{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2018:2HDEA6OTHMBRGQIXPFVI7AE7Y3","short_pith_number":"pith:2HDEA6OT","schema_version":"1.0","canonical_sha256":"d1c64079d33b03134117796a8f809fc6de853635f226952f55762339c799d80b","source":{"kind":"arxiv","id":"1811.08915","version":1},"attestation_state":"computed","paper":{"title":"Telluric correction in the near-infrared: Standard star or synthetic transmission?","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.IM","authors_text":"J. J. Neal, M. Bonnefoy, N. C. Santos, P. Figueira, S. Ulmer-Moll","submitted_at":"2018-11-21T19:05:06Z","abstract_excerpt":"Context. The atmospheric absorption of the Earth is an important limiting factor for ground-based spectroscopic observations and the near-infrared and infrared regions are the most affected. Several software packages that produce a synthetic atmospheric transmission spectrum have been developed to correct for the telluric absorption; these are Molecfit, TelFit, and TAPAS. Aims. Our goal is to compare the correction achieved using these three telluric correction packages and the division by a telluric standard star. We want to evaluate the best method to correct near-infrared high-resolution sp"},"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":"1811.08915","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.IM","submitted_at":"2018-11-21T19:05:06Z","cross_cats_sorted":[],"title_canon_sha256":"2667dd03d761270a03d6a4e77c61d5c1d146e4134b2226794a68023d63bee969","abstract_canon_sha256":"e004c6534598e8ef91a06b6e975dbf8ed5e4445feb2c3517694f4e5496ced420"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-17T23:56:16.717441Z","signature_b64":"NpXrXK84byShK80vqX6iMm7dAjrG4LYL8mtSMJOtVam0Ru2UrtDREB31wwJP/sbB/xJC60fDYs4JOuI2GukPDA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"d1c64079d33b03134117796a8f809fc6de853635f226952f55762339c799d80b","last_reissued_at":"2026-05-17T23:56:16.716799Z","signature_status":"signed_v1","first_computed_at":"2026-05-17T23:56:16.716799Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Telluric correction in the near-infrared: Standard star or synthetic transmission?","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.IM","authors_text":"J. J. Neal, M. Bonnefoy, N. C. Santos, P. Figueira, S. Ulmer-Moll","submitted_at":"2018-11-21T19:05:06Z","abstract_excerpt":"Context. The atmospheric absorption of the Earth is an important limiting factor for ground-based spectroscopic observations and the near-infrared and infrared regions are the most affected. Several software packages that produce a synthetic atmospheric transmission spectrum have been developed to correct for the telluric absorption; these are Molecfit, TelFit, and TAPAS. Aims. Our goal is to compare the correction achieved using these three telluric correction packages and the division by a telluric standard star. We want to evaluate the best method to correct near-infrared high-resolution sp"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1811.08915","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":"1811.08915","created_at":"2026-05-17T23:56:16.716902+00:00"},{"alias_kind":"arxiv_version","alias_value":"1811.08915v1","created_at":"2026-05-17T23:56:16.716902+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1811.08915","created_at":"2026-05-17T23:56:16.716902+00:00"},{"alias_kind":"pith_short_12","alias_value":"2HDEA6OTHMBR","created_at":"2026-05-18T12:32:02.567920+00:00"},{"alias_kind":"pith_short_16","alias_value":"2HDEA6OTHMBRGQIX","created_at":"2026-05-18T12:32:02.567920+00:00"},{"alias_kind":"pith_short_8","alias_value":"2HDEA6OT","created_at":"2026-05-18T12:32:02.567920+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/2HDEA6OTHMBRGQIXPFVI7AE7Y3","json":"https://pith.science/pith/2HDEA6OTHMBRGQIXPFVI7AE7Y3.json","graph_json":"https://pith.science/api/pith-number/2HDEA6OTHMBRGQIXPFVI7AE7Y3/graph.json","events_json":"https://pith.science/api/pith-number/2HDEA6OTHMBRGQIXPFVI7AE7Y3/events.json","paper":"https://pith.science/paper/2HDEA6OT"},"agent_actions":{"view_html":"https://pith.science/pith/2HDEA6OTHMBRGQIXPFVI7AE7Y3","download_json":"https://pith.science/pith/2HDEA6OTHMBRGQIXPFVI7AE7Y3.json","view_paper":"https://pith.science/paper/2HDEA6OT","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1811.08915&json=true","fetch_graph":"https://pith.science/api/pith-number/2HDEA6OTHMBRGQIXPFVI7AE7Y3/graph.json","fetch_events":"https://pith.science/api/pith-number/2HDEA6OTHMBRGQIXPFVI7AE7Y3/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/2HDEA6OTHMBRGQIXPFVI7AE7Y3/action/timestamp_anchor","attest_storage":"https://pith.science/pith/2HDEA6OTHMBRGQIXPFVI7AE7Y3/action/storage_attestation","attest_author":"https://pith.science/pith/2HDEA6OTHMBRGQIXPFVI7AE7Y3/action/author_attestation","sign_citation":"https://pith.science/pith/2HDEA6OTHMBRGQIXPFVI7AE7Y3/action/citation_signature","submit_replication":"https://pith.science/pith/2HDEA6OTHMBRGQIXPFVI7AE7Y3/action/replication_record"}},"created_at":"2026-05-17T23:56:16.716902+00:00","updated_at":"2026-05-17T23:56:16.716902+00:00"}