{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2024:GYVC5MGVD73UPHYB3CUQQVGMFD","short_pith_number":"pith:GYVC5MGV","schema_version":"1.0","canonical_sha256":"362a2eb0d51ff7479f01d8a90854cc28c1efd834d76dc778f1ef90fdbf3f4c9e","source":{"kind":"arxiv","id":"2401.04483","version":1},"attestation_state":"computed","paper":{"title":"The Lockman-SpReSO project. Galactic flows in a sample of far-infrared galaxies","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Ana Mar\\'ia P\\'erez Garc\\'ia, \\'Angel Bongiovanni, Bernab\\'e Cedr\\'es Jos\\'e A. de Diego, C. Alenka Negrete, Carmen P. Padilla-Torres, Erika Ben\\'itez, H\\'ector Hern\\'andez-Toledo, H\\'ector J. Ibarra-Medel, Irene Cruz-Gonz\\'alez, Jakub Nadolny, Jes\\'us Gallego, J. Ignacio Gonz\\'alez-Serrano, J. Jes\\'us Gonz\\'alez, Jordi Cepa, Maritza A. Lara-L\\'opez, Mart\\'in Herrera-Endoqui, Mauro Gonz\\'alez-Otero, Miguel Cervi\\~no, Miguel S\\'anchez-Portal, Mirjana Povic, Ricardo P\\'erez-Mart\\'inez, Roc\\'io Navarro Mart\\'inez, Yair Krongold","submitted_at":"2024-01-09T10:43:38Z","abstract_excerpt":"Methods. We performed measurements of the \\MgII, \\MgI, \\FeIIa, \\FeIIb, and \\FeIIc\\ spectral lines present in the spectra of the selected sample to determine the EW and velocity of the flows observed in the star-forming galaxies. Subsequently, we conducted $10^7$ bootstrap simulations using Spearman's rank correlation coefficient ($\\rho_s$) to explore correlations with galaxy properties. Furthermore, we calculated the covering factor, gas density, and optical depth for the measured \\ion{Fe}{II} doublets.\n  Results. Our analysis revealed strong correlations between the EW of \\ion{Mg}{II} lines a"},"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":"2401.04483","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.GA","submitted_at":"2024-01-09T10:43:38Z","cross_cats_sorted":[],"title_canon_sha256":"0153cdfd0ff7ee3aa1930e6e7980ed20f08c4417e12612bf4bcbfe8fe0fdcbfa","abstract_canon_sha256":"0577b05f883a3b9c9ee73abce54d569d34891b6a1d9565da72fb06ea7a5c0226"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T08:03:47.732450Z","signature_b64":"HPebFpRihVUd2tKbtd+B4Pr6o+I8ZTn34TV0bjIRYM2Xtae1CMenCq9ge9uTUXDpjcAPyuX8A8vOSoUJ3KgmCA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"362a2eb0d51ff7479f01d8a90854cc28c1efd834d76dc778f1ef90fdbf3f4c9e","last_reissued_at":"2026-07-05T08:03:47.731946Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T08:03:47.731946Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The Lockman-SpReSO project. Galactic flows in a sample of far-infrared galaxies","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Ana Mar\\'ia P\\'erez Garc\\'ia, \\'Angel Bongiovanni, Bernab\\'e Cedr\\'es Jos\\'e A. de Diego, C. Alenka Negrete, Carmen P. Padilla-Torres, Erika Ben\\'itez, H\\'ector Hern\\'andez-Toledo, H\\'ector J. Ibarra-Medel, Irene Cruz-Gonz\\'alez, Jakub Nadolny, Jes\\'us Gallego, J. Ignacio Gonz\\'alez-Serrano, J. Jes\\'us Gonz\\'alez, Jordi Cepa, Maritza A. Lara-L\\'opez, Mart\\'in Herrera-Endoqui, Mauro Gonz\\'alez-Otero, Miguel Cervi\\~no, Miguel S\\'anchez-Portal, Mirjana Povic, Ricardo P\\'erez-Mart\\'inez, Roc\\'io Navarro Mart\\'inez, Yair Krongold","submitted_at":"2024-01-09T10:43:38Z","abstract_excerpt":"Methods. We performed measurements of the \\MgII, \\MgI, \\FeIIa, \\FeIIb, and \\FeIIc\\ spectral lines present in the spectra of the selected sample to determine the EW and velocity of the flows observed in the star-forming galaxies. Subsequently, we conducted $10^7$ bootstrap simulations using Spearman's rank correlation coefficient ($\\rho_s$) to explore correlations with galaxy properties. Furthermore, we calculated the covering factor, gas density, and optical depth for the measured \\ion{Fe}{II} doublets.\n  Results. Our analysis revealed strong correlations between the EW of \\ion{Mg}{II} lines a"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2401.04483","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2401.04483/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":"2401.04483","created_at":"2026-07-05T08:03:47.732006+00:00"},{"alias_kind":"arxiv_version","alias_value":"2401.04483v1","created_at":"2026-07-05T08:03:47.732006+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2401.04483","created_at":"2026-07-05T08:03:47.732006+00:00"},{"alias_kind":"pith_short_12","alias_value":"GYVC5MGVD73U","created_at":"2026-07-05T08:03:47.732006+00:00"},{"alias_kind":"pith_short_16","alias_value":"GYVC5MGVD73UPHYB","created_at":"2026-07-05T08:03:47.732006+00:00"},{"alias_kind":"pith_short_8","alias_value":"GYVC5MGV","created_at":"2026-07-05T08:03:47.732006+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/GYVC5MGVD73UPHYB3CUQQVGMFD","json":"https://pith.science/pith/GYVC5MGVD73UPHYB3CUQQVGMFD.json","graph_json":"https://pith.science/api/pith-number/GYVC5MGVD73UPHYB3CUQQVGMFD/graph.json","events_json":"https://pith.science/api/pith-number/GYVC5MGVD73UPHYB3CUQQVGMFD/events.json","paper":"https://pith.science/paper/GYVC5MGV"},"agent_actions":{"view_html":"https://pith.science/pith/GYVC5MGVD73UPHYB3CUQQVGMFD","download_json":"https://pith.science/pith/GYVC5MGVD73UPHYB3CUQQVGMFD.json","view_paper":"https://pith.science/paper/GYVC5MGV","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2401.04483&json=true","fetch_graph":"https://pith.science/api/pith-number/GYVC5MGVD73UPHYB3CUQQVGMFD/graph.json","fetch_events":"https://pith.science/api/pith-number/GYVC5MGVD73UPHYB3CUQQVGMFD/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/GYVC5MGVD73UPHYB3CUQQVGMFD/action/timestamp_anchor","attest_storage":"https://pith.science/pith/GYVC5MGVD73UPHYB3CUQQVGMFD/action/storage_attestation","attest_author":"https://pith.science/pith/GYVC5MGVD73UPHYB3CUQQVGMFD/action/author_attestation","sign_citation":"https://pith.science/pith/GYVC5MGVD73UPHYB3CUQQVGMFD/action/citation_signature","submit_replication":"https://pith.science/pith/GYVC5MGVD73UPHYB3CUQQVGMFD/action/replication_record"}},"created_at":"2026-07-05T08:03:47.732006+00:00","updated_at":"2026-07-05T08:03:47.732006+00:00"}