{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2018:UOLDVEIFUZBI2EDPIWCPCDEJKQ","short_pith_number":"pith:UOLDVEIF","schema_version":"1.0","canonical_sha256":"a3963a9105a6428d106f4584f10c895403a1d5236d413f115d09219a8248163e","source":{"kind":"arxiv","id":"1806.00311","version":1},"attestation_state":"computed","paper":{"title":"Herschel spectral-line mapping of the HH211 protostellar system","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.GA"],"primary_cat":"astro-ph.SR","authors_text":"1180, ((1) University of Vienna, (2) Astronomy & Astrophysics Section, Austria, Department of Astrophysics, Dublin Institute for Advanced Studies, Ireland), Manuel Guedel (1), Odysseas Dionatos (1), Tom Ray (2), Vienna","submitted_at":"2018-06-01T12:32:35Z","abstract_excerpt":"(Abridged) Mid- and far-infrared observations of the environment around embedded protostars reveal a plethora of high excitation molecular and atomic emission lines. In this work we present spectro-imaging observations of the HH211 system with Herschel/PACS that record emission from major molecular (CO, H2O and OH) and atomic coolants (e.g. [OI]). Molecular lines are mainly exited at the terminal bowshocks of the outflow and around the position of the protostar. All lines show maxima at the southeast bowshock with the exception of water emission that peaks around the central source. Excitation"},"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":"1806.00311","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2018-06-01T12:32:35Z","cross_cats_sorted":["astro-ph.GA"],"title_canon_sha256":"62d602dc8c4f1473ea92ce16af257f36f8e79b3e71c1f639fc81f6395ac4ec69","abstract_canon_sha256":"623d50df83194a87fba428e65949fad26704a0aad828c7bb46358ffb4fd022b4"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:07:34.141278Z","signature_b64":"9UhnaP24+rv4i+XUcC565AHOSTM1zo7cSC1ReG6hOg8AiylemVNYhOOAnQK+jQ+UmsiukfBpW83CoWRwh8xKDQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"a3963a9105a6428d106f4584f10c895403a1d5236d413f115d09219a8248163e","last_reissued_at":"2026-05-18T00:07:34.140371Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:07:34.140371Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Herschel spectral-line mapping of the HH211 protostellar system","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.GA"],"primary_cat":"astro-ph.SR","authors_text":"1180, ((1) University of Vienna, (2) Astronomy & Astrophysics Section, Austria, Department of Astrophysics, Dublin Institute for Advanced Studies, Ireland), Manuel Guedel (1), Odysseas Dionatos (1), Tom Ray (2), Vienna","submitted_at":"2018-06-01T12:32:35Z","abstract_excerpt":"(Abridged) Mid- and far-infrared observations of the environment around embedded protostars reveal a plethora of high excitation molecular and atomic emission lines. In this work we present spectro-imaging observations of the HH211 system with Herschel/PACS that record emission from major molecular (CO, H2O and OH) and atomic coolants (e.g. [OI]). Molecular lines are mainly exited at the terminal bowshocks of the outflow and around the position of the protostar. All lines show maxima at the southeast bowshock with the exception of water emission that peaks around the central source. Excitation"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1806.00311","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":"1806.00311","created_at":"2026-05-18T00:07:34.140533+00:00"},{"alias_kind":"arxiv_version","alias_value":"1806.00311v1","created_at":"2026-05-18T00:07:34.140533+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1806.00311","created_at":"2026-05-18T00:07:34.140533+00:00"},{"alias_kind":"pith_short_12","alias_value":"UOLDVEIFUZBI","created_at":"2026-05-18T12:32:56.356000+00:00"},{"alias_kind":"pith_short_16","alias_value":"UOLDVEIFUZBI2EDP","created_at":"2026-05-18T12:32:56.356000+00:00"},{"alias_kind":"pith_short_8","alias_value":"UOLDVEIF","created_at":"2026-05-18T12:32:56.356000+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/UOLDVEIFUZBI2EDPIWCPCDEJKQ","json":"https://pith.science/pith/UOLDVEIFUZBI2EDPIWCPCDEJKQ.json","graph_json":"https://pith.science/api/pith-number/UOLDVEIFUZBI2EDPIWCPCDEJKQ/graph.json","events_json":"https://pith.science/api/pith-number/UOLDVEIFUZBI2EDPIWCPCDEJKQ/events.json","paper":"https://pith.science/paper/UOLDVEIF"},"agent_actions":{"view_html":"https://pith.science/pith/UOLDVEIFUZBI2EDPIWCPCDEJKQ","download_json":"https://pith.science/pith/UOLDVEIFUZBI2EDPIWCPCDEJKQ.json","view_paper":"https://pith.science/paper/UOLDVEIF","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1806.00311&json=true","fetch_graph":"https://pith.science/api/pith-number/UOLDVEIFUZBI2EDPIWCPCDEJKQ/graph.json","fetch_events":"https://pith.science/api/pith-number/UOLDVEIFUZBI2EDPIWCPCDEJKQ/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/UOLDVEIFUZBI2EDPIWCPCDEJKQ/action/timestamp_anchor","attest_storage":"https://pith.science/pith/UOLDVEIFUZBI2EDPIWCPCDEJKQ/action/storage_attestation","attest_author":"https://pith.science/pith/UOLDVEIFUZBI2EDPIWCPCDEJKQ/action/author_attestation","sign_citation":"https://pith.science/pith/UOLDVEIFUZBI2EDPIWCPCDEJKQ/action/citation_signature","submit_replication":"https://pith.science/pith/UOLDVEIFUZBI2EDPIWCPCDEJKQ/action/replication_record"}},"created_at":"2026-05-18T00:07:34.140533+00:00","updated_at":"2026-05-18T00:07:34.140533+00:00"}