{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2019:7INWYI34KWGW2TJ7EL6QHTVPFE","short_pith_number":"pith:7INWYI34","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"},"canonical_sha256":"fa1b6c237c558d6d4d3f22fd03ceaf291b454a4d53fd36e72e4f8a71cd07115f","source":{"kind":"arxiv","id":"1905.11413","version":1},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1905.11413","created_at":"2026-05-17T23:43:49Z"},{"alias_kind":"arxiv_version","alias_value":"1905.11413v1","created_at":"2026-05-17T23:43:49Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1905.11413","created_at":"2026-05-17T23:43:49Z"},{"alias_kind":"pith_short_12","alias_value":"7INWYI34KWGW","created_at":"2026-05-18T12:33:12Z"},{"alias_kind":"pith_short_16","alias_value":"7INWYI34KWGW2TJ7","created_at":"2026-05-18T12:33:12Z"},{"alias_kind":"pith_short_8","alias_value":"7INWYI34","created_at":"2026-05-18T12:33:12Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2019:7INWYI34KWGW2TJ7EL6QHTVPFE","target":"record","payload":{"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"},"canonical_sha256":"fa1b6c237c558d6d4d3f22fd03ceaf291b454a4d53fd36e72e4f8a71cd07115f","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"},"source_kind":"arxiv","source_id":"1905.11413","source_version":1,"attestation_state":"computed"},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-05-17T23:43:49Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"DEDq0IPTQTg1k1KhG3XhBzNvT6KklaM9cKWdaWcF6qpxbY7MVyO4L5UsUKU8u2nQaaQZ7AWCDQrTbaK3r7OaBQ==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-19T11:58:30.947617Z"},"content_sha256":"ba9b5ffd89a88847715966f1d249028b84dc3058c4b3353354862661f59282cc","schema_version":"1.0","event_id":"sha256:ba9b5ffd89a88847715966f1d249028b84dc3058c4b3353354862661f59282cc"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2019:7INWYI34KWGW2TJ7EL6QHTVPFE","target":"graph","payload":{"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"},"verdict_id":null},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-05-17T23:43:49Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"DTExhsP0u+K0QEAU1yqgqmBOKud3wdpOC4WK147MsfF8Mzn3koE99mC5OiLMDoqmCgwupCNiK+gGpuQhtP1NCQ==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-19T11:58:30.948270Z"},"content_sha256":"fcaf417714abb53fb613b0c119f869bdfee29df918ce0d653ac6d2b3b789c028","schema_version":"1.0","event_id":"sha256:fcaf417714abb53fb613b0c119f869bdfee29df918ce0d653ac6d2b3b789c028"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/7INWYI34KWGW2TJ7EL6QHTVPFE/bundle.json","state_url":"https://pith.science/pith/7INWYI34KWGW2TJ7EL6QHTVPFE/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/7INWYI34KWGW2TJ7EL6QHTVPFE/bundle.json","status":"primary"}],"public_keys":[{"key_id":"pith-v1-2026-05","algorithm":"ed25519","format":"raw","public_key_b64":"stVStoiQhXFxp4s2pdzPNoqVNBMojDU/fJ2db5S3CbM=","public_key_hex":"b2d552b68890857171a78b36a5dccf368a953413288c353f7c9d9d6f94b709b3","fingerprint_sha256_b32_first128bits":"RVFV5Z2OI2J3ZUO7ERDEBCYNKS","fingerprint_sha256_hex":"8d4b5ee74e4693bcd1df2446408b0d54","rotates_at":null,"url":"https://pith.science/pith-signing-key.json","notes":"Pith uses this Ed25519 key to sign canonical record SHA-256 digests. Verify with: ed25519_verify(public_key, message=canonical_sha256_bytes, signature=base64decode(signature_b64))."}],"merge_version":"pith-open-graph-merge-v1","built_at":"2026-05-19T11:58:30Z","links":{"resolver":"https://pith.science/pith/7INWYI34KWGW2TJ7EL6QHTVPFE","bundle":"https://pith.science/pith/7INWYI34KWGW2TJ7EL6QHTVPFE/bundle.json","state":"https://pith.science/pith/7INWYI34KWGW2TJ7EL6QHTVPFE/state.json","well_known_bundle":"https://pith.science/.well-known/pith/7INWYI34KWGW2TJ7EL6QHTVPFE/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2019:7INWYI34KWGW2TJ7EL6QHTVPFE","merge_version":"pith-open-graph-merge-v1","event_count":2,"valid_event_count":2,"invalid_event_count":0,"equivocation_count":0,"current":{"canonical_record":{"metadata":{"abstract_canon_sha256":"9560228a781fc4229b22d613850682628d7491fac716ddb46a1208d49a889811","cross_cats_sorted":["astro-ph.CO"],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