{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2013:NDMYULUOXMTGEDJRKYBFWMOXHS","short_pith_number":"pith:NDMYULUO","schema_version":"1.0","canonical_sha256":"68d98a2e8ebb26620d3156025b31d73c9e8c02d82533036c85b30c90bbce1f2b","source":{"kind":"arxiv","id":"1301.1331","version":1},"attestation_state":"computed","paper":{"title":"Asteroid Belts in Debris Disk Twins: VEGA and FOMALHAUT","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.EP","authors_text":"A. Bonsor, A. M. Hughes, D. J. Wilner, D. M. Watson, G. H. Rieke, K. A. Misselt, Kate Y. L. Su, K. R. Stapelfeldt, M. W. Werner, R. Malhotra, Z. Balog","submitted_at":"2013-01-07T20:49:54Z","abstract_excerpt":"Vega and Fomalhaut, are similar in terms of mass, ages, and global debris disk properties; therefore, they are often referred as \"debris disk twins\". We present Spitzer 10-35 um spectroscopic data centered at both stars, and identify warm, unresolved excess emission in the close vicinity of Vega for the first time. The properties of the warm excess in Vega are further characterized with ancillary photometry in the mid infrared and resolved images in the far-infrared and submillimeter wavelengths. The Vega warm excess shares many similar properties with the one found around Fomalhaut. The emiss"},"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":"1301.1331","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.EP","submitted_at":"2013-01-07T20:49:54Z","cross_cats_sorted":[],"title_canon_sha256":"dc859a4c163892539733d314d360d194b014031d932f180fcc086e47aaf7a6c4","abstract_canon_sha256":"2a3eeb59d3a4408a794b3f584eb9300932f1d672338a64f4908603bbf9ebae5d"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:52:20.898869Z","signature_b64":"AAedWsvxnUlIOiclc5A0kZX4jQW9N6hTe7wYbPoY/6eHbWS3Infa+y/EOTnjbYry8+X3baWvQLOmm9Kn/SNUBg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"68d98a2e8ebb26620d3156025b31d73c9e8c02d82533036c85b30c90bbce1f2b","last_reissued_at":"2026-05-18T01:52:20.898479Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:52:20.898479Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Asteroid Belts in Debris Disk Twins: VEGA and FOMALHAUT","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.EP","authors_text":"A. Bonsor, A. M. Hughes, D. J. Wilner, D. M. Watson, G. H. Rieke, K. A. Misselt, Kate Y. L. Su, K. R. Stapelfeldt, M. W. Werner, R. Malhotra, Z. Balog","submitted_at":"2013-01-07T20:49:54Z","abstract_excerpt":"Vega and Fomalhaut, are similar in terms of mass, ages, and global debris disk properties; therefore, they are often referred as \"debris disk twins\". We present Spitzer 10-35 um spectroscopic data centered at both stars, and identify warm, unresolved excess emission in the close vicinity of Vega for the first time. The properties of the warm excess in Vega are further characterized with ancillary photometry in the mid infrared and resolved images in the far-infrared and submillimeter wavelengths. The Vega warm excess shares many similar properties with the one found around Fomalhaut. The emiss"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1301.1331","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":"1301.1331","created_at":"2026-05-18T01:52:20.898544+00:00"},{"alias_kind":"arxiv_version","alias_value":"1301.1331v1","created_at":"2026-05-18T01:52:20.898544+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1301.1331","created_at":"2026-05-18T01:52:20.898544+00:00"},{"alias_kind":"pith_short_12","alias_value":"NDMYULUOXMTG","created_at":"2026-05-18T12:27:52.871228+00:00"},{"alias_kind":"pith_short_16","alias_value":"NDMYULUOXMTGEDJR","created_at":"2026-05-18T12:27:52.871228+00:00"},{"alias_kind":"pith_short_8","alias_value":"NDMYULUO","created_at":"2026-05-18T12:27:52.871228+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/NDMYULUOXMTGEDJRKYBFWMOXHS","json":"https://pith.science/pith/NDMYULUOXMTGEDJRKYBFWMOXHS.json","graph_json":"https://pith.science/api/pith-number/NDMYULUOXMTGEDJRKYBFWMOXHS/graph.json","events_json":"https://pith.science/api/pith-number/NDMYULUOXMTGEDJRKYBFWMOXHS/events.json","paper":"https://pith.science/paper/NDMYULUO"},"agent_actions":{"view_html":"https://pith.science/pith/NDMYULUOXMTGEDJRKYBFWMOXHS","download_json":"https://pith.science/pith/NDMYULUOXMTGEDJRKYBFWMOXHS.json","view_paper":"https://pith.science/paper/NDMYULUO","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1301.1331&json=true","fetch_graph":"https://pith.science/api/pith-number/NDMYULUOXMTGEDJRKYBFWMOXHS/graph.json","fetch_events":"https://pith.science/api/pith-number/NDMYULUOXMTGEDJRKYBFWMOXHS/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/NDMYULUOXMTGEDJRKYBFWMOXHS/action/timestamp_anchor","attest_storage":"https://pith.science/pith/NDMYULUOXMTGEDJRKYBFWMOXHS/action/storage_attestation","attest_author":"https://pith.science/pith/NDMYULUOXMTGEDJRKYBFWMOXHS/action/author_attestation","sign_citation":"https://pith.science/pith/NDMYULUOXMTGEDJRKYBFWMOXHS/action/citation_signature","submit_replication":"https://pith.science/pith/NDMYULUOXMTGEDJRKYBFWMOXHS/action/replication_record"}},"created_at":"2026-05-18T01:52:20.898544+00:00","updated_at":"2026-05-18T01:52:20.898544+00:00"}