{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2017:DQHSPALDSVR5ARW7UOANOHT73P","short_pith_number":"pith:DQHSPALD","schema_version":"1.0","canonical_sha256":"1c0f2781639563d046dfa380d71e7fdbc615f54adbeb0a94d3d2cdaf6e87c339","source":{"kind":"arxiv","id":"1710.00705","version":1},"attestation_state":"computed","paper":{"title":"Observing the Next Galactic Supernova with the NOvA Detectors","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-ex","physics.ins-det"],"primary_cat":"astro-ph.IM","authors_text":"Alec Habig (the NOvA Collaboration), Andrey Sheshukov, Justin A. Vasel","submitted_at":"2017-10-02T14:57:10Z","abstract_excerpt":"The next galactic core-collapse supernova will deliver a wealth of neutrinos which for the first time we are well-situated to measure. These explosions produce neutrinos with energies between 10 and 100 MeV over a period of tens of seconds. Galactic supernovae are relatively rare events, occurring with a frequency of just a few per century. It is therefore essential that all neutrino detectors capable of detecting these neutrinos are ready to trigger on this signal when it occurs. This poster describes a data-driven trigger which is designed to detect the neutrino signal from a galactic core-c"},"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":"1710.00705","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.IM","submitted_at":"2017-10-02T14:57:10Z","cross_cats_sorted":["hep-ex","physics.ins-det"],"title_canon_sha256":"de93cd22ab084f7ad2bab017b0f865f6013fa770927059e6abedc1b408576a21","abstract_canon_sha256":"f4b958b490502db10e14e6d3d3a532e3c701aedfaf72de85d7cd69dc0db68e76"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:33:53.969483Z","signature_b64":"JBJqPjRWejI50CmG5zFWZpBHtN/tLbTYCntoPf7fidEqBOVUKdkRptpuPY6BAd0wa2OM46w56JXW7fJoLZJABg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"1c0f2781639563d046dfa380d71e7fdbc615f54adbeb0a94d3d2cdaf6e87c339","last_reissued_at":"2026-05-18T00:33:53.968990Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:33:53.968990Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Observing the Next Galactic Supernova with the NOvA Detectors","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-ex","physics.ins-det"],"primary_cat":"astro-ph.IM","authors_text":"Alec Habig (the NOvA Collaboration), Andrey Sheshukov, Justin A. Vasel","submitted_at":"2017-10-02T14:57:10Z","abstract_excerpt":"The next galactic core-collapse supernova will deliver a wealth of neutrinos which for the first time we are well-situated to measure. These explosions produce neutrinos with energies between 10 and 100 MeV over a period of tens of seconds. Galactic supernovae are relatively rare events, occurring with a frequency of just a few per century. It is therefore essential that all neutrino detectors capable of detecting these neutrinos are ready to trigger on this signal when it occurs. This poster describes a data-driven trigger which is designed to detect the neutrino signal from a galactic core-c"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1710.00705","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":"1710.00705","created_at":"2026-05-18T00:33:53.969063+00:00"},{"alias_kind":"arxiv_version","alias_value":"1710.00705v1","created_at":"2026-05-18T00:33:53.969063+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1710.00705","created_at":"2026-05-18T00:33:53.969063+00:00"},{"alias_kind":"pith_short_12","alias_value":"DQHSPALDSVR5","created_at":"2026-05-18T12:31:12.930513+00:00"},{"alias_kind":"pith_short_16","alias_value":"DQHSPALDSVR5ARW7","created_at":"2026-05-18T12:31:12.930513+00:00"},{"alias_kind":"pith_short_8","alias_value":"DQHSPALD","created_at":"2026-05-18T12:31:12.930513+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/DQHSPALDSVR5ARW7UOANOHT73P","json":"https://pith.science/pith/DQHSPALDSVR5ARW7UOANOHT73P.json","graph_json":"https://pith.science/api/pith-number/DQHSPALDSVR5ARW7UOANOHT73P/graph.json","events_json":"https://pith.science/api/pith-number/DQHSPALDSVR5ARW7UOANOHT73P/events.json","paper":"https://pith.science/paper/DQHSPALD"},"agent_actions":{"view_html":"https://pith.science/pith/DQHSPALDSVR5ARW7UOANOHT73P","download_json":"https://pith.science/pith/DQHSPALDSVR5ARW7UOANOHT73P.json","view_paper":"https://pith.science/paper/DQHSPALD","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1710.00705&json=true","fetch_graph":"https://pith.science/api/pith-number/DQHSPALDSVR5ARW7UOANOHT73P/graph.json","fetch_events":"https://pith.science/api/pith-number/DQHSPALDSVR5ARW7UOANOHT73P/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/DQHSPALDSVR5ARW7UOANOHT73P/action/timestamp_anchor","attest_storage":"https://pith.science/pith/DQHSPALDSVR5ARW7UOANOHT73P/action/storage_attestation","attest_author":"https://pith.science/pith/DQHSPALDSVR5ARW7UOANOHT73P/action/author_attestation","sign_citation":"https://pith.science/pith/DQHSPALDSVR5ARW7UOANOHT73P/action/citation_signature","submit_replication":"https://pith.science/pith/DQHSPALDSVR5ARW7UOANOHT73P/action/replication_record"}},"created_at":"2026-05-18T00:33:53.969063+00:00","updated_at":"2026-05-18T00:33:53.969063+00:00"}