{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2016:RKJSKNGBPIK6HU4XPZ6DVQ6WMO","short_pith_number":"pith:RKJSKNGB","schema_version":"1.0","canonical_sha256":"8a932534c17a15e3d3977e7c3ac3d66398d4c45578ed2b8a7be352edc228197b","source":{"kind":"arxiv","id":"1612.00535","version":2},"attestation_state":"computed","paper":{"title":"Deep Chandra observations of NGC 1404: cluster plasma physics revealed by an infalling early-type galaxy","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.GA"],"primary_cat":"astro-ph.HE","authors_text":"(2) Univ. of Hull, (3) MPA), Christine Jones (1), Elke Roediger (2), Eugene Churazov (3), Marie E. Machacek (1) ((1) Harvard-Smithsonian Center for Astrophysics, Paul E. J. Nulsen (1), Ralph P. Kraft (1), Scott W. Randall (1), William R. Forman (1), Yuanyuan Su (1)","submitted_at":"2016-12-02T01:30:28Z","abstract_excerpt":"The intracluster medium (ICM), as a magnetized and highly ionized fluid, provides an ideal laboratory to study plasma physics under extreme conditions that cannot yet be achieved on Earth. NGC 1404 is a bright elliptical galaxy that is being gas stripped as it falls through the ICM of the Fornax Cluster. We use the new {\\sl Chandra} X-ray observations of NGC 1404 to study ICM microphysics. The interstellar medium (ISM) of NGC 1404 is characterized by a sharp leading edge, 8 kpc from the galaxy center, and a short downstream gaseous tail. Contact discontinuities are resolved on unprecedented sp"},"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":"1612.00535","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2016-12-02T01:30:28Z","cross_cats_sorted":["astro-ph.GA"],"title_canon_sha256":"9d2ede98a844329258d3e1772fd89f27815c8244367e539ba9b3cccac2fd8020","abstract_canon_sha256":"ed62728698df9b2da9ab6a7a2be9959c44ea81e8a68498af62df2455dbe52210"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:53:04.926972Z","signature_b64":"M4LTGiEaDs4eeXW6Bzy51VELb/XW5imm4zZBXnPW21zLOYrmYB0z1/VGZQHsZ4lXAsL29e4znVzJmNngsl7VBA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"8a932534c17a15e3d3977e7c3ac3d66398d4c45578ed2b8a7be352edc228197b","last_reissued_at":"2026-05-18T00:53:04.926435Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:53:04.926435Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Deep Chandra observations of NGC 1404: cluster plasma physics revealed by an infalling early-type galaxy","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.GA"],"primary_cat":"astro-ph.HE","authors_text":"(2) Univ. of Hull, (3) MPA), Christine Jones (1), Elke Roediger (2), Eugene Churazov (3), Marie E. Machacek (1) ((1) Harvard-Smithsonian Center for Astrophysics, Paul E. J. Nulsen (1), Ralph P. Kraft (1), Scott W. Randall (1), William R. Forman (1), Yuanyuan Su (1)","submitted_at":"2016-12-02T01:30:28Z","abstract_excerpt":"The intracluster medium (ICM), as a magnetized and highly ionized fluid, provides an ideal laboratory to study plasma physics under extreme conditions that cannot yet be achieved on Earth. NGC 1404 is a bright elliptical galaxy that is being gas stripped as it falls through the ICM of the Fornax Cluster. We use the new {\\sl Chandra} X-ray observations of NGC 1404 to study ICM microphysics. The interstellar medium (ISM) of NGC 1404 is characterized by a sharp leading edge, 8 kpc from the galaxy center, and a short downstream gaseous tail. Contact discontinuities are resolved on unprecedented sp"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1612.00535","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":"1612.00535","created_at":"2026-05-18T00:53:04.926532+00:00"},{"alias_kind":"arxiv_version","alias_value":"1612.00535v2","created_at":"2026-05-18T00:53:04.926532+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1612.00535","created_at":"2026-05-18T00:53:04.926532+00:00"},{"alias_kind":"pith_short_12","alias_value":"RKJSKNGBPIK6","created_at":"2026-05-18T12:30:41.710351+00:00"},{"alias_kind":"pith_short_16","alias_value":"RKJSKNGBPIK6HU4X","created_at":"2026-05-18T12:30:41.710351+00:00"},{"alias_kind":"pith_short_8","alias_value":"RKJSKNGB","created_at":"2026-05-18T12:30:41.710351+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2606.17371","citing_title":"Reduced Effective Viscosity from Anisotropic Transport and Plasma Instabilities in the Sloshing Cores of Galaxy Clusters","ref_index":35,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/RKJSKNGBPIK6HU4XPZ6DVQ6WMO","json":"https://pith.science/pith/RKJSKNGBPIK6HU4XPZ6DVQ6WMO.json","graph_json":"https://pith.science/api/pith-number/RKJSKNGBPIK6HU4XPZ6DVQ6WMO/graph.json","events_json":"https://pith.science/api/pith-number/RKJSKNGBPIK6HU4XPZ6DVQ6WMO/events.json","paper":"https://pith.science/paper/RKJSKNGB"},"agent_actions":{"view_html":"https://pith.science/pith/RKJSKNGBPIK6HU4XPZ6DVQ6WMO","download_json":"https://pith.science/pith/RKJSKNGBPIK6HU4XPZ6DVQ6WMO.json","view_paper":"https://pith.science/paper/RKJSKNGB","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1612.00535&json=true","fetch_graph":"https://pith.science/api/pith-number/RKJSKNGBPIK6HU4XPZ6DVQ6WMO/graph.json","fetch_events":"https://pith.science/api/pith-number/RKJSKNGBPIK6HU4XPZ6DVQ6WMO/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/RKJSKNGBPIK6HU4XPZ6DVQ6WMO/action/timestamp_anchor","attest_storage":"https://pith.science/pith/RKJSKNGBPIK6HU4XPZ6DVQ6WMO/action/storage_attestation","attest_author":"https://pith.science/pith/RKJSKNGBPIK6HU4XPZ6DVQ6WMO/action/author_attestation","sign_citation":"https://pith.science/pith/RKJSKNGBPIK6HU4XPZ6DVQ6WMO/action/citation_signature","submit_replication":"https://pith.science/pith/RKJSKNGBPIK6HU4XPZ6DVQ6WMO/action/replication_record"}},"created_at":"2026-05-18T00:53:04.926532+00:00","updated_at":"2026-05-18T00:53:04.926532+00:00"}