{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2022:EK2LBXP5PJKAXTDHEQQ7ZYD2JT","short_pith_number":"pith:EK2LBXP5","schema_version":"1.0","canonical_sha256":"22b4b0ddfd7a540bcc672421fce07a4cc737a59c80fbdffada374272352ce236","source":{"kind":"arxiv","id":"2209.00006","version":2},"attestation_state":"computed","paper":{"title":"A Phantom Menace: On the Morphology of the Galactic Center Excess","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":"Ilias Cholis, Samuel D. McDermott, Yi-Ming Zhong","submitted_at":"2022-08-31T18:00:00Z","abstract_excerpt":"The characteristics of the Galactic Center Excess (GCE) emission observed in gamma-ray energies -- especially the morphology of the GCE -- remain a hotly debated subject. The manner in which the dominant diffuse gamma-ray background is modeled has been claimed to have a determining effect on the preferred morphology. In this work, we compare two distinct approaches to the galactic diffuse gamma-ray emission background: the first approach models this emission through templates calculated from a sequence of well-defined astrophysical assumptions, while the second approach divides surrogates for "},"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":"2209.00006","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2022-08-31T18:00:00Z","cross_cats_sorted":["astro-ph.CO","astro-ph.GA","hep-ph"],"title_canon_sha256":"9af8bdaee6b2fe6fea88a8b7b42bf0b11c0e4b8d72da2debbff187e5bd3c7df9","abstract_canon_sha256":"12a86e94cd422c264fa048d3de050526f17996290b777fb2de6a497582be2b46"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T06:58:05.840641Z","signature_b64":"uOK6TkNJCgIywneZgVpe4COFyRoodxVGoqdGrvP/3c3Zeq4b2026kKG3pckGqDqAA6TPJrjoYtB5+sW0EBoYAg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"22b4b0ddfd7a540bcc672421fce07a4cc737a59c80fbdffada374272352ce236","last_reissued_at":"2026-07-05T06:58:05.840122Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T06:58:05.840122Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"A Phantom Menace: On the Morphology of the Galactic Center Excess","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":"Ilias Cholis, Samuel D. McDermott, Yi-Ming Zhong","submitted_at":"2022-08-31T18:00:00Z","abstract_excerpt":"The characteristics of the Galactic Center Excess (GCE) emission observed in gamma-ray energies -- especially the morphology of the GCE -- remain a hotly debated subject. The manner in which the dominant diffuse gamma-ray background is modeled has been claimed to have a determining effect on the preferred morphology. In this work, we compare two distinct approaches to the galactic diffuse gamma-ray emission background: the first approach models this emission through templates calculated from a sequence of well-defined astrophysical assumptions, while the second approach divides surrogates for "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2209.00006","kind":"arxiv","version":2},"verdict":{"id":null,"model_set":{},"created_at":null,"strongest_claim":"","one_line_summary":"","pipeline_version":null,"weakest_assumption":"","pith_extraction_headline":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2209.00006/integrity.json","findings":[],"available":true,"detectors_run":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938"},"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":"2209.00006","created_at":"2026-07-05T06:58:05.840180+00:00"},{"alias_kind":"arxiv_version","alias_value":"2209.00006v2","created_at":"2026-07-05T06:58:05.840180+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2209.00006","created_at":"2026-07-05T06:58:05.840180+00:00"},{"alias_kind":"pith_short_12","alias_value":"EK2LBXP5PJKA","created_at":"2026-07-05T06:58:05.840180+00:00"},{"alias_kind":"pith_short_16","alias_value":"EK2LBXP5PJKAXTDH","created_at":"2026-07-05T06:58:05.840180+00:00"},{"alias_kind":"pith_short_8","alias_value":"EK2LBXP5","created_at":"2026-07-05T06:58:05.840180+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":5,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2605.22913","citing_title":"A Precise Measurement of the Fermi-LAT Galactic Center Excess Morphology and Spectrum","ref_index":62,"is_internal_anchor":false},{"citing_arxiv_id":"2605.22913","citing_title":"A Precise Measurement of the Fermi-LAT Galactic Center Excess Morphology and Spectrum","ref_index":62,"is_internal_anchor":false},{"citing_arxiv_id":"2509.08043","citing_title":"Testing Viability of Benchmark Dark Matter Models for the Galactic Center Excess","ref_index":22,"is_internal_anchor":false},{"citing_arxiv_id":"2604.08648","citing_title":"High-dimensional inference for the $\\gamma$-ray sky with differentiable programming","ref_index":10,"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":75,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/EK2LBXP5PJKAXTDHEQQ7ZYD2JT","json":"https://pith.science/pith/EK2LBXP5PJKAXTDHEQQ7ZYD2JT.json","graph_json":"https://pith.science/api/pith-number/EK2LBXP5PJKAXTDHEQQ7ZYD2JT/graph.json","events_json":"https://pith.science/api/pith-number/EK2LBXP5PJKAXTDHEQQ7ZYD2JT/events.json","paper":"https://pith.science/paper/EK2LBXP5"},"agent_actions":{"view_html":"https://pith.science/pith/EK2LBXP5PJKAXTDHEQQ7ZYD2JT","download_json":"https://pith.science/pith/EK2LBXP5PJKAXTDHEQQ7ZYD2JT.json","view_paper":"https://pith.science/paper/EK2LBXP5","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2209.00006&json=true","fetch_graph":"https://pith.science/api/pith-number/EK2LBXP5PJKAXTDHEQQ7ZYD2JT/graph.json","fetch_events":"https://pith.science/api/pith-number/EK2LBXP5PJKAXTDHEQQ7ZYD2JT/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/EK2LBXP5PJKAXTDHEQQ7ZYD2JT/action/timestamp_anchor","attest_storage":"https://pith.science/pith/EK2LBXP5PJKAXTDHEQQ7ZYD2JT/action/storage_attestation","attest_author":"https://pith.science/pith/EK2LBXP5PJKAXTDHEQQ7ZYD2JT/action/author_attestation","sign_citation":"https://pith.science/pith/EK2LBXP5PJKAXTDHEQQ7ZYD2JT/action/citation_signature","submit_replication":"https://pith.science/pith/EK2LBXP5PJKAXTDHEQQ7ZYD2JT/action/replication_record"}},"created_at":"2026-07-05T06:58:05.840180+00:00","updated_at":"2026-07-05T06:58:05.840180+00:00"}