{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2022:SV6TGCHWIWXBJPUSKZF2AZHS6X","short_pith_number":"pith:SV6TGCHW","schema_version":"1.0","canonical_sha256":"957d3308f645ae14be92564ba064f2f5f26654230eac384ae6a642e3aacc25ca","source":{"kind":"arxiv","id":"2210.03212","version":1},"attestation_state":"computed","paper":{"title":"The luminous Type IIN supernova SN 2017hcc: Infrared bright, X-ray and radio faint","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Nicholas J. H. James, Ori D. Fox, Poonam Chandra, Roger A. Chevalier","submitted_at":"2022-10-06T21:15:57Z","abstract_excerpt":"We present multiwavelength observations of supernova (SN) 2017hcc with the Chandra X-ray telescope and the X-ray telescope onboard Swift (Swift-XRT) in X-ray bands, with the Spitzer and the TripleSpec spectrometer in near-infrared (IR) and mid-IR bands and with the Karl G. Jansky Very Large Array (VLA) for radio bands. The X-ray observations cover a period of 29 to 1310 days, with the first X-ray detection on day 727 with the Chandra. The SN was subsequently detected in the VLA radio bands from day 1000 onwards. While the radio data are sparse, synchrotron-self absorption is clearly ruled out "},"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":"2210.03212","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.HE","submitted_at":"2022-10-06T21:15:57Z","cross_cats_sorted":[],"title_canon_sha256":"b1e023e38a3a782f5ecdc05512a7f3d7d35fc031184558c4145483d7f1207eee","abstract_canon_sha256":"cb75cada61dea6ce5ba9d0c5f18a907b10668b75f1d4ccfee979fa0ac9c3396b"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T05:10:16.328100Z","signature_b64":"GjrKIrZBxqfASGz/nxKFNCGMlnR3WiDcFXjqIsEHtnQKlA/nyHHhla+kYFHqCnXp+EE5eq3O11i86U0xGAinAA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"957d3308f645ae14be92564ba064f2f5f26654230eac384ae6a642e3aacc25ca","last_reissued_at":"2026-07-05T05:10:16.327645Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T05:10:16.327645Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The luminous Type IIN supernova SN 2017hcc: Infrared bright, X-ray and radio faint","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Nicholas J. H. James, Ori D. Fox, Poonam Chandra, Roger A. Chevalier","submitted_at":"2022-10-06T21:15:57Z","abstract_excerpt":"We present multiwavelength observations of supernova (SN) 2017hcc with the Chandra X-ray telescope and the X-ray telescope onboard Swift (Swift-XRT) in X-ray bands, with the Spitzer and the TripleSpec spectrometer in near-infrared (IR) and mid-IR bands and with the Karl G. Jansky Very Large Array (VLA) for radio bands. The X-ray observations cover a period of 29 to 1310 days, with the first X-ray detection on day 727 with the Chandra. The SN was subsequently detected in the VLA radio bands from day 1000 onwards. While the radio data are sparse, synchrotron-self absorption is clearly ruled out "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2210.03212","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/2210.03212/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":"2210.03212","created_at":"2026-07-05T05:10:16.327700+00:00"},{"alias_kind":"arxiv_version","alias_value":"2210.03212v1","created_at":"2026-07-05T05:10:16.327700+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2210.03212","created_at":"2026-07-05T05:10:16.327700+00:00"},{"alias_kind":"pith_short_12","alias_value":"SV6TGCHWIWXB","created_at":"2026-07-05T05:10:16.327700+00:00"},{"alias_kind":"pith_short_16","alias_value":"SV6TGCHWIWXBJPUS","created_at":"2026-07-05T05:10:16.327700+00:00"},{"alias_kind":"pith_short_8","alias_value":"SV6TGCHW","created_at":"2026-07-05T05:10:16.327700+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/SV6TGCHWIWXBJPUSKZF2AZHS6X","json":"https://pith.science/pith/SV6TGCHWIWXBJPUSKZF2AZHS6X.json","graph_json":"https://pith.science/api/pith-number/SV6TGCHWIWXBJPUSKZF2AZHS6X/graph.json","events_json":"https://pith.science/api/pith-number/SV6TGCHWIWXBJPUSKZF2AZHS6X/events.json","paper":"https://pith.science/paper/SV6TGCHW"},"agent_actions":{"view_html":"https://pith.science/pith/SV6TGCHWIWXBJPUSKZF2AZHS6X","download_json":"https://pith.science/pith/SV6TGCHWIWXBJPUSKZF2AZHS6X.json","view_paper":"https://pith.science/paper/SV6TGCHW","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2210.03212&json=true","fetch_graph":"https://pith.science/api/pith-number/SV6TGCHWIWXBJPUSKZF2AZHS6X/graph.json","fetch_events":"https://pith.science/api/pith-number/SV6TGCHWIWXBJPUSKZF2AZHS6X/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/SV6TGCHWIWXBJPUSKZF2AZHS6X/action/timestamp_anchor","attest_storage":"https://pith.science/pith/SV6TGCHWIWXBJPUSKZF2AZHS6X/action/storage_attestation","attest_author":"https://pith.science/pith/SV6TGCHWIWXBJPUSKZF2AZHS6X/action/author_attestation","sign_citation":"https://pith.science/pith/SV6TGCHWIWXBJPUSKZF2AZHS6X/action/citation_signature","submit_replication":"https://pith.science/pith/SV6TGCHWIWXBJPUSKZF2AZHS6X/action/replication_record"}},"created_at":"2026-07-05T05:10:16.327700+00:00","updated_at":"2026-07-05T05:10:16.327700+00:00"}