{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2015:WC3OWKLUURFSQHO3IBFN4L7P5J","short_pith_number":"pith:WC3OWKLU","schema_version":"1.0","canonical_sha256":"b0b6eb2974a44b281ddb404ade2fefea5b4e7dc86cd5429aaa6d6e0fd50716be","source":{"kind":"arxiv","id":"1509.05272","version":1},"attestation_state":"computed","paper":{"title":"Broad-band spectrophotometry of the hot Jupiter HAT-P-12b from the near-UV to the near-IR","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.SR"],"primary_cat":"astro-ph.EP","authors_text":"A. K\\\"unstler, C. von Essen, E. Herrero, G. Piotto, G. Scandariato, I. Bernt, I. Pagano, J. Weingrill, K. G. Strassmeier, M. Mallonn, P. V. Sada, Sz. Csizmadia, T. Granzer, T. R. Marsh, V. Nascimbeni, V. S. Dhillon","submitted_at":"2015-09-17T14:36:45Z","abstract_excerpt":"The detection of trends or gradients in the transmission spectrum of extrasolar planets is possible with observations at very low spectral resolution. Transit measurements of sufficient accuracy using selected broad-band filters allow for an initial characterization of the atmosphere of the planet. We obtained time series photometry of 20 transit events and analyzed them homogeneously, along with eight light curves obtained from the literature. In total, the light curves span a range from 0.35 to 1.25 microns. During two observing seasons over four months each, we monitored the host star to co"},"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":"1509.05272","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.EP","submitted_at":"2015-09-17T14:36:45Z","cross_cats_sorted":["astro-ph.SR"],"title_canon_sha256":"0ee5af80624c5cadf50aec21602d5777ccef98eab6bbdc1daf435712cbd65601","abstract_canon_sha256":"b763b344271f0835d277b705c7cbad981b2a7fef007c8ea595c93aea74d2e901"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:27:22.566421Z","signature_b64":"g2eWHkqmR4TqKIakxrE7C6zHr/8geIDSL84IMrLXaI5uv7/B5P4Y2tsT0d09iyLtS1jirCOplSzQ7EtyBKStBw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"b0b6eb2974a44b281ddb404ade2fefea5b4e7dc86cd5429aaa6d6e0fd50716be","last_reissued_at":"2026-05-18T01:27:22.565810Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:27:22.565810Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Broad-band spectrophotometry of the hot Jupiter HAT-P-12b from the near-UV to the near-IR","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.SR"],"primary_cat":"astro-ph.EP","authors_text":"A. K\\\"unstler, C. von Essen, E. Herrero, G. Piotto, G. Scandariato, I. Bernt, I. Pagano, J. Weingrill, K. G. Strassmeier, M. Mallonn, P. V. Sada, Sz. Csizmadia, T. Granzer, T. R. Marsh, V. Nascimbeni, V. S. Dhillon","submitted_at":"2015-09-17T14:36:45Z","abstract_excerpt":"The detection of trends or gradients in the transmission spectrum of extrasolar planets is possible with observations at very low spectral resolution. Transit measurements of sufficient accuracy using selected broad-band filters allow for an initial characterization of the atmosphere of the planet. We obtained time series photometry of 20 transit events and analyzed them homogeneously, along with eight light curves obtained from the literature. In total, the light curves span a range from 0.35 to 1.25 microns. During two observing seasons over four months each, we monitored the host star to co"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1509.05272","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":"1509.05272","created_at":"2026-05-18T01:27:22.565897+00:00"},{"alias_kind":"arxiv_version","alias_value":"1509.05272v1","created_at":"2026-05-18T01:27:22.565897+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1509.05272","created_at":"2026-05-18T01:27:22.565897+00:00"},{"alias_kind":"pith_short_12","alias_value":"WC3OWKLUURFS","created_at":"2026-05-18T12:29:47.479230+00:00"},{"alias_kind":"pith_short_16","alias_value":"WC3OWKLUURFSQHO3","created_at":"2026-05-18T12:29:47.479230+00:00"},{"alias_kind":"pith_short_8","alias_value":"WC3OWKLU","created_at":"2026-05-18T12:29:47.479230+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/WC3OWKLUURFSQHO3IBFN4L7P5J","json":"https://pith.science/pith/WC3OWKLUURFSQHO3IBFN4L7P5J.json","graph_json":"https://pith.science/api/pith-number/WC3OWKLUURFSQHO3IBFN4L7P5J/graph.json","events_json":"https://pith.science/api/pith-number/WC3OWKLUURFSQHO3IBFN4L7P5J/events.json","paper":"https://pith.science/paper/WC3OWKLU"},"agent_actions":{"view_html":"https://pith.science/pith/WC3OWKLUURFSQHO3IBFN4L7P5J","download_json":"https://pith.science/pith/WC3OWKLUURFSQHO3IBFN4L7P5J.json","view_paper":"https://pith.science/paper/WC3OWKLU","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1509.05272&json=true","fetch_graph":"https://pith.science/api/pith-number/WC3OWKLUURFSQHO3IBFN4L7P5J/graph.json","fetch_events":"https://pith.science/api/pith-number/WC3OWKLUURFSQHO3IBFN4L7P5J/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/WC3OWKLUURFSQHO3IBFN4L7P5J/action/timestamp_anchor","attest_storage":"https://pith.science/pith/WC3OWKLUURFSQHO3IBFN4L7P5J/action/storage_attestation","attest_author":"https://pith.science/pith/WC3OWKLUURFSQHO3IBFN4L7P5J/action/author_attestation","sign_citation":"https://pith.science/pith/WC3OWKLUURFSQHO3IBFN4L7P5J/action/citation_signature","submit_replication":"https://pith.science/pith/WC3OWKLUURFSQHO3IBFN4L7P5J/action/replication_record"}},"created_at":"2026-05-18T01:27:22.565897+00:00","updated_at":"2026-05-18T01:27:22.565897+00:00"}