{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2017:TMVOFHI62LGBQ2CEDIJBPP5F6V","short_pith_number":"pith:TMVOFHI6","schema_version":"1.0","canonical_sha256":"9b2ae29d1ed2cc1868441a1217bfa5f554676b6cec1743aa83879d5bd3549dd8","source":{"kind":"arxiv","id":"1711.08438","version":1},"attestation_state":"computed","paper":{"title":"Simulating the galaxy cluster \"El Gordo\": gas motion, kinetic Sunyaev-Zel'dovich signal, and X-ray line features","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.GA"],"primary_cat":"astro-ph.CO","authors_text":"2), (2) KIAA, (3) NAOC, 4) ((1) MPA, (4) UCAS), Congyao Zhang (1, Qingjuan Yu (2), Youjun Lu (3","submitted_at":"2017-11-22T18:34:40Z","abstract_excerpt":"The massive galaxy cluster \"El Gordo\" (ACT-CL J0102--4915) is a rare merging system with a high collision speed suggested by multi-wavelength observations and the theoretical modeling. Zhang et al. (2015) propose two types of mergers, a nearly head-on merger and an off-axis merger with a large impact parameter, to reproduce most of the observational features of the cluster, by using numerical simulations. The different merger configurations of the two models result in different gas motion in the simulated clusters. In this paper, we predict the kinetic Sunyaev-Zel'dovich (kSZ) effect, the rela"},"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":"1711.08438","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2017-11-22T18:34:40Z","cross_cats_sorted":["astro-ph.GA"],"title_canon_sha256":"221f018163404f68f0afca79b66400ff3456a5d5bd1bdf520d3ae5b5e7b2dd1d","abstract_canon_sha256":"ae34e3725032959e780ba8ac872d76e2dd7d1ef0427cee56e9fcd9f0a78c5062"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:20:38.223112Z","signature_b64":"ixvZHQJJILozQhz9vElaLHnFYB2uIkULLr0nTjZ20eXO8fJc/4aBUVrYzJo+6Fi0f7GXc6+t4nPMAFlcX4R2CQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"9b2ae29d1ed2cc1868441a1217bfa5f554676b6cec1743aa83879d5bd3549dd8","last_reissued_at":"2026-05-18T00:20:38.222590Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:20:38.222590Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Simulating the galaxy cluster \"El Gordo\": gas motion, kinetic Sunyaev-Zel'dovich signal, and X-ray line features","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.GA"],"primary_cat":"astro-ph.CO","authors_text":"2), (2) KIAA, (3) NAOC, 4) ((1) MPA, (4) UCAS), Congyao Zhang (1, Qingjuan Yu (2), Youjun Lu (3","submitted_at":"2017-11-22T18:34:40Z","abstract_excerpt":"The massive galaxy cluster \"El Gordo\" (ACT-CL J0102--4915) is a rare merging system with a high collision speed suggested by multi-wavelength observations and the theoretical modeling. Zhang et al. (2015) propose two types of mergers, a nearly head-on merger and an off-axis merger with a large impact parameter, to reproduce most of the observational features of the cluster, by using numerical simulations. The different merger configurations of the two models result in different gas motion in the simulated clusters. In this paper, we predict the kinetic Sunyaev-Zel'dovich (kSZ) effect, the rela"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1711.08438","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":""},"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":"1711.08438","created_at":"2026-05-18T00:20:38.222669+00:00"},{"alias_kind":"arxiv_version","alias_value":"1711.08438v1","created_at":"2026-05-18T00:20:38.222669+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1711.08438","created_at":"2026-05-18T00:20:38.222669+00:00"},{"alias_kind":"pith_short_12","alias_value":"TMVOFHI62LGB","created_at":"2026-05-18T12:31:46.661854+00:00"},{"alias_kind":"pith_short_16","alias_value":"TMVOFHI62LGBQ2CE","created_at":"2026-05-18T12:31:46.661854+00:00"},{"alias_kind":"pith_short_8","alias_value":"TMVOFHI6","created_at":"2026-05-18T12:31:46.661854+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/TMVOFHI62LGBQ2CEDIJBPP5F6V","json":"https://pith.science/pith/TMVOFHI62LGBQ2CEDIJBPP5F6V.json","graph_json":"https://pith.science/api/pith-number/TMVOFHI62LGBQ2CEDIJBPP5F6V/graph.json","events_json":"https://pith.science/api/pith-number/TMVOFHI62LGBQ2CEDIJBPP5F6V/events.json","paper":"https://pith.science/paper/TMVOFHI6"},"agent_actions":{"view_html":"https://pith.science/pith/TMVOFHI62LGBQ2CEDIJBPP5F6V","download_json":"https://pith.science/pith/TMVOFHI62LGBQ2CEDIJBPP5F6V.json","view_paper":"https://pith.science/paper/TMVOFHI6","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1711.08438&json=true","fetch_graph":"https://pith.science/api/pith-number/TMVOFHI62LGBQ2CEDIJBPP5F6V/graph.json","fetch_events":"https://pith.science/api/pith-number/TMVOFHI62LGBQ2CEDIJBPP5F6V/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/TMVOFHI62LGBQ2CEDIJBPP5F6V/action/timestamp_anchor","attest_storage":"https://pith.science/pith/TMVOFHI62LGBQ2CEDIJBPP5F6V/action/storage_attestation","attest_author":"https://pith.science/pith/TMVOFHI62LGBQ2CEDIJBPP5F6V/action/author_attestation","sign_citation":"https://pith.science/pith/TMVOFHI62LGBQ2CEDIJBPP5F6V/action/citation_signature","submit_replication":"https://pith.science/pith/TMVOFHI62LGBQ2CEDIJBPP5F6V/action/replication_record"}},"created_at":"2026-05-18T00:20:38.222669+00:00","updated_at":"2026-05-18T00:20:38.222669+00:00"}