{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2016:TGLWYZIKHTPK5VPAFIRGE5F322","short_pith_number":"pith:TGLWYZIK","schema_version":"1.0","canonical_sha256":"99976c650a3cdeaed5e02a226274bbd6ac4d5db83bfc90aa5c1bc3443cd5b002","source":{"kind":"arxiv","id":"1608.07417","version":1},"attestation_state":"computed","paper":{"title":"Probing the dynamical and X-ray mass proxies of the cluster of galaxies Abell S1101","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.GA"],"primary_cat":"astro-ph.CO","authors_text":"Andreas Rabitz, Axel Schwope, Matthias Klein, Miguel Verdugo, Thomas H. Reiprich, Yu-Ying Zhang","submitted_at":"2016-08-26T10:28:13Z","abstract_excerpt":"Context: The galaxy cluster Abell S1101 (S1101 hereafter) deviates significantly from the X-ray luminosity versus velocity dispersion relation (L-sigma) of galaxy clusters in our previous study. Given reliable X-ray luminosity measurement combining XMM-Newton and ROSAT, this could most likely be caused by the bias in the velocity dispersion due to interlopers and low member statistic in the previous sample of member galaxies, which was solely based on 20 galaxy redshifts drawn from the literature. Aims: We intend to increase the galaxy member statistic to perform a precision measurement of the"},"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":"1608.07417","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2016-08-26T10:28:13Z","cross_cats_sorted":["astro-ph.GA"],"title_canon_sha256":"44b3c3ba12c48fc8db524c1090dc8facc5183e7863168119dbcc9599b787524e","abstract_canon_sha256":"256bec9c6113c58724ddf0e8aa3eb18d3920f2f6d5af0c8159b22750274e6338"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:54:19.731592Z","signature_b64":"ANikBDR9HtxTWtZZ0qSP4O2qwTxRjaUy0U/qnlpNTJ6S+njZSUVFitkbMxI4D6jWMdlRss7vj+RlJL5mw/0FCQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"99976c650a3cdeaed5e02a226274bbd6ac4d5db83bfc90aa5c1bc3443cd5b002","last_reissued_at":"2026-05-18T00:54:19.731142Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:54:19.731142Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Probing the dynamical and X-ray mass proxies of the cluster of galaxies Abell S1101","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.GA"],"primary_cat":"astro-ph.CO","authors_text":"Andreas Rabitz, Axel Schwope, Matthias Klein, Miguel Verdugo, Thomas H. Reiprich, Yu-Ying Zhang","submitted_at":"2016-08-26T10:28:13Z","abstract_excerpt":"Context: The galaxy cluster Abell S1101 (S1101 hereafter) deviates significantly from the X-ray luminosity versus velocity dispersion relation (L-sigma) of galaxy clusters in our previous study. Given reliable X-ray luminosity measurement combining XMM-Newton and ROSAT, this could most likely be caused by the bias in the velocity dispersion due to interlopers and low member statistic in the previous sample of member galaxies, which was solely based on 20 galaxy redshifts drawn from the literature. Aims: We intend to increase the galaxy member statistic to perform a precision measurement of the"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1608.07417","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":"1608.07417","created_at":"2026-05-18T00:54:19.731211+00:00"},{"alias_kind":"arxiv_version","alias_value":"1608.07417v1","created_at":"2026-05-18T00:54:19.731211+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1608.07417","created_at":"2026-05-18T00:54:19.731211+00:00"},{"alias_kind":"pith_short_12","alias_value":"TGLWYZIKHTPK","created_at":"2026-05-18T12:30:44.179134+00:00"},{"alias_kind":"pith_short_16","alias_value":"TGLWYZIKHTPK5VPA","created_at":"2026-05-18T12:30:44.179134+00:00"},{"alias_kind":"pith_short_8","alias_value":"TGLWYZIK","created_at":"2026-05-18T12:30:44.179134+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/TGLWYZIKHTPK5VPAFIRGE5F322","json":"https://pith.science/pith/TGLWYZIKHTPK5VPAFIRGE5F322.json","graph_json":"https://pith.science/api/pith-number/TGLWYZIKHTPK5VPAFIRGE5F322/graph.json","events_json":"https://pith.science/api/pith-number/TGLWYZIKHTPK5VPAFIRGE5F322/events.json","paper":"https://pith.science/paper/TGLWYZIK"},"agent_actions":{"view_html":"https://pith.science/pith/TGLWYZIKHTPK5VPAFIRGE5F322","download_json":"https://pith.science/pith/TGLWYZIKHTPK5VPAFIRGE5F322.json","view_paper":"https://pith.science/paper/TGLWYZIK","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1608.07417&json=true","fetch_graph":"https://pith.science/api/pith-number/TGLWYZIKHTPK5VPAFIRGE5F322/graph.json","fetch_events":"https://pith.science/api/pith-number/TGLWYZIKHTPK5VPAFIRGE5F322/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/TGLWYZIKHTPK5VPAFIRGE5F322/action/timestamp_anchor","attest_storage":"https://pith.science/pith/TGLWYZIKHTPK5VPAFIRGE5F322/action/storage_attestation","attest_author":"https://pith.science/pith/TGLWYZIKHTPK5VPAFIRGE5F322/action/author_attestation","sign_citation":"https://pith.science/pith/TGLWYZIKHTPK5VPAFIRGE5F322/action/citation_signature","submit_replication":"https://pith.science/pith/TGLWYZIKHTPK5VPAFIRGE5F322/action/replication_record"}},"created_at":"2026-05-18T00:54:19.731211+00:00","updated_at":"2026-05-18T00:54:19.731211+00:00"}