{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2014:L6DWQEANLXEQCKBE45DHA7A7U2","short_pith_number":"pith:L6DWQEAN","schema_version":"1.0","canonical_sha256":"5f8768100d5dc9012824e746707c1fa69124da84d0e01107ff0a9e68ac5b5702","source":{"kind":"arxiv","id":"1402.1184","version":1},"attestation_state":"computed","paper":{"title":"Spatially resolved imaging of the two-component eta Crv debris disk with Herschel","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"B. Matthews, B. Sibthorpe, C. Lisse, C. Pinte, D. Wilner, G. Duchene, G. Kennedy, J. Greaves, J. Horner, J. Wisniewski, M. Booth, M. Clampin, M. Wyatt, P. Arriaga, P. Kalas, W. Holland","submitted_at":"2014-02-05T21:17:44Z","abstract_excerpt":"We present far-infrared and sub-millimeter images of the eta Crv debris disk system obtained with Herschel and SCUBA-2, as well as Hubble Space Telescope visible and near-infrared coronagraphic images. In the 70 micron Herschel image, we clearly separate the thermal emission from the warm and cold belts in the system, find no evidence for a putative dust population located between them, and precisely determine the geometry of the outer belt. We also find marginal evidence for azimuthal asymmetries and a global offset of the outer debris ring relative to the central star. Finally, we place stri"},"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":"1402.1184","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2014-02-05T21:17:44Z","cross_cats_sorted":[],"title_canon_sha256":"787560043e4090ca008bb4f825c7ef2416f0ddb8e0fa28f5e2a36c92ffb2765a","abstract_canon_sha256":"d549b8104b799f71c2a213f6fb4efda9ef992559b630ed7f809474c8e397b466"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:39:16.541856Z","signature_b64":"PchnF9MGXJLBVN1/vv8Lc0v4dCwzVwWcU8J0HIrlI5WRQJboqJipa2WtNPFHuG7jg9zrHIN5daIV6mQIoNqyBQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"5f8768100d5dc9012824e746707c1fa69124da84d0e01107ff0a9e68ac5b5702","last_reissued_at":"2026-05-18T02:39:16.541337Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:39:16.541337Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Spatially resolved imaging of the two-component eta Crv debris disk with Herschel","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"B. Matthews, B. Sibthorpe, C. Lisse, C. Pinte, D. Wilner, G. Duchene, G. Kennedy, J. Greaves, J. Horner, J. Wisniewski, M. Booth, M. Clampin, M. Wyatt, P. Arriaga, P. Kalas, W. Holland","submitted_at":"2014-02-05T21:17:44Z","abstract_excerpt":"We present far-infrared and sub-millimeter images of the eta Crv debris disk system obtained with Herschel and SCUBA-2, as well as Hubble Space Telescope visible and near-infrared coronagraphic images. In the 70 micron Herschel image, we clearly separate the thermal emission from the warm and cold belts in the system, find no evidence for a putative dust population located between them, and precisely determine the geometry of the outer belt. We also find marginal evidence for azimuthal asymmetries and a global offset of the outer debris ring relative to the central star. Finally, we place stri"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1402.1184","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":"1402.1184","created_at":"2026-05-18T02:39:16.541399+00:00"},{"alias_kind":"arxiv_version","alias_value":"1402.1184v1","created_at":"2026-05-18T02:39:16.541399+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1402.1184","created_at":"2026-05-18T02:39:16.541399+00:00"},{"alias_kind":"pith_short_12","alias_value":"L6DWQEANLXEQ","created_at":"2026-05-18T12:28:35.611951+00:00"},{"alias_kind":"pith_short_16","alias_value":"L6DWQEANLXEQCKBE","created_at":"2026-05-18T12:28:35.611951+00:00"},{"alias_kind":"pith_short_8","alias_value":"L6DWQEAN","created_at":"2026-05-18T12:28:35.611951+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/L6DWQEANLXEQCKBE45DHA7A7U2","json":"https://pith.science/pith/L6DWQEANLXEQCKBE45DHA7A7U2.json","graph_json":"https://pith.science/api/pith-number/L6DWQEANLXEQCKBE45DHA7A7U2/graph.json","events_json":"https://pith.science/api/pith-number/L6DWQEANLXEQCKBE45DHA7A7U2/events.json","paper":"https://pith.science/paper/L6DWQEAN"},"agent_actions":{"view_html":"https://pith.science/pith/L6DWQEANLXEQCKBE45DHA7A7U2","download_json":"https://pith.science/pith/L6DWQEANLXEQCKBE45DHA7A7U2.json","view_paper":"https://pith.science/paper/L6DWQEAN","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1402.1184&json=true","fetch_graph":"https://pith.science/api/pith-number/L6DWQEANLXEQCKBE45DHA7A7U2/graph.json","fetch_events":"https://pith.science/api/pith-number/L6DWQEANLXEQCKBE45DHA7A7U2/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/L6DWQEANLXEQCKBE45DHA7A7U2/action/timestamp_anchor","attest_storage":"https://pith.science/pith/L6DWQEANLXEQCKBE45DHA7A7U2/action/storage_attestation","attest_author":"https://pith.science/pith/L6DWQEANLXEQCKBE45DHA7A7U2/action/author_attestation","sign_citation":"https://pith.science/pith/L6DWQEANLXEQCKBE45DHA7A7U2/action/citation_signature","submit_replication":"https://pith.science/pith/L6DWQEANLXEQCKBE45DHA7A7U2/action/replication_record"}},"created_at":"2026-05-18T02:39:16.541399+00:00","updated_at":"2026-05-18T02:39:16.541399+00:00"}