{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2017:NFH6GCQDE6IDW5J2GDH5GTHZ4F","short_pith_number":"pith:NFH6GCQD","schema_version":"1.0","canonical_sha256":"694fe30a0327903b753a30cfd34cf9e178a306db096c27c5f6f58be3bd939f59","source":{"kind":"arxiv","id":"1703.09721","version":3},"attestation_state":"computed","paper":{"title":"The Galactic Contribution to IceCube's Astrophysical Neutrino Flux","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-ph"],"primary_cat":"astro-ph.HE","authors_text":"Danny Marfatia, Peter B. Denton, Thomas J. Weiler","submitted_at":"2017-03-28T18:00:14Z","abstract_excerpt":"High energy neutrinos have been detected by IceCube, but their origin remains a mystery. Determining the sources of this flux is a crucial first step towards multi-messenger studies. In this work we systematically compare two classes of sources with the data: Galactic and extragalactic. We assume that the neutrino sources are distributed according to a class of Galactic models. We build a likelihood function on an event by event basis including energy, event topology, absorption, and direction information. We present the probability that each high energy event with deposited energy $E_{\\rm dep"},"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":"1703.09721","kind":"arxiv","version":3},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2017-03-28T18:00:14Z","cross_cats_sorted":["hep-ph"],"title_canon_sha256":"f25c392a7b82b0726667f570d98646768b6605913a180e6ecc00baf45535ffe4","abstract_canon_sha256":"866b187d3ca7b0a437aa648e8d993e1fd51df1ae46a8e2862136fc1f9ff98982"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:36:24.294544Z","signature_b64":"Ic6u62WbGA6nL/h3WlL/BsxD/7iJNh14Ua5m1C0ym3YXBNGagBRVpAQAqCFDvmodj9mM6Kp52vUxfBV/CBtIDw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"694fe30a0327903b753a30cfd34cf9e178a306db096c27c5f6f58be3bd939f59","last_reissued_at":"2026-05-18T00:36:24.293930Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:36:24.293930Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The Galactic Contribution to IceCube's Astrophysical Neutrino Flux","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-ph"],"primary_cat":"astro-ph.HE","authors_text":"Danny Marfatia, Peter B. Denton, Thomas J. Weiler","submitted_at":"2017-03-28T18:00:14Z","abstract_excerpt":"High energy neutrinos have been detected by IceCube, but their origin remains a mystery. Determining the sources of this flux is a crucial first step towards multi-messenger studies. In this work we systematically compare two classes of sources with the data: Galactic and extragalactic. We assume that the neutrino sources are distributed according to a class of Galactic models. We build a likelihood function on an event by event basis including energy, event topology, absorption, and direction information. We present the probability that each high energy event with deposited energy $E_{\\rm dep"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1703.09721","kind":"arxiv","version":3},"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":"1703.09721","created_at":"2026-05-18T00:36:24.294038+00:00"},{"alias_kind":"arxiv_version","alias_value":"1703.09721v3","created_at":"2026-05-18T00:36:24.294038+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1703.09721","created_at":"2026-05-18T00:36:24.294038+00:00"},{"alias_kind":"pith_short_12","alias_value":"NFH6GCQDE6ID","created_at":"2026-05-18T12:31:31.346846+00:00"},{"alias_kind":"pith_short_16","alias_value":"NFH6GCQDE6IDW5J2","created_at":"2026-05-18T12:31:31.346846+00:00"},{"alias_kind":"pith_short_8","alias_value":"NFH6GCQD","created_at":"2026-05-18T12:31:31.346846+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/NFH6GCQDE6IDW5J2GDH5GTHZ4F","json":"https://pith.science/pith/NFH6GCQDE6IDW5J2GDH5GTHZ4F.json","graph_json":"https://pith.science/api/pith-number/NFH6GCQDE6IDW5J2GDH5GTHZ4F/graph.json","events_json":"https://pith.science/api/pith-number/NFH6GCQDE6IDW5J2GDH5GTHZ4F/events.json","paper":"https://pith.science/paper/NFH6GCQD"},"agent_actions":{"view_html":"https://pith.science/pith/NFH6GCQDE6IDW5J2GDH5GTHZ4F","download_json":"https://pith.science/pith/NFH6GCQDE6IDW5J2GDH5GTHZ4F.json","view_paper":"https://pith.science/paper/NFH6GCQD","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1703.09721&json=true","fetch_graph":"https://pith.science/api/pith-number/NFH6GCQDE6IDW5J2GDH5GTHZ4F/graph.json","fetch_events":"https://pith.science/api/pith-number/NFH6GCQDE6IDW5J2GDH5GTHZ4F/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/NFH6GCQDE6IDW5J2GDH5GTHZ4F/action/timestamp_anchor","attest_storage":"https://pith.science/pith/NFH6GCQDE6IDW5J2GDH5GTHZ4F/action/storage_attestation","attest_author":"https://pith.science/pith/NFH6GCQDE6IDW5J2GDH5GTHZ4F/action/author_attestation","sign_citation":"https://pith.science/pith/NFH6GCQDE6IDW5J2GDH5GTHZ4F/action/citation_signature","submit_replication":"https://pith.science/pith/NFH6GCQDE6IDW5J2GDH5GTHZ4F/action/replication_record"}},"created_at":"2026-05-18T00:36:24.294038+00:00","updated_at":"2026-05-18T00:36:24.294038+00:00"}