{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2015:DTR6Z5MLSMHSJR4UOYE3NUA53N","short_pith_number":"pith:DTR6Z5ML","schema_version":"1.0","canonical_sha256":"1ce3ecf58b930f24c7947609b6d01ddb5a7641c125ccc8f4d48c5fdc7dc4132e","source":{"kind":"arxiv","id":"1504.03401","version":1},"attestation_state":"computed","paper":{"title":"Wide Field Multiband Imaging of Low Redshift Quasar Environments","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Alireza Rafiee, Christopher Thibodeau, Erica Ellingson, Jennifer E. Scott, Jill Bechtold, Michael Richmond","submitted_at":"2015-04-14T02:12:37Z","abstract_excerpt":"We present photometry of the large scale environments of a sample of twelve broad line AGN with $0.06 < z < 0.37$ from deep images in the SDSS $u$, $g$, $r$, and $i$ filters taken with the 90Prime prime focus camera on the Steward Observatory Bok Telescope. We measure galaxy clustering around these AGN using two standard techniques: correlation amplitude (B$_{gq}$) and the two point correlation function. We find average correlation amplitudes for the 10 radio quiet objects in the sample equal to (9$\\pm$18, 144$\\pm$114, -39$\\pm$56, 295$\\pm$260) Mpc$^{1.77}$ in ($u$, $g$, $r$, $i$), all consiste"},"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":"1504.03401","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2015-04-14T02:12:37Z","cross_cats_sorted":[],"title_canon_sha256":"4698568459a973030c2e8724d0c53ffed52f6095571f57300b19d0f83da50f31","abstract_canon_sha256":"2a740142d8e009f014209f36be314bb9c16fc43d8d3db1828f3d8628af11c850"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:18:52.284695Z","signature_b64":"rwyGLxGbXOXrUxuH4NeS3LPBjdJCroptDmIjWebdeg+ywXcyTljlSdwm9545SxJ0wKfBxskdqgpObWDNwrH6Dw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"1ce3ecf58b930f24c7947609b6d01ddb5a7641c125ccc8f4d48c5fdc7dc4132e","last_reissued_at":"2026-05-18T02:18:52.284156Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:18:52.284156Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Wide Field Multiband Imaging of Low Redshift Quasar Environments","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Alireza Rafiee, Christopher Thibodeau, Erica Ellingson, Jennifer E. Scott, Jill Bechtold, Michael Richmond","submitted_at":"2015-04-14T02:12:37Z","abstract_excerpt":"We present photometry of the large scale environments of a sample of twelve broad line AGN with $0.06 < z < 0.37$ from deep images in the SDSS $u$, $g$, $r$, and $i$ filters taken with the 90Prime prime focus camera on the Steward Observatory Bok Telescope. We measure galaxy clustering around these AGN using two standard techniques: correlation amplitude (B$_{gq}$) and the two point correlation function. We find average correlation amplitudes for the 10 radio quiet objects in the sample equal to (9$\\pm$18, 144$\\pm$114, -39$\\pm$56, 295$\\pm$260) Mpc$^{1.77}$ in ($u$, $g$, $r$, $i$), all consiste"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1504.03401","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":"1504.03401","created_at":"2026-05-18T02:18:52.284243+00:00"},{"alias_kind":"arxiv_version","alias_value":"1504.03401v1","created_at":"2026-05-18T02:18:52.284243+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1504.03401","created_at":"2026-05-18T02:18:52.284243+00:00"},{"alias_kind":"pith_short_12","alias_value":"DTR6Z5MLSMHS","created_at":"2026-05-18T12:29:17.054201+00:00"},{"alias_kind":"pith_short_16","alias_value":"DTR6Z5MLSMHSJR4U","created_at":"2026-05-18T12:29:17.054201+00:00"},{"alias_kind":"pith_short_8","alias_value":"DTR6Z5ML","created_at":"2026-05-18T12:29:17.054201+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/DTR6Z5MLSMHSJR4UOYE3NUA53N","json":"https://pith.science/pith/DTR6Z5MLSMHSJR4UOYE3NUA53N.json","graph_json":"https://pith.science/api/pith-number/DTR6Z5MLSMHSJR4UOYE3NUA53N/graph.json","events_json":"https://pith.science/api/pith-number/DTR6Z5MLSMHSJR4UOYE3NUA53N/events.json","paper":"https://pith.science/paper/DTR6Z5ML"},"agent_actions":{"view_html":"https://pith.science/pith/DTR6Z5MLSMHSJR4UOYE3NUA53N","download_json":"https://pith.science/pith/DTR6Z5MLSMHSJR4UOYE3NUA53N.json","view_paper":"https://pith.science/paper/DTR6Z5ML","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1504.03401&json=true","fetch_graph":"https://pith.science/api/pith-number/DTR6Z5MLSMHSJR4UOYE3NUA53N/graph.json","fetch_events":"https://pith.science/api/pith-number/DTR6Z5MLSMHSJR4UOYE3NUA53N/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/DTR6Z5MLSMHSJR4UOYE3NUA53N/action/timestamp_anchor","attest_storage":"https://pith.science/pith/DTR6Z5MLSMHSJR4UOYE3NUA53N/action/storage_attestation","attest_author":"https://pith.science/pith/DTR6Z5MLSMHSJR4UOYE3NUA53N/action/author_attestation","sign_citation":"https://pith.science/pith/DTR6Z5MLSMHSJR4UOYE3NUA53N/action/citation_signature","submit_replication":"https://pith.science/pith/DTR6Z5MLSMHSJR4UOYE3NUA53N/action/replication_record"}},"created_at":"2026-05-18T02:18:52.284243+00:00","updated_at":"2026-05-18T02:18:52.284243+00:00"}