{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2013:HSXVXYKWXMCTMLTZPBT2REHSAI","short_pith_number":"pith:HSXVXYKW","schema_version":"1.0","canonical_sha256":"3caf5be156bb05362e797867a890f202298b8a3ab5363d6596c8d2c5365b03b3","source":{"kind":"arxiv","id":"1304.7245","version":1},"attestation_state":"computed","paper":{"title":"Numerical modelling of gamma-ray emission produced by electrons originating from the magnetospheres of millisecond pulsars in globular clusters","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"A. Zajczyk, B. Rudak, W. Bednarek","submitted_at":"2013-04-26T18:03:27Z","abstract_excerpt":"Globular clusters are source of gamma-ray radiation. At GeV energies, their emission is attributed to magnetospheric activity of millisecond pulsars residing in the clusters. Inverse Compton scattering of ambient photon fields on relativistic particles diffusing through cluster environment is thought to be the source of GeV-TeV emission of globular clusters. Using pair starved polar cap model gamma-ray emission from synthetic millisecond pulsar was modelled. In addition to pulsar emission characteristics, the synthetic pulsar model yielded spectra of electrons escaping pulsar magnetosphere. To"},"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":"1304.7245","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2013-04-26T18:03:27Z","cross_cats_sorted":[],"title_canon_sha256":"a0bf3540965593349e9db5ce71e57f496ceb7321eb0b7d095e2caaa570536b51","abstract_canon_sha256":"9dfd7f7f309f3cbdccb279e09c4334027faee21bbb3f4d3fa4a54b35d9780cb6"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T03:25:15.634332Z","signature_b64":"nos6o3DQaLpMBL4g37drka1xuOukw+CBlbfZjqbgenbQIQWcFW83dGaoG/Sknv4Jl+ZPjb7e401AMW5p7gIPDQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"3caf5be156bb05362e797867a890f202298b8a3ab5363d6596c8d2c5365b03b3","last_reissued_at":"2026-05-18T03:25:15.633596Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T03:25:15.633596Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Numerical modelling of gamma-ray emission produced by electrons originating from the magnetospheres of millisecond pulsars in globular clusters","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"A. Zajczyk, B. Rudak, W. Bednarek","submitted_at":"2013-04-26T18:03:27Z","abstract_excerpt":"Globular clusters are source of gamma-ray radiation. At GeV energies, their emission is attributed to magnetospheric activity of millisecond pulsars residing in the clusters. Inverse Compton scattering of ambient photon fields on relativistic particles diffusing through cluster environment is thought to be the source of GeV-TeV emission of globular clusters. Using pair starved polar cap model gamma-ray emission from synthetic millisecond pulsar was modelled. In addition to pulsar emission characteristics, the synthetic pulsar model yielded spectra of electrons escaping pulsar magnetosphere. To"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1304.7245","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":"1304.7245","created_at":"2026-05-18T03:25:15.633726+00:00"},{"alias_kind":"arxiv_version","alias_value":"1304.7245v1","created_at":"2026-05-18T03:25:15.633726+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1304.7245","created_at":"2026-05-18T03:25:15.633726+00:00"},{"alias_kind":"pith_short_12","alias_value":"HSXVXYKWXMCT","created_at":"2026-05-18T12:27:46.883200+00:00"},{"alias_kind":"pith_short_16","alias_value":"HSXVXYKWXMCTMLTZ","created_at":"2026-05-18T12:27:46.883200+00:00"},{"alias_kind":"pith_short_8","alias_value":"HSXVXYKW","created_at":"2026-05-18T12:27:46.883200+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/HSXVXYKWXMCTMLTZPBT2REHSAI","json":"https://pith.science/pith/HSXVXYKWXMCTMLTZPBT2REHSAI.json","graph_json":"https://pith.science/api/pith-number/HSXVXYKWXMCTMLTZPBT2REHSAI/graph.json","events_json":"https://pith.science/api/pith-number/HSXVXYKWXMCTMLTZPBT2REHSAI/events.json","paper":"https://pith.science/paper/HSXVXYKW"},"agent_actions":{"view_html":"https://pith.science/pith/HSXVXYKWXMCTMLTZPBT2REHSAI","download_json":"https://pith.science/pith/HSXVXYKWXMCTMLTZPBT2REHSAI.json","view_paper":"https://pith.science/paper/HSXVXYKW","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1304.7245&json=true","fetch_graph":"https://pith.science/api/pith-number/HSXVXYKWXMCTMLTZPBT2REHSAI/graph.json","fetch_events":"https://pith.science/api/pith-number/HSXVXYKWXMCTMLTZPBT2REHSAI/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/HSXVXYKWXMCTMLTZPBT2REHSAI/action/timestamp_anchor","attest_storage":"https://pith.science/pith/HSXVXYKWXMCTMLTZPBT2REHSAI/action/storage_attestation","attest_author":"https://pith.science/pith/HSXVXYKWXMCTMLTZPBT2REHSAI/action/author_attestation","sign_citation":"https://pith.science/pith/HSXVXYKWXMCTMLTZPBT2REHSAI/action/citation_signature","submit_replication":"https://pith.science/pith/HSXVXYKWXMCTMLTZPBT2REHSAI/action/replication_record"}},"created_at":"2026-05-18T03:25:15.633726+00:00","updated_at":"2026-05-18T03:25:15.633726+00:00"}