{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2013:5VDGW7DD7PBN3G6BS6LXBXYNJX","short_pith_number":"pith:5VDGW7DD","schema_version":"1.0","canonical_sha256":"ed466b7c63fbc2dd9bc1979770df0d4dc4ef68501d983b15005dd43ca6e27ba1","source":{"kind":"arxiv","id":"1310.2569","version":1},"attestation_state":"computed","paper":{"title":"Four new X-ray-selected supernova remnants in the Large Magellanic Cloud","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"F. Haberl, J. Dickel, L. M. Bozzetto, M.D. Filipovic, M. Sasaki, P. J. Kavanagh, P. Maggi, R. A. Gruendl, S. D. Points, W. Pietsch, Y.-H. Chu","submitted_at":"2013-10-09T18:24:53Z","abstract_excerpt":"Aims: We present a detailed multi-wavelength study of four new supernova remnants (SNRs) in the Large Magellanic Cloud (LMC). The objects were identified as SNR candidates in X-ray observations performed during the survey of the LMC with XMM-Newton.\n  Methods: Data obained with XMM-Newton are used to investigate the morphological and spectral features of the remnants in X-rays. We measure the plasma conditions, look for supernova (SN) ejecta emission, and constrain some of the SNR properties (e.g. age and ambient density). We supplement the X-ray data with optical, infrared, and radio-continuu"},"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":"1310.2569","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2013-10-09T18:24:53Z","cross_cats_sorted":[],"title_canon_sha256":"62c223871eebadbb6b7395330e758a1a7e4f61fc2490c48aa6a39bfe390de3bf","abstract_canon_sha256":"07ba42e3e4c7c0e30fdfc70f10ca0ba1ca05f27f6e91f3bd0c01d9f7ac3f59bc"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T03:02:34.300515Z","signature_b64":"1ZEtdXrOqh5bpmB9ZYv3/Nin7WCPM3UZgGfH9dEIHJWOA3CCNcT+inqodWLSX7MdT2rNtwXQrt+oOr4ROtZwAg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"ed466b7c63fbc2dd9bc1979770df0d4dc4ef68501d983b15005dd43ca6e27ba1","last_reissued_at":"2026-05-18T03:02:34.299637Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T03:02:34.299637Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Four new X-ray-selected supernova remnants in the Large Magellanic Cloud","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"F. Haberl, J. Dickel, L. M. Bozzetto, M.D. Filipovic, M. Sasaki, P. J. Kavanagh, P. Maggi, R. A. Gruendl, S. D. Points, W. Pietsch, Y.-H. Chu","submitted_at":"2013-10-09T18:24:53Z","abstract_excerpt":"Aims: We present a detailed multi-wavelength study of four new supernova remnants (SNRs) in the Large Magellanic Cloud (LMC). The objects were identified as SNR candidates in X-ray observations performed during the survey of the LMC with XMM-Newton.\n  Methods: Data obained with XMM-Newton are used to investigate the morphological and spectral features of the remnants in X-rays. We measure the plasma conditions, look for supernova (SN) ejecta emission, and constrain some of the SNR properties (e.g. age and ambient density). We supplement the X-ray data with optical, infrared, and radio-continuu"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1310.2569","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":"1310.2569","created_at":"2026-05-18T03:02:34.299777+00:00"},{"alias_kind":"arxiv_version","alias_value":"1310.2569v1","created_at":"2026-05-18T03:02:34.299777+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1310.2569","created_at":"2026-05-18T03:02:34.299777+00:00"},{"alias_kind":"pith_short_12","alias_value":"5VDGW7DD7PBN","created_at":"2026-05-18T12:27:34.582898+00:00"},{"alias_kind":"pith_short_16","alias_value":"5VDGW7DD7PBN3G6B","created_at":"2026-05-18T12:27:34.582898+00:00"},{"alias_kind":"pith_short_8","alias_value":"5VDGW7DD","created_at":"2026-05-18T12:27:34.582898+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/5VDGW7DD7PBN3G6BS6LXBXYNJX","json":"https://pith.science/pith/5VDGW7DD7PBN3G6BS6LXBXYNJX.json","graph_json":"https://pith.science/api/pith-number/5VDGW7DD7PBN3G6BS6LXBXYNJX/graph.json","events_json":"https://pith.science/api/pith-number/5VDGW7DD7PBN3G6BS6LXBXYNJX/events.json","paper":"https://pith.science/paper/5VDGW7DD"},"agent_actions":{"view_html":"https://pith.science/pith/5VDGW7DD7PBN3G6BS6LXBXYNJX","download_json":"https://pith.science/pith/5VDGW7DD7PBN3G6BS6LXBXYNJX.json","view_paper":"https://pith.science/paper/5VDGW7DD","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1310.2569&json=true","fetch_graph":"https://pith.science/api/pith-number/5VDGW7DD7PBN3G6BS6LXBXYNJX/graph.json","fetch_events":"https://pith.science/api/pith-number/5VDGW7DD7PBN3G6BS6LXBXYNJX/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/5VDGW7DD7PBN3G6BS6LXBXYNJX/action/timestamp_anchor","attest_storage":"https://pith.science/pith/5VDGW7DD7PBN3G6BS6LXBXYNJX/action/storage_attestation","attest_author":"https://pith.science/pith/5VDGW7DD7PBN3G6BS6LXBXYNJX/action/author_attestation","sign_citation":"https://pith.science/pith/5VDGW7DD7PBN3G6BS6LXBXYNJX/action/citation_signature","submit_replication":"https://pith.science/pith/5VDGW7DD7PBN3G6BS6LXBXYNJX/action/replication_record"}},"created_at":"2026-05-18T03:02:34.299777+00:00","updated_at":"2026-05-18T03:02:34.299777+00:00"}