{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2024:RRJZAMBX4QHBRQC6AZ64PS5FZY","short_pith_number":"pith:RRJZAMBX","schema_version":"1.0","canonical_sha256":"8c53903037e40e18c05e067dc7cba5ce29cb8352f9632f53db196210336f0b92","source":{"kind":"arxiv","id":"2411.11952","version":1},"attestation_state":"computed","paper":{"title":"The host galaxies of radio-loud quasars at z>5 with ALMA","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"A. B. Drake, A.-C. Eilers, B. P. Venemans, C. Mazzucchelli, E. Ba\\~nados, E. Momjian, E. P. Farina, F. Walter, F. Wang, M. Onoue, R. A. Meyer, R. Decarli, S. Belladitta, S. Rojas-Ruiz, T. Connor, Y. Khusanova","submitted_at":"2024-11-18T19:00:01Z","abstract_excerpt":"The interaction between radio-jets and quasar host galaxies plays a paramount role in quasar/galaxy co-evolution. However, very little has been known so far about this interaction at very high-z. Here, we present new Atacama Large Millimeter/submillimeter Array (ALMA) observations in Band 7 and Band 3 of six radio-loud quasars' host galaxies at $z > 5$. We recover [CII] 158 $\\mu$m line and underlying dust continuum emission at $>2\\sigma$ for five sources, while we obtain upper limits for the CO(6-5) emission line and continuum for the remaining source. At the spatial resolution of our observat"},"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":"2411.11952","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.GA","submitted_at":"2024-11-18T19:00:01Z","cross_cats_sorted":[],"title_canon_sha256":"62130a44ec75e94ccfd62a489a9912d1375ff9615d78b195cc3538f29a5e4647","abstract_canon_sha256":"af41c92c75d674f27c9ff728e01d59de79049ee3205d9a7a2f7e3da270031360"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T10:12:50.017258Z","signature_b64":"2F64sRk6H89gijProP+ZNWKdfkbSqpZF94Bw1oH58dXIsossQFcMa2uhVYuehDUQj4C3GVDk14Oq0Fl/Cx9HDw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"8c53903037e40e18c05e067dc7cba5ce29cb8352f9632f53db196210336f0b92","last_reissued_at":"2026-07-05T10:12:50.016741Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T10:12:50.016741Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The host galaxies of radio-loud quasars at z>5 with ALMA","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"A. B. Drake, A.-C. Eilers, B. P. Venemans, C. Mazzucchelli, E. Ba\\~nados, E. Momjian, E. P. Farina, F. Walter, F. Wang, M. Onoue, R. A. Meyer, R. Decarli, S. Belladitta, S. Rojas-Ruiz, T. Connor, Y. Khusanova","submitted_at":"2024-11-18T19:00:01Z","abstract_excerpt":"The interaction between radio-jets and quasar host galaxies plays a paramount role in quasar/galaxy co-evolution. However, very little has been known so far about this interaction at very high-z. Here, we present new Atacama Large Millimeter/submillimeter Array (ALMA) observations in Band 7 and Band 3 of six radio-loud quasars' host galaxies at $z > 5$. We recover [CII] 158 $\\mu$m line and underlying dust continuum emission at $>2\\sigma$ for five sources, while we obtain upper limits for the CO(6-5) emission line and continuum for the remaining source. At the spatial resolution of our observat"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2411.11952","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2411.11952/integrity.json","findings":[],"available":true,"detectors_run":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938"},"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":"2411.11952","created_at":"2026-07-05T10:12:50.016805+00:00"},{"alias_kind":"arxiv_version","alias_value":"2411.11952v1","created_at":"2026-07-05T10:12:50.016805+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2411.11952","created_at":"2026-07-05T10:12:50.016805+00:00"},{"alias_kind":"pith_short_12","alias_value":"RRJZAMBX4QHB","created_at":"2026-07-05T10:12:50.016805+00:00"},{"alias_kind":"pith_short_16","alias_value":"RRJZAMBX4QHBRQC6","created_at":"2026-07-05T10:12:50.016805+00:00"},{"alias_kind":"pith_short_8","alias_value":"RRJZAMBX","created_at":"2026-07-05T10:12:50.016805+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2605.20698","citing_title":"CO(7-6) and [C I](2-1) survey in z > 6 quasars","ref_index":84,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/RRJZAMBX4QHBRQC6AZ64PS5FZY","json":"https://pith.science/pith/RRJZAMBX4QHBRQC6AZ64PS5FZY.json","graph_json":"https://pith.science/api/pith-number/RRJZAMBX4QHBRQC6AZ64PS5FZY/graph.json","events_json":"https://pith.science/api/pith-number/RRJZAMBX4QHBRQC6AZ64PS5FZY/events.json","paper":"https://pith.science/paper/RRJZAMBX"},"agent_actions":{"view_html":"https://pith.science/pith/RRJZAMBX4QHBRQC6AZ64PS5FZY","download_json":"https://pith.science/pith/RRJZAMBX4QHBRQC6AZ64PS5FZY.json","view_paper":"https://pith.science/paper/RRJZAMBX","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2411.11952&json=true","fetch_graph":"https://pith.science/api/pith-number/RRJZAMBX4QHBRQC6AZ64PS5FZY/graph.json","fetch_events":"https://pith.science/api/pith-number/RRJZAMBX4QHBRQC6AZ64PS5FZY/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/RRJZAMBX4QHBRQC6AZ64PS5FZY/action/timestamp_anchor","attest_storage":"https://pith.science/pith/RRJZAMBX4QHBRQC6AZ64PS5FZY/action/storage_attestation","attest_author":"https://pith.science/pith/RRJZAMBX4QHBRQC6AZ64PS5FZY/action/author_attestation","sign_citation":"https://pith.science/pith/RRJZAMBX4QHBRQC6AZ64PS5FZY/action/citation_signature","submit_replication":"https://pith.science/pith/RRJZAMBX4QHBRQC6AZ64PS5FZY/action/replication_record"}},"created_at":"2026-07-05T10:12:50.016805+00:00","updated_at":"2026-07-05T10:12:50.016805+00:00"}