{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2016:6YF6L63C3T52OVXWOFCET76X7X","short_pith_number":"pith:6YF6L63C","schema_version":"1.0","canonical_sha256":"f60be5fb62dcfba756f6714449ffd7fdfa6ec236410ef91a9514c317e45fccc6","source":{"kind":"arxiv","id":"1610.03504","version":2},"attestation_state":"computed","paper":{"title":"The Broadband and Spectrally-Resolved H-band Eclipse of KELT-1b and the Role of Surface Gravity in Stratospheric Inversions in Hot Jupiters","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.EP","authors_text":"Allyson Bierlya, B. Scott Gaudi, David W. Latham, Nikku Madhusudhan, Richard Pogge, Sun Mi Chung, Thomas G. Beatty","submitted_at":"2016-10-11T20:03:04Z","abstract_excerpt":"We present a high precision H-band emission spectrum of the transiting brown dwarf KELT-1b, which we spectrophotometrically observed during a single secondary eclipse using the LUCI1 multi-object spectrograph on the Large Binocular Telescope. Using a Gaussian-process regression model, we are able to clearly measure the broadband eclipse depth as Delta-H=1418+/-94ppm. We are also able to spectrally-resolve the H-band into five separate wavechannels and measure the eclipse spectrum of KELT-1b at R~50 with an average precision of +/-135ppm. We find that the day side has an average brightness temp"},"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":"1610.03504","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.EP","submitted_at":"2016-10-11T20:03:04Z","cross_cats_sorted":[],"title_canon_sha256":"35caf91b4b140d8b241b599583ec055001ad54064e354a79d3ab16e63aba60b5","abstract_canon_sha256":"12d8e788a30e92cbad6391145fe47aea2513ecf54c40035df9462c476a6a0590"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:28:56.807570Z","signature_b64":"epiQoT3DNBuqXGCpcJrqsU6stLp4g8EJJ354tttW6t7oieVQCpX3Ax6z8YMFhjL5/JSwcwbRxqIJ7H2lnkh9DA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"f60be5fb62dcfba756f6714449ffd7fdfa6ec236410ef91a9514c317e45fccc6","last_reissued_at":"2026-05-18T00:28:56.807134Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:28:56.807134Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The Broadband and Spectrally-Resolved H-band Eclipse of KELT-1b and the Role of Surface Gravity in Stratospheric Inversions in Hot Jupiters","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.EP","authors_text":"Allyson Bierlya, B. Scott Gaudi, David W. Latham, Nikku Madhusudhan, Richard Pogge, Sun Mi Chung, Thomas G. Beatty","submitted_at":"2016-10-11T20:03:04Z","abstract_excerpt":"We present a high precision H-band emission spectrum of the transiting brown dwarf KELT-1b, which we spectrophotometrically observed during a single secondary eclipse using the LUCI1 multi-object spectrograph on the Large Binocular Telescope. Using a Gaussian-process regression model, we are able to clearly measure the broadband eclipse depth as Delta-H=1418+/-94ppm. We are also able to spectrally-resolve the H-band into five separate wavechannels and measure the eclipse spectrum of KELT-1b at R~50 with an average precision of +/-135ppm. We find that the day side has an average brightness temp"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1610.03504","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":""},"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":"1610.03504","created_at":"2026-05-18T00:28:56.807203+00:00"},{"alias_kind":"arxiv_version","alias_value":"1610.03504v2","created_at":"2026-05-18T00:28:56.807203+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1610.03504","created_at":"2026-05-18T00:28:56.807203+00:00"},{"alias_kind":"pith_short_12","alias_value":"6YF6L63C3T52","created_at":"2026-05-18T12:30:04.600751+00:00"},{"alias_kind":"pith_short_16","alias_value":"6YF6L63C3T52OVXW","created_at":"2026-05-18T12:30:04.600751+00:00"},{"alias_kind":"pith_short_8","alias_value":"6YF6L63C","created_at":"2026-05-18T12:30:04.600751+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2606.04144","citing_title":"Characterizing Transiting Exoplanet Atmospheres in the 2030s with the Hubble Space Telescope","ref_index":82,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/6YF6L63C3T52OVXWOFCET76X7X","json":"https://pith.science/pith/6YF6L63C3T52OVXWOFCET76X7X.json","graph_json":"https://pith.science/api/pith-number/6YF6L63C3T52OVXWOFCET76X7X/graph.json","events_json":"https://pith.science/api/pith-number/6YF6L63C3T52OVXWOFCET76X7X/events.json","paper":"https://pith.science/paper/6YF6L63C"},"agent_actions":{"view_html":"https://pith.science/pith/6YF6L63C3T52OVXWOFCET76X7X","download_json":"https://pith.science/pith/6YF6L63C3T52OVXWOFCET76X7X.json","view_paper":"https://pith.science/paper/6YF6L63C","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1610.03504&json=true","fetch_graph":"https://pith.science/api/pith-number/6YF6L63C3T52OVXWOFCET76X7X/graph.json","fetch_events":"https://pith.science/api/pith-number/6YF6L63C3T52OVXWOFCET76X7X/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/6YF6L63C3T52OVXWOFCET76X7X/action/timestamp_anchor","attest_storage":"https://pith.science/pith/6YF6L63C3T52OVXWOFCET76X7X/action/storage_attestation","attest_author":"https://pith.science/pith/6YF6L63C3T52OVXWOFCET76X7X/action/author_attestation","sign_citation":"https://pith.science/pith/6YF6L63C3T52OVXWOFCET76X7X/action/citation_signature","submit_replication":"https://pith.science/pith/6YF6L63C3T52OVXWOFCET76X7X/action/replication_record"}},"created_at":"2026-05-18T00:28:56.807203+00:00","updated_at":"2026-05-18T00:28:56.807203+00:00"}