{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2016:EAJIELSRSCMABIMPS2ND5QEINM","short_pith_number":"pith:EAJIELSR","schema_version":"1.0","canonical_sha256":"2012822e51909800a18f969a3ec0886b1f1119527749dfba89d2f0e7911371d0","source":{"kind":"arxiv","id":"1605.02656","version":1},"attestation_state":"computed","paper":{"title":"Dynamical analysis of the cluster pair: A3407 + A3408","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"A.L.B. Ribeiro, E. R. Carrasco, H. Plana, M. Trevisan, R. Dupke, R.S. Nascimento","submitted_at":"2016-05-09T16:56:52Z","abstract_excerpt":"We carried out a dynamical study of the galaxy cluster pair A3407 \\& A3408 based on a spectroscopic survey obtained with the 4 meter Blanco telescope at the CTIO, plus 6dF data, and ROSAT All-Sky-Survey. The sample consists of 122 member galaxies brighter than $m_R=20$. Our main goal is to probe the galaxy dynamics in this field and verify if the sample constitutes a single galaxy system or corresponds to an ongoing merging process. Statistical tests were applied to clusters members showing that both the composite system A3407 + A3408 as well as each individual cluster have Gaussian velocity d"},"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":"1605.02656","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2016-05-09T16:56:52Z","cross_cats_sorted":[],"title_canon_sha256":"c687c75f64e57d4360166455bf3110ab6efa092b95536b03f110b2ac1c35c857","abstract_canon_sha256":"0d4efd11eccf29cde96059f71ebd3bd553fa8fa390b66b512b500f68956e0c74"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:10:30.192822Z","signature_b64":"FFNV+URNG978uHu1QHZP4zL66fGhtnnaGiDkarv9ZkFqNli8UCtsCHY5HwuO7ItU3faYBzj8fti4PrfO3H/cBA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"2012822e51909800a18f969a3ec0886b1f1119527749dfba89d2f0e7911371d0","last_reissued_at":"2026-05-18T01:10:30.192374Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:10:30.192374Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Dynamical analysis of the cluster pair: A3407 + A3408","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"A.L.B. Ribeiro, E. R. Carrasco, H. Plana, M. Trevisan, R. Dupke, R.S. Nascimento","submitted_at":"2016-05-09T16:56:52Z","abstract_excerpt":"We carried out a dynamical study of the galaxy cluster pair A3407 \\& A3408 based on a spectroscopic survey obtained with the 4 meter Blanco telescope at the CTIO, plus 6dF data, and ROSAT All-Sky-Survey. The sample consists of 122 member galaxies brighter than $m_R=20$. Our main goal is to probe the galaxy dynamics in this field and verify if the sample constitutes a single galaxy system or corresponds to an ongoing merging process. Statistical tests were applied to clusters members showing that both the composite system A3407 + A3408 as well as each individual cluster have Gaussian velocity d"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1605.02656","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":"1605.02656","created_at":"2026-05-18T01:10:30.192446+00:00"},{"alias_kind":"arxiv_version","alias_value":"1605.02656v1","created_at":"2026-05-18T01:10:30.192446+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1605.02656","created_at":"2026-05-18T01:10:30.192446+00:00"},{"alias_kind":"pith_short_12","alias_value":"EAJIELSRSCMA","created_at":"2026-05-18T12:30:12.583610+00:00"},{"alias_kind":"pith_short_16","alias_value":"EAJIELSRSCMABIMP","created_at":"2026-05-18T12:30:12.583610+00:00"},{"alias_kind":"pith_short_8","alias_value":"EAJIELSR","created_at":"2026-05-18T12:30:12.583610+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/EAJIELSRSCMABIMPS2ND5QEINM","json":"https://pith.science/pith/EAJIELSRSCMABIMPS2ND5QEINM.json","graph_json":"https://pith.science/api/pith-number/EAJIELSRSCMABIMPS2ND5QEINM/graph.json","events_json":"https://pith.science/api/pith-number/EAJIELSRSCMABIMPS2ND5QEINM/events.json","paper":"https://pith.science/paper/EAJIELSR"},"agent_actions":{"view_html":"https://pith.science/pith/EAJIELSRSCMABIMPS2ND5QEINM","download_json":"https://pith.science/pith/EAJIELSRSCMABIMPS2ND5QEINM.json","view_paper":"https://pith.science/paper/EAJIELSR","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1605.02656&json=true","fetch_graph":"https://pith.science/api/pith-number/EAJIELSRSCMABIMPS2ND5QEINM/graph.json","fetch_events":"https://pith.science/api/pith-number/EAJIELSRSCMABIMPS2ND5QEINM/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/EAJIELSRSCMABIMPS2ND5QEINM/action/timestamp_anchor","attest_storage":"https://pith.science/pith/EAJIELSRSCMABIMPS2ND5QEINM/action/storage_attestation","attest_author":"https://pith.science/pith/EAJIELSRSCMABIMPS2ND5QEINM/action/author_attestation","sign_citation":"https://pith.science/pith/EAJIELSRSCMABIMPS2ND5QEINM/action/citation_signature","submit_replication":"https://pith.science/pith/EAJIELSRSCMABIMPS2ND5QEINM/action/replication_record"}},"created_at":"2026-05-18T01:10:30.192446+00:00","updated_at":"2026-05-18T01:10:30.192446+00:00"}