{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2018:RDF5TTKP65DYCGAXPD4TN3IGXT","short_pith_number":"pith:RDF5TTKP","schema_version":"1.0","canonical_sha256":"88cbd9cd4ff74781181778f936ed06bcca142231d4ddb21d03850f5e32e40d3f","source":{"kind":"arxiv","id":"1803.07414","version":2},"attestation_state":"computed","paper":{"title":"The VANDELS ESO public spectroscopic survey","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"A. Bongiorno, A. C. Carnall, A. Cimatti, A. Citro, A. Fontana, A. Galametz, A. Gargiulo, A. Georgakakis, A. Grazian, A. Iovino, A. M. Koekemoer, A. Mortlock, B. Garilli, C. C. Williams, C. Papovich, C. Schreiber, D. Elbaz, D. J. McLeod, D. Maccagni, D. P. Rosario, D. P. Stark, D. Schaerer, D. T. Maltby, E. Curtis-Lake, E. F. Bell, E. Marmol-Queralto, E. Pompei, E. Vanzella, E. Zucca, F. Buitrago, F. Cullen, F. Fiore, F. Fontanot, F. Mannucci, F. Marchi, G. Cresci, G. G. Fazio, G. Zamorani, H. C. Ferguson, H. Mendez-Hernandez, I. Balestra, I. Jung, J. Mendez-Abreu, J. M. Lotz, J. P. U. Fynbo, J. S. Dunlop, K. I. Caputi, K. Matsuoka, K. Nandra, L. A. M. Tasca, L. Guaita, L. Pentericci, L. Pozzetti, M. Bolzonella, M. Brusa, M. Castellano, M. Cirasuolo, M. Dickinson, M. Franco, M. Fumana, M. Giavalisco, M. J. Jarvis, M. Mignoli, M. Moresco, M. Nonino, M. Pannella, M. Salvato, M. Scodeggio, M. Talia, N. Bourne, N. P. Hathi, O. Almaini, O. Cucciati, O. Le Fevre, P. Cassata, P. Franzetti, P. Popesso, P. Santini, R. A. A. Bowler, R. Amorin, R. J. McLure, R. Thomas, S. Bardelli, S. Charlot, S. Cristiani, S. de Barros, S. Juneau, S. Kim, S. L. Finkelstein, T. Treu, V. Sommariva, V. Wild, W. G. Hartley, W. Karman, Y. Khusanova","submitted_at":"2018-03-20T13:25:37Z","abstract_excerpt":"VANDELS is a uniquely-deep spectroscopic survey of high-redshift galaxies with the VIMOS spectrograph on ESO's Very Large Telescope (VLT). The survey has obtained ultra-deep optical (0.48 < lambda < 1.0 micron) spectroscopy of ~2100 galaxies within the redshift interval 1.0 < z < 7.0, over a total area of ~0.2 sq. degrees centred on the CANDELS UDS and CDFS fields. Based on accurate photometric redshift pre-selection, 85% of the galaxies targeted by VANDELS were selected to be at z>=3. Exploiting the red sensitivity of the refurbished VIMOS spectrograph, the fundamental aim of the survey is to"},"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":"1803.07414","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2018-03-20T13:25:37Z","cross_cats_sorted":[],"title_canon_sha256":"d03b8601f9d0b7e184097a661d76021f2ca126990c0bbdf4e5e12c3330083880","abstract_canon_sha256":"bc231fab9c3a5a0d8bb4bbc932e67c343db78f4efe59f65a2dd1c7bc8f88da2f"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:11:49.585030Z","signature_b64":"7sNB0iR8Sp9ZZSwjUHa+NNRBstRs0/lR0wdL+K/9ZIheAf9DHWG8nUVsuopzWbRzvqhiv5sbO1fJ0lg2lLAeDA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"88cbd9cd4ff74781181778f936ed06bcca142231d4ddb21d03850f5e32e40d3f","last_reissued_at":"2026-05-18T00:11:49.584542Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:11:49.584542Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The VANDELS ESO public spectroscopic survey","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"A. Bongiorno, A. C. Carnall, A. Cimatti, A. Citro, A. Fontana, A. Galametz, A. Gargiulo, A. Georgakakis, A. Grazian, A. Iovino, A. M. Koekemoer, A. Mortlock, B. Garilli, C. C. Williams, C. Papovich, C. Schreiber, D. Elbaz, D. J. McLeod, D. Maccagni, D. P. Rosario, D. P. Stark, D. Schaerer, D. T. Maltby, E. Curtis-Lake, E. F. Bell, E. Marmol-Queralto, E. Pompei, E. Vanzella, E. Zucca, F. Buitrago, F. Cullen, F. Fiore, F. Fontanot, F. Mannucci, F. Marchi, G. Cresci, G. G. Fazio, G. Zamorani, H. C. Ferguson, H. Mendez-Hernandez, I. Balestra, I. Jung, J. Mendez-Abreu, J. M. Lotz, J. P. U. Fynbo, J. S. Dunlop, K. I. Caputi, K. Matsuoka, K. Nandra, L. A. M. Tasca, L. Guaita, L. Pentericci, L. Pozzetti, M. Bolzonella, M. Brusa, M. Castellano, M. Cirasuolo, M. Dickinson, M. Franco, M. Fumana, M. Giavalisco, M. J. Jarvis, M. Mignoli, M. Moresco, M. Nonino, M. Pannella, M. Salvato, M. Scodeggio, M. Talia, N. Bourne, N. P. Hathi, O. Almaini, O. Cucciati, O. Le