{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:1999:UG7SS7LAWYS4UBYCGVZN5RFAN4","short_pith_number":"pith:UG7SS7LA","schema_version":"1.0","canonical_sha256":"a1bf297d60b625ca07023572dec4a06f275436bd39db46ac2f320398e23328b0","source":{"kind":"arxiv","id":"astro-ph/9912090","version":1},"attestation_state":"computed","paper":{"title":"New infrared object in the field of the SMC cluster NGC 330","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"A. Kucinskas, M. Sauvage, T. Tanab\\'e, V. Vansevicius","submitted_at":"1999-12-06T14:03:12Z","abstract_excerpt":"We report ISO (Infrared Space Observatory) observations of a new infrared source discovered in the vicinity of the young populous cluster NGC 330 in the Small Magellanic Cloud. The object was observed with ISOCAM at 4.5, 6.75 and 11.5 $\\mu$m and shows a prominent mid-infrared excess, indicating the presence of a dust shell. The available observations of the optical counterpart together with the mid-infrared ISOCAM data suggest that this object is most likely a post-AGB star, or a Be supergiant. Cluster membership and candidate evolutionary scenarios are discussed briefly."},"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":"astro-ph/9912090","kind":"arxiv","version":1},"metadata":{"license":"","primary_cat":"astro-ph","submitted_at":"1999-12-06T14:03:12Z","cross_cats_sorted":[],"title_canon_sha256":"827494afa8e3b07e9a9adbe6f1cbcfca360072f7c9118dccd0cdc87816b213aa","abstract_canon_sha256":"f01ce76fabe1c99e30ffddf8aa76dfca7f2c505fc3cba1ba0a86e50067b6c889"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:09:21.317944Z","signature_b64":"vuXlkmNr7SnyNr5ngOx0VaH37gnmNxy4rflHjmGBVviY620vqLBKra+qQNX3wOEQnAzEo+oVv2AbAOqD4nzjCw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"a1bf297d60b625ca07023572dec4a06f275436bd39db46ac2f320398e23328b0","last_reissued_at":"2026-05-18T01:09:21.317420Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:09:21.317420Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"New infrared object in the field of the SMC cluster NGC 330","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"A. Kucinskas, M. Sauvage, T. Tanab\\'e, V. Vansevicius","submitted_at":"1999-12-06T14:03:12Z","abstract_excerpt":"We report ISO (Infrared Space Observatory) observations of a new infrared source discovered in the vicinity of the young populous cluster NGC 330 in the Small Magellanic Cloud. The object was observed with ISOCAM at 4.5, 6.75 and 11.5 $\\mu$m and shows a prominent mid-infrared excess, indicating the presence of a dust shell. The available observations of the optical counterpart together with the mid-infrared ISOCAM data suggest that this object is most likely a post-AGB star, or a Be supergiant. Cluster membership and candidate evolutionary scenarios are discussed briefly."},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"astro-ph/9912090","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":"astro-ph/9912090","created_at":"2026-05-18T01:09:21.317519+00:00"},{"alias_kind":"arxiv_version","alias_value":"astro-ph/9912090v1","created_at":"2026-05-18T01:09:21.317519+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.astro-ph/9912090","created_at":"2026-05-18T01:09:21.317519+00:00"},{"alias_kind":"pith_short_12","alias_value":"UG7SS7LAWYS4","created_at":"2026-05-18T12:25:49.631198+00:00"},{"alias_kind":"pith_short_16","alias_value":"UG7SS7LAWYS4UBYC","created_at":"2026-05-18T12:25:49.631198+00:00"},{"alias_kind":"pith_short_8","alias_value":"UG7SS7LA","created_at":"2026-05-18T12:25:49.631198+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/UG7SS7LAWYS4UBYCGVZN5RFAN4","json":"https://pith.science/pith/UG7SS7LAWYS4UBYCGVZN5RFAN4.json","graph_json":"https://pith.science/api/pith-number/UG7SS7LAWYS4UBYCGVZN5RFAN4/graph.json","events_json":"https://pith.science/api/pith-number/UG7SS7LAWYS4UBYCGVZN5RFAN4/events.json","paper":"https://pith.science/paper/UG7SS7LA"},"agent_actions":{"view_html":"https://pith.science/pith/UG7SS7LAWYS4UBYCGVZN5RFAN4","download_json":"https://pith.science/pith/UG7SS7LAWYS4UBYCGVZN5RFAN4.json","view_paper":"https://pith.science/paper/UG7SS7LA","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=astro-ph/9912090&json=true","fetch_graph":"https://pith.science/api/pith-number/UG7SS7LAWYS4UBYCGVZN5RFAN4/graph.json","fetch_events":"https://pith.science/api/pith-number/UG7SS7LAWYS4UBYCGVZN5RFAN4/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/UG7SS7LAWYS4UBYCGVZN5RFAN4/action/timestamp_anchor","attest_storage":"https://pith.science/pith/UG7SS7LAWYS4UBYCGVZN5RFAN4/action/storage_attestation","attest_author":"https://pith.science/pith/UG7SS7LAWYS4UBYCGVZN5RFAN4/action/author_attestation","sign_citation":"https://pith.science/pith/UG7SS7LAWYS4UBYCGVZN5RFAN4/action/citation_signature","submit_replication":"https://pith.science/pith/UG7SS7LAWYS4UBYCGVZN5RFAN4/action/replication_record"}},"created_at":"2026-05-18T01:09:21.317519+00:00","updated_at":"2026-05-18T01:09:21.317519+00:00"}