{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2019:KP4MJDD72GHB4UN242G5I2ZEIK","short_pith_number":"pith:KP4MJDD7","schema_version":"1.0","canonical_sha256":"53f8c48c7fd18e1e51bae68dd46b2442a4fa4daaa2674e4e38ba9fc691219499","source":{"kind":"arxiv","id":"1905.12662","version":1},"attestation_state":"computed","paper":{"title":"Reflected Light Phase Curves in the TESS Era","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.EP","authors_text":"L. C. Mayorga, M. S. Marley, N. E. Batalha, N. K. Lewis","submitted_at":"2019-05-29T18:15:39Z","abstract_excerpt":"The reflected light signal from a planet throughout its orbit is a powerful probe of a planet's atmospheric properties. There are a number of planets that are amenable to reflected light phase curve studies with present and future space-based instrumentation and here we assess our ability to characterize these worlds. Using simulated TESS populations we identify the Nine, a set of archetypal exoplanets with the potential to be bright in reflected light, because of their radii and proximity to their star, while still being cool enough to have minimal thermal contamination at optical wavelengths"},"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":"1905.12662","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.EP","submitted_at":"2019-05-29T18:15:39Z","cross_cats_sorted":[],"title_canon_sha256":"62d5f5303a64149b9f77a72a81e9d8d32538493a6a97ed57e7abba072d473d7c","abstract_canon_sha256":"c5731160223aebf3a8da16fd968c1b20bc67c31e1e3b931d8d6670035327850b"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-17T23:39:43.393567Z","signature_b64":"FnJ6/k8/m5fiAFvCdQ4iz5wXq85EQA2O1AneINyrTV3kYleDwulX3JNx37PeiqkBvmX/0L+LZfGo27PUuCFpAA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"53f8c48c7fd18e1e51bae68dd46b2442a4fa4daaa2674e4e38ba9fc691219499","last_reissued_at":"2026-05-17T23:39:43.392929Z","signature_status":"signed_v1","first_computed_at":"2026-05-17T23:39:43.392929Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Reflected Light Phase Curves in the TESS Era","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.EP","authors_text":"L. C. Mayorga, M. S. Marley, N. E. Batalha, N. K. Lewis","submitted_at":"2019-05-29T18:15:39Z","abstract_excerpt":"The reflected light signal from a planet throughout its orbit is a powerful probe of a planet's atmospheric properties. There are a number of planets that are amenable to reflected light phase curve studies with present and future space-based instrumentation and here we assess our ability to characterize these worlds. Using simulated TESS populations we identify the Nine, a set of archetypal exoplanets with the potential to be bright in reflected light, because of their radii and proximity to their star, while still being cool enough to have minimal thermal contamination at optical wavelengths"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1905.12662","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":"1905.12662","created_at":"2026-05-17T23:39:43.393054+00:00"},{"alias_kind":"arxiv_version","alias_value":"1905.12662v1","created_at":"2026-05-17T23:39:43.393054+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1905.12662","created_at":"2026-05-17T23:39:43.393054+00:00"},{"alias_kind":"pith_short_12","alias_value":"KP4MJDD72GHB","created_at":"2026-05-18T12:33:21.387695+00:00"},{"alias_kind":"pith_short_16","alias_value":"KP4MJDD72GHB4UN2","created_at":"2026-05-18T12:33:21.387695+00:00"},{"alias_kind":"pith_short_8","alias_value":"KP4MJDD7","created_at":"2026-05-18T12:33:21.387695+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/KP4MJDD72GHB4UN242G5I2ZEIK","json":"https://pith.science/pith/KP4MJDD72GHB4UN242G5I2ZEIK.json","graph_json":"https://pith.science/api/pith-number/KP4MJDD72GHB4UN242G5I2ZEIK/graph.json","events_json":"https://pith.science/api/pith-number/KP4MJDD72GHB4UN242G5I2ZEIK/events.json","paper":"https://pith.science/paper/KP4MJDD7"},"agent_actions":{"view_html":"https://pith.science/pith/KP4MJDD72GHB4UN242G5I2ZEIK","download_json":"https://pith.science/pith/KP4MJDD72GHB4UN242G5I2ZEIK.json","view_paper":"https://pith.science/paper/KP4MJDD7","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1905.12662&json=true","fetch_graph":"https://pith.science/api/pith-number/KP4MJDD72GHB4UN242G5I2ZEIK/graph.json","fetch_events":"https://pith.science/api/pith-number/KP4MJDD72GHB4UN242G5I2ZEIK/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/KP4MJDD72GHB4UN242G5I2ZEIK/action/timestamp_anchor","attest_storage":"https://pith.science/pith/KP4MJDD72GHB4UN242G5I2ZEIK/action/storage_attestation","attest_author":"https://pith.science/pith/KP4MJDD72GHB4UN242G5I2ZEIK/action/author_attestation","sign_citation":"https://pith.science/pith/KP4MJDD72GHB4UN242G5I2ZEIK/action/citation_signature","submit_replication":"https://pith.science/pith/KP4MJDD72GHB4UN242G5I2ZEIK/action/replication_record"}},"created_at":"2026-05-17T23:39:43.393054+00:00","updated_at":"2026-05-17T23:39:43.393054+00:00"}