{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2018:GJXS4V7BN5LHINGYPB3Q3W3UN5","short_pith_number":"pith:GJXS4V7B","schema_version":"1.0","canonical_sha256":"326f2e57e16f567434d878770ddb746f49f33b560f5165acf040fc8748279d34","source":{"kind":"arxiv","id":"1812.01149","version":1},"attestation_state":"computed","paper":{"title":"A Northern Ecliptic Survey for Solar System Science","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.IM"],"primary_cat":"astro-ph.EP","authors_text":"Colin Snodgrass, Darin Ragozzine, Henry H. Hsieh, Hsing Wen (Edward) Lin, Kathryn Volk, Marc W. Buie, Mario Juric, Megan E. Schwamb, Michael Mommert, Michael S. P. Kelley, Michele T. Bannister, R. Lynne Jones, Scott S. Sheppard, Steven R. Chesley","submitted_at":"2018-12-04T00:52:31Z","abstract_excerpt":"Making an inventory of the Solar System is one of the four fundamental science requirements for the Large Synoptic Survey Telescope (LSST). The current baseline footprint for LSST's main Wide-Fast-Deep (WFD) Survey observes the sky below 0$^\\circ$ declination, which includes only half of the ecliptic plane. Critically, key Solar System populations are asymmetrically distributed on the sky: they will be entirely missed, or only partially mapped, if only the WFD occurs. We propose a Northern Ecliptic Spur (NES) mini survey, observing the northern sky up to +10$^\\circ$ ecliptic latitude, to maxim"},"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":"1812.01149","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.EP","submitted_at":"2018-12-04T00:52:31Z","cross_cats_sorted":["astro-ph.IM"],"title_canon_sha256":"8adf4b7bf8c844907d0544de9ccad9f3cca534bd0e928ff33972224b5ae55a01","abstract_canon_sha256":"7d850b2d4193e896435b6bf23306cb0fc394cb83be123631feca6c3d10608ad1"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-17T23:59:13.220809Z","signature_b64":"r8iZCVBeUgR1DJOxhwLLoOMBF7ShYpwEQPZuHd9AN0EOXzXElrqjVCDafKzrBBd9lOCJ7FR3rODSGjGmn4nVDQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"326f2e57e16f567434d878770ddb746f49f33b560f5165acf040fc8748279d34","last_reissued_at":"2026-05-17T23:59:13.220247Z","signature_status":"signed_v1","first_computed_at":"2026-05-17T23:59:13.220247Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"A Northern Ecliptic Survey for Solar System Science","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.IM"],"primary_cat":"astro-ph.EP","authors_text":"Colin Snodgrass, Darin Ragozzine, Henry H. Hsieh, Hsing Wen (Edward) Lin, Kathryn Volk, Marc W. Buie, Mario Juric, Megan E. Schwamb, Michael Mommert, Michael S. P. Kelley, Michele T. Bannister, R. Lynne Jones, Scott S. Sheppard, Steven R. Chesley","submitted_at":"2018-12-04T00:52:31Z","abstract_excerpt":"Making an inventory of the Solar System is one of the four fundamental science requirements for the Large Synoptic Survey Telescope (LSST). The current baseline footprint for LSST's main Wide-Fast-Deep (WFD) Survey observes the sky below 0$^\\circ$ declination, which includes only half of the ecliptic plane. Critically, key Solar System populations are asymmetrically distributed on the sky: they will be entirely missed, or only partially mapped, if only the WFD occurs. We propose a Northern Ecliptic Spur (NES) mini survey, observing the northern sky up to +10$^\\circ$ ecliptic latitude, to maxim"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1812.01149","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":"1812.01149","created_at":"2026-05-17T23:59:13.220322+00:00"},{"alias_kind":"arxiv_version","alias_value":"1812.01149v1","created_at":"2026-05-17T23:59:13.220322+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1812.01149","created_at":"2026-05-17T23:59:13.220322+00:00"},{"alias_kind":"pith_short_12","alias_value":"GJXS4V7BN5LH","created_at":"2026-05-18T12:32:25.280505+00:00"},{"alias_kind":"pith_short_16","alias_value":"GJXS4V7BN5LHINGY","created_at":"2026-05-18T12:32:25.280505+00:00"},{"alias_kind":"pith_short_8","alias_value":"GJXS4V7B","created_at":"2026-05-18T12:32:25.280505+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2411.07970","citing_title":"MUltiplexed Survey Telescope (MUST) Science White Paper I: Overview of Large-Scale Structure Cosmology in the Era of Stage-V Spectroscopic Surveys","ref_index":218,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/GJXS4V7BN5LHINGYPB3Q3W3UN5","json":"https://pith.science/pith/GJXS4V7BN5LHINGYPB3Q3W3UN5.json","graph_json":"https://pith.science/api/pith-number/GJXS4V7BN5LHINGYPB3Q3W3UN5/graph.json","events_json":"https://pith.science/api/pith-number/GJXS4V7BN5LHINGYPB3Q3W3UN5/events.json","paper":"https://pith.science/paper/GJXS4V7B"},"agent_actions":{"view_html":"https://pith.science/pith/GJXS4V7BN5LHINGYPB3Q3W3UN5","download_json":"https://pith.science/pith/GJXS4V7BN5LHINGYPB3Q3W3UN5.json","view_paper":"https://pith.science/paper/GJXS4V7B","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1812.01149&json=true","fetch_graph":"https://pith.science/api/pith-number/GJXS4V7BN5LHINGYPB3Q3W3UN5/graph.json","fetch_events":"https://pith.science/api/pith-number/GJXS4V7BN5LHINGYPB3Q3W3UN5/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/GJXS4V7BN5LHINGYPB3Q3W3UN5/action/timestamp_anchor","attest_storage":"https://pith.science/pith/GJXS4V7BN5LHINGYPB3Q3W3UN5/action/storage_attestation","attest_author":"https://pith.science/pith/GJXS4V7BN5LHINGYPB3Q3W3UN5/action/author_attestation","sign_citation":"https://pith.science/pith/GJXS4V7BN5LHINGYPB3Q3W3UN5/action/citation_signature","submit_replication":"https://pith.science/pith/GJXS4V7BN5LHINGYPB3Q3W3UN5/action/replication_record"}},"created_at":"2026-05-17T23:59:13.220322+00:00","updated_at":"2026-05-17T23:59:13.220322+00:00"}