{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2026:LZ3A5BX55WAWUS32YNJ5TEEFON","short_pith_number":"pith:LZ3A5BX5","schema_version":"1.0","canonical_sha256":"5e760e86fded816a4b7ac353d99085737317bdb8d232b36923355b6354575272","source":{"kind":"arxiv","id":"2606.03342","version":1},"attestation_state":"computed","paper":{"title":"The caustic method applied to The Three Hundred: prospects for upcoming CATARSIS and other surveys","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["astro-ph.GA"],"primary_cat":"astro-ph.CO","authors_text":"A. Gil de Paz, A. Knebe, B. Callejas C\\'ordoba, C. Catal\\'an Torrecilla, P. S\\'anchez Bl\\'azquez, R. Dave, W. Cui","submitted_at":"2026-06-02T08:53:06Z","abstract_excerpt":"We investigate the expected uncertainties in recovering galaxy cluster mass profiles from upcoming spectroscopic survey data using The Three Hundred Project. Using the caustic technique, which leverages galaxy positions and line-of-sight velocities, we assess the systematic errors introduced by assumptions regarding velocity anisotropy and demonstrate how an iterative correction method can minimize these errors. We also assess the impact of survey magnitude limits on cluster mass estimates, highlighting potential biases across different observational strategies. We focus the analysis on our ow"},"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":"2606.03342","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.CO","submitted_at":"2026-06-02T08:53:06Z","cross_cats_sorted":["astro-ph.GA"],"title_canon_sha256":"06dbcd0c83216186cf2f511107659b8d78a1ae72ff9091ab8bdceac259c33059","abstract_canon_sha256":"f26fb0b021de6a574722537a745913591e9a8d3ea1827f887e1d0cf3d1b5bcb1"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-06-03T01:05:55.491006Z","signature_b64":"YMiJAIUqwYiNpEL4An7VZhXCKpgXUcfLks0TsQgTt5CjtvXUiYBclGAi7iyDxQdpiQORNa5QnX29DIiIYdy9DQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"5e760e86fded816a4b7ac353d99085737317bdb8d232b36923355b6354575272","last_reissued_at":"2026-06-03T01:05:55.490593Z","signature_status":"signed_v1","first_computed_at":"2026-06-03T01:05:55.490593Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The caustic method applied to The Three Hundred: prospects for upcoming CATARSIS and other surveys","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["astro-ph.GA"],"primary_cat":"astro-ph.CO","authors_text":"A. Gil de Paz, A. Knebe, B. Callejas C\\'ordoba, C. Catal\\'an Torrecilla, P. S\\'anchez Bl\\'azquez, R. Dave, W. Cui","submitted_at":"2026-06-02T08:53:06Z","abstract_excerpt":"We investigate the expected uncertainties in recovering galaxy cluster mass profiles from upcoming spectroscopic survey data using The Three Hundred Project. Using the caustic technique, which leverages galaxy positions and line-of-sight velocities, we assess the systematic errors introduced by assumptions regarding velocity anisotropy and demonstrate how an iterative correction method can minimize these errors. We also assess the impact of survey magnitude limits on cluster mass estimates, highlighting potential biases across different observational strategies. We focus the analysis on our ow"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2606.03342","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/2606.03342/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":"2606.03342","created_at":"2026-06-03T01:05:55.490651+00:00"},{"alias_kind":"arxiv_version","alias_value":"2606.03342v1","created_at":"2026-06-03T01:05:55.490651+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2606.03342","created_at":"2026-06-03T01:05:55.490651+00:00"},{"alias_kind":"pith_short_12","alias_value":"LZ3A5BX55WAW","created_at":"2026-06-03T01:05:55.490651+00:00"},{"alias_kind":"pith_short_16","alias_value":"LZ3A5BX55WAWUS32","created_at":"2026-06-03T01:05:55.490651+00:00"},{"alias_kind":"pith_short_8","alias_value":"LZ3A5BX5","created_at":"2026-06-03T01:05:55.490651+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/LZ3A5BX55WAWUS32YNJ5TEEFON","json":"https://pith.science/pith/LZ3A5BX55WAWUS32YNJ5TEEFON.json","graph_json":"https://pith.science/api/pith-number/LZ3A5BX55WAWUS32YNJ5TEEFON/graph.json","events_json":"https://pith.science/api/pith-number/LZ3A5BX55WAWUS32YNJ5TEEFON/events.json","paper":"https://pith.science/paper/LZ3A5BX5"},"agent_actions":{"view_html":"https://pith.science/pith/LZ3A5BX55WAWUS32YNJ5TEEFON","download_json":"https://pith.science/pith/LZ3A5BX55WAWUS32YNJ5TEEFON.json","view_paper":"https://pith.science/paper/LZ3A5BX5","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2606.03342&json=true","fetch_graph":"https://pith.science/api/pith-number/LZ3A5BX55WAWUS32YNJ5TEEFON/graph.json","fetch_events":"https://pith.science/api/pith-number/LZ3A5BX55WAWUS32YNJ5TEEFON/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/LZ3A5BX55WAWUS32YNJ5TEEFON/action/timestamp_anchor","attest_storage":"https://pith.science/pith/LZ3A5BX55WAWUS32YNJ5TEEFON/action/storage_attestation","attest_author":"https://pith.science/pith/LZ3A5BX55WAWUS32YNJ5TEEFON/action/author_attestation","sign_citation":"https://pith.science/pith/LZ3A5BX55WAWUS32YNJ5TEEFON/action/citation_signature","submit_replication":"https://pith.science/pith/LZ3A5BX55WAWUS32YNJ5TEEFON/action/replication_record"}},"created_at":"2026-06-03T01:05:55.490651+00:00","updated_at":"2026-06-03T01:05:55.490651+00:00"}