{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2011:3NT4MZIG74EQDJ4AB6NUO4OCLD","short_pith_number":"pith:3NT4MZIG","schema_version":"1.0","canonical_sha256":"db67c66506ff0901a7800f9b4771c258d89878f89f3325fc0bea4b16cd92ed51","source":{"kind":"arxiv","id":"1101.4842","version":1},"attestation_state":"computed","paper":{"title":"On the Detectability of High-Energy Galactic Neutrino Sources","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Felix Aharonian, Francesco Vissani, Narek Sahakyan","submitted_at":"2011-01-25T15:09:47Z","abstract_excerpt":"With the arrival of km**3 volume scale neutrino detectors the chances to detect the first astronomical sources of TeV neutrinos will be dramatically increased. While the theoretical estimates of the neutrino fluxes contain large uncertainties, we can formulate the conditions for the detectability of certain neutrino sources phenomenologically. In fact, since most galactic neutrino sources are transparent for TeV gamma-rays, their detectability implies a minimum flux of the accompanying gamma-rays. For a typical energy-dependence of detection areas of km**3 volume neutrino detectors, we obtain "},"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":"1101.4842","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2011-01-25T15:09:47Z","cross_cats_sorted":[],"title_canon_sha256":"79d45c36b41f6498e079ed146f7face6cbf999d88378a91b3c16eaa59ce2e160","abstract_canon_sha256":"64cea9b2b06ab2cf9920c4343a23a6e9550b8b839dcec3ee3aa2f6270fa7c499"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T04:23:22.826861Z","signature_b64":"ejNlGkMdpzJwdBrYrj7KhkCMyUHMoH/5DixYVsxjfC2rTIVcAnn3TnRHSksUSTtKzBhOJ7Xxh9hHIF33/ivUBg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"db67c66506ff0901a7800f9b4771c258d89878f89f3325fc0bea4b16cd92ed51","last_reissued_at":"2026-05-18T04:23:22.826423Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T04:23:22.826423Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"On the Detectability of High-Energy Galactic Neutrino Sources","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Felix Aharonian, Francesco Vissani, Narek Sahakyan","submitted_at":"2011-01-25T15:09:47Z","abstract_excerpt":"With the arrival of km**3 volume scale neutrino detectors the chances to detect the first astronomical sources of TeV neutrinos will be dramatically increased. While the theoretical estimates of the neutrino fluxes contain large uncertainties, we can formulate the conditions for the detectability of certain neutrino sources phenomenologically. In fact, since most galactic neutrino sources are transparent for TeV gamma-rays, their detectability implies a minimum flux of the accompanying gamma-rays. For a typical energy-dependence of detection areas of km**3 volume neutrino detectors, we obtain "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1101.4842","kind":"arxiv","version":1},"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":"1101.4842","created_at":"2026-05-18T04:23:22.826483+00:00"},{"alias_kind":"arxiv_version","alias_value":"1101.4842v1","created_at":"2026-05-18T04:23:22.826483+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1101.4842","created_at":"2026-05-18T04:23:22.826483+00:00"},{"alias_kind":"pith_short_12","alias_value":"3NT4MZIG74EQ","created_at":"2026-05-18T12:26:18.847500+00:00"},{"alias_kind":"pith_short_16","alias_value":"3NT4MZIG74EQDJ4A","created_at":"2026-05-18T12:26:18.847500+00:00"},{"alias_kind":"pith_short_8","alias_value":"3NT4MZIG","created_at":"2026-05-18T12:26:18.847500+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/3NT4MZIG74EQDJ4AB6NUO4OCLD","json":"https://pith.science/pith/3NT4MZIG74EQDJ4AB6NUO4OCLD.json","graph_json":"https://pith.science/api/pith-number/3NT4MZIG74EQDJ4AB6NUO4OCLD/graph.json","events_json":"https://pith.science/api/pith-number/3NT4MZIG74EQDJ4AB6NUO4OCLD/events.json","paper":"https://pith.science/paper/3NT4MZIG"},"agent_actions":{"view_html":"https://pith.science/pith/3NT4MZIG74EQDJ4AB6NUO4OCLD","download_json":"https://pith.science/pith/3NT4MZIG74EQDJ4AB6NUO4OCLD.json","view_paper":"https://pith.science/paper/3NT4MZIG","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1101.4842&json=true","fetch_graph":"https://pith.science/api/pith-number/3NT4MZIG74EQDJ4AB6NUO4OCLD/graph.json","fetch_events":"https://pith.science/api/pith-number/3NT4MZIG74EQDJ4AB6NUO4OCLD/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/3NT4MZIG74EQDJ4AB6NUO4OCLD/action/timestamp_anchor","attest_storage":"https://pith.science/pith/3NT4MZIG74EQDJ4AB6NUO4OCLD/action/storage_attestation","attest_author":"https://pith.science/pith/3NT4MZIG74EQDJ4AB6NUO4OCLD/action/author_attestation","sign_citation":"https://pith.science/pith/3NT4MZIG74EQDJ4AB6NUO4OCLD/action/citation_signature","submit_replication":"https://pith.science/pith/3NT4MZIG74EQDJ4AB6NUO4OCLD/action/replication_record"}},"created_at":"2026-05-18T04:23:22.826483+00:00","updated_at":"2026-05-18T04:23:22.826483+00:00"}