{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2017:OHAWVURSP3JHYEZ5SFWX2CHF6O","short_pith_number":"pith:OHAWVURS","schema_version":"1.0","canonical_sha256":"71c16ad2327ed27c133d916d7d08e5f3aab25732eacd825947865352f7afb3ec","source":{"kind":"arxiv","id":"1710.08686","version":1},"attestation_state":"computed","paper":{"title":"A 1.3 mm SMA Survey of 29 Variable Young Stellar Objects","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"\\'Agnes K\\'osp\\'al, Aina Palau, Carlo F. Manara, Carlos Carrasco-Gonz\\'alez, Carmen Ju\\'arez, Eduard I. Vorobyov, Hauyu Baobab Liu, Ilaria Pascucci, Jan Forbrich, Joel D. Green, Josep M. Girart, Leonardo Testi, Michael M. Dunham, Michihiro Takami, Naomi Hirano, Roberto Galv\\'an-Madrid, Sean Andrews, Steven Longmore, Tyler L. Bourke","submitted_at":"2017-10-24T10:08:48Z","abstract_excerpt":"Young stellar objects (YSOs) may undergo periods of active accretion (outbursts), during which the protostellar accretion rate is temporarily enhanced by a few orders of magnitude. Whether or not these accretion outburst YSOs possess similar dust/gas reservoirs to each other, and whether or not their dust/gas reservoirs are similar as quiescent YSOs, are issues not yet clarified. The aim of this work is to characterize the millimeter thermal dust emission properties of a statistically significant sample of long and short duration accretion outburst YSOs (i.e., FUors and EXors) and the spectros"},"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":"1710.08686","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2017-10-24T10:08:48Z","cross_cats_sorted":[],"title_canon_sha256":"4e7bcb80e66ac274d3ef6c7edb0a22d478563e52e1001f006b1301c740820e51","abstract_canon_sha256":"b4a598d32008eeea0891c62fc96a7076f97dd0b201cbf0e7520d45ccc3d70a18"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:17:42.604552Z","signature_b64":"CL6liL4sjPoGyVRfg4zfDI4p/y/nUBwz9F+4TNVSE/mDKmhA+CkP2LX0qSUb/dStPjEYS1H1NH45lQhxq0eTBw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"71c16ad2327ed27c133d916d7d08e5f3aab25732eacd825947865352f7afb3ec","last_reissued_at":"2026-05-18T00:17:42.603889Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:17:42.603889Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"A 1.3 mm SMA Survey of 29 Variable Young Stellar Objects","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"\\'Agnes K\\'osp\\'al, Aina Palau, Carlo F. Manara, Carlos Carrasco-Gonz\\'alez, Carmen Ju\\'arez, Eduard I. Vorobyov, Hauyu Baobab Liu, Ilaria Pascucci, Jan Forbrich, Joel D. Green, Josep M. Girart, Leonardo Testi, Michael M. Dunham, Michihiro Takami, Naomi Hirano, Roberto Galv\\'an-Madrid, Sean Andrews, Steven Longmore, Tyler L. Bourke","submitted_at":"2017-10-24T10:08:48Z","abstract_excerpt":"Young stellar objects (YSOs) may undergo periods of active accretion (outbursts), during which the protostellar accretion rate is temporarily enhanced by a few orders of magnitude. Whether or not these accretion outburst YSOs possess similar dust/gas reservoirs to each other, and whether or not their dust/gas reservoirs are similar as quiescent YSOs, are issues not yet clarified. The aim of this work is to characterize the millimeter thermal dust emission properties of a statistically significant sample of long and short duration accretion outburst YSOs (i.e., FUors and EXors) and the spectros"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1710.08686","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":"1710.08686","created_at":"2026-05-18T00:17:42.603994+00:00"},{"alias_kind":"arxiv_version","alias_value":"1710.08686v1","created_at":"2026-05-18T00:17:42.603994+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1710.08686","created_at":"2026-05-18T00:17:42.603994+00:00"},{"alias_kind":"pith_short_12","alias_value":"OHAWVURSP3JH","created_at":"2026-05-18T12:31:34.259226+00:00"},{"alias_kind":"pith_short_16","alias_value":"OHAWVURSP3JHYEZ5","created_at":"2026-05-18T12:31:34.259226+00:00"},{"alias_kind":"pith_short_8","alias_value":"OHAWVURS","created_at":"2026-05-18T12:31:34.259226+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/OHAWVURSP3JHYEZ5SFWX2CHF6O","json":"https://pith.science/pith/OHAWVURSP3JHYEZ5SFWX2CHF6O.json","graph_json":"https://pith.science/api/pith-number/OHAWVURSP3JHYEZ5SFWX2CHF6O/graph.json","events_json":"https://pith.science/api/pith-number/OHAWVURSP3JHYEZ5SFWX2CHF6O/events.json","paper":"https://pith.science/paper/OHAWVURS"},"agent_actions":{"view_html":"https://pith.science/pith/OHAWVURSP3JHYEZ5SFWX2CHF6O","download_json":"https://pith.science/pith/OHAWVURSP3JHYEZ5SFWX2CHF6O.json","view_paper":"https://pith.science/paper/OHAWVURS","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1710.08686&json=true","fetch_graph":"https://pith.science/api/pith-number/OHAWVURSP3JHYEZ5SFWX2CHF6O/graph.json","fetch_events":"https://pith.science/api/pith-number/OHAWVURSP3JHYEZ5SFWX2CHF6O/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/OHAWVURSP3JHYEZ5SFWX2CHF6O/action/timestamp_anchor","attest_storage":"https://pith.science/pith/OHAWVURSP3JHYEZ5SFWX2CHF6O/action/storage_attestation","attest_author":"https://pith.science/pith/OHAWVURSP3JHYEZ5SFWX2CHF6O/action/author_attestation","sign_citation":"https://pith.science/pith/OHAWVURSP3JHYEZ5SFWX2CHF6O/action/citation_signature","submit_replication":"https://pith.science/pith/OHAWVURSP3JHYEZ5SFWX2CHF6O/action/replication_record"}},"created_at":"2026-05-18T00:17:42.603994+00:00","updated_at":"2026-05-18T00:17:42.603994+00:00"}