{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2009:P3SSUZUE34CLUX2HMP2UI2VRA5","short_pith_number":"pith:P3SSUZUE","schema_version":"1.0","canonical_sha256":"7ee52a6684df04ba5f4763f5446ab10755498a5c50c6d4083001597dbe30dbff","source":{"kind":"arxiv","id":"0912.1133","version":2},"attestation_state":"computed","paper":{"title":"Nightside Pollution of Exoplanet Transit Depths","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.EP","authors_text":"David M. Kipping, Giovanna Tinetti","submitted_at":"2009-12-06T20:55:12Z","abstract_excerpt":"Out of the known transiting extrasolar planets, the majority are gas giants orbiting their host star at close proximity. Both theoretical and observational studies support the hypothesis that such bodies emit significant amounts of flux relative to the host star, increasing towards infrared wavelengths. For the dayside of the exoplanet, this phenomenon typically permits detectable secondary eclipses at such wavelengths, which may be used to infer atmospheric composition. In this paper, we explore the effects of emission from the nightside of the exoplanet on the primary transit lightcurve, whi"},"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":"0912.1133","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.EP","submitted_at":"2009-12-06T20:55:12Z","cross_cats_sorted":[],"title_canon_sha256":"d8d48efcd6ee2bbf2211f03cc8b543790c4728c0ef36521a5b9debe6e98da72c","abstract_canon_sha256":"e72d649be51eef4e72af2a7a374a9217b27df7fedb736f62c08f6efcaaeddd5a"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T04:25:01.688909Z","signature_b64":"7U2dLJskN5psMo161Itgh3ijux9kOIWczKvYRfvWLDXF5D4EJvWdpwPJCbSi7mq15+LXWF8UNfBY6bEqer8qBQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"7ee52a6684df04ba5f4763f5446ab10755498a5c50c6d4083001597dbe30dbff","last_reissued_at":"2026-05-18T04:25:01.688364Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T04:25:01.688364Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Nightside Pollution of Exoplanet Transit Depths","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.EP","authors_text":"David M. Kipping, Giovanna Tinetti","submitted_at":"2009-12-06T20:55:12Z","abstract_excerpt":"Out of the known transiting extrasolar planets, the majority are gas giants orbiting their host star at close proximity. Both theoretical and observational studies support the hypothesis that such bodies emit significant amounts of flux relative to the host star, increasing towards infrared wavelengths. For the dayside of the exoplanet, this phenomenon typically permits detectable secondary eclipses at such wavelengths, which may be used to infer atmospheric composition. In this paper, we explore the effects of emission from the nightside of the exoplanet on the primary transit lightcurve, whi"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"0912.1133","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":"0912.1133","created_at":"2026-05-18T04:25:01.688477+00:00"},{"alias_kind":"arxiv_version","alias_value":"0912.1133v2","created_at":"2026-05-18T04:25:01.688477+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.0912.1133","created_at":"2026-05-18T04:25:01.688477+00:00"},{"alias_kind":"pith_short_12","alias_value":"P3SSUZUE34CL","created_at":"2026-05-18T12:26:01.383474+00:00"},{"alias_kind":"pith_short_16","alias_value":"P3SSUZUE34CLUX2H","created_at":"2026-05-18T12:26:01.383474+00:00"},{"alias_kind":"pith_short_8","alias_value":"P3SSUZUE","created_at":"2026-05-18T12:26:01.383474+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/P3SSUZUE34CLUX2HMP2UI2VRA5","json":"https://pith.science/pith/P3SSUZUE34CLUX2HMP2UI2VRA5.json","graph_json":"https://pith.science/api/pith-number/P3SSUZUE34CLUX2HMP2UI2VRA5/graph.json","events_json":"https://pith.science/api/pith-number/P3SSUZUE34CLUX2HMP2UI2VRA5/events.json","paper":"https://pith.science/paper/P3SSUZUE"},"agent_actions":{"view_html":"https://pith.science/pith/P3SSUZUE34CLUX2HMP2UI2VRA5","download_json":"https://pith.science/pith/P3SSUZUE34CLUX2HMP2UI2VRA5.json","view_paper":"https://pith.science/paper/P3SSUZUE","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=0912.1133&json=true","fetch_graph":"https://pith.science/api/pith-number/P3SSUZUE34CLUX2HMP2UI2VRA5/graph.json","fetch_events":"https://pith.science/api/pith-number/P3SSUZUE34CLUX2HMP2UI2VRA5/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/P3SSUZUE34CLUX2HMP2UI2VRA5/action/timestamp_anchor","attest_storage":"https://pith.science/pith/P3SSUZUE34CLUX2HMP2UI2VRA5/action/storage_attestation","attest_author":"https://pith.science/pith/P3SSUZUE34CLUX2HMP2UI2VRA5/action/author_attestation","sign_citation":"https://pith.science/pith/P3SSUZUE34CLUX2HMP2UI2VRA5/action/citation_signature","submit_replication":"https://pith.science/pith/P3SSUZUE34CLUX2HMP2UI2VRA5/action/replication_record"}},"created_at":"2026-05-18T04:25:01.688477+00:00","updated_at":"2026-05-18T04:25:01.688477+00:00"}