{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2023:ROCA5ID2CERPJHMC3TTXWJTCOM","short_pith_number":"pith:ROCA5ID2","schema_version":"1.0","canonical_sha256":"8b840ea07a1122f49d82dce77b2662733026f2a9b69ae1685a376eaa7e5115e5","source":{"kind":"arxiv","id":"2308.09176","version":2},"attestation_state":"computed","paper":{"title":"First spatio-spectral Bayesian imaging of SN1006 in X-ray","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.IM"],"primary_cat":"astro-ph.HE","authors_text":"Jakob Knollm\\\"uller, Julia Stadler, Lukas Platz, Margret Westerkamp, Matteo Guardiani, Philipp Arras, Philipp Frank, Torsten En{\\ss}lin, Vincent Eberle","submitted_at":"2023-08-17T20:28:37Z","abstract_excerpt":"Supernovae are an important source of energy in the interstellar medium. Young remnants of supernovae have a peak emission in the X-ray region, making them interesting objects for X-ray observations. In particular, the supernova remnant SN1006 is of great interest due to its historical record, proximity and brightness. It has therefore been studied by several X-ray telescopes. Improving the X-ray imaging of this and other remnants is important but challenging as it requires to address a spatially varying instrument response in order to achieve a high signal-to-noise ratio. Here, we use Chandra"},"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":"2308.09176","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2023-08-17T20:28:37Z","cross_cats_sorted":["astro-ph.IM"],"title_canon_sha256":"04fdc7dbe9f2e6471c3f9195f95134c444c83a65404007901a218a1516db5cae","abstract_canon_sha256":"b0f560e71ac0e985472b8a1691dab495e7774cdae3f898b88907726f46ba83a1"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T09:40:36.783159Z","signature_b64":"bth08vOcBeHf/wsHn+M/HjMfyW0cpXdacb0FJd55Q/GNbTLNrdmWyRzBmGMewWVCqv7yVLgiuEuBxf+XEMjuAw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"8b840ea07a1122f49d82dce77b2662733026f2a9b69ae1685a376eaa7e5115e5","last_reissued_at":"2026-07-05T09:40:36.782665Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T09:40:36.782665Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"First spatio-spectral Bayesian imaging of SN1006 in X-ray","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.IM"],"primary_cat":"astro-ph.HE","authors_text":"Jakob Knollm\\\"uller, Julia Stadler, Lukas Platz, Margret Westerkamp, Matteo Guardiani, Philipp Arras, Philipp Frank, Torsten En{\\ss}lin, Vincent Eberle","submitted_at":"2023-08-17T20:28:37Z","abstract_excerpt":"Supernovae are an important source of energy in the interstellar medium. Young remnants of supernovae have a peak emission in the X-ray region, making them interesting objects for X-ray observations. In particular, the supernova remnant SN1006 is of great interest due to its historical record, proximity and brightness. It has therefore been studied by several X-ray telescopes. Improving the X-ray imaging of this and other remnants is important but challenging as it requires to address a spatially varying instrument response in order to achieve a high signal-to-noise ratio. Here, we use Chandra"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2308.09176","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2308.09176/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":"2308.09176","created_at":"2026-07-05T09:40:36.782726+00:00"},{"alias_kind":"arxiv_version","alias_value":"2308.09176v2","created_at":"2026-07-05T09:40:36.782726+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2308.09176","created_at":"2026-07-05T09:40:36.782726+00:00"},{"alias_kind":"pith_short_12","alias_value":"ROCA5ID2CERP","created_at":"2026-07-05T09:40:36.782726+00:00"},{"alias_kind":"pith_short_16","alias_value":"ROCA5ID2CERPJHMC","created_at":"2026-07-05T09:40:36.782726+00:00"},{"alias_kind":"pith_short_8","alias_value":"ROCA5ID2","created_at":"2026-07-05T09:40:36.782726+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/ROCA5ID2CERPJHMC3TTXWJTCOM","json":"https://pith.science/pith/ROCA5ID2CERPJHMC3TTXWJTCOM.json","graph_json":"https://pith.science/api/pith-number/ROCA5ID2CERPJHMC3TTXWJTCOM/graph.json","events_json":"https://pith.science/api/pith-number/ROCA5ID2CERPJHMC3TTXWJTCOM/events.json","paper":"https://pith.science/paper/ROCA5ID2"},"agent_actions":{"view_html":"https://pith.science/pith/ROCA5ID2CERPJHMC3TTXWJTCOM","download_json":"https://pith.science/pith/ROCA5ID2CERPJHMC3TTXWJTCOM.json","view_paper":"https://pith.science/paper/ROCA5ID2","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2308.09176&json=true","fetch_graph":"https://pith.science/api/pith-number/ROCA5ID2CERPJHMC3TTXWJTCOM/graph.json","fetch_events":"https://pith.science/api/pith-number/ROCA5ID2CERPJHMC3TTXWJTCOM/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/ROCA5ID2CERPJHMC3TTXWJTCOM/action/timestamp_anchor","attest_storage":"https://pith.science/pith/ROCA5ID2CERPJHMC3TTXWJTCOM/action/storage_attestation","attest_author":"https://pith.science/pith/ROCA5ID2CERPJHMC3TTXWJTCOM/action/author_attestation","sign_citation":"https://pith.science/pith/ROCA5ID2CERPJHMC3TTXWJTCOM/action/citation_signature","submit_replication":"https://pith.science/pith/ROCA5ID2CERPJHMC3TTXWJTCOM/action/replication_record"}},"created_at":"2026-07-05T09:40:36.782726+00:00","updated_at":"2026-07-05T09:40:36.782726+00:00"}