{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2013:5MZQWNZW5FUMHAQX4HXOG5MZCV","short_pith_number":"pith:5MZQWNZW","schema_version":"1.0","canonical_sha256":"eb330b3736e968c38217e1eee37599154709ed88aea8cc32baff4515be2c2c49","source":{"kind":"arxiv","id":"1310.3822","version":2},"attestation_state":"computed","paper":{"title":"The dynamics of z=0.8 H-alpha-selected star-forming galaxies from KMOS/CF-HiZELS","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.GA","astro-ph.IM"],"primary_cat":"astro-ph.CO","authors_text":"A. M. Swinbank, David Sobral, Ian Smail, James E. Geach, John Stott, Jorryt Matthee, Philip N. Best, Ray M. Sharples, Richard G. Bower","submitted_at":"2013-10-14T20:00:01Z","abstract_excerpt":"We present the spatially resolved H-alpha (Ha) dynamics of sixteen star-forming galaxies at z~0.81 using the new KMOS multi-object integral field spectrograph on the ESO VLT. These galaxies were selected using 1.18 um narrow-band imaging from the 10 deg^2 CFHT-HiZELS survey of the SA22hr field, are found in a ~4Mpc over-density of Ha emitters and likely reside in a group/intermediate environment, but not a cluster. We confirm and identify a rich group of star-forming galaxies at z=0.813+-0.003, with thirteen galaxies within 1000 km/s of each other, and 7 within a diameter of 3Mpc. All our gala"},"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":"1310.3822","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2013-10-14T20:00:01Z","cross_cats_sorted":["astro-ph.GA","astro-ph.IM"],"title_canon_sha256":"12429a732123492091801b914911aa2008d685a5f98cbb6e2943b7035a54ee90","abstract_canon_sha256":"833374bfefe0a85041ba1e3ac03dca548c03c910ab7328645593a48e77f24cf0"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T03:05:17.972001Z","signature_b64":"lu2pEVSDJGvAQf4w7XckarweHmeMfuPx2f44kg68HQ9VWnVuFIUErVmn5W+G4UbF+CCgasEgYzOzNguw8LuGDg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"eb330b3736e968c38217e1eee37599154709ed88aea8cc32baff4515be2c2c49","last_reissued_at":"2026-05-18T03:05:17.971385Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T03:05:17.971385Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The dynamics of z=0.8 H-alpha-selected star-forming galaxies from KMOS/CF-HiZELS","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.GA","astro-ph.IM"],"primary_cat":"astro-ph.CO","authors_text":"A. M. Swinbank, David Sobral, Ian Smail, James E. Geach, John Stott, Jorryt Matthee, Philip N. Best, Ray M. Sharples, Richard G. Bower","submitted_at":"2013-10-14T20:00:01Z","abstract_excerpt":"We present the spatially resolved H-alpha (Ha) dynamics of sixteen star-forming galaxies at z~0.81 using the new KMOS multi-object integral field spectrograph on the ESO VLT. These galaxies were selected using 1.18 um narrow-band imaging from the 10 deg^2 CFHT-HiZELS survey of the SA22hr field, are found in a ~4Mpc over-density of Ha emitters and likely reside in a group/intermediate environment, but not a cluster. We confirm and identify a rich group of star-forming galaxies at z=0.813+-0.003, with thirteen galaxies within 1000 km/s of each other, and 7 within a diameter of 3Mpc. All our gala"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1310.3822","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":"1310.3822","created_at":"2026-05-18T03:05:17.971479+00:00"},{"alias_kind":"arxiv_version","alias_value":"1310.3822v2","created_at":"2026-05-18T03:05:17.971479+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1310.3822","created_at":"2026-05-18T03:05:17.971479+00:00"},{"alias_kind":"pith_short_12","alias_value":"5MZQWNZW5FUM","created_at":"2026-05-18T12:27:34.582898+00:00"},{"alias_kind":"pith_short_16","alias_value":"5MZQWNZW5FUMHAQX","created_at":"2026-05-18T12:27:34.582898+00:00"},{"alias_kind":"pith_short_8","alias_value":"5MZQWNZW","created_at":"2026-05-18T12:27:34.582898+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/5MZQWNZW5FUMHAQX4HXOG5MZCV","json":"https://pith.science/pith/5MZQWNZW5FUMHAQX4HXOG5MZCV.json","graph_json":"https://pith.science/api/pith-number/5MZQWNZW5FUMHAQX4HXOG5MZCV/graph.json","events_json":"https://pith.science/api/pith-number/5MZQWNZW5FUMHAQX4HXOG5MZCV/events.json","paper":"https://pith.science/paper/5MZQWNZW"},"agent_actions":{"view_html":"https://pith.science/pith/5MZQWNZW5FUMHAQX4HXOG5MZCV","download_json":"https://pith.science/pith/5MZQWNZW5FUMHAQX4HXOG5MZCV.json","view_paper":"https://pith.science/paper/5MZQWNZW","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1310.3822&json=true","fetch_graph":"https://pith.science/api/pith-number/5MZQWNZW5FUMHAQX4HXOG5MZCV/graph.json","fetch_events":"https://pith.science/api/pith-number/5MZQWNZW5FUMHAQX4HXOG5MZCV/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/5MZQWNZW5FUMHAQX4HXOG5MZCV/action/timestamp_anchor","attest_storage":"https://pith.science/pith/5MZQWNZW5FUMHAQX4HXOG5MZCV/action/storage_attestation","attest_author":"https://pith.science/pith/5MZQWNZW5FUMHAQX4HXOG5MZCV/action/author_attestation","sign_citation":"https://pith.science/pith/5MZQWNZW5FUMHAQX4HXOG5MZCV/action/citation_signature","submit_replication":"https://pith.science/pith/5MZQWNZW5FUMHAQX4HXOG5MZCV/action/replication_record"}},"created_at":"2026-05-18T03:05:17.971479+00:00","updated_at":"2026-05-18T03:05:17.971479+00:00"}