{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2014:FG4J3EVV6M622Y6HQDGJDPG6BZ","short_pith_number":"pith:FG4J3EVV","schema_version":"1.0","canonical_sha256":"29b89d92b5f33dad63c780cc91bcde0e5bb669e4e0018f7192e18d4cb8b6ec23","source":{"kind":"arxiv","id":"1401.3335","version":3},"attestation_state":"computed","paper":{"title":"Discovery and Observations of ASASSN-13db, an EX Lupi-Type Accretion Event on a Low-Mass T Tauri Star","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"A. Sicilia-Aguilar, B. J. Shappee, C. E. Woodward, Christopher S. Kochanek, D. Bersier, D. Grupe, D. M. Szczygie{\\l}, G. Pojmanski, J. Brimacombe, J. D. Simon, J. F.Beacom, J. J. Adams, J. Jencson, Jose L. Prieto, K. Croxall, Krzysztof Z. Stanek, N. Morell S. M. McGraw, R. M. Wagner, S. G. Starrfield, Thomas W.-S. Holoien, U. Basu, Z. Zhu","submitted_at":"2014-01-14T21:00:06Z","abstract_excerpt":"We discuss ASASSN-13db, an EX Lupi-type (\"EXor\") accretion event on the young stellar object (YSO) SDSS J051011.01$-$032826.2 (hereafter SDSSJ0510) discovered by the All-Sky Automated Survey for SuperNovae (ASAS-SN). Using archival photometric data of SDSSJ0510 we construct a pre-outburst spectral energy distribution (SED) and find that it is consistent with a low-mass class II YSO near the Orion star forming region ($d \\sim 420$ pc). We present follow-up photometric and spectroscopic observations of the source after the $\\Delta V \\sim-$5.4 magnitude outburst that began in September 2013 and e"},"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":"1401.3335","kind":"arxiv","version":3},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2014-01-14T21:00:06Z","cross_cats_sorted":[],"title_canon_sha256":"19fbf256101435808a8841038608a7f08adf5ed5cb71e8f7975fafbce3987238","abstract_canon_sha256":"8000bbe7133b9b08b620760f4213b39a607f3a33d597b2b4b74ba628344c756d"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:45:25.564418Z","signature_b64":"baO/bUeX66BpXzY3zYtwQS6DxK2yY2u8p74+86uGDV8jL3j7bsfN2U+4EW4AvB7MmlDaTGFcVi09ePuofeqFAA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"29b89d92b5f33dad63c780cc91bcde0e5bb669e4e0018f7192e18d4cb8b6ec23","last_reissued_at":"2026-05-18T01:45:25.563893Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:45:25.563893Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Discovery and Observations of ASASSN-13db, an EX Lupi-Type Accretion Event on a Low-Mass T Tauri Star","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"A. Sicilia-Aguilar, B. J. Shappee, C. E. Woodward, Christopher S. Kochanek, D. Bersier, D. Grupe, D. M. Szczygie{\\l}, G. Pojmanski, J. Brimacombe, J. D. Simon, J. F.Beacom, J. J. Adams, J. Jencson, Jose L. Prieto, K. Croxall, Krzysztof Z. Stanek, N. Morell S. M. McGraw, R. M. Wagner, S. G. Starrfield, Thomas W.-S. Holoien, U. Basu, Z. Zhu","submitted_at":"2014-01-14T21:00:06Z","abstract_excerpt":"We discuss ASASSN-13db, an EX Lupi-type (\"EXor\") accretion event on the young stellar object (YSO) SDSS J051011.01$-$032826.2 (hereafter SDSSJ0510) discovered by the All-Sky Automated Survey for SuperNovae (ASAS-SN). Using archival photometric data of SDSSJ0510 we construct a pre-outburst spectral energy distribution (SED) and find that it is consistent with a low-mass class II YSO near the Orion star forming region ($d \\sim 420$ pc). We present follow-up photometric and spectroscopic observations of the source after the $\\Delta V \\sim-$5.4 magnitude outburst that began in September 2013 and e"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1401.3335","kind":"arxiv","version":3},"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":"1401.3335","created_at":"2026-05-18T01:45:25.563979+00:00"},{"alias_kind":"arxiv_version","alias_value":"1401.3335v3","created_at":"2026-05-18T01:45:25.563979+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1401.3335","created_at":"2026-05-18T01:45:25.563979+00:00"},{"alias_kind":"pith_short_12","alias_value":"FG4J3EVV6M62","created_at":"2026-05-18T12:28:28.263976+00:00"},{"alias_kind":"pith_short_16","alias_value":"FG4J3EVV6M622Y6H","created_at":"2026-05-18T12:28:28.263976+00:00"},{"alias_kind":"pith_short_8","alias_value":"FG4J3EVV","created_at":"2026-05-18T12:28:28.263976+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/FG4J3EVV6M622Y6HQDGJDPG6BZ","json":"https://pith.science/pith/FG4J3EVV6M622Y6HQDGJDPG6BZ.json","graph_json":"https://pith.science/api/pith-number/FG4J3EVV6M622Y6HQDGJDPG6BZ/graph.json","events_json":"https://pith.science/api/pith-number/FG4J3EVV6M622Y6HQDGJDPG6BZ/events.json","paper":"https://pith.science/paper/FG4J3EVV"},"agent_actions":{"view_html":"https://pith.science/pith/FG4J3EVV6M622Y6HQDGJDPG6BZ","download_json":"https://pith.science/pith/FG4J3EVV6M622Y6HQDGJDPG6BZ.json","view_paper":"https://pith.science/paper/FG4J3EVV","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1401.3335&json=true","fetch_graph":"https://pith.science/api/pith-number/FG4J3EVV6M622Y6HQDGJDPG6BZ/graph.json","fetch_events":"https://pith.science/api/pith-number/FG4J3EVV6M622Y6HQDGJDPG6BZ/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/FG4J3EVV6M622Y6HQDGJDPG6BZ/action/timestamp_anchor","attest_storage":"https://pith.science/pith/FG4J3EVV6M622Y6HQDGJDPG6BZ/action/storage_attestation","attest_author":"https://pith.science/pith/FG4J3EVV6M622Y6HQDGJDPG6BZ/action/author_attestation","sign_citation":"https://pith.science/pith/FG4J3EVV6M622Y6HQDGJDPG6BZ/action/citation_signature","submit_replication":"https://pith.science/pith/FG4J3EVV6M622Y6HQDGJDPG6BZ/action/replication_record"}},"created_at":"2026-05-18T01:45:25.563979+00:00","updated_at":"2026-05-18T01:45:25.563979+00:00"}