{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2014:EAKRTAKGDFSQPEXINI55236IUG","short_pith_number":"pith:EAKRTAKG","schema_version":"1.0","canonical_sha256":"201519814619650792e86a3bdd6fc8a1a78abc3a291719ea782baafb1ddff1b3","source":{"kind":"arxiv","id":"1406.3356","version":1},"attestation_state":"computed","paper":{"title":"On the lack of correlation between Mg II 2796, 2803 Angstrom and Lyman alpha emission in lensed star-forming galaxies","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"E. Wuyts, H. Dahle, J. R. Rigby, K. Sharon, M. B. Bayliss, M. D. Gladders","submitted_at":"2014-06-12T20:00:23Z","abstract_excerpt":"We examine the Mg II 2796, 2803 Angstrom, Lyman alpha, and nebular line emission in five bright star-forming galaxies at 1.66<z<1.91 that have been gravitationally lensed by foreground galaxy clusters. All five galaxies show prominent Mg II emission and absorption in a P Cygni profile. We find no correlation between the equivalent widths of Mg II and Lyman alpha emission. The Mg II emission has a broader range of velocities than do the nebular emission line profiles; the Mg II emission is redshifted with respect to systemic by 100 to 200 km/s. When present, Lyman alpha is even more redshifted."},"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":"1406.3356","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2014-06-12T20:00:23Z","cross_cats_sorted":[],"title_canon_sha256":"4ba08ab1f0eaafcf12e642451a8e05acf041f14fdd7acb4fad339c05eff3a561","abstract_canon_sha256":"a61f33a7b3cb15a03175e20acdbae914dea5866131d93b2482cb7e24bf857be1"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:42:57.876769Z","signature_b64":"aFuQnTaJyYtqLdCOuHU99kgRgUx3ti11ttp49+YNABG5KnUUQQY4lA9Qf8azNJsfQTle85ACgzvhDmMDEGw6DQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"201519814619650792e86a3bdd6fc8a1a78abc3a291719ea782baafb1ddff1b3","last_reissued_at":"2026-05-18T01:42:57.876019Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:42:57.876019Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"On the lack of correlation between Mg II 2796, 2803 Angstrom and Lyman alpha emission in lensed star-forming galaxies","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"E. Wuyts, H. Dahle, J. R. Rigby, K. Sharon, M. B. Bayliss, M. D. Gladders","submitted_at":"2014-06-12T20:00:23Z","abstract_excerpt":"We examine the Mg II 2796, 2803 Angstrom, Lyman alpha, and nebular line emission in five bright star-forming galaxies at 1.66<z<1.91 that have been gravitationally lensed by foreground galaxy clusters. All five galaxies show prominent Mg II emission and absorption in a P Cygni profile. We find no correlation between the equivalent widths of Mg II and Lyman alpha emission. The Mg II emission has a broader range of velocities than do the nebular emission line profiles; the Mg II emission is redshifted with respect to systemic by 100 to 200 km/s. When present, Lyman alpha is even more redshifted."},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1406.3356","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":"1406.3356","created_at":"2026-05-18T01:42:57.876143+00:00"},{"alias_kind":"arxiv_version","alias_value":"1406.3356v1","created_at":"2026-05-18T01:42:57.876143+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1406.3356","created_at":"2026-05-18T01:42:57.876143+00:00"},{"alias_kind":"pith_short_12","alias_value":"EAKRTAKGDFSQ","created_at":"2026-05-18T12:28:25.294606+00:00"},{"alias_kind":"pith_short_16","alias_value":"EAKRTAKGDFSQPEXI","created_at":"2026-05-18T12:28:25.294606+00:00"},{"alias_kind":"pith_short_8","alias_value":"EAKRTAKG","created_at":"2026-05-18T12:28:25.294606+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/EAKRTAKGDFSQPEXINI55236IUG","json":"https://pith.science/pith/EAKRTAKGDFSQPEXINI55236IUG.json","graph_json":"https://pith.science/api/pith-number/EAKRTAKGDFSQPEXINI55236IUG/graph.json","events_json":"https://pith.science/api/pith-number/EAKRTAKGDFSQPEXINI55236IUG/events.json","paper":"https://pith.science/paper/EAKRTAKG"},"agent_actions":{"view_html":"https://pith.science/pith/EAKRTAKGDFSQPEXINI55236IUG","download_json":"https://pith.science/pith/EAKRTAKGDFSQPEXINI55236IUG.json","view_paper":"https://pith.science/paper/EAKRTAKG","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1406.3356&json=true","fetch_graph":"https://pith.science/api/pith-number/EAKRTAKGDFSQPEXINI55236IUG/graph.json","fetch_events":"https://pith.science/api/pith-number/EAKRTAKGDFSQPEXINI55236IUG/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/EAKRTAKGDFSQPEXINI55236IUG/action/timestamp_anchor","attest_storage":"https://pith.science/pith/EAKRTAKGDFSQPEXINI55236IUG/action/storage_attestation","attest_author":"https://pith.science/pith/EAKRTAKGDFSQPEXINI55236IUG/action/author_attestation","sign_citation":"https://pith.science/pith/EAKRTAKGDFSQPEXINI55236IUG/action/citation_signature","submit_replication":"https://pith.science/pith/EAKRTAKGDFSQPEXINI55236IUG/action/replication_record"}},"created_at":"2026-05-18T01:42:57.876143+00:00","updated_at":"2026-05-18T01:42:57.876143+00:00"}