{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2022:346LWYI645RXIVRBFEPN52MZP7","short_pith_number":"pith:346LWYI6","schema_version":"1.0","canonical_sha256":"df3cbb611ee763745621291edee9997fc0e0856c7a90ff31449c99c3058292dd","source":{"kind":"arxiv","id":"2205.11326","version":2},"attestation_state":"computed","paper":{"title":"CHEX-MATE: Morphological analysis of the sample","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"Ben Maughan, Dominique Eckert, Elena Rasia, Etienne Pointecouteau, Fabio Gastaldello, Federico De Luca, Gabriel W. Pratt, Iacopo Bartalucci, Lorenzo Lovisari, Marco De Petris, Mariachiara Rossetti, Maria Giulia Campitiello, Massimo Gaspari, Mauro Sereno, Pasquale Mazzotta, Silvano Molendi, Simona Ghizzardi, Stefano Borgani, Stefano Ettori, Veronica Biffi","submitted_at":"2022-05-23T14:15:14Z","abstract_excerpt":"In this work, we performed an analysis of the X-ray morphology of the 118 CHEX-MATE (Cluster HEritage project with XMM-Newton - Mass Assembly and Thermodynamics at the Endpoint of structure formation) galaxy clusters, with the aim to provide a classification of their dynamical state. To investigate the link between the X-ray appearance and the dynamical state, we considered four morphological parameters: the surface brightness concentration, the centroid shift, and the second- and third-order power ratios. These indicators result to be: strongly correlated with each other, powerful in identify"},"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":"2205.11326","kind":"arxiv","version":2},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.CO","submitted_at":"2022-05-23T14:15:14Z","cross_cats_sorted":[],"title_canon_sha256":"72202da1031f077dc8aab4e334b371831644ac918ac87e1b6516d2621e100134","abstract_canon_sha256":"b9ad8e58a70b23e3944c3eeecbe3cadf5133786d3fa58b03746b7be2e5a72474"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T04:59:24.145384Z","signature_b64":"3wMaHQLlPqFs9DOF7xPw1UyLsrUxJe6rB91s9/ISlb5tQ62qj/c7qLaYyMib/x7L88k0dce22wdDeoCPiDsPBg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"df3cbb611ee763745621291edee9997fc0e0856c7a90ff31449c99c3058292dd","last_reissued_at":"2026-07-05T04:59:24.144923Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T04:59:24.144923Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"CHEX-MATE: Morphological analysis of the sample","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"Ben Maughan, Dominique Eckert, Elena Rasia, Etienne Pointecouteau, Fabio Gastaldello, Federico De Luca, Gabriel W. Pratt, Iacopo Bartalucci, Lorenzo Lovisari, Marco De Petris, Mariachiara Rossetti, Maria Giulia Campitiello, Massimo Gaspari, Mauro Sereno, Pasquale Mazzotta, Silvano Molendi, Simona Ghizzardi, Stefano Borgani, Stefano Ettori, Veronica Biffi","submitted_at":"2022-05-23T14:15:14Z","abstract_excerpt":"In this work, we performed an analysis of the X-ray morphology of the 118 CHEX-MATE (Cluster HEritage project with XMM-Newton - Mass Assembly and Thermodynamics at the Endpoint of structure formation) galaxy clusters, with the aim to provide a classification of their dynamical state. To investigate the link between the X-ray appearance and the dynamical state, we considered four morphological parameters: the surface brightness concentration, the centroid shift, and the second- and third-order power ratios. These indicators result to be: strongly correlated with each other, powerful in identify"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2205.11326","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2205.11326/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":"2205.11326","created_at":"2026-07-05T04:59:24.144980+00:00"},{"alias_kind":"arxiv_version","alias_value":"2205.11326v2","created_at":"2026-07-05T04:59:24.144980+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2205.11326","created_at":"2026-07-05T04:59:24.144980+00:00"},{"alias_kind":"pith_short_12","alias_value":"346LWYI645RX","created_at":"2026-07-05T04:59:24.144980+00:00"},{"alias_kind":"pith_short_16","alias_value":"346LWYI645RXIVRB","created_at":"2026-07-05T04:59:24.144980+00:00"},{"alias_kind":"pith_short_8","alias_value":"346LWYI6","created_at":"2026-07-05T04:59:24.144980+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/346LWYI645RXIVRBFEPN52MZP7","json":"https://pith.science/pith/346LWYI645RXIVRBFEPN52MZP7.json","graph_json":"https://pith.science/api/pith-number/346LWYI645RXIVRBFEPN52MZP7/graph.json","events_json":"https://pith.science/api/pith-number/346LWYI645RXIVRBFEPN52MZP7/events.json","paper":"https://pith.science/paper/346LWYI6"},"agent_actions":{"view_html":"https://pith.science/pith/346LWYI645RXIVRBFEPN52MZP7","download_json":"https://pith.science/pith/346LWYI645RXIVRBFEPN52MZP7.json","view_paper":"https://pith.science/paper/346LWYI6","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2205.11326&json=true","fetch_graph":"https://pith.science/api/pith-number/346LWYI645RXIVRBFEPN52MZP7/graph.json","fetch_events":"https://pith.science/api/pith-number/346LWYI645RXIVRBFEPN52MZP7/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/346LWYI645RXIVRBFEPN52MZP7/action/timestamp_anchor","attest_storage":"https://pith.science/pith/346LWYI645RXIVRBFEPN52MZP7/action/storage_attestation","attest_author":"https://pith.science/pith/346LWYI645RXIVRBFEPN52MZP7/action/author_attestation","sign_citation":"https://pith.science/pith/346LWYI645RXIVRBFEPN52MZP7/action/citation_signature","submit_replication":"https://pith.science/pith/346LWYI645RXIVRBFEPN52MZP7/action/replication_record"}},"created_at":"2026-07-05T04:59:24.144980+00:00","updated_at":"2026-07-05T04:59:24.144980+00:00"}