{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2019:ECO2JSN3AM6WWG2AQKMCMYA5O3","short_pith_number":"pith:ECO2JSN3","schema_version":"1.0","canonical_sha256":"209da4c9bb033d6b1b40829826601d76f00d0a78bd61814ace2fd9826dbbd415","source":{"kind":"arxiv","id":"1905.04870","version":1},"attestation_state":"computed","paper":{"title":"KMT-2018-BLG-1292: A Super-Jovian Microlens Planet in the Galactic Plane","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.EP","authors_text":"Andrew Gould, Byeong-Gon Park, Cheongho Han, Chung-Uk Lee, Dante Minniti, Dong-Jin Kim, Dong-Joo Lee, Hyoun-Woo Kim, In-Gu Shin, Javier Alonso-Garcia, Jennifer C. Yee, Kyu-Ha Hwang, Maria Gabriela Navarro, Matthew T. Penny, Michael D.Albrow, Richard W. Pogge, Roberto K. Saito, Sang-Mok Cha, Seung-Lee Kim, Sun-Ju Chung, Weicheng Zang, Yongseok Lee, Yoon-Hyun Ryu, Yossi Shvartzvald, Youn Kil Jung","submitted_at":"2019-05-13T05:48:16Z","abstract_excerpt":"We report the discovery of KMT-2018-BLG-1292Lb, a super-Jovian $M_{\\rm planet} = 4.5\\pm 1.3\\,M_J$ planet orbiting an F or G dwarf $M_{\\rm host} = 1.5\\pm 0.4\\,M_\\odot$, which lies physically within ${\\cal O}(10\\,\\pc)$ of the Galactic plane. The source star is a heavily extincted $A_I\\sim 5.2$ luminous giant that has the lowest Galactic latitude, $b=-0.28^\\circ$, of any planetary microlensing event. The relatively blue blended light is almost certainly either the host or its binary companion, with the first explanation being substantially more likely. This blend dominates the light at $I$ band 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":"1905.04870","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.EP","submitted_at":"2019-05-13T05:48:16Z","cross_cats_sorted":[],"title_canon_sha256":"cf0039c9f6ca5e3a07818816236780a0e47e09baa825f43ac28a623dde2217c8","abstract_canon_sha256":"18979a249a6c8ef0d49bf6cb138fbcdd96283c97b03e75436e330e990e0e28f6"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T00:36:23.250125Z","signature_b64":"GXuKRDHFeQ8UjTtvGEQV4jfndLA8BzXpK7QGVh/KG144asUjhhsZUtf1fAjwoK2RgbWeBu9v6Wqd0SfVd3h9Bw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"209da4c9bb033d6b1b40829826601d76f00d0a78bd61814ace2fd9826dbbd415","last_reissued_at":"2026-07-05T00:36:23.249627Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T00:36:23.249627Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"KMT-2018-BLG-1292: A Super-Jovian Microlens Planet in the Galactic Plane","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.EP","authors_text":"Andrew Gould, Byeong-Gon Park, Cheongho Han, Chung-Uk Lee, Dante Minniti, Dong-Jin Kim, Dong-Joo Lee, Hyoun-Woo Kim, In-Gu Shin, Javier Alonso-Garcia, Jennifer C. Yee, Kyu-Ha Hwang, Maria Gabriela Navarro, Matthew T. Penny, Michael D.Albrow, Richard W. Pogge, Roberto K. Saito, Sang-Mok Cha, Seung-Lee Kim, Sun-Ju Chung, Weicheng Zang, Yongseok Lee, Yoon-Hyun Ryu, Yossi Shvartzvald, Youn Kil Jung","submitted_at":"2019-05-13T05:48:16Z","abstract_excerpt":"We report the discovery of KMT-2018-BLG-1292Lb, a super-Jovian $M_{\\rm planet} = 4.5\\pm 1.3\\,M_J$ planet orbiting an F or G dwarf $M_{\\rm host} = 1.5\\pm 0.4\\,M_\\odot$, which lies physically within ${\\cal O}(10\\,\\pc)$ of the Galactic plane. The source star is a heavily extincted $A_I\\sim 5.2$ luminous giant that has the lowest Galactic latitude, $b=-0.28^\\circ$, of any planetary microlensing event. The relatively blue blended light is almost certainly either the host or its binary companion, with the first explanation being substantially more likely. This blend dominates the light at $I$ band a"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1905.04870","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/1905.04870/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":"1905.04870","created_at":"2026-07-05T00:36:23.249686+00:00"},{"alias_kind":"arxiv_version","alias_value":"1905.04870v1","created_at":"2026-07-05T00:36:23.249686+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1905.04870","created_at":"2026-07-05T00:36:23.249686+00:00"},{"alias_kind":"pith_short_12","alias_value":"ECO2JSN3AM6W","created_at":"2026-07-05T00:36:23.249686+00:00"},{"alias_kind":"pith_short_16","alias_value":"ECO2JSN3AM6WWG2A","created_at":"2026-07-05T00:36:23.249686+00:00"},{"alias_kind":"pith_short_8","alias_value":"ECO2JSN3","created_at":"2026-07-05T00:36:23.249686+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/ECO2JSN3AM6WWG2AQKMCMYA5O3","json":"https://pith.science/pith/ECO2JSN3AM6WWG2AQKMCMYA5O3.json","graph_json":"https://pith.science/api/pith-number/ECO2JSN3AM6WWG2AQKMCMYA5O3/graph.json","events_json":"https://pith.science/api/pith-number/ECO2JSN3AM6WWG2AQKMCMYA5O3/events.json","paper":"https://pith.science/paper/ECO2JSN3"},"agent_actions":{"view_html":"https://pith.science/pith/ECO2JSN3AM6WWG2AQKMCMYA5O3","download_json":"https://pith.science/pith/ECO2JSN3AM6WWG2AQKMCMYA5O3.json","view_paper":"https://pith.science/paper/ECO2JSN3","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1905.04870&json=true","fetch_graph":"https://pith.science/api/pith-number/ECO2JSN3AM6WWG2AQKMCMYA5O3/graph.json","fetch_events":"https://pith.science/api/pith-number/ECO2JSN3AM6WWG2AQKMCMYA5O3/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/ECO2JSN3AM6WWG2AQKMCMYA5O3/action/timestamp_anchor","attest_storage":"https://pith.science/pith/ECO2JSN3AM6WWG2AQKMCMYA5O3/action/storage_attestation","attest_author":"https://pith.science/pith/ECO2JSN3AM6WWG2AQKMCMYA5O3/action/author_attestation","sign_citation":"https://pith.science/pith/ECO2JSN3AM6WWG2AQKMCMYA5O3/action/citation_signature","submit_replication":"https://pith.science/pith/ECO2JSN3AM6WWG2AQKMCMYA5O3/action/replication_record"}},"created_at":"2026-07-05T00:36:23.249686+00:00","updated_at":"2026-07-05T00:36:23.249686+00:00"}