{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2018:ZAY5IJ7PQ4F5I7A6FOMPA3OYOG","short_pith_number":"pith:ZAY5IJ7P","schema_version":"1.0","canonical_sha256":"c831d427ef870bd47c1e2b98f06dd871ab1c948207766fd52d082ca44a4e7264","source":{"kind":"arxiv","id":"1806.10211","version":2},"attestation_state":"computed","paper":{"title":"LBT/ARGOS adaptive optics observations of z$\\sim 2$ lensed galaxies","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"A. Contursi, C. Grillo, D. Lutz, D. Peter, F. Mannucci, G. Cresci, G. Orban de Xivry, G. Rahmer, H. Gemperlein, I. Georgiev, J. Borelli, J. Ziegler, L. Busoni, M. Bonaglia, M. Curti, M. Deysenroth, M. Kulas, M. Perna, M. Rosensteiner, P. Buschkamp, S. Belli, S. Esposito, S. Rabien, S. Zibetti, T. Mazzoni, W. Gaessler, W. Raab","submitted_at":"2018-06-26T21:11:28Z","abstract_excerpt":"Gravitationally lensed systems allow a detailed view of galaxies at high redshift. High spatial- and spectral-resolution measurements of arc-like structures can offer unique constraints on the physical and dynamical properties of high-z systems. We present near-infrared spectra centred on the gravitational arcs of six known z ~ 2 lensed star-forming galaxies of stellar masses of 10^9-10^11 Msun and star formation rate (SFR) in the range between 10 and 400 Msun/yr. Ground layer adaptive optics (AO)-assisted observations are obtained at the Large Binocular Telescope (LBT) with the LUCI spectrogr"},"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":"1806.10211","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2018-06-26T21:11:28Z","cross_cats_sorted":[],"title_canon_sha256":"683d3e3b55bbbdf04dd8fe8f0f55040e7aa5ac6886c64f2d532cfe9ff41f1aec","abstract_canon_sha256":"ec95620b0597d79887e82459042f3f0a0a8a485e05bda058fd5d12e77ef6acdb"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:03:04.973802Z","signature_b64":"pXJIxeTyMU2R7UvmTQPl5gjJOJrxU5iZxfO0xkS1WwmR26828EzOmgC/SODsbHwf9IPMon+mjkJgOQQRBN79Ag==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"c831d427ef870bd47c1e2b98f06dd871ab1c948207766fd52d082ca44a4e7264","last_reissued_at":"2026-05-18T00:03:04.973147Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:03:04.973147Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"LBT/ARGOS adaptive optics observations of z$\\sim 2$ lensed galaxies","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"A. Contursi, C. Grillo, D. Lutz, D. Peter, F. Mannucci, G. Cresci, G. Orban de Xivry, G. Rahmer, H. Gemperlein, I. Georgiev, J. Borelli, J. Ziegler, L. Busoni, M. Bonaglia, M. Curti, M. Deysenroth, M. Kulas, M. Perna, M. Rosensteiner, P. Buschkamp, S. Belli, S. Esposito, S. Rabien, S. Zibetti, T. Mazzoni, W. Gaessler, W. Raab","submitted_at":"2018-06-26T21:11:28Z","abstract_excerpt":"Gravitationally lensed systems allow a detailed view of galaxies at high redshift. High spatial- and spectral-resolution measurements of arc-like structures can offer unique constraints on the physical and dynamical properties of high-z systems. We present near-infrared spectra centred on the gravitational arcs of six known z ~ 2 lensed star-forming galaxies of stellar masses of 10^9-10^11 Msun and star formation rate (SFR) in the range between 10 and 400 Msun/yr. Ground layer adaptive optics (AO)-assisted observations are obtained at the Large Binocular Telescope (LBT) with the LUCI spectrogr"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1806.10211","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":""},"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":"1806.10211","created_at":"2026-05-18T00:03:04.973234+00:00"},{"alias_kind":"arxiv_version","alias_value":"1806.10211v2","created_at":"2026-05-18T00:03:04.973234+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1806.10211","created_at":"2026-05-18T00:03:04.973234+00:00"},{"alias_kind":"pith_short_12","alias_value":"ZAY5IJ7PQ4F5","created_at":"2026-05-18T12:33:04.347982+00:00"},{"alias_kind":"pith_short_16","alias_value":"ZAY5IJ7PQ4F5I7A6","created_at":"2026-05-18T12:33:04.347982+00:00"},{"alias_kind":"pith_short_8","alias_value":"ZAY5IJ7P","created_at":"2026-05-18T12:33:04.347982+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/ZAY5IJ7PQ4F5I7A6FOMPA3OYOG","json":"https://pith.science/pith/ZAY5IJ7PQ4F5I7A6FOMPA3OYOG.json","graph_json":"https://pith.science/api/pith-number/ZAY5IJ7PQ4F5I7A6FOMPA3OYOG/graph.json","events_json":"https://pith.science/api/pith-number/ZAY5IJ7PQ4F5I7A6FOMPA3OYOG/events.json","paper":"https://pith.science/paper/ZAY5IJ7P"},"agent_actions":{"view_html":"https://pith.science/pith/ZAY5IJ7PQ4F5I7A6FOMPA3OYOG","download_json":"https://pith.science/pith/ZAY5IJ7PQ4F5I7A6FOMPA3OYOG.json","view_paper":"https://pith.science/paper/ZAY5IJ7P","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1806.10211&json=true","fetch_graph":"https://pith.science/api/pith-number/ZAY5IJ7PQ4F5I7A6FOMPA3OYOG/graph.json","fetch_events":"https://pith.science/api/pith-number/ZAY5IJ7PQ4F5I7A6FOMPA3OYOG/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/ZAY5IJ7PQ4F5I7A6FOMPA3OYOG/action/timestamp_anchor","attest_storage":"https://pith.science/pith/ZAY5IJ7PQ4F5I7A6FOMPA3OYOG/action/storage_attestation","attest_author":"https://pith.science/pith/ZAY5IJ7PQ4F5I7A6FOMPA3OYOG/action/author_attestation","sign_citation":"https://pith.science/pith/ZAY5IJ7PQ4F5I7A6FOMPA3OYOG/action/citation_signature","submit_replication":"https://pith.science/pith/ZAY5IJ7PQ4F5I7A6FOMPA3OYOG/action/replication_record"}},"created_at":"2026-05-18T00:03:04.973234+00:00","updated_at":"2026-05-18T00:03:04.973234+00:00"}