{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2014:XI3HMOZXY3G6DG3F5PLHC5Z2ME","short_pith_number":"pith:XI3HMOZX","schema_version":"1.0","canonical_sha256":"ba36763b37c6cde19b65ebd671773a6120831ed3e3c429e6fc7a1e0a0bf892c3","source":{"kind":"arxiv","id":"1406.5188","version":1},"attestation_state":"computed","paper":{"title":"ALP Conversion and the Soft X-ray Excess in the Outskirts of the Coma Cluster","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO","astro-ph.HE","hep-th"],"primary_cat":"hep-ph","authors_text":"David Kraljic, Joseph P. Conlon, Markus Rummel","submitted_at":"2014-06-19T20:00:22Z","abstract_excerpt":"It was recently found that the soft X-ray excess in the center of the Coma cluster can be fitted by conversion of axion-like-particles (ALPs) of a cosmic axion background (CAB) to photons. We extend this analysis to the outskirts of Coma, including regions up to 5 Mpc from the center of the cluster. We extract the excess soft X-ray flux from ROSAT All-Sky Survey data and compare it to the expected flux from ALP to photon conversion of a CAB. The soft X-ray excess both in the center and the outskirts of Coma can be simultaneously fitted by ALP to photon conversion of a CAB. Given the uncertaint"},"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":"1406.5188","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-ph","submitted_at":"2014-06-19T20:00:22Z","cross_cats_sorted":["astro-ph.CO","astro-ph.HE","hep-th"],"title_canon_sha256":"9286e6848297c3ab426346e380fd0c4b7b7ba1680dbdcb81a14d05af99bc9b37","abstract_canon_sha256":"173019ab9b5f32d8f5ea1ec51dd6bf2e4eb67d1d5ead12d3e2fec03070bdc925"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:25:49.135615Z","signature_b64":"YPPdbKPXcT9yb4aQ9lejo+2Yb2o8C5tYbhkRacJ8J5npqCIRYRFAUJPYq+LEm/E+dYzB+BCvMI9bsdAhwZtYDA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"ba36763b37c6cde19b65ebd671773a6120831ed3e3c429e6fc7a1e0a0bf892c3","last_reissued_at":"2026-05-18T02:25:49.135196Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:25:49.135196Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"ALP Conversion and the Soft X-ray Excess in the Outskirts of the Coma Cluster","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO","astro-ph.HE","hep-th"],"primary_cat":"hep-ph","authors_text":"David Kraljic, Joseph P. Conlon, Markus Rummel","submitted_at":"2014-06-19T20:00:22Z","abstract_excerpt":"It was recently found that the soft X-ray excess in the center of the Coma cluster can be fitted by conversion of axion-like-particles (ALPs) of a cosmic axion background (CAB) to photons. We extend this analysis to the outskirts of Coma, including regions up to 5 Mpc from the center of the cluster. We extract the excess soft X-ray flux from ROSAT All-Sky Survey data and compare it to the expected flux from ALP to photon conversion of a CAB. The soft X-ray excess both in the center and the outskirts of Coma can be simultaneously fitted by ALP to photon conversion of a CAB. Given the uncertaint"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1406.5188","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":"1406.5188","created_at":"2026-05-18T02:25:49.135251+00:00"},{"alias_kind":"arxiv_version","alias_value":"1406.5188v1","created_at":"2026-05-18T02:25:49.135251+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1406.5188","created_at":"2026-05-18T02:25:49.135251+00:00"},{"alias_kind":"pith_short_12","alias_value":"XI3HMOZXY3G6","created_at":"2026-05-18T12:28:57.508820+00:00"},{"alias_kind":"pith_short_16","alias_value":"XI3HMOZXY3G6DG3F","created_at":"2026-05-18T12:28:57.508820+00:00"},{"alias_kind":"pith_short_8","alias_value":"XI3HMOZX","created_at":"2026-05-18T12:28:57.508820+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/XI3HMOZXY3G6DG3F5PLHC5Z2ME","json":"https://pith.science/pith/XI3HMOZXY3G6DG3F5PLHC5Z2ME.json","graph_json":"https://pith.science/api/pith-number/XI3HMOZXY3G6DG3F5PLHC5Z2ME/graph.json","events_json":"https://pith.science/api/pith-number/XI3HMOZXY3G6DG3F5PLHC5Z2ME/events.json","paper":"https://pith.science/paper/XI3HMOZX"},"agent_actions":{"view_html":"https://pith.science/pith/XI3HMOZXY3G6DG3F5PLHC5Z2ME","download_json":"https://pith.science/pith/XI3HMOZXY3G6DG3F5PLHC5Z2ME.json","view_paper":"https://pith.science/paper/XI3HMOZX","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1406.5188&json=true","fetch_graph":"https://pith.science/api/pith-number/XI3HMOZXY3G6DG3F5PLHC5Z2ME/graph.json","fetch_events":"https://pith.science/api/pith-number/XI3HMOZXY3G6DG3F5PLHC5Z2ME/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/XI3HMOZXY3G6DG3F5PLHC5Z2ME/action/timestamp_anchor","attest_storage":"https://pith.science/pith/XI3HMOZXY3G6DG3F5PLHC5Z2ME/action/storage_attestation","attest_author":"https://pith.science/pith/XI3HMOZXY3G6DG3F5PLHC5Z2ME/action/author_attestation","sign_citation":"https://pith.science/pith/XI3HMOZXY3G6DG3F5PLHC5Z2ME/action/citation_signature","submit_replication":"https://pith.science/pith/XI3HMOZXY3G6DG3F5PLHC5Z2ME/action/replication_record"}},"created_at":"2026-05-18T02:25:49.135251+00:00","updated_at":"2026-05-18T02:25:49.135251+00:00"}