{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2012:TDWUICMLVJ7XESYYCZC7C7R3AX","short_pith_number":"pith:TDWUICML","schema_version":"1.0","canonical_sha256":"98ed44098baa7f724b181645f17e3b05f5e73443f40e7ce062472dff1f0d01b4","source":{"kind":"arxiv","id":"1210.6571","version":2},"attestation_state":"computed","paper":{"title":"Low Density Structures in the Local Universe. I. Diffuse Agglomerates of Galaxies","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"A. A. Elyiv, D. I. Makarov, I. D. Karachentsev, O. V. Melnyk, V. E. Karachentseva","submitted_at":"2012-10-24T15:24:25Z","abstract_excerpt":"This paper is the first of a series considering the properties of distribution of nearby galaxies in the low density regions. Among 7596 galaxies with radial velocities V_{LG}<3500 km/s, absolute magnitudes M_K<-18.4^m$, and Galactic latitudes |b| >15 degr there are 3168 field galaxies (i.e. 42%) that do not belong to pairs, groups or clusters in the Local universe. Applying to this sample the percolation method with a radius of r_0=2.8 Mpc, we found 226 diffuse agglomerates with n>=4 number of members. The structures of eight most populated objects among them (n>=25) are discussed. These non-"},"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":"1210.6571","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2012-10-24T15:24:25Z","cross_cats_sorted":[],"title_canon_sha256":"1e740bc90cde7c7ec8d344d34a0718f62941707617ad4a35d16f004daaeac664","abstract_canon_sha256":"a5ed6c00aa8f61b8d7e5fe150c96bd61dce8971476d103f1612bb8717ab0f96e"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:53:43.662541Z","signature_b64":"+oyidQ4r/5Or7sW63M3iDMrfW849mqgYLBaMd1SU/LugfEcgQjnoo/OlJxMp2mMOXEx4elMI+ErCXI57PHTkCQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"98ed44098baa7f724b181645f17e3b05f5e73443f40e7ce062472dff1f0d01b4","last_reissued_at":"2026-05-18T01:53:43.661941Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:53:43.661941Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Low Density Structures in the Local Universe. I. Diffuse Agglomerates of Galaxies","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"A. A. Elyiv, D. I. Makarov, I. D. Karachentsev, O. V. Melnyk, V. E. Karachentseva","submitted_at":"2012-10-24T15:24:25Z","abstract_excerpt":"This paper is the first of a series considering the properties of distribution of nearby galaxies in the low density regions. Among 7596 galaxies with radial velocities V_{LG}<3500 km/s, absolute magnitudes M_K<-18.4^m$, and Galactic latitudes |b| >15 degr there are 3168 field galaxies (i.e. 42%) that do not belong to pairs, groups or clusters in the Local universe. Applying to this sample the percolation method with a radius of r_0=2.8 Mpc, we found 226 diffuse agglomerates with n>=4 number of members. The structures of eight most populated objects among them (n>=25) are discussed. These non-"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1210.6571","kind":"arxiv","version":2},"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":"1210.6571","created_at":"2026-05-18T01:53:43.662024+00:00"},{"alias_kind":"arxiv_version","alias_value":"1210.6571v2","created_at":"2026-05-18T01:53:43.662024+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1210.6571","created_at":"2026-05-18T01:53:43.662024+00:00"},{"alias_kind":"pith_short_12","alias_value":"TDWUICMLVJ7X","created_at":"2026-05-18T12:27:23.164592+00:00"},{"alias_kind":"pith_short_16","alias_value":"TDWUICMLVJ7XESYY","created_at":"2026-05-18T12:27:23.164592+00:00"},{"alias_kind":"pith_short_8","alias_value":"TDWUICML","created_at":"2026-05-18T12:27:23.164592+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/TDWUICMLVJ7XESYYCZC7C7R3AX","json":"https://pith.science/pith/TDWUICMLVJ7XESYYCZC7C7R3AX.json","graph_json":"https://pith.science/api/pith-number/TDWUICMLVJ7XESYYCZC7C7R3AX/graph.json","events_json":"https://pith.science/api/pith-number/TDWUICMLVJ7XESYYCZC7C7R3AX/events.json","paper":"https://pith.science/paper/TDWUICML"},"agent_actions":{"view_html":"https://pith.science/pith/TDWUICMLVJ7XESYYCZC7C7R3AX","download_json":"https://pith.science/pith/TDWUICMLVJ7XESYYCZC7C7R3AX.json","view_paper":"https://pith.science/paper/TDWUICML","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1210.6571&json=true","fetch_graph":"https://pith.science/api/pith-number/TDWUICMLVJ7XESYYCZC7C7R3AX/graph.json","fetch_events":"https://pith.science/api/pith-number/TDWUICMLVJ7XESYYCZC7C7R3AX/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/TDWUICMLVJ7XESYYCZC7C7R3AX/action/timestamp_anchor","attest_storage":"https://pith.science/pith/TDWUICMLVJ7XESYYCZC7C7R3AX/action/storage_attestation","attest_author":"https://pith.science/pith/TDWUICMLVJ7XESYYCZC7C7R3AX/action/author_attestation","sign_citation":"https://pith.science/pith/TDWUICMLVJ7XESYYCZC7C7R3AX/action/citation_signature","submit_replication":"https://pith.science/pith/TDWUICMLVJ7XESYYCZC7C7R3AX/action/replication_record"}},"created_at":"2026-05-18T01:53:43.662024+00:00","updated_at":"2026-05-18T01:53:43.662024+00:00"}