{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2009:7MSMEFD5RM5CIQ7LNFC4ZEEETS","short_pith_number":"pith:7MSMEFD5","schema_version":"1.0","canonical_sha256":"fb24c2147d8b3a2443eb6945cc90849c93638d9910541d93c348501f536b2dd9","source":{"kind":"arxiv","id":"0905.4624","version":1},"attestation_state":"computed","paper":{"title":"Detection and evolution of the CO (v = 2) emission in nova V2615 Ophiuchi (2007)","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"Dipankar P. K. Banerjee, N. M. Ashok, Ramkrishna Das","submitted_at":"2009-05-28T12:00:31Z","abstract_excerpt":"We present near-infrared (1 - 2.5 micron) spectroscopic and photometric results of Nova V2615 Ophiuchi which was discovered in outburst in 2007 March. Our observations span a period of ~ 80 days starting from 2007 March 28 when the nova was at its maximum light. The evolution of the spectra are shown from the initial P-Cygni phase to an emission-line phase and finally to a dust formation stage. The characteristics of the JHK spectra are very similar to those observed in a nova outburst occurring on a carbon-oxygen white dwarf. We analyse an observed line at 2.088 micron and suggest it could be"},"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":"0905.4624","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2009-05-28T12:00:31Z","cross_cats_sorted":[],"title_canon_sha256":"26273fc0fbdbd27e3571380789b33ee27064601ae73aa0f501e9d26760e8b25b","abstract_canon_sha256":"01d5ba3802e5b29707f4c58279eef2fdac74acac825b90505e5f9352bce6b8e5"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:13:31.223731Z","signature_b64":"KPBl7iq9gnEf3PVNhHio+pdV3OEVFvc8+gWUGgMUaSIkeRmF7Thz1U8qINvXtOVskSWgJrviySdZth4/B21ZCg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"fb24c2147d8b3a2443eb6945cc90849c93638d9910541d93c348501f536b2dd9","last_reissued_at":"2026-05-18T02:13:31.222950Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:13:31.222950Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Detection and evolution of the CO (v = 2) emission in nova V2615 Ophiuchi (2007)","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"Dipankar P. K. Banerjee, N. M. Ashok, Ramkrishna Das","submitted_at":"2009-05-28T12:00:31Z","abstract_excerpt":"We present near-infrared (1 - 2.5 micron) spectroscopic and photometric results of Nova V2615 Ophiuchi which was discovered in outburst in 2007 March. Our observations span a period of ~ 80 days starting from 2007 March 28 when the nova was at its maximum light. The evolution of the spectra are shown from the initial P-Cygni phase to an emission-line phase and finally to a dust formation stage. The characteristics of the JHK spectra are very similar to those observed in a nova outburst occurring on a carbon-oxygen white dwarf. We analyse an observed line at 2.088 micron and suggest it could be"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"0905.4624","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":"0905.4624","created_at":"2026-05-18T02:13:31.223087+00:00"},{"alias_kind":"arxiv_version","alias_value":"0905.4624v1","created_at":"2026-05-18T02:13:31.223087+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.0905.4624","created_at":"2026-05-18T02:13:31.223087+00:00"},{"alias_kind":"pith_short_12","alias_value":"7MSMEFD5RM5C","created_at":"2026-05-18T12:25:58.837520+00:00"},{"alias_kind":"pith_short_16","alias_value":"7MSMEFD5RM5CIQ7L","created_at":"2026-05-18T12:25:58.837520+00:00"},{"alias_kind":"pith_short_8","alias_value":"7MSMEFD5","created_at":"2026-05-18T12:25:58.837520+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/7MSMEFD5RM5CIQ7LNFC4ZEEETS","json":"https://pith.science/pith/7MSMEFD5RM5CIQ7LNFC4ZEEETS.json","graph_json":"https://pith.science/api/pith-number/7MSMEFD5RM5CIQ7LNFC4ZEEETS/graph.json","events_json":"https://pith.science/api/pith-number/7MSMEFD5RM5CIQ7LNFC4ZEEETS/events.json","paper":"https://pith.science/paper/7MSMEFD5"},"agent_actions":{"view_html":"https://pith.science/pith/7MSMEFD5RM5CIQ7LNFC4ZEEETS","download_json":"https://pith.science/pith/7MSMEFD5RM5CIQ7LNFC4ZEEETS.json","view_paper":"https://pith.science/paper/7MSMEFD5","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=0905.4624&json=true","fetch_graph":"https://pith.science/api/pith-number/7MSMEFD5RM5CIQ7LNFC4ZEEETS/graph.json","fetch_events":"https://pith.science/api/pith-number/7MSMEFD5RM5CIQ7LNFC4ZEEETS/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/7MSMEFD5RM5CIQ7LNFC4ZEEETS/action/timestamp_anchor","attest_storage":"https://pith.science/pith/7MSMEFD5RM5CIQ7LNFC4ZEEETS/action/storage_attestation","attest_author":"https://pith.science/pith/7MSMEFD5RM5CIQ7LNFC4ZEEETS/action/author_attestation","sign_citation":"https://pith.science/pith/7MSMEFD5RM5CIQ7LNFC4ZEEETS/action/citation_signature","submit_replication":"https://pith.science/pith/7MSMEFD5RM5CIQ7LNFC4ZEEETS/action/replication_record"}},"created_at":"2026-05-18T02:13:31.223087+00:00","updated_at":"2026-05-18T02:13:31.223087+00:00"}