{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2014:GFJMFHMH5NUH7WFOMQRZDIWJUO","short_pith_number":"pith:GFJMFHMH","schema_version":"1.0","canonical_sha256":"3152c29d87eb687fd8ae642391a2c9a3a446636ddb349c3b8691b6aef43272a6","source":{"kind":"arxiv","id":"1410.0968","version":1},"attestation_state":"computed","paper":{"title":"Characterization of the atmosphere of the hot Jupiter HAT-P-32Ab and the M-dwarf companion HAT-P-32B","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.EP","authors_text":"(10) The University of Arizona, (11) Jet Propulsion Laboratory), 2), (2) Center for Exoplanets, (3) California Institute of Technology, (4) Princeton University, (5) University of California, (6) University of Hawaii at Manoa, (7) California Institute of Technology, (8) University of North Carolina at Chapel Hill, (9) Boston University, Adam Burrows (4), Adam P. Showman (10), Benjamin J. Fulton (6), Christoph Baranec (6), Habitable Worlds, Heather A. Knutson (3), Henry Ngo (3), Jason Curtis (1, Jason T. Wright (1, Johnathan Fortney (5), Joseph G. O'Rourke (3), Ming Zhao (1, Nicholas M. Law (8), Philip S. Muirhead (9), Reed Riddle (7), Rick Burruss (11) ((1) Pennsylvania State University, Santa Cruz, Sasha Hinkley (7)","submitted_at":"2014-10-03T20:07:15Z","abstract_excerpt":"We report secondary eclipse photometry of the hot Jupiter HAT-P-32Ab, taken with Hale/WIRC in H and Ks bands and with Spitzer/IRAC at 3.6 and 4.5 micron. We carried out adaptive optics imaging of the planet host star HAT-P-32A and its companion HAT-P-32B in the near-IR and the visible. We clearly resolve the two stars from each other and find a separation of 2.923\" +/- 0. 004\" and a position angle 110.64 deg +/- 0.12 deg. We measure the flux ratios of the binary in g' r' i' z' and H & Ks bands, and determine Teff = 3565 +/- 82 K for the companion star, corresponding to an M1.5 dwarf. We use PH"},"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":"1410.0968","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.EP","submitted_at":"2014-10-03T20:07:15Z","cross_cats_sorted":[],"title_canon_sha256":"4361087cb8741ab6e25f6e869cc962713dd9d2c7be95a5d84c47ed713d8035b1","abstract_canon_sha256":"fbb71a9e119fa51ecfdb74075fc64c4bb8bf0f82f441d14193d46824c9657bad"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:41:52.655249Z","signature_b64":"nPtYL0Y/+mnOYFC90DhoazZEDWUTlnnU+yBceSO6LgTF/khOph9a4FOWnxY3N0QvLlwdtjdSiLKcmzZmObfPDA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"3152c29d87eb687fd8ae642391a2c9a3a446636ddb349c3b8691b6aef43272a6","last_reissued_at":"2026-05-18T01:41:52.654672Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:41:52.654672Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Characterization of the atmosphere of the hot Jupiter HAT-P-32Ab and the M-dwarf companion HAT-P-32B","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.EP","authors_text":"(10) The University of Arizona, (11) Jet Propulsion Laboratory), 2), (2) Center for Exoplanets, (3) California Institute of Technology, (4) Princeton University, (5) University of California, (6) University of Hawaii at Manoa, (7) California Institute of Technology, (8) University of North Carolina at Chapel Hill, (9) Boston University, Adam Burrows (4), Adam P. Showman (10), Benjamin J. Fulton (6), Christoph Baranec (6), Habitable Worlds, Heather A. Knutson (3), Henry Ngo (3), Jason Curtis (1, Jason T. Wright (1, Johnathan Fortney (5), Joseph G. O'Rourke (3), Ming Zhao (1, Nicholas M. Law (8), Philip S. Muirhead (9), Reed Riddle (7), Rick Burruss (11) ((1) Pennsylvania State University, Santa Cruz, Sasha Hinkley (7)","submitted_at":"2014-10-03T20:07:15Z","abstract_excerpt":"We report secondary eclipse photometry of the hot Jupiter HAT-P-32Ab, taken with Hale/WIRC in H and Ks bands and with Spitzer/IRAC at 3.6 and 4.5 micron. We carried out adaptive optics imaging of the planet host star HAT-P-32A and its companion HAT-P-32B in the near-IR and the visible. We clearly resolve the two stars from each other and find a separation of 2.923\" +/- 0. 004\" and a position angle 110.64 deg +/- 0.12 deg. We measure the flux ratios of the binary in g' r' i' z' and H & Ks bands, and determine Teff = 3565 +/- 82 K for the companion star, corresponding to an M1.5 dwarf. We use PH"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1410.0968","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":"1410.0968","created_at":"2026-05-18T01:41:52.654764+00:00"},{"alias_kind":"arxiv_version","alias_value":"1410.0968v1","created_at":"2026-05-18T01:41:52.654764+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1410.0968","created_at":"2026-05-18T01:41:52.654764+00:00"},{"alias_kind":"pith_short_12","alias_value":"GFJMFHMH5NUH","created_at":"2026-05-18T12:28:30.664211+00:00"},{"alias_kind":"pith_short_16","alias_value":"GFJMFHMH5NUH7WFO","created_at":"2026-05-18T12:28:30.664211+00:00"},{"alias_kind":"pith_short_8","alias_value":"GFJMFHMH","created_at":"2026-05-18T12:28:30.664211+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/GFJMFHMH5NUH7WFOMQRZDIWJUO","json":"https://pith.science/pith/GFJMFHMH5NUH7WFOMQRZDIWJUO.json","graph_json":"https://pith.science/api/pith-number/GFJMFHMH5NUH7WFOMQRZDIWJUO/graph.json","events_json":"https://pith.science/api/pith-number/GFJMFHMH5NUH7WFOMQRZDIWJUO/events.json","paper":"https://pith.science/paper/GFJMFHMH"},"agent_actions":{"view_html":"https://pith.science/pith/GFJMFHMH5NUH7WFOMQRZDIWJUO","download_json":"https://pith.science/pith/GFJMFHMH5NUH7WFOMQRZDIWJUO.json","view_paper":"https://pith.science/paper/GFJMFHMH","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1410.0968&json=true","fetch_graph":"https://pith.science/api/pith-number/GFJMFHMH5NUH7WFOMQRZDIWJUO/graph.json","fetch_events":"https://pith.science/api/pith-number/GFJMFHMH5NUH7WFOMQRZDIWJUO/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/GFJMFHMH5NUH7WFOMQRZDIWJUO/action/timestamp_anchor","attest_storage":"https://pith.science/pith/GFJMFHMH5NUH7WFOMQRZDIWJUO/action/storage_attestation","attest_author":"https://pith.science/pith/GFJMFHMH5NUH7WFOMQRZDIWJUO/action/author_attestation","sign_citation":"https://pith.science/pith/GFJMFHMH5NUH7WFOMQRZDIWJUO/action/citation_signature","submit_replication":"https://pith.science/pith/GFJMFHMH5NUH7WFOMQRZDIWJUO/action/replication_record"}},"created_at":"2026-05-18T01:41:52.654764+00:00","updated_at":"2026-05-18T01:41:52.654764+00:00"}