{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2021:YGP6HTIOVEUYMJB6H3X5JPNMNE","short_pith_number":"pith:YGP6HTIO","schema_version":"1.0","canonical_sha256":"c19fe3cd0ea92986243e3eefd4bdac6914629acf9f86796483461aa8601fa024","source":{"kind":"arxiv","id":"2101.02216","version":2},"attestation_state":"computed","paper":{"title":"Multiwavelength view of SPT-CL J2106-5844. The radio galaxies and the thermal and relativistic plasmas in a massive galaxy cluster merger at z~1.13","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.GA"],"primary_cat":"astro-ph.CO","authors_text":"Andrew M. Hopkins, B\\\"arbel S. Koribalski, Eugene Churazov, Jennifer L. West, Jinhyub Kim, Jordan D. Collier, Jose M. Diego, Joshua D. Marvil, Kim HyeongHan, Lawrence Rudnick, Luca Di Mascolo, M. James Jee, Remco van der Burg, Tony Mroczkowski, Yvette Perrott","submitted_at":"2021-01-06T19:00:02Z","abstract_excerpt":"SPT-CL J2106-5844 is among the most massive galaxy clusters at z>1 yet discovered. While initially used in cosmological tests to assess the compatibility with $\\Lambda$CDM cosmology of such a massive virialized object at this redshift, more recent studies indicate SPT-CL J2106-5844 is undergoing a major merger, and is not an isolated system with a singular, well-defined halo. We use sensitive, high spatial resolution measurements from ALMA and ACA of the thermal SZ effect to reconstruct the pressure distribution of the intracluster medium in this system. These measurements are coupled with rad"},"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":"2101.02216","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2021-01-06T19:00:02Z","cross_cats_sorted":["astro-ph.GA"],"title_canon_sha256":"e1b9ccaf3a3f91ebd843b61a3f3f4694ef598614a0ae83b7d85095a721d94603","abstract_canon_sha256":"90efa01489afeba19e0713979b0503e7b30c9d4ec518345a719a757c5c155536"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T02:53:32.300355Z","signature_b64":"pVUXLDVzu7CjctJCWS86cw2VwRmIxyDV+61hgd4tVwijL6Yrv1V47gKv//e80c/kzAGGJLEi0U5Hf1CascenDw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"c19fe3cd0ea92986243e3eefd4bdac6914629acf9f86796483461aa8601fa024","last_reissued_at":"2026-07-05T02:53:32.299893Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T02:53:32.299893Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Multiwavelength view of SPT-CL J2106-5844. The radio galaxies and the thermal and relativistic plasmas in a massive galaxy cluster merger at z~1.13","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.GA"],"primary_cat":"astro-ph.CO","authors_text":"Andrew M. Hopkins, B\\\"arbel S. Koribalski, Eugene Churazov, Jennifer L. West, Jinhyub Kim, Jordan D. Collier, Jose M. Diego, Joshua D. Marvil, Kim HyeongHan, Lawrence Rudnick, Luca Di Mascolo, M. James Jee, Remco van der Burg, Tony Mroczkowski, Yvette Perrott","submitted_at":"2021-01-06T19:00:02Z","abstract_excerpt":"SPT-CL J2106-5844 is among the most massive galaxy clusters at z>1 yet discovered. While initially used in cosmological tests to assess the compatibility with $\\Lambda$CDM cosmology of such a massive virialized object at this redshift, more recent studies indicate SPT-CL J2106-5844 is undergoing a major merger, and is not an isolated system with a singular, well-defined halo. We use sensitive, high spatial resolution measurements from ALMA and ACA of the thermal SZ effect to reconstruct the pressure distribution of the intracluster medium in this system. These measurements are coupled with rad"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2101.02216","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/2101.02216/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":"2101.02216","created_at":"2026-07-05T02:53:32.299944+00:00"},{"alias_kind":"arxiv_version","alias_value":"2101.02216v2","created_at":"2026-07-05T02:53:32.299944+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2101.02216","created_at":"2026-07-05T02:53:32.299944+00:00"},{"alias_kind":"pith_short_12","alias_value":"YGP6HTIOVEUY","created_at":"2026-07-05T02:53:32.299944+00:00"},{"alias_kind":"pith_short_16","alias_value":"YGP6HTIOVEUYMJB6","created_at":"2026-07-05T02:53:32.299944+00:00"},{"alias_kind":"pith_short_8","alias_value":"YGP6HTIO","created_at":"2026-07-05T02:53:32.299944+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/YGP6HTIOVEUYMJB6H3X5JPNMNE","json":"https://pith.science/pith/YGP6HTIOVEUYMJB6H3X5JPNMNE.json","graph_json":"https://pith.science/api/pith-number/YGP6HTIOVEUYMJB6H3X5JPNMNE/graph.json","events_json":"https://pith.science/api/pith-number/YGP6HTIOVEUYMJB6H3X5JPNMNE/events.json","paper":"https://pith.science/paper/YGP6HTIO"},"agent_actions":{"view_html":"https://pith.science/pith/YGP6HTIOVEUYMJB6H3X5JPNMNE","download_json":"https://pith.science/pith/YGP6HTIOVEUYMJB6H3X5JPNMNE.json","view_paper":"https://pith.science/paper/YGP6HTIO","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2101.02216&json=true","fetch_graph":"https://pith.science/api/pith-number/YGP6HTIOVEUYMJB6H3X5JPNMNE/graph.json","fetch_events":"https://pith.science/api/pith-number/YGP6HTIOVEUYMJB6H3X5JPNMNE/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/YGP6HTIOVEUYMJB6H3X5JPNMNE/action/timestamp_anchor","attest_storage":"https://pith.science/pith/YGP6HTIOVEUYMJB6H3X5JPNMNE/action/storage_attestation","attest_author":"https://pith.science/pith/YGP6HTIOVEUYMJB6H3X5JPNMNE/action/author_attestation","sign_citation":"https://pith.science/pith/YGP6HTIOVEUYMJB6H3X5JPNMNE/action/citation_signature","submit_replication":"https://pith.science/pith/YGP6HTIOVEUYMJB6H3X5JPNMNE/action/replication_record"}},"created_at":"2026-07-05T02:53:32.299944+00:00","updated_at":"2026-07-05T02:53:32.299944+00:00"}