{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2017:BRMDTNJJQ63J5WNCMDGLGYQKTH","short_pith_number":"pith:BRMDTNJJ","schema_version":"1.0","canonical_sha256":"0c5839b52987b69ed9a260ccb3620a99efd4a2ca85dd11af52b19bad6d10d0ff","source":{"kind":"arxiv","id":"1705.09384","version":2},"attestation_state":"computed","paper":{"title":"Multiwavelength Analysis of Dark Matter Annihilation and RX-DMFIT","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO","hep-ph"],"primary_cat":"astro-ph.HE","authors_text":"Alex McDaniel, Emma Storm, Stefano Profumo, Tesla Jeltema","submitted_at":"2017-05-25T22:38:10Z","abstract_excerpt":"Dark matter (DM) particles are predicted by several well motivated models to yield Standard Model particles through self-annihilation that can potentially be detected by astrophysical observations. In particular, the production of charged particles from DM annihilation in astrophysical systems that contain magnetic fields yields radio emission through synchrotron radiation and X-ray emission through inverse Compton scattering of ambient photons. We introduce RX-DMFIT, a tool used for calculating the expected secondary emission from DM annihilation. RX-DMFIT includes a wide range of customizabl"},"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":"1705.09384","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2017-05-25T22:38:10Z","cross_cats_sorted":["astro-ph.CO","hep-ph"],"title_canon_sha256":"c91ef055b553dd87bf4d0cd30b757dc082c216c5582f01c9edaadfdf383c765e","abstract_canon_sha256":"1f1d923eecab651ed04c516d5c97619ab2d173dedd22ba98514600793af88602"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:16:09.058576Z","signature_b64":"aSH4oBT3cbzsdHDnwyI6OYphqsHwUXa0O6cONY02/ft4uspurSnRLl8cYNGRuikJzwiXqvNvUnVzZ3Q3CZOqCA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"0c5839b52987b69ed9a260ccb3620a99efd4a2ca85dd11af52b19bad6d10d0ff","last_reissued_at":"2026-05-18T00:16:09.057806Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:16:09.057806Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Multiwavelength Analysis of Dark Matter Annihilation and RX-DMFIT","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO","hep-ph"],"primary_cat":"astro-ph.HE","authors_text":"Alex McDaniel, Emma Storm, Stefano Profumo, Tesla Jeltema","submitted_at":"2017-05-25T22:38:10Z","abstract_excerpt":"Dark matter (DM) particles are predicted by several well motivated models to yield Standard Model particles through self-annihilation that can potentially be detected by astrophysical observations. In particular, the production of charged particles from DM annihilation in astrophysical systems that contain magnetic fields yields radio emission through synchrotron radiation and X-ray emission through inverse Compton scattering of ambient photons. We introduce RX-DMFIT, a tool used for calculating the expected secondary emission from DM annihilation. RX-DMFIT includes a wide range of customizabl"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1705.09384","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":"1705.09384","created_at":"2026-05-18T00:16:09.057941+00:00"},{"alias_kind":"arxiv_version","alias_value":"1705.09384v2","created_at":"2026-05-18T00:16:09.057941+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1705.09384","created_at":"2026-05-18T00:16:09.057941+00:00"},{"alias_kind":"pith_short_12","alias_value":"BRMDTNJJQ63J","created_at":"2026-05-18T12:31:08.081275+00:00"},{"alias_kind":"pith_short_16","alias_value":"BRMDTNJJQ63J5WNC","created_at":"2026-05-18T12:31:08.081275+00:00"},{"alias_kind":"pith_short_8","alias_value":"BRMDTNJJ","created_at":"2026-05-18T12:31:08.081275+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/BRMDTNJJQ63J5WNCMDGLGYQKTH","json":"https://pith.science/pith/BRMDTNJJQ63J5WNCMDGLGYQKTH.json","graph_json":"https://pith.science/api/pith-number/BRMDTNJJQ63J5WNCMDGLGYQKTH/graph.json","events_json":"https://pith.science/api/pith-number/BRMDTNJJQ63J5WNCMDGLGYQKTH/events.json","paper":"https://pith.science/paper/BRMDTNJJ"},"agent_actions":{"view_html":"https://pith.science/pith/BRMDTNJJQ63J5WNCMDGLGYQKTH","download_json":"https://pith.science/pith/BRMDTNJJQ63J5WNCMDGLGYQKTH.json","view_paper":"https://pith.science/paper/BRMDTNJJ","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1705.09384&json=true","fetch_graph":"https://pith.science/api/pith-number/BRMDTNJJQ63J5WNCMDGLGYQKTH/graph.json","fetch_events":"https://pith.science/api/pith-number/BRMDTNJJQ63J5WNCMDGLGYQKTH/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/BRMDTNJJQ63J5WNCMDGLGYQKTH/action/timestamp_anchor","attest_storage":"https://pith.science/pith/BRMDTNJJQ63J5WNCMDGLGYQKTH/action/storage_attestation","attest_author":"https://pith.science/pith/BRMDTNJJQ63J5WNCMDGLGYQKTH/action/author_attestation","sign_citation":"https://pith.science/pith/BRMDTNJJQ63J5WNCMDGLGYQKTH/action/citation_signature","submit_replication":"https://pith.science/pith/BRMDTNJJQ63J5WNCMDGLGYQKTH/action/replication_record"}},"created_at":"2026-05-18T00:16:09.057941+00:00","updated_at":"2026-05-18T00:16:09.057941+00:00"}