{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2014:43SKNB74M4VYR4S5YVKSQTIQMM","short_pith_number":"pith:43SKNB74","schema_version":"1.0","canonical_sha256":"e6e4a687fc672b88f25dc555284d106320b8c24565d44444b68939d3580b94d8","source":{"kind":"arxiv","id":"1406.5531","version":2},"attestation_state":"computed","paper":{"title":"Near infrared spectroscopy of the type IIn SN 2010jl: evidence for high velocity ejecta","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE"],"primary_cat":"astro-ph.SR","authors_text":"Aaron M. Kingery, Benjamin M. Breslauer, Chenliang Huang, George C. Privon, H. Jacob Borish, Roger A. Chevalier","submitted_at":"2014-06-20T20:33:11Z","abstract_excerpt":"The Type IIn supernova SN 2010jl was relatively nearby and luminous, allowing detailed studies of the near-infrared (NIR) emission. We present 1 - 2.4 micron spectroscopy over the age range of 36 - 565 days from the earliest detection of the supernova. On day 36, the H lines show an unresolved narrow emission component along with a symmetric broad component that can be modeled as the result of electron scattering by a thermal distribution of electrons. Over the next hundreds of days, the broad components of the H lines shift to the blue by 700 km/s, as is also observed in optical lines. The na"},"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":"1406.5531","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2014-06-20T20:33:11Z","cross_cats_sorted":["astro-ph.HE"],"title_canon_sha256":"eba2ae7533719be19da5ec29d08dc6e3366a63555a2fe0ef59d69d547f57b4ab","abstract_canon_sha256":"e92bc55c1e5dba7c23b128d8115bdcd3d02132030432510d67a46dbd0dabdc0b"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:25:49.123577Z","signature_b64":"pva7sC6TFt6S8oKfgA37mo1r282YWSnrJHGmvWqNa1RKDbxGbYc/YE8t7Y6qkgGWCUGKSL0/QmX6AMVC4VN+Cg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"e6e4a687fc672b88f25dc555284d106320b8c24565d44444b68939d3580b94d8","last_reissued_at":"2026-05-18T02:25:49.123193Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:25:49.123193Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Near infrared spectroscopy of the type IIn SN 2010jl: evidence for high velocity ejecta","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE"],"primary_cat":"astro-ph.SR","authors_text":"Aaron M. Kingery, Benjamin M. Breslauer, Chenliang Huang, George C. Privon, H. Jacob Borish, Roger A. Chevalier","submitted_at":"2014-06-20T20:33:11Z","abstract_excerpt":"The Type IIn supernova SN 2010jl was relatively nearby and luminous, allowing detailed studies of the near-infrared (NIR) emission. We present 1 - 2.4 micron spectroscopy over the age range of 36 - 565 days from the earliest detection of the supernova. On day 36, the H lines show an unresolved narrow emission component along with a symmetric broad component that can be modeled as the result of electron scattering by a thermal distribution of electrons. Over the next hundreds of days, the broad components of the H lines shift to the blue by 700 km/s, as is also observed in optical lines. The na"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1406.5531","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":""},"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":"1406.5531","created_at":"2026-05-18T02:25:49.123246+00:00"},{"alias_kind":"arxiv_version","alias_value":"1406.5531v2","created_at":"2026-05-18T02:25:49.123246+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1406.5531","created_at":"2026-05-18T02:25:49.123246+00:00"},{"alias_kind":"pith_short_12","alias_value":"43SKNB74M4VY","created_at":"2026-05-18T12:28:11.866339+00:00"},{"alias_kind":"pith_short_16","alias_value":"43SKNB74M4VYR4S5","created_at":"2026-05-18T12:28:11.866339+00:00"},{"alias_kind":"pith_short_8","alias_value":"43SKNB74","created_at":"2026-05-18T12:28:11.866339+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/43SKNB74M4VYR4S5YVKSQTIQMM","json":"https://pith.science/pith/43SKNB74M4VYR4S5YVKSQTIQMM.json","graph_json":"https://pith.science/api/pith-number/43SKNB74M4VYR4S5YVKSQTIQMM/graph.json","events_json":"https://pith.science/api/pith-number/43SKNB74M4VYR4S5YVKSQTIQMM/events.json","paper":"https://pith.science/paper/43SKNB74"},"agent_actions":{"view_html":"https://pith.science/pith/43SKNB74M4VYR4S5YVKSQTIQMM","download_json":"https://pith.science/pith/43SKNB74M4VYR4S5YVKSQTIQMM.json","view_paper":"https://pith.science/paper/43SKNB74","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1406.5531&json=true","fetch_graph":"https://pith.science/api/pith-number/43SKNB74M4VYR4S5YVKSQTIQMM/graph.json","fetch_events":"https://pith.science/api/pith-number/43SKNB74M4VYR4S5YVKSQTIQMM/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/43SKNB74M4VYR4S5YVKSQTIQMM/action/timestamp_anchor","attest_storage":"https://pith.science/pith/43SKNB74M4VYR4S5YVKSQTIQMM/action/storage_attestation","attest_author":"https://pith.science/pith/43SKNB74M4VYR4S5YVKSQTIQMM/action/author_attestation","sign_citation":"https://pith.science/pith/43SKNB74M4VYR4S5YVKSQTIQMM/action/citation_signature","submit_replication":"https://pith.science/pith/43SKNB74M4VYR4S5YVKSQTIQMM/action/replication_record"}},"created_at":"2026-05-18T02:25:49.123246+00:00","updated_at":"2026-05-18T02:25:49.123246+00:00"}