{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2023:GULFAYSWWIYVEJKOGFWSNTJBX7","short_pith_number":"pith:GULFAYSW","schema_version":"1.0","canonical_sha256":"3516506256b23152254e316d26cd21bfe18708cd1f36a0aa8c104b7cf5e36a31","source":{"kind":"arxiv","id":"2303.13732","version":2},"attestation_state":"computed","paper":{"title":"Thermal Emission from the hot Jupiter WASP-103b in J and Ks Bands","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.EP","authors_text":"Gang Zhao, Guo Chen, Jingkun Zhao, Meng Zhai, Nicolas Crouzet, Qinglin Ouyang, Roy van Boekel, Thomas Henning, Wei Wang, Yaqing Shi, Zewen Jiang","submitted_at":"2023-03-24T01:08:50Z","abstract_excerpt":"Hot Jupiters, particularly those with temperature higher than 2000 K are the best sample of planets that allow in-depth characterization of their atmospheres. We present here a thermal emission study of the ultra hot Jupiter WASP-103 b observed in two secondary eclipses with CFHT/WIRCam in J and Ks bands. By means of high precision differential photometry, we determine eclipse depths in J and Ks to an accuracy of 220 and 270 ppm, which are combined with the published HST/WFC3 and Spitzer data to retrieve a joint constraints on the properties of WASP-103 b dayside atmosphere. We find that the a"},"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":"2303.13732","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.EP","submitted_at":"2023-03-24T01:08:50Z","cross_cats_sorted":[],"title_canon_sha256":"89ca27db0f38b257c3438f20074ce63b7bc875c28fbd21d2e3d192a4b34507d8","abstract_canon_sha256":"deae1837cf6239f8ab62856e3e2159b5923660d690154d2084299a802eca9843"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T05:58:10.774446Z","signature_b64":"RPDhlFzHa8Y20ecjG0D7phFtV+RngpUu0/jGQiulFHx3xAC9nNMQEYMTnF9n7+4ZjoirFZnFqxE3BSJreHByDw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"3516506256b23152254e316d26cd21bfe18708cd1f36a0aa8c104b7cf5e36a31","last_reissued_at":"2026-07-05T05:58:10.774050Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T05:58:10.774050Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Thermal Emission from the hot Jupiter WASP-103b in J and Ks Bands","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.EP","authors_text":"Gang Zhao, Guo Chen, Jingkun Zhao, Meng Zhai, Nicolas Crouzet, Qinglin Ouyang, Roy van Boekel, Thomas Henning, Wei Wang, Yaqing Shi, Zewen Jiang","submitted_at":"2023-03-24T01:08:50Z","abstract_excerpt":"Hot Jupiters, particularly those with temperature higher than 2000 K are the best sample of planets that allow in-depth characterization of their atmospheres. We present here a thermal emission study of the ultra hot Jupiter WASP-103 b observed in two secondary eclipses with CFHT/WIRCam in J and Ks bands. By means of high precision differential photometry, we determine eclipse depths in J and Ks to an accuracy of 220 and 270 ppm, which are combined with the published HST/WFC3 and Spitzer data to retrieve a joint constraints on the properties of WASP-103 b dayside atmosphere. We find that the a"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2303.13732","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2303.13732/integrity.json","findings":[],"available":true,"detectors_run":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938"},"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":"2303.13732","created_at":"2026-07-05T05:58:10.774110+00:00"},{"alias_kind":"arxiv_version","alias_value":"2303.13732v2","created_at":"2026-07-05T05:58:10.774110+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2303.13732","created_at":"2026-07-05T05:58:10.774110+00:00"},{"alias_kind":"pith_short_12","alias_value":"GULFAYSWWIYV","created_at":"2026-07-05T05:58:10.774110+00:00"},{"alias_kind":"pith_short_16","alias_value":"GULFAYSWWIYVEJKO","created_at":"2026-07-05T05:58:10.774110+00:00"},{"alias_kind":"pith_short_8","alias_value":"GULFAYSW","created_at":"2026-07-05T05:58:10.774110+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/GULFAYSWWIYVEJKOGFWSNTJBX7","json":"https://pith.science/pith/GULFAYSWWIYVEJKOGFWSNTJBX7.json","graph_json":"https://pith.science/api/pith-number/GULFAYSWWIYVEJKOGFWSNTJBX7/graph.json","events_json":"https://pith.science/api/pith-number/GULFAYSWWIYVEJKOGFWSNTJBX7/events.json","paper":"https://pith.science/paper/GULFAYSW"},"agent_actions":{"view_html":"https://pith.science/pith/GULFAYSWWIYVEJKOGFWSNTJBX7","download_json":"https://pith.science/pith/GULFAYSWWIYVEJKOGFWSNTJBX7.json","view_paper":"https://pith.science/paper/GULFAYSW","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2303.13732&json=true","fetch_graph":"https://pith.science/api/pith-number/GULFAYSWWIYVEJKOGFWSNTJBX7/graph.json","fetch_events":"https://pith.science/api/pith-number/GULFAYSWWIYVEJKOGFWSNTJBX7/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/GULFAYSWWIYVEJKOGFWSNTJBX7/action/timestamp_anchor","attest_storage":"https://pith.science/pith/GULFAYSWWIYVEJKOGFWSNTJBX7/action/storage_attestation","attest_author":"https://pith.science/pith/GULFAYSWWIYVEJKOGFWSNTJBX7/action/author_attestation","sign_citation":"https://pith.science/pith/GULFAYSWWIYVEJKOGFWSNTJBX7/action/citation_signature","submit_replication":"https://pith.science/pith/GULFAYSWWIYVEJKOGFWSNTJBX7/action/replication_record"}},"created_at":"2026-07-05T05:58:10.774110+00:00","updated_at":"2026-07-05T05:58:10.774110+00:00"}