{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2016:B6NNPD2FZFSKGD5BYPYUAFOOYT","short_pith_number":"pith:B6NNPD2F","schema_version":"1.0","canonical_sha256":"0f9ad78f45c964a30fa1c3f14015cec4ef8ad9825c9a666d58dd321b862258c9","source":{"kind":"arxiv","id":"1605.07595","version":2},"attestation_state":"computed","paper":{"title":"The merger history of the complex cluster Abell 1758: a combined weak lensing and spectroscopic view","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.GA"],"primary_cat":"astro-ph.CO","authors_text":"Andr\\'e L. B. Ribeiro, Eduardo S. Cypriano, Gast\\~ao B. Lima-Neto, Laerte Sodr\\'e Jr, Renato A. Dupke, Rog\\'erio Monteiro-Oliveira, Rubens E. G. Machado","submitted_at":"2016-05-24T19:33:25Z","abstract_excerpt":"We present a weak-lensing and dynamical study of the complex cluster Abell 1758 (A1758, z = 0.278) supported by hydrodynamical simulations. This cluster is composed of two main structures, called A1758N and A1758S. The Northern structure is composed of A1758NW & A1758NE, with lensing determined masses of 7.90_{-1.55}^{+1.89} X 10^{14} M_\\odot and 5.49_{-1.33}^{+1.67} X 10^{14} M_\\odot, respectively. They show a remarkable feature: while in A1758NW there is a spatial agreement among weak lensing mass distribution, intracluster medium and its brightest cluster galaxy (BCG) in A1758NE the X-ray p"},"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":"1605.07595","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2016-05-24T19:33:25Z","cross_cats_sorted":["astro-ph.GA"],"title_canon_sha256":"ff9777c92a7c48a70edc00764ac682a782dc2b7e84249e6d3a607e77abd68fa1","abstract_canon_sha256":"adc7b36b512a9fa3ed902cba35079166ab325d56f9074627476c8d542fcb599f"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:52:17.215224Z","signature_b64":"793L2L9YiX0CIOiRopmTVk0MBI82G9WiLN2xMwsvZwvqqWdUYrMji+KU5SVYi5LaQi91kC7ZRP+Iq6ByYO/wBw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"0f9ad78f45c964a30fa1c3f14015cec4ef8ad9825c9a666d58dd321b862258c9","last_reissued_at":"2026-05-18T00:52:17.214722Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:52:17.214722Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The merger history of the complex cluster Abell 1758: a combined weak lensing and spectroscopic view","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.GA"],"primary_cat":"astro-ph.CO","authors_text":"Andr\\'e L. B. Ribeiro, Eduardo S. Cypriano, Gast\\~ao B. Lima-Neto, Laerte Sodr\\'e Jr, Renato A. Dupke, Rog\\'erio Monteiro-Oliveira, Rubens E. G. Machado","submitted_at":"2016-05-24T19:33:25Z","abstract_excerpt":"We present a weak-lensing and dynamical study of the complex cluster Abell 1758 (A1758, z = 0.278) supported by hydrodynamical simulations. This cluster is composed of two main structures, called A1758N and A1758S. The Northern structure is composed of A1758NW & A1758NE, with lensing determined masses of 7.90_{-1.55}^{+1.89} X 10^{14} M_\\odot and 5.49_{-1.33}^{+1.67} X 10^{14} M_\\odot, respectively. They show a remarkable feature: while in A1758NW there is a spatial agreement among weak lensing mass distribution, intracluster medium and its brightest cluster galaxy (BCG) in A1758NE the X-ray p"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1605.07595","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":"1605.07595","created_at":"2026-05-18T00:52:17.214808+00:00"},{"alias_kind":"arxiv_version","alias_value":"1605.07595v2","created_at":"2026-05-18T00:52:17.214808+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1605.07595","created_at":"2026-05-18T00:52:17.214808+00:00"},{"alias_kind":"pith_short_12","alias_value":"B6NNPD2FZFSK","created_at":"2026-05-18T12:30:07.202191+00:00"},{"alias_kind":"pith_short_16","alias_value":"B6NNPD2FZFSKGD5B","created_at":"2026-05-18T12:30:07.202191+00:00"},{"alias_kind":"pith_short_8","alias_value":"B6NNPD2F","created_at":"2026-05-18T12:30:07.202191+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/B6NNPD2FZFSKGD5BYPYUAFOOYT","json":"https://pith.science/pith/B6NNPD2FZFSKGD5BYPYUAFOOYT.json","graph_json":"https://pith.science/api/pith-number/B6NNPD2FZFSKGD5BYPYUAFOOYT/graph.json","events_json":"https://pith.science/api/pith-number/B6NNPD2FZFSKGD5BYPYUAFOOYT/events.json","paper":"https://pith.science/paper/B6NNPD2F"},"agent_actions":{"view_html":"https://pith.science/pith/B6NNPD2FZFSKGD5BYPYUAFOOYT","download_json":"https://pith.science/pith/B6NNPD2FZFSKGD5BYPYUAFOOYT.json","view_paper":"https://pith.science/paper/B6NNPD2F","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1605.07595&json=true","fetch_graph":"https://pith.science/api/pith-number/B6NNPD2FZFSKGD5BYPYUAFOOYT/graph.json","fetch_events":"https://pith.science/api/pith-number/B6NNPD2FZFSKGD5BYPYUAFOOYT/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/B6NNPD2FZFSKGD5BYPYUAFOOYT/action/timestamp_anchor","attest_storage":"https://pith.science/pith/B6NNPD2FZFSKGD5BYPYUAFOOYT/action/storage_attestation","attest_author":"https://pith.science/pith/B6NNPD2FZFSKGD5BYPYUAFOOYT/action/author_attestation","sign_citation":"https://pith.science/pith/B6NNPD2FZFSKGD5BYPYUAFOOYT/action/citation_signature","submit_replication":"https://pith.science/pith/B6NNPD2FZFSKGD5BYPYUAFOOYT/action/replication_record"}},"created_at":"2026-05-18T00:52:17.214808+00:00","updated_at":"2026-05-18T00:52:17.214808+00:00"}