{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2018:ZYN3A66SRPHKQ2ZN3MVDVS2TSN","short_pith_number":"pith:ZYN3A66S","schema_version":"1.0","canonical_sha256":"ce1bb07bd28bcea86b2ddb2a3acb539360f739967dead8fbb2632b859d8d7a9d","source":{"kind":"arxiv","id":"1812.07094","version":1},"attestation_state":"computed","paper":{"title":"Water and OH Emission from the inner disk of a Herbig Ae/Be star","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.GA"],"primary_cat":"astro-ph.SR","authors_text":"Joan R. Najita, John S. Carr, M\\'at\\'e \\'Ad\\'amkovics, Sean D. Brittain, Steven C. Adams","submitted_at":"2018-12-17T23:20:20Z","abstract_excerpt":"We report the detection of hot H$_{2}$O and OH emission from the Herbig Ae/Be star HD$~101412$ using the Cryogenic Infrared Echelle Spectrograph on the $\\textit{Very Large Telescope}$. Previous studies of Herbig Ae/Be stars have shown the presence of OH around some of these sources, but H$_{2}$O has proven more elusive. While marginal water emission has been reported in the mid-infrared, and a few Herbig Ae/Be stars show water emission in the far-infrared, water emission near 2.9 $\\mu$m has not been previously detected. We apply slab models to the ro-vibrational OH, H$_{2}$O, and CO spectra of"},"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":"1812.07094","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2018-12-17T23:20:20Z","cross_cats_sorted":["astro-ph.GA"],"title_canon_sha256":"591010d286b923cc8a4a1d73bdce2d567a916ec2cb7b2e6790a7ccc202496327","abstract_canon_sha256":"f24f0703e240924c5951eb6ac9cb588d2601a53b8dd729a0e9590448f32dbb74"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-17T23:52:58.452096Z","signature_b64":"tpLujPaNoBsH9/4Kn2+6+eEDsVKt/hk8GQ1+m4D4ASEJKtvIf0g1lJEFazf34XWYG0UdWg8S4fmMnjY73n2fDA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"ce1bb07bd28bcea86b2ddb2a3acb539360f739967dead8fbb2632b859d8d7a9d","last_reissued_at":"2026-05-17T23:52:58.451655Z","signature_status":"signed_v1","first_computed_at":"2026-05-17T23:52:58.451655Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Water and OH Emission from the inner disk of a Herbig Ae/Be star","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.GA"],"primary_cat":"astro-ph.SR","authors_text":"Joan R. Najita, John S. Carr, M\\'at\\'e \\'Ad\\'amkovics, Sean D. Brittain, Steven C. Adams","submitted_at":"2018-12-17T23:20:20Z","abstract_excerpt":"We report the detection of hot H$_{2}$O and OH emission from the Herbig Ae/Be star HD$~101412$ using the Cryogenic Infrared Echelle Spectrograph on the $\\textit{Very Large Telescope}$. Previous studies of Herbig Ae/Be stars have shown the presence of OH around some of these sources, but H$_{2}$O has proven more elusive. While marginal water emission has been reported in the mid-infrared, and a few Herbig Ae/Be stars show water emission in the far-infrared, water emission near 2.9 $\\mu$m has not been previously detected. We apply slab models to the ro-vibrational OH, H$_{2}$O, and CO spectra of"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1812.07094","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":"1812.07094","created_at":"2026-05-17T23:52:58.451717+00:00"},{"alias_kind":"arxiv_version","alias_value":"1812.07094v1","created_at":"2026-05-17T23:52:58.451717+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1812.07094","created_at":"2026-05-17T23:52:58.451717+00:00"},{"alias_kind":"pith_short_12","alias_value":"ZYN3A66SRPHK","created_at":"2026-05-18T12:33:07.085635+00:00"},{"alias_kind":"pith_short_16","alias_value":"ZYN3A66SRPHKQ2ZN","created_at":"2026-05-18T12:33:07.085635+00:00"},{"alias_kind":"pith_short_8","alias_value":"ZYN3A66S","created_at":"2026-05-18T12:33:07.085635+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/ZYN3A66SRPHKQ2ZN3MVDVS2TSN","json":"https://pith.science/pith/ZYN3A66SRPHKQ2ZN3MVDVS2TSN.json","graph_json":"https://pith.science/api/pith-number/ZYN3A66SRPHKQ2ZN3MVDVS2TSN/graph.json","events_json":"https://pith.science/api/pith-number/ZYN3A66SRPHKQ2ZN3MVDVS2TSN/events.json","paper":"https://pith.science/paper/ZYN3A66S"},"agent_actions":{"view_html":"https://pith.science/pith/ZYN3A66SRPHKQ2ZN3MVDVS2TSN","download_json":"https://pith.science/pith/ZYN3A66SRPHKQ2ZN3MVDVS2TSN.json","view_paper":"https://pith.science/paper/ZYN3A66S","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1812.07094&json=true","fetch_graph":"https://pith.science/api/pith-number/ZYN3A66SRPHKQ2ZN3MVDVS2TSN/graph.json","fetch_events":"https://pith.science/api/pith-number/ZYN3A66SRPHKQ2ZN3MVDVS2TSN/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/ZYN3A66SRPHKQ2ZN3MVDVS2TSN/action/timestamp_anchor","attest_storage":"https://pith.science/pith/ZYN3A66SRPHKQ2ZN3MVDVS2TSN/action/storage_attestation","attest_author":"https://pith.science/pith/ZYN3A66SRPHKQ2ZN3MVDVS2TSN/action/author_attestation","sign_citation":"https://pith.science/pith/ZYN3A66SRPHKQ2ZN3MVDVS2TSN/action/citation_signature","submit_replication":"https://pith.science/pith/ZYN3A66SRPHKQ2ZN3MVDVS2TSN/action/replication_record"}},"created_at":"2026-05-17T23:52:58.451717+00:00","updated_at":"2026-05-17T23:52:58.451717+00:00"}