{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2018:VVTZEV7AJ6ITV7QLXJIPNQTF6Q","short_pith_number":"pith:VVTZEV7A","schema_version":"1.0","canonical_sha256":"ad679257e04f913afe0bba50f6c265f424550a4962c1111f40727cd63c140e7a","source":{"kind":"arxiv","id":"1812.08152","version":2},"attestation_state":"computed","paper":{"title":"Joint cluster reconstructions: Combining free-form lensing and X-rays","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"Celine Tchernin, Julian Merten, Korbinian Huber, Matthias Bartelmann, Stefan Hilbert","submitted_at":"2018-12-19T18:47:42Z","abstract_excerpt":"Galaxy clusters provide a multitude of observational data across wavelengths and their structure and morphology are of considerable interest in cosmology as well as astrophysics. We develop a framework that allows the combination of lensing and non-lensing observations in a free-form and mesh-free approach to infer the projected mass distribution of individual galaxy clusters. This method can be used to test common assumptions on the morphology of clusters in parametric models. We make use of the lensing reconstruction code SaWLens2 and expand its capabilities by incorporating an estimate of t"},"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":"1812.08152","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2018-12-19T18:47:42Z","cross_cats_sorted":[],"title_canon_sha256":"be07d950356fc9cab49eb3699a18e91e9113f5bad7f2b86ac4339b0f3c186177","abstract_canon_sha256":"1f8a069734b714b6901a9755e96cd7514cf97388d7392542e65b4c6315102ab8"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-17T23:40:33.877118Z","signature_b64":"RnaVNDCTuG5311BiK9cXgOwKLwdwYik81K/6nDhWzlBtdgbb8sbfOaUtV3ZHcn8ZJwvFSnN8daAsoSrxeL2IBg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"ad679257e04f913afe0bba50f6c265f424550a4962c1111f40727cd63c140e7a","last_reissued_at":"2026-05-17T23:40:33.876675Z","signature_status":"signed_v1","first_computed_at":"2026-05-17T23:40:33.876675Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Joint cluster reconstructions: Combining free-form lensing and X-rays","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"Celine Tchernin, Julian Merten, Korbinian Huber, Matthias Bartelmann, Stefan Hilbert","submitted_at":"2018-12-19T18:47:42Z","abstract_excerpt":"Galaxy clusters provide a multitude of observational data across wavelengths and their structure and morphology are of considerable interest in cosmology as well as astrophysics. We develop a framework that allows the combination of lensing and non-lensing observations in a free-form and mesh-free approach to infer the projected mass distribution of individual galaxy clusters. This method can be used to test common assumptions on the morphology of clusters in parametric models. We make use of the lensing reconstruction code SaWLens2 and expand its capabilities by incorporating an estimate of t"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1812.08152","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":"1812.08152","created_at":"2026-05-17T23:40:33.876743+00:00"},{"alias_kind":"arxiv_version","alias_value":"1812.08152v2","created_at":"2026-05-17T23:40:33.876743+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1812.08152","created_at":"2026-05-17T23:40:33.876743+00:00"},{"alias_kind":"pith_short_12","alias_value":"VVTZEV7AJ6IT","created_at":"2026-05-18T12:32:59.047623+00:00"},{"alias_kind":"pith_short_16","alias_value":"VVTZEV7AJ6ITV7QL","created_at":"2026-05-18T12:32:59.047623+00:00"},{"alias_kind":"pith_short_8","alias_value":"VVTZEV7A","created_at":"2026-05-18T12:32:59.047623+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/VVTZEV7AJ6ITV7QLXJIPNQTF6Q","json":"https://pith.science/pith/VVTZEV7AJ6ITV7QLXJIPNQTF6Q.json","graph_json":"https://pith.science/api/pith-number/VVTZEV7AJ6ITV7QLXJIPNQTF6Q/graph.json","events_json":"https://pith.science/api/pith-number/VVTZEV7AJ6ITV7QLXJIPNQTF6Q/events.json","paper":"https://pith.science/paper/VVTZEV7A"},"agent_actions":{"view_html":"https://pith.science/pith/VVTZEV7AJ6ITV7QLXJIPNQTF6Q","download_json":"https://pith.science/pith/VVTZEV7AJ6ITV7QLXJIPNQTF6Q.json","view_paper":"https://pith.science/paper/VVTZEV7A","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1812.08152&json=true","fetch_graph":"https://pith.science/api/pith-number/VVTZEV7AJ6ITV7QLXJIPNQTF6Q/graph.json","fetch_events":"https://pith.science/api/pith-number/VVTZEV7AJ6ITV7QLXJIPNQTF6Q/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/VVTZEV7AJ6ITV7QLXJIPNQTF6Q/action/timestamp_anchor","attest_storage":"https://pith.science/pith/VVTZEV7AJ6ITV7QLXJIPNQTF6Q/action/storage_attestation","attest_author":"https://pith.science/pith/VVTZEV7AJ6ITV7QLXJIPNQTF6Q/action/author_attestation","sign_citation":"https://pith.science/pith/VVTZEV7AJ6ITV7QLXJIPNQTF6Q/action/citation_signature","submit_replication":"https://pith.science/pith/VVTZEV7AJ6ITV7QLXJIPNQTF6Q/action/replication_record"}},"created_at":"2026-05-17T23:40:33.876743+00:00","updated_at":"2026-05-17T23:40:33.876743+00:00"}