{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2016:XVPXP22R5ISKQEUUUSCCFWOQT3","short_pith_number":"pith:XVPXP22R","schema_version":"1.0","canonical_sha256":"bd5f77eb51ea24a81294a48422d9d09ecb49b33ca19a25a70e70ae3818dc7454","source":{"kind":"arxiv","id":"1606.05474","version":2},"attestation_state":"computed","paper":{"title":"HELIOS: An Open-source, GPU-accelerated Radiative Transfer Code For Self-consistent Exoplanetary Atmospheres","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["physics.ao-ph"],"primary_cat":"astro-ph.EP","authors_text":"Adam Burrows, Baptiste Lavie, Daniel Kitzmann, Jacob L. Bean, Jo\\~ao M. Mendon\\c{c}a, Kevin B. Stevenson, Kevin Heng, Laura Kreidberg, Luc Grosheintz, Matej Malik, Megan Bedell, Shang-Min Tsai, Simon L. Grimm","submitted_at":"2016-06-17T11:01:09Z","abstract_excerpt":"We present the open-source radiative transfer code named HELIOS, which is constructed for studying exoplanetary atmospheres. In its initial version, the model atmospheres of HELIOS are one-dimensional and plane-parallel, and the equation of radiative transfer is solved in the two-stream approximation with non-isotropic scattering. A small set of the main infrared absorbers is employed, computed with the opacity calculator HELIOS-K and combined using a correlated-$k$ approximation. The molecular abundances originate from validated analytical formulae for equilibrium chemistry. We compare HELIOS"},"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":"1606.05474","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.EP","submitted_at":"2016-06-17T11:01:09Z","cross_cats_sorted":["physics.ao-ph"],"title_canon_sha256":"ff5bb9b20d2c95752311eef67e5895150a952b76f94abe187fb46982a9406e28","abstract_canon_sha256":"c0dcddd16db2c3de5d00f9fd4758427e669343c6b31a6790e5bd39270b7f00a3"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:52:39.467307Z","signature_b64":"fBfJ7HrR3IwD1iXNsnUMYjamzU/Rw9lDTayRDEehyleZT/YFtezXgmqX6JQtq/0tor4n/FM7g3xafrbeMt/4DQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"bd5f77eb51ea24a81294a48422d9d09ecb49b33ca19a25a70e70ae3818dc7454","last_reissued_at":"2026-05-18T00:52:39.466733Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:52:39.466733Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"HELIOS: An Open-source, GPU-accelerated Radiative Transfer Code For Self-consistent Exoplanetary Atmospheres","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["physics.ao-ph"],"primary_cat":"astro-ph.EP","authors_text":"Adam Burrows, Baptiste Lavie, Daniel Kitzmann, Jacob L. Bean, Jo\\~ao M. Mendon\\c{c}a, Kevin B. Stevenson, Kevin Heng, Laura Kreidberg, Luc Grosheintz, Matej Malik, Megan Bedell, Shang-Min Tsai, Simon L. Grimm","submitted_at":"2016-06-17T11:01:09Z","abstract_excerpt":"We present the open-source radiative transfer code named HELIOS, which is constructed for studying exoplanetary atmospheres. In its initial version, the model atmospheres of HELIOS are one-dimensional and plane-parallel, and the equation of radiative transfer is solved in the two-stream approximation with non-isotropic scattering. A small set of the main infrared absorbers is employed, computed with the opacity calculator HELIOS-K and combined using a correlated-$k$ approximation. The molecular abundances originate from validated analytical formulae for equilibrium chemistry. We compare HELIOS"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1606.05474","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":"1606.05474","created_at":"2026-05-18T00:52:39.466829+00:00"},{"alias_kind":"arxiv_version","alias_value":"1606.05474v2","created_at":"2026-05-18T00:52:39.466829+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1606.05474","created_at":"2026-05-18T00:52:39.466829+00:00"},{"alias_kind":"pith_short_12","alias_value":"XVPXP22R5ISK","created_at":"2026-05-18T12:30:51.357362+00:00"},{"alias_kind":"pith_short_16","alias_value":"XVPXP22R5ISKQEUU","created_at":"2026-05-18T12:30:51.357362+00:00"},{"alias_kind":"pith_short_8","alias_value":"XVPXP22R","created_at":"2026-05-18T12:30:51.357362+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/XVPXP22R5ISKQEUUUSCCFWOQT3","json":"https://pith.science/pith/XVPXP22R5ISKQEUUUSCCFWOQT3.json","graph_json":"https://pith.science/api/pith-number/XVPXP22R5ISKQEUUUSCCFWOQT3/graph.json","events_json":"https://pith.science/api/pith-number/XVPXP22R5ISKQEUUUSCCFWOQT3/events.json","paper":"https://pith.science/paper/XVPXP22R"},"agent_actions":{"view_html":"https://pith.science/pith/XVPXP22R5ISKQEUUUSCCFWOQT3","download_json":"https://pith.science/pith/XVPXP22R5ISKQEUUUSCCFWOQT3.json","view_paper":"https://pith.science/paper/XVPXP22R","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1606.05474&json=true","fetch_graph":"https://pith.science/api/pith-number/XVPXP22R5ISKQEUUUSCCFWOQT3/graph.json","fetch_events":"https://pith.science/api/pith-number/XVPXP22R5ISKQEUUUSCCFWOQT3/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/XVPXP22R5ISKQEUUUSCCFWOQT3/action/timestamp_anchor","attest_storage":"https://pith.science/pith/XVPXP22R5ISKQEUUUSCCFWOQT3/action/storage_attestation","attest_author":"https://pith.science/pith/XVPXP22R5ISKQEUUUSCCFWOQT3/action/author_attestation","sign_citation":"https://pith.science/pith/XVPXP22R5ISKQEUUUSCCFWOQT3/action/citation_signature","submit_replication":"https://pith.science/pith/XVPXP22R5ISKQEUUUSCCFWOQT3/action/replication_record"}},"created_at":"2026-05-18T00:52:39.466829+00:00","updated_at":"2026-05-18T00:52:39.466829+00:00"}