{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2017:3LROR4S2EK74CRZFQRP2RDC3D2","short_pith_number":"pith:3LROR4S2","schema_version":"1.0","canonical_sha256":"dae2e8f25a22bfc14725845fa88c5b1ea14fbaec49cc4c5f62f25bcb3ca2a62a","source":{"kind":"arxiv","id":"1701.05561","version":2},"attestation_state":"computed","paper":{"title":"The KMOS Redshift One Spectroscopic Survey (KROSS): rotational velocities and angular momentum of z~0.9 galaxies","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"astro-ph.GA","authors_text":"A. J. Bunker, A.L. Tiley, A.M. Swinbank, C.M. Harrison (Durham, D. Sobral, ESO), G. Magdis, H.L. Johnson, Ian Smail, J.P. Stott, M. Bureau, M. Cirasuolo, M.J. Jarvis, P. Best, R.G. Bower, R.M. Sharples","submitted_at":"2017-01-19T19:00:05Z","abstract_excerpt":"We present dynamical measurements for 586 H-alpha detected star-forming galaxies from the KMOS (K-band Multi-Object Spectrograph) Redshift One Spectroscopic Survey (KROSS). The sample represents typical star-forming galaxies at this redshift (z=0.6-1.0), with a median star formation rate of ~7 Msol/yr and a stellar mass range of log[M/Msol]~9-11. We find that the rotation velocity-stellar mass relationship (the inverse of the Tully-Fisher relationship) for our rotationally-dominated sources (v/sigma>1) has a consistent slope and normalisation as that observed for z=0 disks. In contrast, the sp"},"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":"1701.05561","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2017-01-19T19:00:05Z","cross_cats_sorted":["astro-ph.CO"],"title_canon_sha256":"b8f24c3180db5f256df461bc9d17ce4edab4b4edee111bf18019baf26de1ffae","abstract_canon_sha256":"4ab95634b4294e4105d27c7edc6b492d178a4133f828609701c9932531e1719f"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:48:15.239122Z","signature_b64":"DoqdSJIoo7QR5h1AhvCXqHMEJN2H8L3buLvT6hbELq0QwJ+AzpetJs2NIkcjo/nbjtqfIi0vnTqxkzSyCLbdAA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"dae2e8f25a22bfc14725845fa88c5b1ea14fbaec49cc4c5f62f25bcb3ca2a62a","last_reissued_at":"2026-05-18T00:48:15.238524Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:48:15.238524Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The KMOS Redshift One Spectroscopic Survey (KROSS): rotational velocities and angular momentum of z~0.9 galaxies","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"astro-ph.GA","authors_text":"A. J. Bunker, A.L. Tiley, A.M. Swinbank, C.M. Harrison (Durham, D. Sobral, ESO), G. Magdis, H.L. Johnson, Ian Smail, J.P. Stott, M. Bureau, M. Cirasuolo, M.J. Jarvis, P. Best, R.G. Bower, R.M. Sharples","submitted_at":"2017-01-19T19:00:05Z","abstract_excerpt":"We present dynamical measurements for 586 H-alpha detected star-forming galaxies from the KMOS (K-band Multi-Object Spectrograph) Redshift One Spectroscopic Survey (KROSS). The sample represents typical star-forming galaxies at this redshift (z=0.6-1.0), with a median star formation rate of ~7 Msol/yr and a stellar mass range of log[M/Msol]~9-11. We find that the rotation velocity-stellar mass relationship (the inverse of the Tully-Fisher relationship) for our rotationally-dominated sources (v/sigma>1) has a consistent slope and normalisation as that observed for z=0 disks. In contrast, the sp"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1701.05561","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":"1701.05561","created_at":"2026-05-18T00:48:15.238620+00:00"},{"alias_kind":"arxiv_version","alias_value":"1701.05561v2","created_at":"2026-05-18T00:48:15.238620+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1701.05561","created_at":"2026-05-18T00:48:15.238620+00:00"},{"alias_kind":"pith_short_12","alias_value":"3LROR4S2EK74","created_at":"2026-05-18T12:30:58.224056+00:00"},{"alias_kind":"pith_short_16","alias_value":"3LROR4S2EK74CRZF","created_at":"2026-05-18T12:30:58.224056+00:00"},{"alias_kind":"pith_short_8","alias_value":"3LROR4S2","created_at":"2026-05-18T12:30:58.224056+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/3LROR4S2EK74CRZFQRP2RDC3D2","json":"https://pith.science/pith/3LROR4S2EK74CRZFQRP2RDC3D2.json","graph_json":"https://pith.science/api/pith-number/3LROR4S2EK74CRZFQRP2RDC3D2/graph.json","events_json":"https://pith.science/api/pith-number/3LROR4S2EK74CRZFQRP2RDC3D2/events.json","paper":"https://pith.science/paper/3LROR4S2"},"agent_actions":{"view_html":"https://pith.science/pith/3LROR4S2EK74CRZFQRP2RDC3D2","download_json":"https://pith.science/pith/3LROR4S2EK74CRZFQRP2RDC3D2.json","view_paper":"https://pith.science/paper/3LROR4S2","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1701.05561&json=true","fetch_graph":"https://pith.science/api/pith-number/3LROR4S2EK74CRZFQRP2RDC3D2/graph.json","fetch_events":"https://pith.science/api/pith-number/3LROR4S2EK74CRZFQRP2RDC3D2/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/3LROR4S2EK74CRZFQRP2RDC3D2/action/timestamp_anchor","attest_storage":"https://pith.science/pith/3LROR4S2EK74CRZFQRP2RDC3D2/action/storage_attestation","attest_author":"https://pith.science/pith/3LROR4S2EK74CRZFQRP2RDC3D2/action/author_attestation","sign_citation":"https://pith.science/pith/3LROR4S2EK74CRZFQRP2RDC3D2/action/citation_signature","submit_replication":"https://pith.science/pith/3LROR4S2EK74CRZFQRP2RDC3D2/action/replication_record"}},"created_at":"2026-05-18T00:48:15.238620+00:00","updated_at":"2026-05-18T00:48:15.238620+00:00"}