{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2016:VHHM4EPH72ZFVECUJ6A3WICQVI","short_pith_number":"pith:VHHM4EPH","schema_version":"1.0","canonical_sha256":"a9cece11e7feb25a90544f81bb2050aa316de3664befac50326bcaf98c97fdf7","source":{"kind":"arxiv","id":"1611.03871","version":1},"attestation_state":"computed","paper":{"title":"Exo-Transmit: An Open-Source Code for Calculating Transmission Spectra for Exoplanet Atmospheres of Varied Composition","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.EP","authors_text":"Albert Owusu-Asare, Bryson Cale, Eliza M.-R. Kempton, Patrick Slough, Roxana E. Lupu","submitted_at":"2016-11-11T21:00:13Z","abstract_excerpt":"We present Exo-Transmit, a software package to calculate exoplanet transmission spectra for planets of varied composition. The code is designed to generate spectra of planets with a wide range of atmospheric composition, temperature, surface gravity, and size, and is therefore applicable to exoplanets ranging in mass and size from hot Jupiters down to rocky super-Earths. Spectra can be generated with or without clouds or hazes with options to (1) include an optically thick cloud deck at a user-specified atmospheric pressure or (2) to augment the nominal Rayleigh scattering by a user-specified "},"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":"1611.03871","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.EP","submitted_at":"2016-11-11T21:00:13Z","cross_cats_sorted":[],"title_canon_sha256":"ae5df144a9f048aff1a103ef31c7fcceb32e0c3126c1d1584815ba1da2f24654","abstract_canon_sha256":"11a7e41cfd0ef0ff78bce83cc1a52e2099e06767fb1a13c01872fb101c97455a"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:48:16.297790Z","signature_b64":"4Scgm3wRNE/5402Luxnpp0wSGNGLXzalprFXvFd8DyY4qyq0R6aldHCgBzYYXIOAaH18A2JUU1RFyK8QLS8AAA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"a9cece11e7feb25a90544f81bb2050aa316de3664befac50326bcaf98c97fdf7","last_reissued_at":"2026-05-18T00:48:16.296972Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:48:16.296972Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Exo-Transmit: An Open-Source Code for Calculating Transmission Spectra for Exoplanet Atmospheres of Varied Composition","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.EP","authors_text":"Albert Owusu-Asare, Bryson Cale, Eliza M.-R. Kempton, Patrick Slough, Roxana E. Lupu","submitted_at":"2016-11-11T21:00:13Z","abstract_excerpt":"We present Exo-Transmit, a software package to calculate exoplanet transmission spectra for planets of varied composition. The code is designed to generate spectra of planets with a wide range of atmospheric composition, temperature, surface gravity, and size, and is therefore applicable to exoplanets ranging in mass and size from hot Jupiters down to rocky super-Earths. Spectra can be generated with or without clouds or hazes with options to (1) include an optically thick cloud deck at a user-specified atmospheric pressure or (2) to augment the nominal Rayleigh scattering by a user-specified "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1611.03871","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":"1611.03871","created_at":"2026-05-18T00:48:16.297128+00:00"},{"alias_kind":"arxiv_version","alias_value":"1611.03871v1","created_at":"2026-05-18T00:48:16.297128+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1611.03871","created_at":"2026-05-18T00:48:16.297128+00:00"},{"alias_kind":"pith_short_12","alias_value":"VHHM4EPH72ZF","created_at":"2026-05-18T12:30:48.956258+00:00"},{"alias_kind":"pith_short_16","alias_value":"VHHM4EPH72ZFVECU","created_at":"2026-05-18T12:30:48.956258+00:00"},{"alias_kind":"pith_short_8","alias_value":"VHHM4EPH","created_at":"2026-05-18T12:30:48.956258+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/VHHM4EPH72ZFVECUJ6A3WICQVI","json":"https://pith.science/pith/VHHM4EPH72ZFVECUJ6A3WICQVI.json","graph_json":"https://pith.science/api/pith-number/VHHM4EPH72ZFVECUJ6A3WICQVI/graph.json","events_json":"https://pith.science/api/pith-number/VHHM4EPH72ZFVECUJ6A3WICQVI/events.json","paper":"https://pith.science/paper/VHHM4EPH"},"agent_actions":{"view_html":"https://pith.science/pith/VHHM4EPH72ZFVECUJ6A3WICQVI","download_json":"https://pith.science/pith/VHHM4EPH72ZFVECUJ6A3WICQVI.json","view_paper":"https://pith.science/paper/VHHM4EPH","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1611.03871&json=true","fetch_graph":"https://pith.science/api/pith-number/VHHM4EPH72ZFVECUJ6A3WICQVI/graph.json","fetch_events":"https://pith.science/api/pith-number/VHHM4EPH72ZFVECUJ6A3WICQVI/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/VHHM4EPH72ZFVECUJ6A3WICQVI/action/timestamp_anchor","attest_storage":"https://pith.science/pith/VHHM4EPH72ZFVECUJ6A3WICQVI/action/storage_attestation","attest_author":"https://pith.science/pith/VHHM4EPH72ZFVECUJ6A3WICQVI/action/author_attestation","sign_citation":"https://pith.science/pith/VHHM4EPH72ZFVECUJ6A3WICQVI/action/citation_signature","submit_replication":"https://pith.science/pith/VHHM4EPH72ZFVECUJ6A3WICQVI/action/replication_record"}},"created_at":"2026-05-18T00:48:16.297128+00:00","updated_at":"2026-05-18T00:48:16.297128+00:00"}