{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2023:BEBIKEMBQO5HSFQQTRW266AOJF","short_pith_number":"pith:BEBIKEMB","schema_version":"1.0","canonical_sha256":"090285118183ba7916109c6daf780e497dbcb0f63d48975e9e0dd1ca5412a188","source":{"kind":"arxiv","id":"2306.07328","version":2},"attestation_state":"computed","paper":{"title":"Dissecting a 30 kpc galactic outflow at $z \\sim$ 1.7","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Ahmed Shaban, C\\'edric Ledoux, Jane R. Rigby, John Chisholm, Keren Sharon, L. Felipe Barrientos, Matthew B. Bayliss, Michael G. Gladders, Michael K. Florian, Nicolas Tejos, Rongmon Bordoloi, Sebastian Lopez, Soniya Sharma","submitted_at":"2023-06-12T18:00:03Z","abstract_excerpt":"We present the spatially resolved measurements of a cool galactic outflow in the gravitationally lensed galaxy RCS0327 at $z \\approx 1.703$ using VLT/MUSE IFU observations. We probe the cool outflowing gas, traced by blueshifted Mg II and Fe II absorption lines, in 15 distinct regions of the same galaxy in its image-plane. Different physical regions, 5 to 7 kpc apart within the galaxy, drive the outflows at different velocities ($V_{out} \\sim $ $-161$ to $-240$ km s$^{-1}$), and mass outflow rates ($\\dot{M}_{out} \\sim$ 183 to 527 $M_{\\odot}\\ yr^{-1}$). The outflow velocities from different reg"},"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":"2306.07328","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2023-06-12T18:00:03Z","cross_cats_sorted":[],"title_canon_sha256":"aa0febe1f674b5fd1fcb4b6c4e35fc38848c73cd07abf1df22e73d7b9fe1ee09","abstract_canon_sha256":"3e404f623a5854ee22bbf6c086472da05e322bbf8a4e4ecb3795ff009e6df674"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T06:56:34.510867Z","signature_b64":"+yu9uxa0chWKKfQwfV20fp6gLMR9dBybHi6Zf7LuRU06u6UVc0rfAPlQ92ALVg6tVYdMmhFgv/9FkxJ9PEPEBQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"090285118183ba7916109c6daf780e497dbcb0f63d48975e9e0dd1ca5412a188","last_reissued_at":"2026-07-05T06:56:34.510375Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T06:56:34.510375Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Dissecting a 30 kpc galactic outflow at $z \\sim$ 1.7","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Ahmed Shaban, C\\'edric Ledoux, Jane R. Rigby, John Chisholm, Keren Sharon, L. Felipe Barrientos, Matthew B. Bayliss, Michael G. Gladders, Michael K. Florian, Nicolas Tejos, Rongmon Bordoloi, Sebastian Lopez, Soniya Sharma","submitted_at":"2023-06-12T18:00:03Z","abstract_excerpt":"We present the spatially resolved measurements of a cool galactic outflow in the gravitationally lensed galaxy RCS0327 at $z \\approx 1.703$ using VLT/MUSE IFU observations. We probe the cool outflowing gas, traced by blueshifted Mg II and Fe II absorption lines, in 15 distinct regions of the same galaxy in its image-plane. Different physical regions, 5 to 7 kpc apart within the galaxy, drive the outflows at different velocities ($V_{out} \\sim $ $-161$ to $-240$ km s$^{-1}$), and mass outflow rates ($\\dot{M}_{out} \\sim$ 183 to 527 $M_{\\odot}\\ yr^{-1}$). The outflow velocities from different reg"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2306.07328","kind":"arxiv","version":2},"verdict":{"id":null,"model_set":{},"created_at":null,"strongest_claim":"","one_line_summary":"","pipeline_version":null,"weakest_assumption":"","pith_extraction_headline":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2306.07328/integrity.json","findings":[],"available":true,"detectors_run":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938"},"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":"2306.07328","created_at":"2026-07-05T06:56:34.510436+00:00"},{"alias_kind":"arxiv_version","alias_value":"2306.07328v2","created_at":"2026-07-05T06:56:34.510436+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2306.07328","created_at":"2026-07-05T06:56:34.510436+00:00"},{"alias_kind":"pith_short_12","alias_value":"BEBIKEMBQO5H","created_at":"2026-07-05T06:56:34.510436+00:00"},{"alias_kind":"pith_short_16","alias_value":"BEBIKEMBQO5HSFQQ","created_at":"2026-07-05T06:56:34.510436+00:00"},{"alias_kind":"pith_short_8","alias_value":"BEBIKEMB","created_at":"2026-07-05T06:56:34.510436+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/BEBIKEMBQO5HSFQQTRW266AOJF","json":"https://pith.science/pith/BEBIKEMBQO5HSFQQTRW266AOJF.json","graph_json":"https://pith.science/api/pith-number/BEBIKEMBQO5HSFQQTRW266AOJF/graph.json","events_json":"https://pith.science/api/pith-number/BEBIKEMBQO5HSFQQTRW266AOJF/events.json","paper":"https://pith.science/paper/BEBIKEMB"},"agent_actions":{"view_html":"https://pith.science/pith/BEBIKEMBQO5HSFQQTRW266AOJF","download_json":"https://pith.science/pith/BEBIKEMBQO5HSFQQTRW266AOJF.json","view_paper":"https://pith.science/paper/BEBIKEMB","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2306.07328&json=true","fetch_graph":"https://pith.science/api/pith-number/BEBIKEMBQO5HSFQQTRW266AOJF/graph.json","fetch_events":"https://pith.science/api/pith-number/BEBIKEMBQO5HSFQQTRW266AOJF/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/BEBIKEMBQO5HSFQQTRW266AOJF/action/timestamp_anchor","attest_storage":"https://pith.science/pith/BEBIKEMBQO5HSFQQTRW266AOJF/action/storage_attestation","attest_author":"https://pith.science/pith/BEBIKEMBQO5HSFQQTRW266AOJF/action/author_attestation","sign_citation":"https://pith.science/pith/BEBIKEMBQO5HSFQQTRW266AOJF/action/citation_signature","submit_replication":"https://pith.science/pith/BEBIKEMBQO5HSFQQTRW266AOJF/action/replication_record"}},"created_at":"2026-07-05T06:56:34.510436+00:00","updated_at":"2026-07-05T06:56:34.510436+00:00"}