{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2024:6MHH3GGITLG4LVC6AETOTDHZ73","short_pith_number":"pith:6MHH3GGI","schema_version":"1.0","canonical_sha256":"f30e7d98c89acdc5d45e0126e98cf9feff081bf7f721ef51233e9ff993a24d2d","source":{"kind":"arxiv","id":"2403.14313","version":1},"attestation_state":"computed","paper":{"title":"Gaia23ckh: Symbiotic outburst of the assumed Mira variable V390 Sco","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"Jan Skowron, Jaroslav Merc, Lionel Mulato, Olivier Garde, Pascal le D\\^u, Peter Velez, St\\'ephane Charbonnel, Thomas Petit","submitted_at":"2024-03-21T11:35:13Z","abstract_excerpt":"The poorly studied variable star V390 Sco, previously classified as a Mira pulsator, was detected in a brightening event by the ESA Gaia satellite in September 2023. This work presents an analysis of available archival multifrequency photometric data of this target, along with our spectroscopic observations. Our findings lead to the conclusion that V390 Sco is a new symbiotic star identified by Gaia, currently undergoing a classical symbiotic outburst. Additionally, we uncovered three prior outbursts of this system through archival photometry. The outbursts recur approximately every 2330 - 240"},"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":"2403.14313","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2024-03-21T11:35:13Z","cross_cats_sorted":[],"title_canon_sha256":"5fe1649fd2f19e8a3d40aa7db8bc443791e14c1fd21c3a32a80b2c93a35a6083","abstract_canon_sha256":"75d6394847ba8bd6eaec957c0c23d1e78c0d06b037d9a6e9fe5990c60220a9d9"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T07:59:06.960124Z","signature_b64":"EonTTUQ55iUWO5qI9t4ZKiJ7C9T8gEChOA8F9lDx4rThCZ0dULHwc8mxKLodTuffmXI4nzFNEBQlUeEabPuFDA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"f30e7d98c89acdc5d45e0126e98cf9feff081bf7f721ef51233e9ff993a24d2d","last_reissued_at":"2026-07-05T07:59:06.959778Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T07:59:06.959778Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Gaia23ckh: Symbiotic outburst of the assumed Mira variable V390 Sco","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"Jan Skowron, Jaroslav Merc, Lionel Mulato, Olivier Garde, Pascal le D\\^u, Peter Velez, St\\'ephane Charbonnel, Thomas Petit","submitted_at":"2024-03-21T11:35:13Z","abstract_excerpt":"The poorly studied variable star V390 Sco, previously classified as a Mira pulsator, was detected in a brightening event by the ESA Gaia satellite in September 2023. This work presents an analysis of available archival multifrequency photometric data of this target, along with our spectroscopic observations. Our findings lead to the conclusion that V390 Sco is a new symbiotic star identified by Gaia, currently undergoing a classical symbiotic outburst. Additionally, we uncovered three prior outbursts of this system through archival photometry. The outbursts recur approximately every 2330 - 240"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2403.14313","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2403.14313/integrity.json","findings":[],"available":true,"detectors_run":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938"},"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":"2403.14313","created_at":"2026-07-05T07:59:06.959836+00:00"},{"alias_kind":"arxiv_version","alias_value":"2403.14313v1","created_at":"2026-07-05T07:59:06.959836+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2403.14313","created_at":"2026-07-05T07:59:06.959836+00:00"},{"alias_kind":"pith_short_12","alias_value":"6MHH3GGITLG4","created_at":"2026-07-05T07:59:06.959836+00:00"},{"alias_kind":"pith_short_16","alias_value":"6MHH3GGITLG4LVC6","created_at":"2026-07-05T07:59:06.959836+00:00"},{"alias_kind":"pith_short_8","alias_value":"6MHH3GGI","created_at":"2026-07-05T07:59:06.959836+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/6MHH3GGITLG4LVC6AETOTDHZ73","json":"https://pith.science/pith/6MHH3GGITLG4LVC6AETOTDHZ73.json","graph_json":"https://pith.science/api/pith-number/6MHH3GGITLG4LVC6AETOTDHZ73/graph.json","events_json":"https://pith.science/api/pith-number/6MHH3GGITLG4LVC6AETOTDHZ73/events.json","paper":"https://pith.science/paper/6MHH3GGI"},"agent_actions":{"view_html":"https://pith.science/pith/6MHH3GGITLG4LVC6AETOTDHZ73","download_json":"https://pith.science/pith/6MHH3GGITLG4LVC6AETOTDHZ73.json","view_paper":"https://pith.science/paper/6MHH3GGI","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2403.14313&json=true","fetch_graph":"https://pith.science/api/pith-number/6MHH3GGITLG4LVC6AETOTDHZ73/graph.json","fetch_events":"https://pith.science/api/pith-number/6MHH3GGITLG4LVC6AETOTDHZ73/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/6MHH3GGITLG4LVC6AETOTDHZ73/action/timestamp_anchor","attest_storage":"https://pith.science/pith/6MHH3GGITLG4LVC6AETOTDHZ73/action/storage_attestation","attest_author":"https://pith.science/pith/6MHH3GGITLG4LVC6AETOTDHZ73/action/author_attestation","sign_citation":"https://pith.science/pith/6MHH3GGITLG4LVC6AETOTDHZ73/action/citation_signature","submit_replication":"https://pith.science/pith/6MHH3GGITLG4LVC6AETOTDHZ73/action/replication_record"}},"created_at":"2026-07-05T07:59:06.959836+00:00","updated_at":"2026-07-05T07:59:06.959836+00:00"}