{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2010:3IYJVHMQRPTHMJXZBSIPU6GLEM","short_pith_number":"pith:3IYJVHMQ","schema_version":"1.0","canonical_sha256":"da309a9d908be67626f90c90fa78cb230cbcd86be075420d3e1bf36a57155a95","source":{"kind":"arxiv","id":"1007.4199","version":2},"attestation_state":"computed","paper":{"title":"Indirect Dark Matter Detection Limits from the Ultra-Faint Milky Way Satellite Segue 1","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.GA","astro-ph.HE","hep-ph"],"primary_cat":"astro-ph.CO","authors_text":"(2) KIPAC/Stanford/SLAC, (3) Yale, (4) Carnegie Observatories), Joshua D. Simon (4) ((1) SLAC, Louis E. Strigari (2), Marla Geha (3), Neelima Sehgal (2), Rouven Essig (1)","submitted_at":"2010-07-23T20:00:03Z","abstract_excerpt":"We use new kinematic data from the ultra-faint Milky Way satellite Segue 1 to model its dark matter distribution and derive upper limits on the dark matter annihilation cross-section. Using gamma-ray flux upper limits from the Fermi satellite and MAGIC, we determine cross-section exclusion regions for dark matter annihilation into a variety of different particles including charged leptons. We show that these exclusion regions are beginning to probe the regions of interest for a dark matter interpretation of the electron and positron fluxes from PAMELA, Fermi, and HESS, and that future observat"},"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":"1007.4199","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2010-07-23T20:00:03Z","cross_cats_sorted":["astro-ph.GA","astro-ph.HE","hep-ph"],"title_canon_sha256":"824c2bfb59016fa042f2431609d5aa285ee9c9daca8c546d66f729d61609c16f","abstract_canon_sha256":"26df7bf6f151b79c9a49a7aab14a307797ad8fb503df1da1ff61d97ff33a3443"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T04:32:36.336806Z","signature_b64":"HgmERbUVP4XQsaDSzIw6Y4dVdSHjEra7L8afaEfU+zCoOWp/IKF1zXYCTJaegbBWeDwFsyquvO9p2lUMB2fGBw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"da309a9d908be67626f90c90fa78cb230cbcd86be075420d3e1bf36a57155a95","last_reissued_at":"2026-05-18T04:32:36.336126Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T04:32:36.336126Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Indirect Dark Matter Detection Limits from the Ultra-Faint Milky Way Satellite Segue 1","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.GA","astro-ph.HE","hep-ph"],"primary_cat":"astro-ph.CO","authors_text":"(2) KIPAC/Stanford/SLAC, (3) Yale, (4) Carnegie Observatories), Joshua D. Simon (4) ((1) SLAC, Louis E. Strigari (2), Marla Geha (3), Neelima Sehgal (2), Rouven Essig (1)","submitted_at":"2010-07-23T20:00:03Z","abstract_excerpt":"We use new kinematic data from the ultra-faint Milky Way satellite Segue 1 to model its dark matter distribution and derive upper limits on the dark matter annihilation cross-section. Using gamma-ray flux upper limits from the Fermi satellite and MAGIC, we determine cross-section exclusion regions for dark matter annihilation into a variety of different particles including charged leptons. We show that these exclusion regions are beginning to probe the regions of interest for a dark matter interpretation of the electron and positron fluxes from PAMELA, Fermi, and HESS, and that future observat"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1007.4199","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":"1007.4199","created_at":"2026-05-18T04:32:36.336222+00:00"},{"alias_kind":"arxiv_version","alias_value":"1007.4199v2","created_at":"2026-05-18T04:32:36.336222+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1007.4199","created_at":"2026-05-18T04:32:36.336222+00:00"},{"alias_kind":"pith_short_12","alias_value":"3IYJVHMQRPTH","created_at":"2026-05-18T12:26:03.138858+00:00"},{"alias_kind":"pith_short_16","alias_value":"3IYJVHMQRPTHMJXZ","created_at":"2026-05-18T12:26:03.138858+00:00"},{"alias_kind":"pith_short_8","alias_value":"3IYJVHMQ","created_at":"2026-05-18T12:26:03.138858+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/3IYJVHMQRPTHMJXZBSIPU6GLEM","json":"https://pith.science/pith/3IYJVHMQRPTHMJXZBSIPU6GLEM.json","graph_json":"https://pith.science/api/pith-number/3IYJVHMQRPTHMJXZBSIPU6GLEM/graph.json","events_json":"https://pith.science/api/pith-number/3IYJVHMQRPTHMJXZBSIPU6GLEM/events.json","paper":"https://pith.science/paper/3IYJVHMQ"},"agent_actions":{"view_html":"https://pith.science/pith/3IYJVHMQRPTHMJXZBSIPU6GLEM","download_json":"https://pith.science/pith/3IYJVHMQRPTHMJXZBSIPU6GLEM.json","view_paper":"https://pith.science/paper/3IYJVHMQ","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1007.4199&json=true","fetch_graph":"https://pith.science/api/pith-number/3IYJVHMQRPTHMJXZBSIPU6GLEM/graph.json","fetch_events":"https://pith.science/api/pith-number/3IYJVHMQRPTHMJXZBSIPU6GLEM/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/3IYJVHMQRPTHMJXZBSIPU6GLEM/action/timestamp_anchor","attest_storage":"https://pith.science/pith/3IYJVHMQRPTHMJXZBSIPU6GLEM/action/storage_attestation","attest_author":"https://pith.science/pith/3IYJVHMQRPTHMJXZBSIPU6GLEM/action/author_attestation","sign_citation":"https://pith.science/pith/3IYJVHMQRPTHMJXZBSIPU6GLEM/action/citation_signature","submit_replication":"https://pith.science/pith/3IYJVHMQRPTHMJXZBSIPU6GLEM/action/replication_record"}},"created_at":"2026-05-18T04:32:36.336222+00:00","updated_at":"2026-05-18T04:32:36.336222+00:00"}