"https://pith.science/api/pith-number/RXEWA6X7NW33SWROW6LMGOVIZS/graph.json","fetch_events":"https://pith.science/api/pith-number/RXEWA6X7NW33SWROW6LMGOVIZS/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/RXEWA6X7NW33SWROW6LMGOVIZS/action/timestamp_anchor","attest_storage":"https://pith.science/pith/RXEWA6X7NW33SWROW6LMGOVIZS/action/storage_attestation","attest_author":"https://pith.science/pith/RXEWA6X7NW33SWROW6LMGOVIZS/action/author_attestation","sign_citation":"https://pith.science/pith/RXEWA6X7NW33SWROW6LMGOVIZS/action/citation_signature","submit_replication":"https://pith.science/pith/RXEWA6X7NW33SWROW6LMGOVIZS/action/replication_record"}},"created_at":"2026-05-18T04:09:45.258155+00:00","updated_at":"2026-05-18T04:09:45.258155+00:00"}