{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2019:7INWYI34KWGW2TJ7EL6QHTVPFE","short_pith_number":"pith:7INWYI34","schema_version":"1.0","canonical_sha256":"fa1b6c237c558d6d4d3f22fd03ceaf291b454a4d53fd36e72e4f8a71cd07115f","source":{"kind":"arxiv","id":"1905.11413","version":1},"attestation_state":"computed","paper":{"title":"Kinematics of $z\\geq 6$ galaxies from [CII] line emission","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"astro-ph.GA","authors_text":"A. Ferrara, A. Pallottini, A. Zanella, C. Behrens, L. Vallini, M. Kohandel, S. Carniani, S. Gallerani","submitted_at":"2019-05-27T18:00:03Z","abstract_excerpt":"We study the kinematical properties of galaxies in the Epoch of Reionization via the [CII] 158$\\mu$m line emission. The line profile provides information on the kinematics as well as structural properties such as the presence of a disk and satellites. To understand how these properties are encoded in the line profile, first we develop analytical models from which we identify disk inclination and gas turbulent motions as the key parameters affecting the line profile. To gain further insights, we use \"Althaea\", a highly-resolved ($30\\, \\rm pc$) simulated prototypical Lyman Break Galaxy, in the r"},"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":"1905.11413","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2019-05-27T18:00:03Z","cross_cats_sorted":["astro-ph.CO"],"title_canon_sha256":"810689f44f15fabbb8f7730cca8a4e93ac7129ab59f78a5e52e13827b3e378ea","abstract_canon_sha256":"9560228a781fc4229b22d613850682628d7491fac716ddb46a1208d49a889811"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-17T23:43:49.230983Z","signature_b64":"gTqDKBX1w6nFPt1BXoH/n3IiCQQPyHTEXQ7DHA8+bH6lSSIIGDLuiaWhgGmMdzLa1dVdHsiA+arA5Q8WN8NgCQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"fa1b6c237c558d6d4d3f22fd03ceaf291b454a4d53fd36e72e4f8a71cd07115f","last_reissued_at":"2026-05-17T23:43:49.230158Z","signature_status":"signed_v1","first_computed_at":"2026-05-17T23:43:49.230158Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Kinematics of $z\\geq 6$ galaxies from [CII] line emission","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"astro-ph.GA","authors_text":"A. Ferrara, A. Pallottini, A. Zanella, C. Behrens, L. Vallini, M. Kohandel, S. Carniani, S. Gallerani","submitted_at":"2019-05-27T18:00:03Z","abstract_excerpt":"We study the kinematical properties of galaxies in the Epoch of Reionization via the [CII] 158$\\mu$m line emission. The line profile provides information on the kinematics as well as structural properties such as the presence of a disk and satellites. To understand how these properties are encoded in the line profile, first we develop analytical models from which we identify disk inclination and gas turbulent motions as the key parameters affecting the line profile. To gain further insights, we use \"Althaea\", a highly-resolved ($30\\, \\rm pc$) simulated prototypical Lyman Break Galaxy, in the r"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1905.11413","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":"1905.11413","created_at":"2026-05-17T23:43:49.230293+00:00"},{"alias_kind":"arxiv_version","alias_value":"1905.11413v1","created_at":"2026-05-17T23:43:49.230293+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1905.11413","created_at":"2026-05-17T23:43:49.230293+00:00"},{"alias_kind":"pith_short_12","alias_value":"7INWYI34KWGW","created_at":"2026-05-18T12:33:12.712433+00:00"},{"alias_kind":"pith_short_16","alias_value":"7INWYI34KWGW2TJ7","created_at":"2026-05-18T12:33:12.712433+00:00"},{"alias_kind":"pith_short_8","alias_value":"7INWYI34","created_at":"2026-05-18T12:33:12.712433+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/7INWYI34KWGW2TJ7EL6QHTVPFE","json":"https://pith.science/pith/7INWYI34KWGW2TJ7EL6QHTVPFE.json","graph_json":"https://pith.science/api/pith-number/7INWYI34KWGW2TJ7EL6QHTVPFE/graph.json","events_json":"https://pith.science/api/pith-number/7INWYI34KWGW2TJ7EL6QHTVPFE/events.json","paper":"https://pith.science/paper/7INWYI34"},"agent_actions":{"view_html":"https://pith.science/pith/7INWYI34KWGW2TJ7EL6QHTVPFE","download_json":"https://pith.science/pith/7INWYI34KWGW2TJ7EL6QHTVPFE.json","view_paper":"https://pith.science/paper/7INWYI34","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1905.11413&json=true","fetch_graph":"https://pith.science/api/pith-number/7INWYI34KWGW2TJ7EL6QHTVPFE/graph.json","fetch_events":"https://pith.science/api/pith-number/7INWYI34KWGW2TJ7EL6QHTVPFE/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/7INWYI34KWGW2TJ7EL6QHTVPFE/action/timestamp_anchor","attest_storage":"https://pith.science/pith/7INWYI34KWGW2TJ7EL6QHTVPFE/action/storage_attestation","attest_author":"https://pith.science/pith/7INWYI34KWGW2TJ7EL6QHTVPFE/action/author_attestation","sign_citation":"https://pith.science/pith/7INWYI34KWGW2TJ7EL6QHTVPFE/action/citation_signature","submit_replication":"https://pith.science/pith/7INWYI34KWGW2TJ7EL6QHTVPFE/action/replication_record"}},"created_at":"2026-05-17T23:43:49.230293+00:00","updated_at":"2026-05-17T23:43:49.230293+00:00"}