{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2017:HX42MJNLOPMADEB5KEP4XGJLZW","short_pith_number":"pith:HX42MJNL","schema_version":"1.0","canonical_sha256":"3df9a625ab73d801903d511fcb992bcd92de53b54f83f249866fb245cc9f08b1","source":{"kind":"arxiv","id":"1710.07694","version":1},"attestation_state":"computed","paper":{"title":"The MUSE Hubble Ultra Deep Field Survey: V. Spatially resolved stellar kinematics of galaxies at redshift $0.2\\lesssim z \\lesssim 0.8$","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Adrien Guerou, Benoit Epinat, Davor Krajnovic, Eric Emsellem, Johan Richard, Joop Schaye, Leo Michel-Dansac, Mark den Brok, Nicolas Bouche, Peter M. Weilbacher, Raffaella Anna Marino, Roland Bacon, Santiago Erroz-Ferrer, Thierry Contini","submitted_at":"2017-10-20T20:06:33Z","abstract_excerpt":"We present spatially resolved stellar kinematic maps, for the first time, for a sample of 17 intermediate redshift galaxies (0.2 < z < 0.8). We used deep MUSE/VLT integral field spectroscopic observations in the Hubble Deep Field South (HDFS) and Hubble Ultra Deep Field (HUDF), resulting from ~30h integration time per field, each covering 1'x1' field of view, with ~0.65\" spatial resolution. We selected all galaxies brighter than 25mag in the I band and for which the stellar continuum is detected over an area that is at least two times larger than the spatial resolution. The resulting sample co"},"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":"1710.07694","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2017-10-20T20:06:33Z","cross_cats_sorted":[],"title_canon_sha256":"88a7eb2953ce5af3dfdedba3ccc6fafd269238991ac2e051627579ed14327514","abstract_canon_sha256":"88d0bebd7078d428c7938c44a3270105ea54a61bc4e1e845daee6e638449a4ee"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:28:13.222776Z","signature_b64":"hH1A0eR7p6K/btaIsDBzI68uIMQ827sgLny64em/QyHGHltdud60lBQye/7jgt/KDhVEV/RsGb/nvCMkPm2VAA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"3df9a625ab73d801903d511fcb992bcd92de53b54f83f249866fb245cc9f08b1","last_reissued_at":"2026-05-18T00:28:13.222083Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:28:13.222083Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The MUSE Hubble Ultra Deep Field Survey: V. Spatially resolved stellar kinematics of galaxies at redshift $0.2\\lesssim z \\lesssim 0.8$","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Adrien Guerou, Benoit Epinat, Davor Krajnovic, Eric Emsellem, Johan Richard, Joop Schaye, Leo Michel-Dansac, Mark den Brok, Nicolas Bouche, Peter M. Weilbacher, Raffaella Anna Marino, Roland Bacon, Santiago Erroz-Ferrer, Thierry Contini","submitted_at":"2017-10-20T20:06:33Z","abstract_excerpt":"We present spatially resolved stellar kinematic maps, for the first time, for a sample of 17 intermediate redshift galaxies (0.2 < z < 0.8). We used deep MUSE/VLT integral field spectroscopic observations in the Hubble Deep Field South (HDFS) and Hubble Ultra Deep Field (HUDF), resulting from ~30h integration time per field, each covering 1'x1' field of view, with ~0.65\" spatial resolution. We selected all galaxies brighter than 25mag in the I band and for which the stellar continuum is detected over an area that is at least two times larger than the spatial resolution. The resulting sample co"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1710.07694","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":"1710.07694","created_at":"2026-05-18T00:28:13.222190+00:00"},{"alias_kind":"arxiv_version","alias_value":"1710.07694v1","created_at":"2026-05-18T00:28:13.222190+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1710.07694","created_at":"2026-05-18T00:28:13.222190+00:00"},{"alias_kind":"pith_short_12","alias_value":"HX42MJNLOPMA","created_at":"2026-05-18T12:31:21.493067+00:00"},{"alias_kind":"pith_short_16","alias_value":"HX42MJNLOPMADEB5","created_at":"2026-05-18T12:31:21.493067+00:00"},{"alias_kind":"pith_short_8","alias_value":"HX42MJNL","created_at":"2026-05-18T12:31:21.493067+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/HX42MJNLOPMADEB5KEP4XGJLZW","json":"https://pith.science/pith/HX42MJNLOPMADEB5KEP4XGJLZW.json","graph_json":"https://pith.science/api/pith-number/HX42MJNLOPMADEB5KEP4XGJLZW/graph.json","events_json":"https://pith.science/api/pith-number/HX42MJNLOPMADEB5KEP4XGJLZW/events.json","paper":"https://pith.science/paper/HX42MJNL"},"agent_actions":{"view_html":"https://pith.science/pith/HX42MJNLOPMADEB5KEP4XGJLZW","download_json":"https://pith.science/pith/HX42MJNLOPMADEB5KEP4XGJLZW.json","view_paper":"https://pith.science/paper/HX42MJNL","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1710.07694&json=true","fetch_graph":"https://pith.science/api/pith-number/HX42MJNLOPMADEB5KEP4XGJLZW/graph.json","fetch_events":"https://pith.science/api/pith-number/HX42MJNLOPMADEB5KEP4XGJLZW/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/HX42MJNLOPMADEB5KEP4XGJLZW/action/timestamp_anchor","attest_storage":"https://pith.science/pith/HX42MJNLOPMADEB5KEP4XGJLZW/action/storage_attestation","attest_author":"https://pith.science/pith/HX42MJNLOPMADEB5KEP4XGJLZW/action/author_attestation","sign_citation":"https://pith.science/pith/HX42MJNLOPMADEB5KEP4XGJLZW/action/citation_signature","submit_replication":"https://pith.science/pith/HX42MJNLOPMADEB5KEP4XGJLZW/action/replication_record"}},"created_at":"2026-05-18T00:28:13.222190+00:00","updated_at":"2026-05-18T00:28:13.222190+00:00"}