{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2013:6PQB3XFZAY2OVM33OUSCCBNAC6","short_pith_number":"pith:6PQB3XFZ","schema_version":"1.0","canonical_sha256":"f3e01ddcb90634eab37b75242105a017aa2df45bb3aee54b3316d3b14fe8e269","source":{"kind":"arxiv","id":"1308.2106","version":1},"attestation_state":"computed","paper":{"title":"Hubble Space Telescope hot Jupiter Transmission Spectral Survey: detection of water in HAT-P-1b from Wide Field Camera 3 near-infrared spatial scan observations","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.EP","authors_text":"A. Lecavelier des Etangs, A. P. Showman, A. S. Burrows, A. Vidal-Madjar, D. Deming, D. K. Sing, F. Pont, G. Ballester, G. Henry, H. Knutson, H. R. Wakeford, J. J. Fortney, K. Zahnle, N. Nikolov, N. P. Gibson, S. Aigrain","submitted_at":"2013-08-09T12:32:28Z","abstract_excerpt":"We present Hubble Space Telescope near-infrared transmission spectroscopy of the transiting hot-Jupiter HAT-P-1b. We observed one transit with Wide Field Camera 3 using the G141 low-resolution grism to cover the wavelength range 1.087- 1.678 {\\mu}m. These time series observations were taken with the newly available spatial scan mode that increases the duty cycle by nearly a factor of two, thus improving the resulting photometric precision of the data. We measure a planet-to-star radius ratio of Rp/R*=0.11709+/-0.00038 in the white light curve with the centre of transit occurring at 2456114.345"},"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":"1308.2106","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.EP","submitted_at":"2013-08-09T12:32:28Z","cross_cats_sorted":[],"title_canon_sha256":"9a88b46e050c4b00ed95f54f5db46f9440d319c3e95f9ff90607ace797e278c6","abstract_canon_sha256":"5b6cb5febc69d0c39102f631a21f7f909da30cdde7dcd4666844b2d34ee76ee2"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T03:13:09.620778Z","signature_b64":"5+hfOATcFazx56qQxPS6u1Y6M0G8+5K2uWJ9Rzd7OdgtxotJXAWINy7Y0AWSwd8DqwcaZOJEZvkISpIQX4DGCA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"f3e01ddcb90634eab37b75242105a017aa2df45bb3aee54b3316d3b14fe8e269","last_reissued_at":"2026-05-18T03:13:09.620308Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T03:13:09.620308Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Hubble Space Telescope hot Jupiter Transmission Spectral Survey: detection of water in HAT-P-1b from Wide Field Camera 3 near-infrared spatial scan observations","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.EP","authors_text":"A. Lecavelier des Etangs, A. P. Showman, A. S. Burrows, A. Vidal-Madjar, D. Deming, D. K. Sing, F. Pont, G. Ballester, G. Henry, H. Knutson, H. R. Wakeford, J. J. Fortney, K. Zahnle, N. Nikolov, N. P. Gibson, S. Aigrain","submitted_at":"2013-08-09T12:32:28Z","abstract_excerpt":"We present Hubble Space Telescope near-infrared transmission spectroscopy of the transiting hot-Jupiter HAT-P-1b. We observed one transit with Wide Field Camera 3 using the G141 low-resolution grism to cover the wavelength range 1.087- 1.678 {\\mu}m. These time series observations were taken with the newly available spatial scan mode that increases the duty cycle by nearly a factor of two, thus improving the resulting photometric precision of the data. We measure a planet-to-star radius ratio of Rp/R*=0.11709+/-0.00038 in the white light curve with the centre of transit occurring at 2456114.345"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1308.2106","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":"1308.2106","created_at":"2026-05-18T03:13:09.620388+00:00"},{"alias_kind":"arxiv_version","alias_value":"1308.2106v1","created_at":"2026-05-18T03:13:09.620388+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1308.2106","created_at":"2026-05-18T03:13:09.620388+00:00"},{"alias_kind":"pith_short_12","alias_value":"6PQB3XFZAY2O","created_at":"2026-05-18T12:27:36.564083+00:00"},{"alias_kind":"pith_short_16","alias_value":"6PQB3XFZAY2OVM33","created_at":"2026-05-18T12:27:36.564083+00:00"},{"alias_kind":"pith_short_8","alias_value":"6PQB3XFZ","created_at":"2026-05-18T12:27:36.564083+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/6PQB3XFZAY2OVM33OUSCCBNAC6","json":"https://pith.science/pith/6PQB3XFZAY2OVM33OUSCCBNAC6.json","graph_json":"https://pith.science/api/pith-number/6PQB3XFZAY2OVM33OUSCCBNAC6/graph.json","events_json":"https://pith.science/api/pith-number/6PQB3XFZAY2OVM33OUSCCBNAC6/events.json","paper":"https://pith.science/paper/6PQB3XFZ"},"agent_actions":{"view_html":"https://pith.science/pith/6PQB3XFZAY2OVM33OUSCCBNAC6","download_json":"https://pith.science/pith/6PQB3XFZAY2OVM33OUSCCBNAC6.json","view_paper":"https://pith.science/paper/6PQB3XFZ","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1308.2106&json=true","fetch_graph":"https://pith.science/api/pith-number/6PQB3XFZAY2OVM33OUSCCBNAC6/graph.json","fetch_events":"https://pith.science/api/pith-number/6PQB3XFZAY2OVM33OUSCCBNAC6/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/6PQB3XFZAY2OVM33OUSCCBNAC6/action/timestamp_anchor","attest_storage":"https://pith.science/pith/6PQB3XFZAY2OVM33OUSCCBNAC6/action/storage_attestation","attest_author":"https://pith.science/pith/6PQB3XFZAY2OVM33OUSCCBNAC6/action/author_attestation","sign_citation":"https://pith.science/pith/6PQB3XFZAY2OVM33OUSCCBNAC6/action/citation_signature","submit_replication":"https://pith.science/pith/6PQB3XFZAY2OVM33OUSCCBNAC6/action/replication_record"}},"created_at":"2026-05-18T03:13:09.620388+00:00","updated_at":"2026-05-18T03:13:09.620388+00:00"}