{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2015:L7JT4XESXYHKQTRF6YD4QT3KDX","short_pith_number":"pith:L7JT4XES","schema_version":"1.0","canonical_sha256":"5fd33e5c92be0ea84e25f607c84f6a1def9cb03697cc6402c32ba76924f94a55","source":{"kind":"arxiv","id":"1510.01585","version":1},"attestation_state":"computed","paper":{"title":"Multi-wavelength characterisation of z~2 clustered, dusty star forming galaxies discovered by Planck","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"astro-ph.GA","authors_text":"D. Guery, D. Pierini, E. Le Floch, E. Pointecouteau, G. Lagache, G. Soucail, H. Dole, I. Flores-Cacho, L. Montier, N. Nesvadba, R. Canameras, R. Pello","submitted_at":"2015-10-06T14:12:17Z","abstract_excerpt":"(abridged) We report the discovery of PHz G95.5-61.6, a complex structure detected in emission in the Planck all-sky survey that corresponds to two over-densities of high-redshift galaxies. This is the first source from the Planck catalogue of high-z candidates that has been completely characterised with follow-up observations from the optical to the sub-millimetre domain. Herschel/SPIRE observations at 250, 350 and 500 microns reveal the existence of five sources producing a 500 microns emission excess that spatially corresponds to the candidate proto-clusters discovered by Planck. Further ob"},"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":"1510.01585","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2015-10-06T14:12:17Z","cross_cats_sorted":["astro-ph.CO"],"title_canon_sha256":"5f759d7607473f061df0ea45494abb72c8edca6b62af469aab0c59d1f2d475f9","abstract_canon_sha256":"bcbc6e4f70ead37cbec3ceff2f231529fb023a28601c5c409576ee7847132a42"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:23:55.121106Z","signature_b64":"gux9OgzkDkunijgTLWxcpPtMavpZJjeEtyBJT2xN2QuTY8aocCOB1bX6u5il8ppsM+yIWF7w9UO6csZf79SpDw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"5fd33e5c92be0ea84e25f607c84f6a1def9cb03697cc6402c32ba76924f94a55","last_reissued_at":"2026-05-18T01:23:55.120438Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:23:55.120438Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Multi-wavelength characterisation of z~2 clustered, dusty star forming galaxies discovered by Planck","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"astro-ph.GA","authors_text":"D. Guery, D. Pierini, E. Le Floch, E. Pointecouteau, G. Lagache, G. Soucail, H. Dole, I. Flores-Cacho, L. Montier, N. Nesvadba, R. Canameras, R. Pello","submitted_at":"2015-10-06T14:12:17Z","abstract_excerpt":"(abridged) We report the discovery of PHz G95.5-61.6, a complex structure detected in emission in the Planck all-sky survey that corresponds to two over-densities of high-redshift galaxies. This is the first source from the Planck catalogue of high-z candidates that has been completely characterised with follow-up observations from the optical to the sub-millimetre domain. Herschel/SPIRE observations at 250, 350 and 500 microns reveal the existence of five sources producing a 500 microns emission excess that spatially corresponds to the candidate proto-clusters discovered by Planck. Further ob"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1510.01585","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":"1510.01585","created_at":"2026-05-18T01:23:55.120575+00:00"},{"alias_kind":"arxiv_version","alias_value":"1510.01585v1","created_at":"2026-05-18T01:23:55.120575+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1510.01585","created_at":"2026-05-18T01:23:55.120575+00:00"},{"alias_kind":"pith_short_12","alias_value":"L7JT4XESXYHK","created_at":"2026-05-18T12:29:29.992203+00:00"},{"alias_kind":"pith_short_16","alias_value":"L7JT4XESXYHKQTRF","created_at":"2026-05-18T12:29:29.992203+00:00"},{"alias_kind":"pith_short_8","alias_value":"L7JT4XES","created_at":"2026-05-18T12:29:29.992203+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/L7JT4XESXYHKQTRF6YD4QT3KDX","json":"https://pith.science/pith/L7JT4XESXYHKQTRF6YD4QT3KDX.json","graph_json":"https://pith.science/api/pith-number/L7JT4XESXYHKQTRF6YD4QT3KDX/graph.json","events_json":"https://pith.science/api/pith-number/L7JT4XESXYHKQTRF6YD4QT3KDX/events.json","paper":"https://pith.science/paper/L7JT4XES"},"agent_actions":{"view_html":"https://pith.science/pith/L7JT4XESXYHKQTRF6YD4QT3KDX","download_json":"https://pith.science/pith/L7JT4XESXYHKQTRF6YD4QT3KDX.json","view_paper":"https://pith.science/paper/L7JT4XES","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1510.01585&json=true","fetch_graph":"https://pith.science/api/pith-number/L7JT4XESXYHKQTRF6YD4QT3KDX/graph.json","fetch_events":"https://pith.science/api/pith-number/L7JT4XESXYHKQTRF6YD4QT3KDX/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/L7JT4XESXYHKQTRF6YD4QT3KDX/action/timestamp_anchor","attest_storage":"https://pith.science/pith/L7JT4XESXYHKQTRF6YD4QT3KDX/action/storage_attestation","attest_author":"https://pith.science/pith/L7JT4XESXYHKQTRF6YD4QT3KDX/action/author_attestation","sign_citation":"https://pith.science/pith/L7JT4XESXYHKQTRF6YD4QT3KDX/action/citation_signature","submit_replication":"https://pith.science/pith/L7JT4XESXYHKQTRF6YD4QT3KDX/action/replication_record"}},"created_at":"2026-05-18T01:23:55.120575+00:00","updated_at":"2026-05-18T01:23:55.120575+00:00"}