{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2018:CVLZKTUBKMFETNMQFVCB365NSG","short_pith_number":"pith:CVLZKTUB","schema_version":"1.0","canonical_sha256":"1557954e81530a49b5902d441dfbad91810827db139450ec077bea0d8c14db16","source":{"kind":"arxiv","id":"1806.01951","version":1},"attestation_state":"computed","paper":{"title":"A resolved warm/dense gas Schmidt-Kennicutt relationship in a binary HyLIRG at $z=2.41$","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Gustavo Orellana, Hugo Messias, Jonathan S. G\\'omez, Neil M. Nagar, Paul van der Werf, Rob J.Ivison","submitted_at":"2018-06-05T22:18:17Z","abstract_excerpt":"Hyperluminous infrared galaxies (HyLIRGs) provide crucial \"long lever arm\" constraints on galaxy evolution. H-ATLAS $J084933.4+021443$, a $z=2.41$ binary HyLIRG with at least two additional luminous companion galaxies, is thus an optimal test-ground for studies of star formation and galaxy evolution during \"cosmic noon\". We have used ALMA to obtain resolved imaging and kinematics of atomic and molecular emission lines, and rest-frame $340$ to $1160$GHz continuum emission, for the known luminous component galaxies in H-ATLAS $J084933.4+021443$: W, T, M, C. All four component galaxies are spatia"},"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":"1806.01951","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2018-06-05T22:18:17Z","cross_cats_sorted":[],"title_canon_sha256":"b79992f94f8c1e8e0ba575ead445f03651379367e8aa37e72942688dd7935c4f","abstract_canon_sha256":"53f88876fde38e793e0ceebbd21dfa84835bed5d76efe4d2427c8985be426ee1"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:14:03.296669Z","signature_b64":"Pj8c6OxzBQ/1GUaNF4vxdFnSeJi/DsXjxhuXM2cQg1a0AGshagxfc2sMgsb6kEeU/dWTLvha0kt8dQ5PZeAlAA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"1557954e81530a49b5902d441dfbad91810827db139450ec077bea0d8c14db16","last_reissued_at":"2026-05-18T00:14:03.295633Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:14:03.295633Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"A resolved warm/dense gas Schmidt-Kennicutt relationship in a binary HyLIRG at $z=2.41$","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Gustavo Orellana, Hugo Messias, Jonathan S. G\\'omez, Neil M. Nagar, Paul van der Werf, Rob J.Ivison","submitted_at":"2018-06-05T22:18:17Z","abstract_excerpt":"Hyperluminous infrared galaxies (HyLIRGs) provide crucial \"long lever arm\" constraints on galaxy evolution. H-ATLAS $J084933.4+021443$, a $z=2.41$ binary HyLIRG with at least two additional luminous companion galaxies, is thus an optimal test-ground for studies of star formation and galaxy evolution during \"cosmic noon\". We have used ALMA to obtain resolved imaging and kinematics of atomic and molecular emission lines, and rest-frame $340$ to $1160$GHz continuum emission, for the known luminous component galaxies in H-ATLAS $J084933.4+021443$: W, T, M, C. All four component galaxies are spatia"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1806.01951","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":"1806.01951","created_at":"2026-05-18T00:14:03.295945+00:00"},{"alias_kind":"arxiv_version","alias_value":"1806.01951v1","created_at":"2026-05-18T00:14:03.295945+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1806.01951","created_at":"2026-05-18T00:14:03.295945+00:00"},{"alias_kind":"pith_short_12","alias_value":"CVLZKTUBKMFE","created_at":"2026-05-18T12:32:19.392346+00:00"},{"alias_kind":"pith_short_16","alias_value":"CVLZKTUBKMFETNMQ","created_at":"2026-05-18T12:32:19.392346+00:00"},{"alias_kind":"pith_short_8","alias_value":"CVLZKTUB","created_at":"2026-05-18T12:32:19.392346+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/CVLZKTUBKMFETNMQFVCB365NSG","json":"https://pith.science/pith/CVLZKTUBKMFETNMQFVCB365NSG.json","graph_json":"https://pith.science/api/pith-number/CVLZKTUBKMFETNMQFVCB365NSG/graph.json","events_json":"https://pith.science/api/pith-number/CVLZKTUBKMFETNMQFVCB365NSG/events.json","paper":"https://pith.science/paper/CVLZKTUB"},"agent_actions":{"view_html":"https://pith.science/pith/CVLZKTUBKMFETNMQFVCB365NSG","download_json":"https://pith.science/pith/CVLZKTUBKMFETNMQFVCB365NSG.json","view_paper":"https://pith.science/paper/CVLZKTUB","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1806.01951&json=true","fetch_graph":"https://pith.science/api/pith-number/CVLZKTUBKMFETNMQFVCB365NSG/graph.json","fetch_events":"https://pith.science/api/pith-number/CVLZKTUBKMFETNMQFVCB365NSG/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/CVLZKTUBKMFETNMQFVCB365NSG/action/timestamp_anchor","attest_storage":"https://pith.science/pith/CVLZKTUBKMFETNMQFVCB365NSG/action/storage_attestation","attest_author":"https://pith.science/pith/CVLZKTUBKMFETNMQFVCB365NSG/action/author_attestation","sign_citation":"https://pith.science/pith/CVLZKTUBKMFETNMQFVCB365NSG/action/citation_signature","submit_replication":"https://pith.science/pith/CVLZKTUBKMFETNMQFVCB365NSG/action/replication_record"}},"created_at":"2026-05-18T00:14:03.295945+00:00","updated_at":"2026-05-18T00:14:03.295945+00:00"}