{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2018:DUTORXL4GQEGXEULRNXHYCY7AS","short_pith_number":"pith:DUTORXL4","schema_version":"1.0","canonical_sha256":"1d26e8dd7c34086b928b8b6e7c0b1f04a90d3c48784e0a0c9852d1b05633d683","source":{"kind":"arxiv","id":"1808.04388","version":2},"attestation_state":"computed","paper":{"title":"Hunting for Heavy Winos in the Galactic Center","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO","hep-ph"],"primary_cat":"astro-ph.HE","authors_text":"Emmanuel Moulin, Iain W. Stewart, Ian Moult, Lucia Rinchiuso, Matthew Baumgart, Nicholas L. Rodd, Timothy Cohen, Tracy R. Slatyer, Varun Vaidya","submitted_at":"2018-08-13T18:15:57Z","abstract_excerpt":"Observing gamma rays using ground-based atmospheric Cherenkov telescopes provides one of the only probes of heavy weakly interacting dark matter. A canonical target is the thermal wino, for which the strongest limits come from searches for photon lines from annihilations in the Galactic Center. Irreducible finite energy resolution effects motivate refining the prediction for a wino signal beyond the photon line approximation; recently, modern effective field theory techniques have been utilized to obtain a precise calculation of the full photon energy spectrum from wino annihilation. In this p"},"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":"1808.04388","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2018-08-13T18:15:57Z","cross_cats_sorted":["astro-ph.CO","hep-ph"],"title_canon_sha256":"f7e6996338ffdb9c8a3c0432280b61856ee99e405c28e9030360209de1c45b8f","abstract_canon_sha256":"a4944b335045de13535c9a90b992192ebb3ec8499cc05d2105d3d64b78234e9f"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-17T23:57:36.162539Z","signature_b64":"LrNAeCtgXruNqs2TaPMVCom7qJmVrKRDrCY73PPUWVkwJRUmcAohqTnNWpZRjMRml3cdAWTb5thoy4tdy8ZTBw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"1d26e8dd7c34086b928b8b6e7c0b1f04a90d3c48784e0a0c9852d1b05633d683","last_reissued_at":"2026-05-17T23:57:36.162035Z","signature_status":"signed_v1","first_computed_at":"2026-05-17T23:57:36.162035Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Hunting for Heavy Winos in the Galactic Center","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO","hep-ph"],"primary_cat":"astro-ph.HE","authors_text":"Emmanuel Moulin, Iain W. Stewart, Ian Moult, Lucia Rinchiuso, Matthew Baumgart, Nicholas L. Rodd, Timothy Cohen, Tracy R. Slatyer, Varun Vaidya","submitted_at":"2018-08-13T18:15:57Z","abstract_excerpt":"Observing gamma rays using ground-based atmospheric Cherenkov telescopes provides one of the only probes of heavy weakly interacting dark matter. A canonical target is the thermal wino, for which the strongest limits come from searches for photon lines from annihilations in the Galactic Center. Irreducible finite energy resolution effects motivate refining the prediction for a wino signal beyond the photon line approximation; recently, modern effective field theory techniques have been utilized to obtain a precise calculation of the full photon energy spectrum from wino annihilation. In this p"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1808.04388","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":"1808.04388","created_at":"2026-05-17T23:57:36.162119+00:00"},{"alias_kind":"arxiv_version","alias_value":"1808.04388v2","created_at":"2026-05-17T23:57:36.162119+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1808.04388","created_at":"2026-05-17T23:57:36.162119+00:00"},{"alias_kind":"pith_short_12","alias_value":"DUTORXL4GQEG","created_at":"2026-05-18T12:32:19.392346+00:00"},{"alias_kind":"pith_short_16","alias_value":"DUTORXL4GQEGXEUL","created_at":"2026-05-18T12:32:19.392346+00:00"},{"alias_kind":"pith_short_8","alias_value":"DUTORXL4","created_at":"2026-05-18T12:32:19.392346+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/DUTORXL4GQEGXEULRNXHYCY7AS","json":"https://pith.science/pith/DUTORXL4GQEGXEULRNXHYCY7AS.json","graph_json":"https://pith.science/api/pith-number/DUTORXL4GQEGXEULRNXHYCY7AS/graph.json","events_json":"https://pith.science/api/pith-number/DUTORXL4GQEGXEULRNXHYCY7AS/events.json","paper":"https://pith.science/paper/DUTORXL4"},"agent_actions":{"view_html":"https://pith.science/pith/DUTORXL4GQEGXEULRNXHYCY7AS","download_json":"https://pith.science/pith/DUTORXL4GQEGXEULRNXHYCY7AS.json","view_paper":"https://pith.science/paper/DUTORXL4","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1808.04388&json=true","fetch_graph":"https://pith.science/api/pith-number/DUTORXL4GQEGXEULRNXHYCY7AS/graph.json","fetch_events":"https://pith.science/api/pith-number/DUTORXL4GQEGXEULRNXHYCY7AS/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/DUTORXL4GQEGXEULRNXHYCY7AS/action/timestamp_anchor","attest_storage":"https://pith.science/pith/DUTORXL4GQEGXEULRNXHYCY7AS/action/storage_attestation","attest_author":"https://pith.science/pith/DUTORXL4GQEGXEULRNXHYCY7AS/action/author_attestation","sign_citation":"https://pith.science/pith/DUTORXL4GQEGXEULRNXHYCY7AS/action/citation_signature","submit_replication":"https://pith.science/pith/DUTORXL4GQEGXEULRNXHYCY7AS/action/replication_record"}},"created_at":"2026-05-17T23:57:36.162119+00:00","updated_at":"2026-05-17T23:57:36.162119+00:00"}