{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2011:5LAOLTEXWQOWZXBG6VS5LZYMUH","short_pith_number":"pith:5LAOLTEX","schema_version":"1.0","canonical_sha256":"eac0e5cc97b41d6cdc26f565d5e70ca1f3ba2f9c3c09ebc3e45baaee7b87c637","source":{"kind":"arxiv","id":"1108.1407","version":2},"attestation_state":"computed","paper":{"title":"Dark Matter Detection with Hard X-ray Telescopes","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO","hep-ph"],"primary_cat":"astro-ph.HE","authors_text":"Stefano Profumo, Tesla E. Jeltema","submitted_at":"2011-08-05T20:18:00Z","abstract_excerpt":"We analyze the impact of future hard X-ray observations on the search for indirect signatures of particle dark matter in large extragalactic systems such as nearby clusters or groups of galaxies. We argue that the hard X-ray energy band falls squarely at the peak of the inverse Compton emission from electrons and positrons produced by dark matter annihilation or decay for a large class of dark matter models. Specifically, the most promising are low-mass models with a hard electron-positron annihilation final state spectrum and intermediate-mass models with a soft electron-positron spectrum. We"},"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":"1108.1407","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2011-08-05T20:18:00Z","cross_cats_sorted":["astro-ph.CO","hep-ph"],"title_canon_sha256":"6bc16932754c8aabffd6f16330773158666e1433294f2ce880437633f9d1c69c","abstract_canon_sha256":"2eba4d67af865197550abce6ee13b8da211ee9cd4d46c6b4cb1cd2f269adcaa4"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:01:00.930685Z","signature_b64":"a+TB9S0fqwU6uGSXVn3k6esbrswGfAmcanR8SyzTPGc9yG0aD1J0Wo42Kzl6ohgnD4EnSowyHkQHp1Xo6ZRCBA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"eac0e5cc97b41d6cdc26f565d5e70ca1f3ba2f9c3c09ebc3e45baaee7b87c637","last_reissued_at":"2026-05-18T02:01:00.930177Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:01:00.930177Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Dark Matter Detection with Hard X-ray Telescopes","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO","hep-ph"],"primary_cat":"astro-ph.HE","authors_text":"Stefano Profumo, Tesla E. Jeltema","submitted_at":"2011-08-05T20:18:00Z","abstract_excerpt":"We analyze the impact of future hard X-ray observations on the search for indirect signatures of particle dark matter in large extragalactic systems such as nearby clusters or groups of galaxies. We argue that the hard X-ray energy band falls squarely at the peak of the inverse Compton emission from electrons and positrons produced by dark matter annihilation or decay for a large class of dark matter models. Specifically, the most promising are low-mass models with a hard electron-positron annihilation final state spectrum and intermediate-mass models with a soft electron-positron spectrum. We"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1108.1407","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":""},"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":"1108.1407","created_at":"2026-05-18T02:01:00.930256+00:00"},{"alias_kind":"arxiv_version","alias_value":"1108.1407v2","created_at":"2026-05-18T02:01:00.930256+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1108.1407","created_at":"2026-05-18T02:01:00.930256+00:00"},{"alias_kind":"pith_short_12","alias_value":"5LAOLTEXWQOW","created_at":"2026-05-18T12:26:20.644004+00:00"},{"alias_kind":"pith_short_16","alias_value":"5LAOLTEXWQOWZXBG","created_at":"2026-05-18T12:26:20.644004+00:00"},{"alias_kind":"pith_short_8","alias_value":"5LAOLTEX","created_at":"2026-05-18T12:26:20.644004+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/5LAOLTEXWQOWZXBG6VS5LZYMUH","json":"https://pith.science/pith/5LAOLTEXWQOWZXBG6VS5LZYMUH.json","graph_json":"https://pith.science/api/pith-number/5LAOLTEXWQOWZXBG6VS5LZYMUH/graph.json","events_json":"https://pith.science/api/pith-number/5LAOLTEXWQOWZXBG6VS5LZYMUH/events.json","paper":"https://pith.science/paper/5LAOLTEX"},"agent_actions":{"view_html":"https://pith.science/pith/5LAOLTEXWQOWZXBG6VS5LZYMUH","download_json":"https://pith.science/pith/5LAOLTEXWQOWZXBG6VS5LZYMUH.json","view_paper":"https://pith.science/paper/5LAOLTEX","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1108.1407&json=true","fetch_graph":"https://pith.science/api/pith-number/5LAOLTEXWQOWZXBG6VS5LZYMUH/graph.json","fetch_events":"https://pith.science/api/pith-number/5LAOLTEXWQOWZXBG6VS5LZYMUH/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/5LAOLTEXWQOWZXBG6VS5LZYMUH/action/timestamp_anchor","attest_storage":"https://pith.science/pith/5LAOLTEXWQOWZXBG6VS5LZYMUH/action/storage_attestation","attest_author":"https://pith.science/pith/5LAOLTEXWQOWZXBG6VS5LZYMUH/action/author_attestation","sign_citation":"https://pith.science/pith/5LAOLTEXWQOWZXBG6VS5LZYMUH/action/citation_signature","submit_replication":"https://pith.science/pith/5LAOLTEXWQOWZXBG6VS5LZYMUH/action/replication_record"}},"created_at":"2026-05-18T02:01:00.930256+00:00","updated_at":"2026-05-18T02:01:00.930256+00:00"}