{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2015:FOG6JHSDKITY2KWDO6HS7JM3GG","short_pith_number":"pith:FOG6JHSD","schema_version":"1.0","canonical_sha256":"2b8de49e4352278d2ac3778f2fa59b319ac85b29be99e57dca35c8e1cc6c472c","source":{"kind":"arxiv","id":"1509.02928","version":1},"attestation_state":"computed","paper":{"title":"Known Radio Pulsars Do Not Contribute to the Galactic Center Gamma-Ray Excess","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.GA","hep-ph"],"primary_cat":"astro-ph.HE","authors_text":"Tim Linden","submitted_at":"2015-09-09T20:15:54Z","abstract_excerpt":"Observations using the Fermi Large Area Telescope (Fermi-LAT) have found a significant gamma-ray excess surrounding the center of the Milky Way (GC). One possible interpretation of this excess invokes gamma-ray emission from an undiscovered population of either young or recycled pulsars densely clustered throughout the inner kiloparsec of the Milky Way. While these systems, by construction, have individual fluxes that lie below the point source sensitivity of the Fermi-LAT, they may already be observed in multiwavelength observations. Notably the Australia Telescope National Facility (ATNF) ca"},"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":"1509.02928","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2015-09-09T20:15:54Z","cross_cats_sorted":["astro-ph.GA","hep-ph"],"title_canon_sha256":"8aadd0893bbf2b3330f0fbe41e723250d9ba1fe5ee1472efc53b97d17a176d22","abstract_canon_sha256":"a191d5adaaa7df2c6f2cebd7b02d4e1eb904bc5f82e9126b108a223a6ee86f92"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:18:33.186306Z","signature_b64":"GhuQwUuNaB5sReLn9pUpPnuk6HLXg+EbBeJkLHTjD9/M952c6EAaAOckOyULGBHO6Pud+pGAj1MViqMYVhIoCg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"2b8de49e4352278d2ac3778f2fa59b319ac85b29be99e57dca35c8e1cc6c472c","last_reissued_at":"2026-05-18T01:18:33.185925Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:18:33.185925Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Known Radio Pulsars Do Not Contribute to the Galactic Center Gamma-Ray Excess","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.GA","hep-ph"],"primary_cat":"astro-ph.HE","authors_text":"Tim Linden","submitted_at":"2015-09-09T20:15:54Z","abstract_excerpt":"Observations using the Fermi Large Area Telescope (Fermi-LAT) have found a significant gamma-ray excess surrounding the center of the Milky Way (GC). One possible interpretation of this excess invokes gamma-ray emission from an undiscovered population of either young or recycled pulsars densely clustered throughout the inner kiloparsec of the Milky Way. While these systems, by construction, have individual fluxes that lie below the point source sensitivity of the Fermi-LAT, they may already be observed in multiwavelength observations. Notably the Australia Telescope National Facility (ATNF) ca"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1509.02928","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":"1509.02928","created_at":"2026-05-18T01:18:33.185988+00:00"},{"alias_kind":"arxiv_version","alias_value":"1509.02928v1","created_at":"2026-05-18T01:18:33.185988+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1509.02928","created_at":"2026-05-18T01:18:33.185988+00:00"},{"alias_kind":"pith_short_12","alias_value":"FOG6JHSDKITY","created_at":"2026-05-18T12:29:19.899920+00:00"},{"alias_kind":"pith_short_16","alias_value":"FOG6JHSDKITY2KWD","created_at":"2026-05-18T12:29:19.899920+00:00"},{"alias_kind":"pith_short_8","alias_value":"FOG6JHSD","created_at":"2026-05-18T12:29:19.899920+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/FOG6JHSDKITY2KWDO6HS7JM3GG","json":"https://pith.science/pith/FOG6JHSDKITY2KWDO6HS7JM3GG.json","graph_json":"https://pith.science/api/pith-number/FOG6JHSDKITY2KWDO6HS7JM3GG/graph.json","events_json":"https://pith.science/api/pith-number/FOG6JHSDKITY2KWDO6HS7JM3GG/events.json","paper":"https://pith.science/paper/FOG6JHSD"},"agent_actions":{"view_html":"https://pith.science/pith/FOG6JHSDKITY2KWDO6HS7JM3GG","download_json":"https://pith.science/pith/FOG6JHSDKITY2KWDO6HS7JM3GG.json","view_paper":"https://pith.science/paper/FOG6JHSD","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1509.02928&json=true","fetch_graph":"https://pith.science/api/pith-number/FOG6JHSDKITY2KWDO6HS7JM3GG/graph.json","fetch_events":"https://pith.science/api/pith-number/FOG6JHSDKITY2KWDO6HS7JM3GG/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/FOG6JHSDKITY2KWDO6HS7JM3GG/action/timestamp_anchor","attest_storage":"https://pith.science/pith/FOG6JHSDKITY2KWDO6HS7JM3GG/action/storage_attestation","attest_author":"https://pith.science/pith/FOG6JHSDKITY2KWDO6HS7JM3GG/action/author_attestation","sign_citation":"https://pith.science/pith/FOG6JHSDKITY2KWDO6HS7JM3GG/action/citation_signature","submit_replication":"https://pith.science/pith/FOG6JHSDKITY2KWDO6HS7JM3GG/action/replication_record"}},"created_at":"2026-05-18T01:18:33.185988+00:00","updated_at":"2026-05-18T01:18:33.185988+00:00"}