{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2018:T6UXLUOTFM7X2FRKIL3ODGXX6P","short_pith_number":"pith:T6UXLUOT","schema_version":"1.0","canonical_sha256":"9fa975d1d32b3f7d162a42f6e19af7f3c75bb9a825d30722e5d658aedf929676","source":{"kind":"arxiv","id":"1804.05052","version":2},"attestation_state":"computed","paper":{"title":"On velocity-dependent dark matter annihilations in dwarf satellites","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO","astro-ph.HE","hep-ph"],"primary_cat":"astro-ph.GA","authors_text":"Mauro Valli, Mihael Petac, Piero Ullio","submitted_at":"2018-04-13T17:43:34Z","abstract_excerpt":"Milky Way dwarf spheroidal satellites are a prime target for Dark Matter (DM) indirect searches. There have been recent reassessments of the expected DM gamma-ray signals in case of long-range interactions, commonly known as Sommerfeld enhancement. Since details of the underlying DM phase-space distribution function become critical, there are potentially large uncertainties in the final result. We provide here a first attempt towards a comprehensive investigation of these systematics, addressing the impact on the expected DM flux from Milky Way dwarfs via Bayesian inference on the available st"},"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":"1804.05052","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2018-04-13T17:43:34Z","cross_cats_sorted":["astro-ph.CO","astro-ph.HE","hep-ph"],"title_canon_sha256":"74b677a17afec274e64a04bdd3971920ab12f7e16684fe0249bc814bd76801e5","abstract_canon_sha256":"e2b0903bf77a09f68f6e3eb17023f45f6db8b962b9e512ce64db0d1443b3f5dc"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-17T23:57:50.700370Z","signature_b64":"C+BqdBPrDPLwJXKBR2Y6AWZaeOfZjL/m3fPPyU8DoPXAeB6NiZONDttGFSQvgOK6BxPSuwEiTEfnrxGthAq+CA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"9fa975d1d32b3f7d162a42f6e19af7f3c75bb9a825d30722e5d658aedf929676","last_reissued_at":"2026-05-17T23:57:50.699770Z","signature_status":"signed_v1","first_computed_at":"2026-05-17T23:57:50.699770Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"On velocity-dependent dark matter annihilations in dwarf satellites","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO","astro-ph.HE","hep-ph"],"primary_cat":"astro-ph.GA","authors_text":"Mauro Valli, Mihael Petac, Piero Ullio","submitted_at":"2018-04-13T17:43:34Z","abstract_excerpt":"Milky Way dwarf spheroidal satellites are a prime target for Dark Matter (DM) indirect searches. There have been recent reassessments of the expected DM gamma-ray signals in case of long-range interactions, commonly known as Sommerfeld enhancement. Since details of the underlying DM phase-space distribution function become critical, there are potentially large uncertainties in the final result. We provide here a first attempt towards a comprehensive investigation of these systematics, addressing the impact on the expected DM flux from Milky Way dwarfs via Bayesian inference on the available st"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1804.05052","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":"1804.05052","created_at":"2026-05-17T23:57:50.699856+00:00"},{"alias_kind":"arxiv_version","alias_value":"1804.05052v2","created_at":"2026-05-17T23:57:50.699856+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1804.05052","created_at":"2026-05-17T23:57:50.699856+00:00"},{"alias_kind":"pith_short_12","alias_value":"T6UXLUOTFM7X","created_at":"2026-05-18T12:32:53.628368+00:00"},{"alias_kind":"pith_short_16","alias_value":"T6UXLUOTFM7X2FRK","created_at":"2026-05-18T12:32:53.628368+00:00"},{"alias_kind":"pith_short_8","alias_value":"T6UXLUOT","created_at":"2026-05-18T12:32:53.628368+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2501.04663","citing_title":"Searching for dark matter annihilating into light long-lived mediators from stars inside dwarf spheroidal galaxies","ref_index":21,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/T6UXLUOTFM7X2FRKIL3ODGXX6P","json":"https://pith.science/pith/T6UXLUOTFM7X2FRKIL3ODGXX6P.json","graph_json":"https://pith.science/api/pith-number/T6UXLUOTFM7X2FRKIL3ODGXX6P/graph.json","events_json":"https://pith.science/api/pith-number/T6UXLUOTFM7X2FRKIL3ODGXX6P/events.json","paper":"https://pith.science/paper/T6UXLUOT"},"agent_actions":{"view_html":"https://pith.science/pith/T6UXLUOTFM7X2FRKIL3ODGXX6P","download_json":"https://pith.science/pith/T6UXLUOTFM7X2FRKIL3ODGXX6P.json","view_paper":"https://pith.science/paper/T6UXLUOT","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1804.05052&json=true","fetch_graph":"https://pith.science/api/pith-number/T6UXLUOTFM7X2FRKIL3ODGXX6P/graph.json","fetch_events":"https://pith.science/api/pith-number/T6UXLUOTFM7X2FRKIL3ODGXX6P/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/T6UXLUOTFM7X2FRKIL3ODGXX6P/action/timestamp_anchor","attest_storage":"https://pith.science/pith/T6UXLUOTFM7X2FRKIL3ODGXX6P/action/storage_attestation","attest_author":"https://pith.science/pith/T6UXLUOTFM7X2FRKIL3ODGXX6P/action/author_attestation","sign_citation":"https://pith.science/pith/T6UXLUOTFM7X2FRKIL3ODGXX6P/action/citation_signature","submit_replication":"https://pith.science/pith/T6UXLUOTFM7X2FRKIL3ODGXX6P/action/replication_record"}},"created_at":"2026-05-17T23:57:50.699856+00:00","updated_at":"2026-05-17T23:57:50.699856+00:00"}