2019-05-27T18:00:03Z","title_canon_sha256":"810689f44f15fabbb8f7730cca8a4e93ac7129ab59f78a5e52e13827b3e378ea"},"schema_version":"1.0","source":{"id":"1905.11413","kind":"arxiv","version":1}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1905.11413","created_at":"2026-05-17T23:43:49Z"},{"alias_kind":"arxiv_version","alias_value":"1905.11413v1","created_at":"2026-05-17T23:43:49Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1905.11413","created_at":"2026-05-17T23:43:49Z"},{"alias_kind":"pith_short_12","alias_value":"7INWYI34KWGW","created_at":"2026-05-18T12:33:12Z"},{"alias_kind":"pith_short_16","alias_value":"7INWYI34KWGW2TJ7","created_at":"2026-05-18T12:33:12Z"},{"alias_kind":"pith_short_8","alias_value":"7INWYI34","created_at":"2026-05-18T12:33:12Z"}],"graph_snapshots":[{"event_id":"sha256:fcaf417714abb53fb613b0c119f869bdfee29df918ce0d653ac6d2b3b789c028","target":"graph","created_at":"2026-05-17T23:43:49Z","signer":{"key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signer_id":"pith.science","signer_type":"pith_registry"},"payload":{"graph_snapshot":{"author_claims":{"count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","strong_count":0},"builder_version":"pith-number-builder-2026-05-17-v1","claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"paper":{"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","authors_text":"A. Ferrara, A. Pallottini, A. Zanella, C. Behrens, L. Vallini, M. Kohandel, S. Carniani, S. Gallerani","cross_cats":["astro-ph.CO"],"headline":"","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2019-05-27T18:00:03Z","title":"Kinematics of $z\\geq 6$ galaxies from [CII] line emission"},"references":{"count":0,"internal_anchors":0,"resolved_work":0,"sample":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1905.11413","kind":"arxiv","version":1},"verdict":{"created_at":null,"id":null,"model_set":{},"one_line_summary":"","pipeline_version":null,"pith_extraction_headline":"","strongest_claim":"","weakest_assumption":""}},"verdict_id":null}}],"author_attestations":[],"timestamp_anchors":[],"storage_attestations":[],"citation_signatures":[],"replication_records":[],"corrections":[],"mirror_hints":[],"record_created":{"event_id":"sha256:ba9b5ffd89a88847715966f1d249028b84dc3058c4b3353354862661f59282cc","target":"record","created_at":"2026-05-17T23:43:49Z","signer":{"key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signer_id":"pith.science","signer_type":"pith_registry"},"payload":{"attestation_state":"computed","canonical_record":{"metadata":{"abstract_canon_sha256":"9560228a781fc4229b22d613850682628d7491fac716ddb46a1208d49a889811","cross_cats_sorted":["astro-ph.CO"],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2019-05-27T18:00:03Z","title_canon_sha256":"810689f44f15fabbb8f7730cca8a4e93ac7129ab59f78a5e52e13827b3e378ea"},"schema_version":"1.0","source":{"id":"1905.11413","kind":"arxiv","version":1}},"canonical_sha256":"fa1b6c237c558d6d4d3f22fd03ceaf291b454a4d53fd36e72e4f8a71cd07115f","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"fa1b6c237c558d6d4d3f22fd03ceaf291b454a4d53fd36e72e4f8a71cd07115f","first_computed_at":"2026-05-17T23:43:49.230158Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-05-17T23:43:49.230158Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"gTqDKBX1w6nFPt1BXoH/n3IiCQQPyHTEXQ7DHA8+bH6lSSIIGDLuiaWhgGmMdzLa1dVdHsiA+arA5Q8WN8NgCQ==","signature_status":"signed_v1","signed_at":"2026-05-17T23:43:49.230983Z","signed_message":"canonical_sha256_bytes"},"source_id":"1905.11413","source_kind":"arxiv","source_version":1}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:ba9b5ffd89a88847715966f1d249028b84dc3058c4b3353354862661f59282cc","sha256:fcaf417714abb53fb613b0c119f869bdfee29df918ce0d653ac6d2b3b789c028"],"state_sha256":"71b0da48a7d44596231e6f3586900d3c7a7fe983e4c9432f3e7cc1781da042fd"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"BnifdDoKOI9MESTkpWcQk1p5MSC4LzK9DfZ5idUf8KQtNcbJte2ueBjMCldmakwjxIKFXoz/7h+A8PFJ8OeRBQ==","signed_message":"bundle_sha256_bytes","signed_at":"2026-05-19T11:58:30.950800Z","bundle_sha256":"a436f92b4f86d5debee08d80c93c45708ba949bc01c0604b5442179aa403dcef"}}