{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2014:RTQYJMHSLP4YBH4V7G4ACZFSCQ","short_pith_number":"pith:RTQYJMHS","schema_version":"1.0","canonical_sha256":"8ce184b0f25bf9809f95f9b80164b214282aab00eb23ae7fe5bfac034ce850de","source":{"kind":"arxiv","id":"1408.5649","version":1},"attestation_state":"computed","paper":{"title":"Interpreting the extended emission around three nearby debris disc host stars","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.EP"],"primary_cat":"astro-ph.SR","authors_text":"B. Matthews, B. Montesinos, C. Eiroa, F. Kirchschlager, G.M. Kennedy, J.-C. Augereau, Jonathan P. Marshall, M. Booth, S. Ertel, S. Wolf","submitted_at":"2014-08-25T01:21:29Z","abstract_excerpt":"Cool debris discs are a relic of the planetesimal formation process around their host star, analogous to the solar system's Edgeworth-Kuiper belt. As such, they can be used as a proxy to probe the origin and formation of planetary systems like our own. The Herschel Open Time Key Programmes \"DUst around NEarby Stars\" (DUNES) and \"Disc Emission via a Bias-free Reconnaissance in the Infrared/Submillimetre\" (DEBRIS) observed many nearby, sun-like stars at far-infrared wavelengths seeking to detect and characterize the emission from their circumstellar dust. Excess emission attributable to the pres"},"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":"1408.5649","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2014-08-25T01:21:29Z","cross_cats_sorted":["astro-ph.EP"],"title_canon_sha256":"d551a615330ecd4955f5ab21da6581b27f8876dd5b020dc687f3754b6306f58c","abstract_canon_sha256":"cef999461b6cc48bbecb49d921f3158a75755253026b8f454a3aa3b54ea54862"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:42:13.454750Z","signature_b64":"40oMAsIwsU2KU3oiVGMBXlXwdha5VRawS7wUO+O+PvWgyp9+QE2ZFjXUT7umIFZnqgxJvPjpzExFcdI65Rz+DA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"8ce184b0f25bf9809f95f9b80164b214282aab00eb23ae7fe5bfac034ce850de","last_reissued_at":"2026-05-18T01:42:13.453925Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:42:13.453925Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Interpreting the extended emission around three nearby debris disc host stars","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.EP"],"primary_cat":"astro-ph.SR","authors_text":"B. Matthews, B. Montesinos, C. Eiroa, F. Kirchschlager, G.M. Kennedy, J.-C. Augereau, Jonathan P. Marshall, M. Booth, S. Ertel, S. Wolf","submitted_at":"2014-08-25T01:21:29Z","abstract_excerpt":"Cool debris discs are a relic of the planetesimal formation process around their host star, analogous to the solar system's Edgeworth-Kuiper belt. As such, they can be used as a proxy to probe the origin and formation of planetary systems like our own. The Herschel Open Time Key Programmes \"DUst around NEarby Stars\" (DUNES) and \"Disc Emission via a Bias-free Reconnaissance in the Infrared/Submillimetre\" (DEBRIS) observed many nearby, sun-like stars at far-infrared wavelengths seeking to detect and characterize the emission from their circumstellar dust. Excess emission attributable to the pres"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1408.5649","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":"1408.5649","created_at":"2026-05-18T01:42:13.454052+00:00"},{"alias_kind":"arxiv_version","alias_value":"1408.5649v1","created_at":"2026-05-18T01:42:13.454052+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1408.5649","created_at":"2026-05-18T01:42:13.454052+00:00"},{"alias_kind":"pith_short_12","alias_value":"RTQYJMHSLP4Y","created_at":"2026-05-18T12:28:46.137349+00:00"},{"alias_kind":"pith_short_16","alias_value":"RTQYJMHSLP4YBH4V","created_at":"2026-05-18T12:28:46.137349+00:00"},{"alias_kind":"pith_short_8","alias_value":"RTQYJMHS","created_at":"2026-05-18T12:28:46.137349+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/RTQYJMHSLP4YBH4V7G4ACZFSCQ","json":"https://pith.science/pith/RTQYJMHSLP4YBH4V7G4ACZFSCQ.json","graph_json":"https://pith.science/api/pith-number/RTQYJMHSLP4YBH4V7G4ACZFSCQ/graph.json","events_json":"https://pith.science/api/pith-number/RTQYJMHSLP4YBH4V7G4ACZFSCQ/events.json","paper":"https://pith.science/paper/RTQYJMHS"},"agent_actions":{"view_html":"https://pith.science/pith/RTQYJMHSLP4YBH4V7G4ACZFSCQ","download_json":"https://pith.science/pith/RTQYJMHSLP4YBH4V7G4ACZFSCQ.json","view_paper":"https://pith.science/paper/RTQYJMHS","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1408.5649&json=true","fetch_graph":"https://pith.science/api/pith-number/RTQYJMHSLP4YBH4V7G4ACZFSCQ/graph.json","fetch_events":"https://pith.science/api/pith-number/RTQYJMHSLP4YBH4V7G4ACZFSCQ/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/RTQYJMHSLP4YBH4V7G4ACZFSCQ/action/timestamp_anchor","attest_storage":"https://pith.science/pith/RTQYJMHSLP4YBH4V7G4ACZFSCQ/action/storage_attestation","attest_author":"https://pith.science/pith/RTQYJMHSLP4YBH4V7G4ACZFSCQ/action/author_attestation","sign_citation":"https://pith.science/pith/RTQYJMHSLP4YBH4V7G4ACZFSCQ/action/citation_signature","submit_replication":"https://pith.science/pith/RTQYJMHSLP4YBH4V7G4ACZFSCQ/action/replication_record"}},"created_at":"2026-05-18T01:42:13.454052+00:00","updated_at":"2026-05-18T01:42:13.454052+00:00"}