{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2017:MKOSFBUMLBPTOTK3OGM6T4JNHV","short_pith_number":"pith:MKOSFBUM","schema_version":"1.0","canonical_sha256":"629d22868c585f374d5b7199e9f12d3d4d100aa3ef4b15eedcbcf674174b05c0","source":{"kind":"arxiv","id":"1710.02360","version":1},"attestation_state":"computed","paper":{"title":"Galaxy overdensities around 3C radio galaxies and quasars at $1<z<2.5$ revealed by Spitzer $3.6/4.5\\mu$m and Pan-STARRS","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"B. J. Wilkes, Ch. Westhues, M. Haas, M.L.N. Ashby, R. Chini, S. P. Willner, Z. Ghaffari","submitted_at":"2017-10-06T11:46:40Z","abstract_excerpt":"Luminous radio sources are thought to lie in galaxy clusters or proto-clusters. The complete sample of 64 high-redshift 3C sources at $1<z<2.5$ has been mapped with the Spitzer Space Telescope. The IRAC $3.6\\mu$m and $4.5\\mu$m 5-$\\sigma$ detection limit of $4\\mu$Jy (22.4 AB mag) allows us to search for the brightest candidate cluster member galaxies associated with the 3C sources. To remove the contamination of foreground stars and galaxies along the lines of sight toward the 3C sources we apply color cuts: removed sources satisfy either the IRAC1/2 cut $[3.6] - [4.5] < -0.3$ or the Pan-STARRS"},"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":"1710.02360","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2017-10-06T11:46:40Z","cross_cats_sorted":[],"title_canon_sha256":"05096ef84bd4d7cc05c0ceec2512760bb12a302aaaef4ac89549fb1a5f3be50f","abstract_canon_sha256":"bf8ecaede65698abe698833ef86a3ef7d7ac3a6e4f99c2c283e01ace1db610bf"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:33:33.624266Z","signature_b64":"BGZmE+v7pvBCuqK/FK4mcL1YsX6Y3f4H57QotPeF2Egp3QCc+t6vXM07r4lJz4dD4DbxSQGlvuVPLrXHe4c9Dw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"629d22868c585f374d5b7199e9f12d3d4d100aa3ef4b15eedcbcf674174b05c0","last_reissued_at":"2026-05-18T00:33:33.623567Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:33:33.623567Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Galaxy overdensities around 3C radio galaxies and quasars at $1<z<2.5$ revealed by Spitzer $3.6/4.5\\mu$m and Pan-STARRS","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"B. J. Wilkes, Ch. Westhues, M. Haas, M.L.N. Ashby, R. Chini, S. P. Willner, Z. Ghaffari","submitted_at":"2017-10-06T11:46:40Z","abstract_excerpt":"Luminous radio sources are thought to lie in galaxy clusters or proto-clusters. The complete sample of 64 high-redshift 3C sources at $1<z<2.5$ has been mapped with the Spitzer Space Telescope. The IRAC $3.6\\mu$m and $4.5\\mu$m 5-$\\sigma$ detection limit of $4\\mu$Jy (22.4 AB mag) allows us to search for the brightest candidate cluster member galaxies associated with the 3C sources. To remove the contamination of foreground stars and galaxies along the lines of sight toward the 3C sources we apply color cuts: removed sources satisfy either the IRAC1/2 cut $[3.6] - [4.5] < -0.3$ or the Pan-STARRS"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1710.02360","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":"1710.02360","created_at":"2026-05-18T00:33:33.623683+00:00"},{"alias_kind":"arxiv_version","alias_value":"1710.02360v1","created_at":"2026-05-18T00:33:33.623683+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1710.02360","created_at":"2026-05-18T00:33:33.623683+00:00"},{"alias_kind":"pith_short_12","alias_value":"MKOSFBUMLBPT","created_at":"2026-05-18T12:31:31.346846+00:00"},{"alias_kind":"pith_short_16","alias_value":"MKOSFBUMLBPTOTK3","created_at":"2026-05-18T12:31:31.346846+00:00"},{"alias_kind":"pith_short_8","alias_value":"MKOSFBUM","created_at":"2026-05-18T12:31:31.346846+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/MKOSFBUMLBPTOTK3OGM6T4JNHV","json":"https://pith.science/pith/MKOSFBUMLBPTOTK3OGM6T4JNHV.json","graph_json":"https://pith.science/api/pith-number/MKOSFBUMLBPTOTK3OGM6T4JNHV/graph.json","events_json":"https://pith.science/api/pith-number/MKOSFBUMLBPTOTK3OGM6T4JNHV/events.json","paper":"https://pith.science/paper/MKOSFBUM"},"agent_actions":{"view_html":"https://pith.science/pith/MKOSFBUMLBPTOTK3OGM6T4JNHV","download_json":"https://pith.science/pith/MKOSFBUMLBPTOTK3OGM6T4JNHV.json","view_paper":"https://pith.science/paper/MKOSFBUM","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1710.02360&json=true","fetch_graph":"https://pith.science/api/pith-number/MKOSFBUMLBPTOTK3OGM6T4JNHV/graph.json","fetch_events":"https://pith.science/api/pith-number/MKOSFBUMLBPTOTK3OGM6T4JNHV/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/MKOSFBUMLBPTOTK3OGM6T4JNHV/action/timestamp_anchor","attest_storage":"https://pith.science/pith/MKOSFBUMLBPTOTK3OGM6T4JNHV/action/storage_attestation","attest_author":"https://pith.science/pith/MKOSFBUMLBPTOTK3OGM6T4JNHV/action/author_attestation","sign_citation":"https://pith.science/pith/MKOSFBUMLBPTOTK3OGM6T4JNHV/action/citation_signature","submit_replication":"https://pith.science/pith/MKOSFBUMLBPTOTK3OGM6T4JNHV/action/replication_record"}},"created_at":"2026-05-18T00:33:33.623683+00:00","updated_at":"2026-05-18T00:33:33.623683+00:00"}