{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2016:MVRVX3JFXWBADQEEUSFS5YMOCW","short_pith_number":"pith:MVRVX3JF","schema_version":"1.0","canonical_sha256":"65635bed25bd8201c084a48b2ee18e15a9b1d67f126ef6a371dda54eec8af3f6","source":{"kind":"arxiv","id":"1611.05925","version":1},"attestation_state":"computed","paper":{"title":"Odd Harmonics in Exoplanet Photometry: Weather or Artifact?","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.SR"],"primary_cat":"astro-ph.EP","authors_text":"Elie Bouffard, Hal M. Haggard, Max Meynig, Nicolas B. Cowan, Victoria Chayes","submitted_at":"2016-11-17T22:28:59Z","abstract_excerpt":"Photometry of short-period planetary systems allows astronomers to monitor exoplanets, their host stars, and their mutual interactions. In addition to the transits of a planet in front of its star and the eclipses of the planet by its star, researchers have reported flux variations at the orbital frequency and its harmonics: planetary reflection and/or emission and Doppler beaming of starlight produce one peak per orbit, while ellipsoidal variations of a tidally distorted star and/or planet produce two maxima per orbit. Researchers have also reported significant photometric variability at thre"},"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":"1611.05925","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.EP","submitted_at":"2016-11-17T22:28:59Z","cross_cats_sorted":["astro-ph.SR"],"title_canon_sha256":"0a435aba1d2f7f7b2d11d3a43f1fd0d220aee2f31d95cc990d66e466f6c0f15c","abstract_canon_sha256":"251d1f824ee95ef187cf5274351a3efa1779d34c5a7ddaa2f2e3fb03e614025f"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:52:13.827264Z","signature_b64":"VSoQnVhIIoXJe1P/i04DjsYIBZJs8At95/uERi33fTJyXsgpy/yusxJ4oBBomRNojgTcX0K9KTQm76+qaRPkAQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"65635bed25bd8201c084a48b2ee18e15a9b1d67f126ef6a371dda54eec8af3f6","last_reissued_at":"2026-05-18T00:52:13.826807Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:52:13.826807Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Odd Harmonics in Exoplanet Photometry: Weather or Artifact?","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.SR"],"primary_cat":"astro-ph.EP","authors_text":"Elie Bouffard, Hal M. Haggard, Max Meynig, Nicolas B. Cowan, Victoria Chayes","submitted_at":"2016-11-17T22:28:59Z","abstract_excerpt":"Photometry of short-period planetary systems allows astronomers to monitor exoplanets, their host stars, and their mutual interactions. In addition to the transits of a planet in front of its star and the eclipses of the planet by its star, researchers have reported flux variations at the orbital frequency and its harmonics: planetary reflection and/or emission and Doppler beaming of starlight produce one peak per orbit, while ellipsoidal variations of a tidally distorted star and/or planet produce two maxima per orbit. Researchers have also reported significant photometric variability at thre"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1611.05925","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":"1611.05925","created_at":"2026-05-18T00:52:13.826868+00:00"},{"alias_kind":"arxiv_version","alias_value":"1611.05925v1","created_at":"2026-05-18T00:52:13.826868+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1611.05925","created_at":"2026-05-18T00:52:13.826868+00:00"},{"alias_kind":"pith_short_12","alias_value":"MVRVX3JFXWBA","created_at":"2026-05-18T12:30:32.724797+00:00"},{"alias_kind":"pith_short_16","alias_value":"MVRVX3JFXWBADQEE","created_at":"2026-05-18T12:30:32.724797+00:00"},{"alias_kind":"pith_short_8","alias_value":"MVRVX3JF","created_at":"2026-05-18T12:30:32.724797+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/MVRVX3JFXWBADQEEUSFS5YMOCW","json":"https://pith.science/pith/MVRVX3JFXWBADQEEUSFS5YMOCW.json","graph_json":"https://pith.science/api/pith-number/MVRVX3JFXWBADQEEUSFS5YMOCW/graph.json","events_json":"https://pith.science/api/pith-number/MVRVX3JFXWBADQEEUSFS5YMOCW/events.json","paper":"https://pith.science/paper/MVRVX3JF"},"agent_actions":{"view_html":"https://pith.science/pith/MVRVX3JFXWBADQEEUSFS5YMOCW","download_json":"https://pith.science/pith/MVRVX3JFXWBADQEEUSFS5YMOCW.json","view_paper":"https://pith.science/paper/MVRVX3JF","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1611.05925&json=true","fetch_graph":"https://pith.science/api/pith-number/MVRVX3JFXWBADQEEUSFS5YMOCW/graph.json","fetch_events":"https://pith.science/api/pith-number/MVRVX3JFXWBADQEEUSFS5YMOCW/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/MVRVX3JFXWBADQEEUSFS5YMOCW/action/timestamp_anchor","attest_storage":"https://pith.science/pith/MVRVX3JFXWBADQEEUSFS5YMOCW/action/storage_attestation","attest_author":"https://pith.science/pith/MVRVX3JFXWBADQEEUSFS5YMOCW/action/author_attestation","sign_citation":"https://pith.science/pith/MVRVX3JFXWBADQEEUSFS5YMOCW/action/citation_signature","submit_replication":"https://pith.science/pith/MVRVX3JFXWBADQEEUSFS5YMOCW/action/replication_record"}},"created_at":"2026-05-18T00:52:13.826868+00:00","updated_at":"2026-05-18T00:52:13.826868+00:00"}