{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2012:YMVUWEN6TE2BVTU3AHH6QF2JD7","short_pith_number":"pith:YMVUWEN6","schema_version":"1.0","canonical_sha256":"c32b4b11be99341ace9b01cfe817491fc08ef802463a2c6f94ef3cf047e8ca32","source":{"kind":"arxiv","id":"1208.0182","version":1},"attestation_state":"computed","paper":{"title":"Multi-frequency study of supernova remnants in the Large Magellanic Cloud. Confirmation of the supernova remnant status of DEM L205","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.GA"],"primary_cat":"astro-ph.HE","authors_text":"A. Y. De Horta, E. J. Crawford, F. Haberl, J. Dickel, L. M. Bozzetto, M. D. Filipovi\\'c, M. Sasaki, P. Maggi, R. A. Gruendl, R. C. Smith, R. Sturm, S. D. Points, W. Pietsch, Y.-H. Chu","submitted_at":"2012-08-01T12:08:01Z","abstract_excerpt":"We present new X-ray and radio data of the LMC SNR candidate DEM L205, obtained by XMM-Newton and ATCA, along with archival optical and infrared observations. We use data at various wavelengths to study this object and its complex neighbourhood, in particular in the context of the star formation activity, past and present, around the source. We analyse the X-ray spectrum to derive some remnant's properties, such as age and explosion energy. Supernova remnant features are detected at all observed wavelengths: soft and extended X-ray emission is observed, arising from a thermal plasma with a tem"},"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":"1208.0182","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2012-08-01T12:08:01Z","cross_cats_sorted":["astro-ph.GA"],"title_canon_sha256":"b2dfb26ec84e52781f9e217047becc5014d064c36799fcb6f0135d79d8a4533b","abstract_canon_sha256":"6984d0938a8230e4ee97d76dac6dd2566e81ae613eaf2f8a5a627282b48b6356"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T03:43:06.971746Z","signature_b64":"Z+wk30UsnB9gpcO5+v2NLO0GEpFZ45yETGcXmISi6FdsqUePtQ650wVXvyO762qOHGarZViTdGGrXDXWI3rvBw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"c32b4b11be99341ace9b01cfe817491fc08ef802463a2c6f94ef3cf047e8ca32","last_reissued_at":"2026-05-18T03:43:06.971060Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T03:43:06.971060Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Multi-frequency study of supernova remnants in the Large Magellanic Cloud. Confirmation of the supernova remnant status of DEM L205","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.GA"],"primary_cat":"astro-ph.HE","authors_text":"A. Y. De Horta, E. J. Crawford, F. Haberl, J. Dickel, L. M. Bozzetto, M. D. Filipovi\\'c, M. Sasaki, P. Maggi, R. A. Gruendl, R. C. Smith, R. Sturm, S. D. Points, W. Pietsch, Y.-H. Chu","submitted_at":"2012-08-01T12:08:01Z","abstract_excerpt":"We present new X-ray and radio data of the LMC SNR candidate DEM L205, obtained by XMM-Newton and ATCA, along with archival optical and infrared observations. We use data at various wavelengths to study this object and its complex neighbourhood, in particular in the context of the star formation activity, past and present, around the source. We analyse the X-ray spectrum to derive some remnant's properties, such as age and explosion energy. Supernova remnant features are detected at all observed wavelengths: soft and extended X-ray emission is observed, arising from a thermal plasma with a tem"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1208.0182","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":"1208.0182","created_at":"2026-05-18T03:43:06.971147+00:00"},{"alias_kind":"arxiv_version","alias_value":"1208.0182v1","created_at":"2026-05-18T03:43:06.971147+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1208.0182","created_at":"2026-05-18T03:43:06.971147+00:00"},{"alias_kind":"pith_short_12","alias_value":"YMVUWEN6TE2B","created_at":"2026-05-18T12:27:27.928770+00:00"},{"alias_kind":"pith_short_16","alias_value":"YMVUWEN6TE2BVTU3","created_at":"2026-05-18T12:27:27.928770+00:00"},{"alias_kind":"pith_short_8","alias_value":"YMVUWEN6","created_at":"2026-05-18T12:27:27.928770+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/YMVUWEN6TE2BVTU3AHH6QF2JD7","json":"https://pith.science/pith/YMVUWEN6TE2BVTU3AHH6QF2JD7.json","graph_json":"https://pith.science/api/pith-number/YMVUWEN6TE2BVTU3AHH6QF2JD7/graph.json","events_json":"https://pith.science/api/pith-number/YMVUWEN6TE2BVTU3AHH6QF2JD7/events.json","paper":"https://pith.science/paper/YMVUWEN6"},"agent_actions":{"view_html":"https://pith.science/pith/YMVUWEN6TE2BVTU3AHH6QF2JD7","download_json":"https://pith.science/pith/YMVUWEN6TE2BVTU3AHH6QF2JD7.json","view_paper":"https://pith.science/paper/YMVUWEN6","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1208.0182&json=true","fetch_graph":"https://pith.science/api/pith-number/YMVUWEN6TE2BVTU3AHH6QF2JD7/graph.json","fetch_events":"https://pith.science/api/pith-number/YMVUWEN6TE2BVTU3AHH6QF2JD7/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/YMVUWEN6TE2BVTU3AHH6QF2JD7/action/timestamp_anchor","attest_storage":"https://pith.science/pith/YMVUWEN6TE2BVTU3AHH6QF2JD7/action/storage_attestation","attest_author":"https://pith.science/pith/YMVUWEN6TE2BVTU3AHH6QF2JD7/action/author_attestation","sign_citation":"https://pith.science/pith/YMVUWEN6TE2BVTU3AHH6QF2JD7/action/citation_signature","submit_replication":"https://pith.science/pith/YMVUWEN6TE2BVTU3AHH6QF2JD7/action/replication_record"}},"created_at":"2026-05-18T03:43:06.971147+00:00","updated_at":"2026-05-18T03:43:06.971147+00:00"}