{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2001:MUFDKZX6RLLPGIZWHBELM2JCNM","short_pith_number":"pith:MUFDKZX6","schema_version":"1.0","canonical_sha256":"650a3566fe8ad6f323363848b669226b1854642ab708219e14ef00c013942806","source":{"kind":"arxiv","id":"astro-ph/0107504","version":1},"attestation_state":"computed","paper":{"title":"Discovery of depressions in the X-ray emission of the distant galaxy cluster RBS797 in a CHANDRA observation","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"A. Castillo-Morales (Liverpool JMU), A. Schwope (Astrophysikalisches Institut Potsdam), E. De Filippis (Liverpool JMU), J. Wambsganss (Univ. Potsdam), S. Schindler (Liverpool JMU)","submitted_at":"2001-07-26T14:27:46Z","abstract_excerpt":"We present CHANDRA observations of the X-ray luminous, distant galaxy cluster RBS797 at z=0.35. In the central region the X-ray emission shows two pronounced X-ray minima, which are located opposite to each other with respect to the cluster centre. These depressions suggest an interaction between the central radio galaxy and the intra-cluster medium, which would be the first detection in such a distant cluster. The minima are symmetric relative to the cluster centre and very deep compared to similar features found in a few other nearby clusters. A spectral and morphological analysis of the ove"},"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":"astro-ph/0107504","kind":"arxiv","version":1},"metadata":{"license":"","primary_cat":"astro-ph","submitted_at":"2001-07-26T14:27:46Z","cross_cats_sorted":[],"title_canon_sha256":"1c85537d50ce1f3fd3b0ccdb5556a591e91a3fad85f214a16cc7961ad5490681","abstract_canon_sha256":"a0d7f47c5cd3729c8a91517ee01f0a30ce5fffaf3caa3c3de503954a50b8fbc4"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-04T16:23:46.197959Z","signature_b64":"3FHgZO5EI1I/O3mngCtWfLZgWdWZhC98M8b7MeJj6LDa8EpcQlbr9eSZTrMkuUEOj/ncxzh7DKDimLknS4uoDA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"650a3566fe8ad6f323363848b669226b1854642ab708219e14ef00c013942806","last_reissued_at":"2026-07-04T16:23:46.197521Z","signature_status":"signed_v1","first_computed_at":"2026-07-04T16:23:46.197521Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Discovery of depressions in the X-ray emission of the distant galaxy cluster RBS797 in a CHANDRA observation","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"A. Castillo-Morales (Liverpool JMU), A. Schwope (Astrophysikalisches Institut Potsdam), E. De Filippis (Liverpool JMU), J. Wambsganss (Univ. Potsdam), S. Schindler (Liverpool JMU)","submitted_at":"2001-07-26T14:27:46Z","abstract_excerpt":"We present CHANDRA observations of the X-ray luminous, distant galaxy cluster RBS797 at z=0.35. In the central region the X-ray emission shows two pronounced X-ray minima, which are located opposite to each other with respect to the cluster centre. These depressions suggest an interaction between the central radio galaxy and the intra-cluster medium, which would be the first detection in such a distant cluster. The minima are symmetric relative to the cluster centre and very deep compared to similar features found in a few other nearby clusters. A spectral and morphological analysis of the ove"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"astro-ph/0107504","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/astro-ph/0107504/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":"astro-ph/0107504","created_at":"2026-07-04T16:23:46.197587+00:00"},{"alias_kind":"arxiv_version","alias_value":"astro-ph/0107504v1","created_at":"2026-07-04T16:23:46.197587+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.astro-ph/0107504","created_at":"2026-07-04T16:23:46.197587+00:00"},{"alias_kind":"pith_short_12","alias_value":"MUFDKZX6RLLP","created_at":"2026-07-04T16:23:46.197587+00:00"},{"alias_kind":"pith_short_16","alias_value":"MUFDKZX6RLLPGIZW","created_at":"2026-07-04T16:23:46.197587+00:00"},{"alias_kind":"pith_short_8","alias_value":"MUFDKZX6","created_at":"2026-07-04T16:23:46.197587+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/MUFDKZX6RLLPGIZWHBELM2JCNM","json":"https://pith.science/pith/MUFDKZX6RLLPGIZWHBELM2JCNM.json","graph_json":"https://pith.science/api/pith-number/MUFDKZX6RLLPGIZWHBELM2JCNM/graph.json","events_json":"https://pith.science/api/pith-number/MUFDKZX6RLLPGIZWHBELM2JCNM/events.json","paper":"https://pith.science/paper/MUFDKZX6"},"agent_actions":{"view_html":"https://pith.science/pith/MUFDKZX6RLLPGIZWHBELM2JCNM","download_json":"https://pith.science/pith/MUFDKZX6RLLPGIZWHBELM2JCNM.json","view_paper":"https://pith.science/paper/MUFDKZX6","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=astro-ph/0107504&json=true","fetch_graph":"https://pith.science/api/pith-number/MUFDKZX6RLLPGIZWHBELM2JCNM/graph.json","fetch_events":"https://pith.science/api/pith-number/MUFDKZX6RLLPGIZWHBELM2JCNM/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/MUFDKZX6RLLPGIZWHBELM2JCNM/action/timestamp_anchor","attest_storage":"https://pith.science/pith/MUFDKZX6RLLPGIZWHBELM2JCNM/action/storage_attestation","attest_author":"https://pith.science/pith/MUFDKZX6RLLPGIZWHBELM2JCNM/action/author_attestation","sign_citation":"https://pith.science/pith/MUFDKZX6RLLPGIZWHBELM2JCNM/action/citation_signature","submit_replication":"https://pith.science/pith/MUFDKZX6RLLPGIZWHBELM2JCNM/action/replication_record"}},"created_at":"2026-07-04T16:23:46.197587+00:00","updated_at":"2026-07-04T16:23:46.197587+00:00"}