{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2016:MPQJ6NIR63LBCR2A4YQY7E24SN","short_pith_number":"pith:MPQJ6NIR","schema_version":"1.0","canonical_sha256":"63e09f3511f6d6114740e6218f935c935ef03ced03e86511bcae49d11ae0b9c2","source":{"kind":"arxiv","id":"1606.01761","version":1},"attestation_state":"computed","paper":{"title":"A multi-resolution, multi-epoch low radio frequency survey of the Kepler K2 mission Campaign 1 field","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.IM"],"primary_cat":"astro-ph.GA","authors_text":"H. Intema, K. Mooley, P. Jagannathan, P.J. Hancock, R.B. Wayth, S.J. Tingay","submitted_at":"2016-06-06T14:30:06Z","abstract_excerpt":"We present the first dedicated radio continuum survey of a Kepler K2 mission field, Field 1 covering the North Galactic Cap. The survey is wide field, contemporaneous, multi-epoch, and multi-resolution in nature and was conducted at low radio frequencies between 140 and 200 MHz. The multi-epoch and ultra wide field (but relatively low resolution) part of the survey was provided by 15 nights of observation with the Murchison Widefield Array (MWA) over a period of approximately a month, contemporaneous with K2 observations of the field. The multi-resolution aspect of the survey was provided by t"},"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":"1606.01761","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2016-06-06T14:30:06Z","cross_cats_sorted":["astro-ph.IM"],"title_canon_sha256":"33372ced60c652073e5c0837c699f2fe344758d3c0c4576fe1ab561812337ea7","abstract_canon_sha256":"ff0679d1722733f6ac9178f44fe1cb2e1cbec879b2c3e18ccf136393b1fe123a"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:04:20.057527Z","signature_b64":"TJE2QNoN1wDOc5ivwFAKSQEFVcShbYBTDsL3bmbzDsjuiFmRb+g2xmtFaBR37rtYoOKoHiPDitKvR4yS9mJXCg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"63e09f3511f6d6114740e6218f935c935ef03ced03e86511bcae49d11ae0b9c2","last_reissued_at":"2026-05-18T01:04:20.056915Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:04:20.056915Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"A multi-resolution, multi-epoch low radio frequency survey of the Kepler K2 mission Campaign 1 field","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.IM"],"primary_cat":"astro-ph.GA","authors_text":"H. Intema, K. Mooley, P. Jagannathan, P.J. Hancock, R.B. Wayth, S.J. Tingay","submitted_at":"2016-06-06T14:30:06Z","abstract_excerpt":"We present the first dedicated radio continuum survey of a Kepler K2 mission field, Field 1 covering the North Galactic Cap. The survey is wide field, contemporaneous, multi-epoch, and multi-resolution in nature and was conducted at low radio frequencies between 140 and 200 MHz. The multi-epoch and ultra wide field (but relatively low resolution) part of the survey was provided by 15 nights of observation with the Murchison Widefield Array (MWA) over a period of approximately a month, contemporaneous with K2 observations of the field. The multi-resolution aspect of the survey was provided by t"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1606.01761","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":"1606.01761","created_at":"2026-05-18T01:04:20.057002+00:00"},{"alias_kind":"arxiv_version","alias_value":"1606.01761v1","created_at":"2026-05-18T01:04:20.057002+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1606.01761","created_at":"2026-05-18T01:04:20.057002+00:00"},{"alias_kind":"pith_short_12","alias_value":"MPQJ6NIR63LB","created_at":"2026-05-18T12:30:32.724797+00:00"},{"alias_kind":"pith_short_16","alias_value":"MPQJ6NIR63LBCR2A","created_at":"2026-05-18T12:30:32.724797+00:00"},{"alias_kind":"pith_short_8","alias_value":"MPQJ6NIR","created_at":"2026-05-18T12:30:32.724797+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/MPQJ6NIR63LBCR2A4YQY7E24SN","json":"https://pith.science/pith/MPQJ6NIR63LBCR2A4YQY7E24SN.json","graph_json":"https://pith.science/api/pith-number/MPQJ6NIR63LBCR2A4YQY7E24SN/graph.json","events_json":"https://pith.science/api/pith-number/MPQJ6NIR63LBCR2A4YQY7E24SN/events.json","paper":"https://pith.science/paper/MPQJ6NIR"},"agent_actions":{"view_html":"https://pith.science/pith/MPQJ6NIR63LBCR2A4YQY7E24SN","download_json":"https://pith.science/pith/MPQJ6NIR63LBCR2A4YQY7E24SN.json","view_paper":"https://pith.science/paper/MPQJ6NIR","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1606.01761&json=true","fetch_graph":"https://pith.science/api/pith-number/MPQJ6NIR63LBCR2A4YQY7E24SN/graph.json","fetch_events":"https://pith.science/api/pith-number/MPQJ6NIR63LBCR2A4YQY7E24SN/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/MPQJ6NIR63LBCR2A4YQY7E24SN/action/timestamp_anchor","attest_storage":"https://pith.science/pith/MPQJ6NIR63LBCR2A4YQY7E24SN/action/storage_attestation","attest_author":"https://pith.science/pith/MPQJ6NIR63LBCR2A4YQY7E24SN/action/author_attestation","sign_citation":"https://pith.science/pith/MPQJ6NIR63LBCR2A4YQY7E24SN/action/citation_signature","submit_replication":"https://pith.science/pith/MPQJ6NIR63LBCR2A4YQY7E24SN/action/replication_record"}},"created_at":"2026-05-18T01:04:20.057002+00:00","updated_at":"2026-05-18T01:04:20.057002+00:00"}