{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2011:2Z3TDZSHWQQBQMK3CGG54J3DII","short_pith_number":"pith:2Z3TDZSH","schema_version":"1.0","canonical_sha256":"d67731e647b42018315b118dde27634233a2e4b7e89f0e159c26b479c57467df","source":{"kind":"arxiv","id":"1103.5919","version":1},"attestation_state":"computed","paper":{"title":"The precession of the HH 111 flow in the infrared","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"(2) ICN UNAM, (3) Universitat Heidelberg, (4) JPL, A. C. Raga (2), A. Noriega-Crespo (1), Caltech, Caltech), K. R. Stapelfeldt (4), S. J. Carey (1) ((1) SSC, V. Lora (3)","submitted_at":"2011-03-30T13:17:54Z","abstract_excerpt":"We present Spitzer IRAC images of the HH 111 outflow, that show a wealth of condensations/knots in both jet and counterjet. Studying the positional distribution of these knots, we find very suggestive evidence of a mirror symmetric pattern in the jet/counterjet flow. We model this pattern as the result of an orbital motion of the jet source around a binary companion. From a fit of an analytic, ballistic model to the observed path of the HH 111 system, we find that the motion in a binary with two approx. 1 Msolar stars (one of them being the HH 111 source), in a circular orbit with a separation"},"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":"1103.5919","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2011-03-30T13:17:54Z","cross_cats_sorted":[],"title_canon_sha256":"6d84d6c43f83282e63ac6a10ba0ee6b0da228ccc6ebd5b130511f8abbc57f53e","abstract_canon_sha256":"c6c07f2490ff809dd8d3aac280588b00785262481d3e340272904dd092b747a4"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:02:42.791751Z","signature_b64":"f9nVamVsKEcTI8rMQFucqBlK0cGjRo91uzKF+xWkJZ/sMqH9GJpiSGdGqFIZKE07FR+ticzKILc+Napbp8vqBw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"d67731e647b42018315b118dde27634233a2e4b7e89f0e159c26b479c57467df","last_reissued_at":"2026-05-18T02:02:42.790980Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:02:42.790980Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The precession of the HH 111 flow in the infrared","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"(2) ICN UNAM, (3) Universitat Heidelberg, (4) JPL, A. C. Raga (2), A. Noriega-Crespo (1), Caltech, Caltech), K. R. Stapelfeldt (4), S. J. Carey (1) ((1) SSC, V. Lora (3)","submitted_at":"2011-03-30T13:17:54Z","abstract_excerpt":"We present Spitzer IRAC images of the HH 111 outflow, that show a wealth of condensations/knots in both jet and counterjet. Studying the positional distribution of these knots, we find very suggestive evidence of a mirror symmetric pattern in the jet/counterjet flow. We model this pattern as the result of an orbital motion of the jet source around a binary companion. From a fit of an analytic, ballistic model to the observed path of the HH 111 system, we find that the motion in a binary with two approx. 1 Msolar stars (one of them being the HH 111 source), in a circular orbit with a separation"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1103.5919","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":"1103.5919","created_at":"2026-05-18T02:02:42.791096+00:00"},{"alias_kind":"arxiv_version","alias_value":"1103.5919v1","created_at":"2026-05-18T02:02:42.791096+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1103.5919","created_at":"2026-05-18T02:02:42.791096+00:00"},{"alias_kind":"pith_short_12","alias_value":"2Z3TDZSHWQQB","created_at":"2026-05-18T12:26:18.847500+00:00"},{"alias_kind":"pith_short_16","alias_value":"2Z3TDZSHWQQBQMK3","created_at":"2026-05-18T12:26:18.847500+00:00"},{"alias_kind":"pith_short_8","alias_value":"2Z3TDZSH","created_at":"2026-05-18T12:26:18.847500+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/2Z3TDZSHWQQBQMK3CGG54J3DII","json":"https://pith.science/pith/2Z3TDZSHWQQBQMK3CGG54J3DII.json","graph_json":"https://pith.science/api/pith-number/2Z3TDZSHWQQBQMK3CGG54J3DII/graph.json","events_json":"https://pith.science/api/pith-number/2Z3TDZSHWQQBQMK3CGG54J3DII/events.json","paper":"https://pith.science/paper/2Z3TDZSH"},"agent_actions":{"view_html":"https://pith.science/pith/2Z3TDZSHWQQBQMK3CGG54J3DII","download_json":"https://pith.science/pith/2Z3TDZSHWQQBQMK3CGG54J3DII.json","view_paper":"https://pith.science/paper/2Z3TDZSH","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1103.5919&json=true","fetch_graph":"https://pith.science/api/pith-number/2Z3TDZSHWQQBQMK3CGG54J3DII/graph.json","fetch_events":"https://pith.science/api/pith-number/2Z3TDZSHWQQBQMK3CGG54J3DII/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/2Z3TDZSHWQQBQMK3CGG54J3DII/action/timestamp_anchor","attest_storage":"https://pith.science/pith/2Z3TDZSHWQQBQMK3CGG54J3DII/action/storage_attestation","attest_author":"https://pith.science/pith/2Z3TDZSHWQQBQMK3CGG54J3DII/action/author_attestation","sign_citation":"https://pith.science/pith/2Z3TDZSHWQQBQMK3CGG54J3DII/action/citation_signature","submit_replication":"https://pith.science/pith/2Z3TDZSHWQQBQMK3CGG54J3DII/action/replication_record"}},"created_at":"2026-05-18T02:02:42.791096+00:00","updated_at":"2026-05-18T02:02:42.791096+00:00"}