{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2007:TYZ2N5INO7ZWO3AIGKBFZUDKTQ","short_pith_number":"pith:TYZ2N5IN","schema_version":"1.0","canonical_sha256":"9e33a6f50d77f3676c0832825cd06a9c3f7c096eaea4f09734569af24516e11b","source":{"kind":"arxiv","id":"0709.0832","version":1},"attestation_state":"computed","paper":{"title":"SPLASH: An interactive visualisation tool for Smoothed Particle Hydrodynamics simulations","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"Daniel J. Price","submitted_at":"2007-09-06T11:17:10Z","abstract_excerpt":"This paper presents SPLASH, a publicly available interactive visualisation tool for Smoothed Particle Hydrodynamics (SPH) simulations. Visualisation of SPH data is more complicated than for grid-based codes because the data is defined on a set of irregular points and therefore requires a mapping procedure to a two dimensional pixel array. This means that, in practise, many authors simply produce particle plots which offer a rather crude representation of the simulation output. Here we describe the techniques and algorithms which are utilised in SPLASH in order to provide the user with a fast, "},"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":"0709.0832","kind":"arxiv","version":1},"metadata":{"license":"","primary_cat":"astro-ph","submitted_at":"2007-09-06T11:17:10Z","cross_cats_sorted":[],"title_canon_sha256":"e3c234d1ad0388e6afe257b448a235c8bfa501f77ddf99d952e675ef1061c9a0","abstract_canon_sha256":"7a462883d50b457ff9521af61d201b40117de177eb37d7b9169f3080a935cbeb"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-04T17:05:29.411863Z","signature_b64":"6ichlDHqO2cz4f327Q25Y8/2H5ZB6zm65aqhCilr96Wh4hPGMyg/6W3Axkhryzwk26B65cQsKMpFaao+1rSBDQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"9e33a6f50d77f3676c0832825cd06a9c3f7c096eaea4f09734569af24516e11b","last_reissued_at":"2026-07-04T17:05:29.411480Z","signature_status":"signed_v1","first_computed_at":"2026-07-04T17:05:29.411480Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"SPLASH: An interactive visualisation tool for Smoothed Particle Hydrodynamics simulations","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"Daniel J. Price","submitted_at":"2007-09-06T11:17:10Z","abstract_excerpt":"This paper presents SPLASH, a publicly available interactive visualisation tool for Smoothed Particle Hydrodynamics (SPH) simulations. Visualisation of SPH data is more complicated than for grid-based codes because the data is defined on a set of irregular points and therefore requires a mapping procedure to a two dimensional pixel array. This means that, in practise, many authors simply produce particle plots which offer a rather crude representation of the simulation output. Here we describe the techniques and algorithms which are utilised in SPLASH in order to provide the user with a fast, "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"0709.0832","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/0709.0832/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":"0709.0832","created_at":"2026-07-04T17:05:29.411535+00:00"},{"alias_kind":"arxiv_version","alias_value":"0709.0832v1","created_at":"2026-07-04T17:05:29.411535+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.0709.0832","created_at":"2026-07-04T17:05:29.411535+00:00"},{"alias_kind":"pith_short_12","alias_value":"TYZ2N5INO7ZW","created_at":"2026-07-04T17:05:29.411535+00:00"},{"alias_kind":"pith_short_16","alias_value":"TYZ2N5INO7ZWO3AI","created_at":"2026-07-04T17:05:29.411535+00:00"},{"alias_kind":"pith_short_8","alias_value":"TYZ2N5IN","created_at":"2026-07-04T17:05:29.411535+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":7,"internal_anchor_count":7,"sample":[{"citing_arxiv_id":"2606.25794","citing_title":"Substructures in Planet-Forming Disks with the SKAO","ref_index":260,"is_internal_anchor":true},{"citing_arxiv_id":"2606.00205","citing_title":"Ultraviolet diversity of Little Red Dots as a probe for direct-collapse black hole ages","ref_index":96,"is_internal_anchor":true},{"citing_arxiv_id":"2606.22919","citing_title":"Are most detected tidal disruption events partial?","ref_index":52,"is_internal_anchor":true},{"citing_arxiv_id":"2606.26495","citing_title":"Dust Formation in Common Envelope Binary Interactions -- III. Lightcurves","ref_index":1,"is_internal_anchor":true},{"citing_arxiv_id":"2606.25794","citing_title":"Substructures in Planet-Forming Disks with the SKAO","ref_index":260,"is_internal_anchor":true},{"citing_arxiv_id":"2111.08065","citing_title":"The Bardeen-Petterson effect in accreting supermassive black-hole binaries: disc breaking and critical obliquity","ref_index":46,"is_internal_anchor":true},{"citing_arxiv_id":"2605.20327","citing_title":"On the origin of anomalous dissipation in simulations of tidal disruption events","ref_index":79,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/TYZ2N5INO7ZWO3AIGKBFZUDKTQ","json":"https://pith.science/pith/TYZ2N5INO7ZWO3AIGKBFZUDKTQ.json","graph_json":"https://pith.science/api/pith-number/TYZ2N5INO7ZWO3AIGKBFZUDKTQ/graph.json","events_json":"https://pith.science/api/pith-number/TYZ2N5INO7ZWO3AIGKBFZUDKTQ/events.json","paper":"https://pith.science/paper/TYZ2N5IN"},"agent_actions":{"view_html":"https://pith.science/pith/TYZ2N5INO7ZWO3AIGKBFZUDKTQ","download_json":"https://pith.science/pith/TYZ2N5INO7ZWO3AIGKBFZUDKTQ.json","view_paper":"https://pith.science/paper/TYZ2N5IN","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=0709.0832&json=true","fetch_graph":"https://pith.science/api/pith-number/TYZ2N5INO7ZWO3AIGKBFZUDKTQ/graph.json","fetch_events":"https://pith.science/api/pith-number/TYZ2N5INO7ZWO3AIGKBFZUDKTQ/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/TYZ2N5INO7ZWO3AIGKBFZUDKTQ/action/timestamp_anchor","attest_storage":"https://pith.science/pith/TYZ2N5INO7ZWO3AIGKBFZUDKTQ/action/storage_attestation","attest_author":"https://pith.science/pith/TYZ2N5INO7ZWO3AIGKBFZUDKTQ/action/author_attestation","sign_citation":"https://pith.science/pith/TYZ2N5INO7ZWO3AIGKBFZUDKTQ/action/citation_signature","submit_replication":"https://pith.science/pith/TYZ2N5INO7ZWO3AIGKBFZUDKTQ/action/replication_record"}},"created_at":"2026-07-04T17:05:29.411535+00:00","updated_at":"2026-07-04T17:05:29.411535+00:00"}