{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2000:64OUYGJF66FAQQXSCPDIHPB2XO","short_pith_number":"pith:64OUYGJF","schema_version":"1.0","canonical_sha256":"f71d4c1925f78a0842f213c683bc3abb81a6b36a9f06e532d6f57c83d43c863a","source":{"kind":"arxiv","id":"astro-ph/0006366","version":1},"attestation_state":"computed","paper":{"title":"Cluster Tempreature Evolution: The Mass-Temperature Relation","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"G. M. Voit (STScI)","submitted_at":"2000-06-26T16:07:00Z","abstract_excerpt":"Evolution of the cluster temperature function is extremely sensitive to the mean matter density of the universe. Current measurements based on cluster temperature surveys indicate that Omega_M ~ 0.3 with a 1-sigma statistical error ~0.1, but the systematic errors in this method are of comparable size. Many more high-z cluster temperatures will be arriving from Chandra and XMM in the near future. In preparation for future cluster temperature surveys, this paper analyses the cluster mass-temperature relation, with the intention of identifying and reducing the systematic errors it introduces into"},"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":"astro-ph/0006366","kind":"arxiv","version":1},"metadata":{"license":"","primary_cat":"astro-ph","submitted_at":"2000-06-26T16:07:00Z","cross_cats_sorted":[],"title_canon_sha256":"3656a344a8867b972669f5ed5c3d0283c4566f8c0a8f453ed7330ba61fc025f7","abstract_canon_sha256":"776dd8976235b8d42229db802fcf6b5f2abce7c23bde7a3d662b46e8b8eceaf3"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-04T16:16:49.955789Z","signature_b64":"o06PWeSIPcagNCw6RHA3TG7TaSIaJXTHtsfv6LgblIEQ2bIAPabypjHXEWk1mY9BdMSSUJHF0KIj/Mrl4vtfAw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"f71d4c1925f78a0842f213c683bc3abb81a6b36a9f06e532d6f57c83d43c863a","last_reissued_at":"2026-07-04T16:16:49.955394Z","signature_status":"signed_v1","first_computed_at":"2026-07-04T16:16:49.955394Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Cluster Tempreature Evolution: The Mass-Temperature Relation","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"G. M. Voit (STScI)","submitted_at":"2000-06-26T16:07:00Z","abstract_excerpt":"Evolution of the cluster temperature function is extremely sensitive to the mean matter density of the universe. Current measurements based on cluster temperature surveys indicate that Omega_M ~ 0.3 with a 1-sigma statistical error ~0.1, but the systematic errors in this method are of comparable size. Many more high-z cluster temperatures will be arriving from Chandra and XMM in the near future. In preparation for future cluster temperature surveys, this paper analyses the cluster mass-temperature relation, with the intention of identifying and reducing the systematic errors it introduces into"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"astro-ph/0006366","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/astro-ph/0006366/integrity.json","findings":[],"available":true,"detectors_run":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938"},"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":"astro-ph/0006366","created_at":"2026-07-04T16:16:49.955450+00:00"},{"alias_kind":"arxiv_version","alias_value":"astro-ph/0006366v1","created_at":"2026-07-04T16:16:49.955450+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.astro-ph/0006366","created_at":"2026-07-04T16:16:49.955450+00:00"},{"alias_kind":"pith_short_12","alias_value":"64OUYGJF66FA","created_at":"2026-07-04T16:16:49.955450+00:00"},{"alias_kind":"pith_short_16","alias_value":"64OUYGJF66FAQQXS","created_at":"2026-07-04T16:16:49.955450+00:00"},{"alias_kind":"pith_short_8","alias_value":"64OUYGJF","created_at":"2026-07-04T16:16:49.955450+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"1908.07322","citing_title":"Mass-Temperature relation in $\\Lambda$CDM and modified gravity","ref_index":91,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/64OUYGJF66FAQQXSCPDIHPB2XO","json":"https://pith.science/pith/64OUYGJF66FAQQXSCPDIHPB2XO.json","graph_json":"https://pith.science/api/pith-number/64OUYGJF66FAQQXSCPDIHPB2XO/graph.json","events_json":"https://pith.science/api/pith-number/64OUYGJF66FAQQXSCPDIHPB2XO/events.json","paper":"https://pith.science/paper/64OUYGJF"},"agent_actions":{"view_html":"https://pith.science/pith/64OUYGJF66FAQQXSCPDIHPB2XO","download_json":"https://pith.science/pith/64OUYGJF66FAQQXSCPDIHPB2XO.json","view_paper":"https://pith.science/paper/64OUYGJF","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=astro-ph/0006366&json=true","fetch_graph":"https://pith.science/api/pith-number/64OUYGJF66FAQQXSCPDIHPB2XO/graph.json","fetch_events":"https://pith.science/api/pith-number/64OUYGJF66FAQQXSCPDIHPB2XO/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/64OUYGJF66FAQQXSCPDIHPB2XO/action/timestamp_anchor","attest_storage":"https://pith.science/pith/64OUYGJF66FAQQXSCPDIHPB2XO/action/storage_attestation","attest_author":"https://pith.science/pith/64OUYGJF66FAQQXSCPDIHPB2XO/action/author_attestation","sign_citation":"https://pith.science/pith/64OUYGJF66FAQQXSCPDIHPB2XO/action/citation_signature","submit_replication":"https://pith.science/pith/64OUYGJF66FAQQXSCPDIHPB2XO/action/replication_record"}},"created_at":"2026-07-04T16:16:49.955450+00:00","updated_at":"2026-07-04T16:16:49.955450+00:00"}