{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2010:Z42NJEHC35SPAOJSAHFM5NP5O5","short_pith_number":"pith:Z42NJEHC","schema_version":"1.0","canonical_sha256":"cf34d490e2df64f0393201caceb5fd774d8ec591eae898678f002b178c3c4609","source":{"kind":"arxiv","id":"1011.4275","version":3},"attestation_state":"computed","paper":{"title":"The Consistency of Fermi-LAT Observations of the Galactic Center with a Millisecond Pulsar Population in the Central Stellar Cluster","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO","astro-ph.GA","hep-ph"],"primary_cat":"astro-ph.HE","authors_text":"Kevork N. Abazajian","submitted_at":"2010-11-18T20:26:44Z","abstract_excerpt":"I show that the spectrum and morphology of a recent Fermi-LAT observation of the Galaxy center are consistent with a millisecond pulsar population in the nuclear Central stellar cluster of the Milky Way. The Galaxy Center gamma-ray spectrum is consistent with the spectrum of four of eight globular clusters that have been detected in the gamma-ray. A dark matter annihilation interpretation cannot be ruled out, though no unique features exist that would require this conclusion."},"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":"1011.4275","kind":"arxiv","version":3},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2010-11-18T20:26:44Z","cross_cats_sorted":["astro-ph.CO","astro-ph.GA","hep-ph"],"title_canon_sha256":"97cf021af5e882cadae266706817736fa92df605a1c9b004a82aab2854aed213","abstract_canon_sha256":"ceb93eb382f62afb6ac8e37ed30fc6ad9acd084a10e16794defe787f0d2ae8eb"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:04:43.816001Z","signature_b64":"SVwMMx8QKU2RANgH0kwPFumLJm4dl7R/+VoNgufK2BdUppqvmQ67Lp7eXw142SMjZ5AmI2kcmsx4uDUzml80Bw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"cf34d490e2df64f0393201caceb5fd774d8ec591eae898678f002b178c3c4609","last_reissued_at":"2026-05-18T02:04:43.815260Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:04:43.815260Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The Consistency of Fermi-LAT Observations of the Galactic Center with a Millisecond Pulsar Population in the Central Stellar Cluster","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO","astro-ph.GA","hep-ph"],"primary_cat":"astro-ph.HE","authors_text":"Kevork N. Abazajian","submitted_at":"2010-11-18T20:26:44Z","abstract_excerpt":"I show that the spectrum and morphology of a recent Fermi-LAT observation of the Galaxy center are consistent with a millisecond pulsar population in the nuclear Central stellar cluster of the Milky Way. The Galaxy Center gamma-ray spectrum is consistent with the spectrum of four of eight globular clusters that have been detected in the gamma-ray. A dark matter annihilation interpretation cannot be ruled out, though no unique features exist that would require this conclusion."},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1011.4275","kind":"arxiv","version":3},"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":"1011.4275","created_at":"2026-05-18T02:04:43.815366+00:00"},{"alias_kind":"arxiv_version","alias_value":"1011.4275v3","created_at":"2026-05-18T02:04:43.815366+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1011.4275","created_at":"2026-05-18T02:04:43.815366+00:00"},{"alias_kind":"pith_short_12","alias_value":"Z42NJEHC35SP","created_at":"2026-05-18T12:26:17.028572+00:00"},{"alias_kind":"pith_short_16","alias_value":"Z42NJEHC35SPAOJS","created_at":"2026-05-18T12:26:17.028572+00:00"},{"alias_kind":"pith_short_8","alias_value":"Z42NJEHC","created_at":"2026-05-18T12:26:17.028572+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":3,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2509.08043","citing_title":"Testing Viability of Benchmark Dark Matter Models for the Galactic Center Excess","ref_index":6,"is_internal_anchor":true},{"citing_arxiv_id":"2604.08648","citing_title":"High-dimensional inference for the $\\gamma$-ray sky with differentiable programming","ref_index":14,"is_internal_anchor":false},{"citing_arxiv_id":"2605.08010","citing_title":"Producing the GeV Galactic Center Excess via Cosmic Ray-Dark Matter Scattering","ref_index":11,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/Z42NJEHC35SPAOJSAHFM5NP5O5","json":"https://pith.science/pith/Z42NJEHC35SPAOJSAHFM5NP5O5.json","graph_json":"https://pith.science/api/pith-number/Z42NJEHC35SPAOJSAHFM5NP5O5/graph.json","events_json":"https://pith.science/api/pith-number/Z42NJEHC35SPAOJSAHFM5NP5O5/events.json","paper":"https://pith.science/paper/Z42NJEHC"},"agent_actions":{"view_html":"https://pith.science/pith/Z42NJEHC35SPAOJSAHFM5NP5O5","download_json":"https://pith.science/pith/Z42NJEHC35SPAOJSAHFM5NP5O5.json","view_paper":"https://pith.science/paper/Z42NJEHC","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1011.4275&json=true","fetch_graph":"https://pith.science/api/pith-number/Z42NJEHC35SPAOJSAHFM5NP5O5/graph.json","fetch_events":"https://pith.science/api/pith-number/Z42NJEHC35SPAOJSAHFM5NP5O5/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/Z42NJEHC35SPAOJSAHFM5NP5O5/action/timestamp_anchor","attest_storage":"https://pith.science/pith/Z42NJEHC35SPAOJSAHFM5NP5O5/action/storage_attestation","attest_author":"https://pith.science/pith/Z42NJEHC35SPAOJSAHFM5NP5O5/action/author_attestation","sign_citation":"https://pith.science/pith/Z42NJEHC35SPAOJSAHFM5NP5O5/action/citation_signature","submit_replication":"https://pith.science/pith/Z42NJEHC35SPAOJSAHFM5NP5O5/action/replication_record"}},"created_at":"2026-05-18T02:04:43.815366+00:00","updated_at":"2026-05-18T02:04:43.815366+00:00"}