{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2023:BIOVC62GOB6SRVA4R74V262EDY","short_pith_number":"pith:BIOVC62G","schema_version":"1.0","canonical_sha256":"0a1d517b46707d28d41c8ff95d7b441e081b7c6bbaaa153a152661d0dada6872","source":{"kind":"arxiv","id":"2305.13234","version":1},"attestation_state":"computed","paper":{"title":"Spitzer IRS Observations of Titan as a Precursor to JWST MIRI Observations","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.EP","authors_text":"Brandon Park Coy, Conor A. Nixon, Leigh N. Fletcher, Naomi Rowe-Gurney, Nicholas A. Lombardo, Patrick Irwin, Richard Achterberg","submitted_at":"2023-05-22T17:06:27Z","abstract_excerpt":"In this work we present, for the first time, infrared spectra of Titan from the Spitzer Space Telescope ($2004-2009$). The data are from both the short wavelength-low resolution (SL, $5.13-14.29\\mathrm{\\mu m}, R\\sim60-127$) and short wavelength-high resolution channels (SH, $9.89 - 19.51\\mathrm{\\mu m}, R\\sim600$) showing the emissions of CH$_{4}$, C$_{2}$H$_{2}$, C$_{2}$H$_{4}$, C$_{2}$H$_{6}$, C$_{3}$H$_{4}$, C$_{3}$H$_{6}$, C$_{3}$H$_{8}$, C$_{4}$H$_{2}$, HCN, HC$_{3}$N, and CO$_{2}$. We compare the results obtained for Titan from Spitzer to those of the Cassini Composite Infrared Spectromet"},"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":"2305.13234","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.EP","submitted_at":"2023-05-22T17:06:27Z","cross_cats_sorted":[],"title_canon_sha256":"35c351dc426fd321a6fb266b22f232b05187e155e48bcceee989be8a3baaaf4d","abstract_canon_sha256":"50f6a22d47055243c0ce1893e2f1eb65e4b79d3463d22aa9b408d77d41a69acd"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T06:33:33.453125Z","signature_b64":"SX6ymsP2tH5Nq7L3rgW3JTSGwcZ0jGI1+2USgo+fEH6B4/vmac8rXnlrb/gWNFRJtPehevJboCGIkoVgIL2CDQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"0a1d517b46707d28d41c8ff95d7b441e081b7c6bbaaa153a152661d0dada6872","last_reissued_at":"2026-07-05T06:33:33.452725Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T06:33:33.452725Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Spitzer IRS Observations of Titan as a Precursor to JWST MIRI Observations","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.EP","authors_text":"Brandon Park Coy, Conor A. Nixon, Leigh N. Fletcher, Naomi Rowe-Gurney, Nicholas A. Lombardo, Patrick Irwin, Richard Achterberg","submitted_at":"2023-05-22T17:06:27Z","abstract_excerpt":"In this work we present, for the first time, infrared spectra of Titan from the Spitzer Space Telescope ($2004-2009$). The data are from both the short wavelength-low resolution (SL, $5.13-14.29\\mathrm{\\mu m}, R\\sim60-127$) and short wavelength-high resolution channels (SH, $9.89 - 19.51\\mathrm{\\mu m}, R\\sim600$) showing the emissions of CH$_{4}$, C$_{2}$H$_{2}$, C$_{2}$H$_{4}$, C$_{2}$H$_{6}$, C$_{3}$H$_{4}$, C$_{3}$H$_{6}$, C$_{3}$H$_{8}$, C$_{4}$H$_{2}$, HCN, HC$_{3}$N, and CO$_{2}$. We compare the results obtained for Titan from Spitzer to those of the Cassini Composite Infrared Spectromet"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2305.13234","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/2305.13234/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":"2305.13234","created_at":"2026-07-05T06:33:33.452781+00:00"},{"alias_kind":"arxiv_version","alias_value":"2305.13234v1","created_at":"2026-07-05T06:33:33.452781+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2305.13234","created_at":"2026-07-05T06:33:33.452781+00:00"},{"alias_kind":"pith_short_12","alias_value":"BIOVC62GOB6S","created_at":"2026-07-05T06:33:33.452781+00:00"},{"alias_kind":"pith_short_16","alias_value":"BIOVC62GOB6SRVA4","created_at":"2026-07-05T06:33:33.452781+00:00"},{"alias_kind":"pith_short_8","alias_value":"BIOVC62G","created_at":"2026-07-05T06:33:33.452781+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/BIOVC62GOB6SRVA4R74V262EDY","json":"https://pith.science/pith/BIOVC62GOB6SRVA4R74V262EDY.json","graph_json":"https://pith.science/api/pith-number/BIOVC62GOB6SRVA4R74V262EDY/graph.json","events_json":"https://pith.science/api/pith-number/BIOVC62GOB6SRVA4R74V262EDY/events.json","paper":"https://pith.science/paper/BIOVC62G"},"agent_actions":{"view_html":"https://pith.science/pith/BIOVC62GOB6SRVA4R74V262EDY","download_json":"https://pith.science/pith/BIOVC62GOB6SRVA4R74V262EDY.json","view_paper":"https://pith.science/paper/BIOVC62G","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2305.13234&json=true","fetch_graph":"https://pith.science/api/pith-number/BIOVC62GOB6SRVA4R74V262EDY/graph.json","fetch_events":"https://pith.science/api/pith-number/BIOVC62GOB6SRVA4R74V262EDY/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/BIOVC62GOB6SRVA4R74V262EDY/action/timestamp_anchor","attest_storage":"https://pith.science/pith/BIOVC62GOB6SRVA4R74V262EDY/action/storage_attestation","attest_author":"https://pith.science/pith/BIOVC62GOB6SRVA4R74V262EDY/action/author_attestation","sign_citation":"https://pith.science/pith/BIOVC62GOB6SRVA4R74V262EDY/action/citation_signature","submit_replication":"https://pith.science/pith/BIOVC62GOB6SRVA4R74V262EDY/action/replication_record"}},"created_at":"2026-07-05T06:33:33.452781+00:00","updated_at":"2026-07-05T06:33:33.452781+00:00"}