Fevre, P. Cassata, P. Franzetti, P. Popesso, P. Santini, R. A. A. Bowler, R. Amorin, R. J. McLure, R. Thomas, S. Bardelli, S. Charlot, S. Cristiani, S. de Barros, S. Juneau, S. Kim, S. L. Finkelstein, T. Treu, V. Sommariva, V. Wild, W. G. Hartley, W. Karman, Y. Khusanova","submitted_at":"2018-03-20T13:25:37Z","abstract_excerpt":"VANDELS is a uniquely-deep spectroscopic survey of high-redshift galaxies with the VIMOS spectrograph on ESO's Very Large Telescope (VLT). The survey has obtained ultra-deep optical (0.48 < lambda < 1.0 micron) spectroscopy of ~2100 galaxies within the redshift interval 1.0 < z < 7.0, over a total area of ~0.2 sq. degrees centred on the CANDELS UDS and CDFS fields. Based on accurate photometric redshift pre-selection, 85% of the galaxies targeted by VANDELS were selected to be at z>=3. Exploiting the red sensitivity of the refurbished VIMOS spectrograph, the fundamental aim of the survey is to"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1803.07414","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":"1803.07414","created_at":"2026-05-18T00:11:49.584625+00:00"},{"alias_kind":"arxiv_version","alias_value":"1803.07414v2","created_at":"2026-05-18T00:11:49.584625+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1803.07414","created_at":"2026-05-18T00:11:49.584625+00:00"},{"alias_kind":"pith_short_12","alias_value":"RDF5TTKP65DY","created_at":"2026-05-18T12:32:50.500415+00:00"},{"alias_kind":"pith_short_16","alias_value":"RDF5TTKP65DYCGAX","created_at":"2026-05-18T12:32:50.500415+00:00"},{"alias_kind":"pith_short_8","alias_value":"RDF5TTKP","created_at":"2026-05-18T12:32:50.500415+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":2,"internal_anchor_count":2,"sample":[{"citing_arxiv_id":"2606.20800","citing_title":"No hidden monsters: Probing recently-quenched galaxies for obscured AGN with JWST-PRIMER MIRI and NIRCam","ref_index":58,"is_internal_anchor":true},{"citing_arxiv_id":"2606.20845","citing_title":"LEGGOS I: The JWST LEGGOS Survey -- LEnsing and Galaxy Growth: Observing Substructures -- Unpacks the Nature of Clumpy Star Formation and Quenching in Gravitationally Lensed Galaxies beyond Cosmic Noo","ref_index":283,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/RDF5TTKP65DYCGAXPD4TN3IGXT","json":"https://pith.science/pith/RDF5TTKP65DYCGAXPD4TN3IGXT.json","graph_json":"https://pith.science/api/pith-number/RDF5TTKP65DYCGAXPD4TN3IGXT/graph.json","events_json":"https://pith.science/api/pith-number/RDF5TTKP65DYCGAXPD4TN3IGXT/events.json","paper":"https://pith.science/paper/RDF5TTKP"},"agent_actions":{"view_html":"https://pith.science/pith/RDF5TTKP65DYCGAXPD4TN3IGXT","download_json":"https://pith.science/pith/RDF5TTKP65DYCGAXPD4TN3IGXT.json","view_paper":"https://pith.science/paper/RDF5TTKP","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1803.07414&json=true","fetch_graph":"https://pith.science/api/pith-number/RDF5TTKP65DYCGAXPD4TN3IGXT/graph.json","fetch_events":"https://pith.science/api/pith-number/RDF5TTKP65DYCGAXPD4TN3IGXT/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/RDF5TTKP65DYCGAXPD4TN3IGXT/action/timestamp_anchor","attest_storage":"https://pith.science/pith/RDF5TTKP65DYCGAXPD4TN3IGXT/action/storage_attestation","attest_author":"https://pith.science/pith/RDF5TTKP65DYCGAXPD4TN3IGXT/action/author_attestation","sign_citation":"https://pith.science/pith/RDF5TTKP65DYCGAXPD4TN3IGXT/action/citation_signature","submit_replication":"https://pith.science/pith/RDF5TTKP65DYCGAXPD4TN3IGXT/action/replication_record"}},"created_at":"2026-05-18T00:11:49.584625+00:00","updated_at":"2026-05-18T00:11:49.584625+00:00"}