{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2015:JTARML74LSFDVBTEGLZHAFBNZD","short_pith_number":"pith:JTARML74","schema_version":"1.0","canonical_sha256":"4cc1162ffc5c8a3a866432f270142dc8d1eec3d1e84663f2aee4aa6835fd6d39","source":{"kind":"arxiv","id":"1510.02165","version":2},"attestation_state":"computed","paper":{"title":"The CO2 Abundance in Comets C/2012 K1 (PanSTARRS), C/2012 K5 (LINEAR), and 290P/Jager as Measured with Spitzer","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.EP","authors_text":"Adam J. McKay, Anita L. Cochran, Carey M. Lisse, Dennis Bodewits, Michael A. DiSanti, Michael S.P. Kelley, Neil Dello Russo","submitted_at":"2015-10-07T23:22:52Z","abstract_excerpt":"We present analysis of observations of CO2 and OI emission in three comets to measure the CO2 abundance and evaluate the possibility of employing observations of OI emission in comets as a proxy for CO2. We obtained NIR imaging sensitive to CO2 of comets C/2012 K1 (PanSTARRS), C/2012 K5 (LINEAR), and 290P/Jager with the IRAC instrument on Spitzer. We acquired observations of OI emission in these comets with the ARCES echelle spectrometer mounted on the 3.5-meter telescope at Apache Point Observatory and observations of OH with the Swift observatory (PanSTARRS) and with Keck HIRES (Jager). The "},"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":"1510.02165","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.EP","submitted_at":"2015-10-07T23:22:52Z","cross_cats_sorted":[],"title_canon_sha256":"5c94555978bf9b603ae7da32bb2e2da76a41838742cbec03da9b7d2e76809976","abstract_canon_sha256":"a0dd0229bfdf6cde6ee569011f37a1bc491eb37491a274dd049975949ed19eb7"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:15:44.434873Z","signature_b64":"xaMrL+pLke0nDcKQc6UEgggSphCx1o3PzhQ/uZsNwyn3Y8N1ijyoGl93It4hTvFt3Adtvg2xgvQpqVGIT+uWBg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"4cc1162ffc5c8a3a866432f270142dc8d1eec3d1e84663f2aee4aa6835fd6d39","last_reissued_at":"2026-05-18T01:15:44.434373Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:15:44.434373Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The CO2 Abundance in Comets C/2012 K1 (PanSTARRS), C/2012 K5 (LINEAR), and 290P/Jager as Measured with Spitzer","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.EP","authors_text":"Adam J. McKay, Anita L. Cochran, Carey M. Lisse, Dennis Bodewits, Michael A. DiSanti, Michael S.P. Kelley, Neil Dello Russo","submitted_at":"2015-10-07T23:22:52Z","abstract_excerpt":"We present analysis of observations of CO2 and OI emission in three comets to measure the CO2 abundance and evaluate the possibility of employing observations of OI emission in comets as a proxy for CO2. We obtained NIR imaging sensitive to CO2 of comets C/2012 K1 (PanSTARRS), C/2012 K5 (LINEAR), and 290P/Jager with the IRAC instrument on Spitzer. We acquired observations of OI emission in these comets with the ARCES echelle spectrometer mounted on the 3.5-meter telescope at Apache Point Observatory and observations of OH with the Swift observatory (PanSTARRS) and with Keck HIRES (Jager). The "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1510.02165","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":"1510.02165","created_at":"2026-05-18T01:15:44.434452+00:00"},{"alias_kind":"arxiv_version","alias_value":"1510.02165v2","created_at":"2026-05-18T01:15:44.434452+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1510.02165","created_at":"2026-05-18T01:15:44.434452+00:00"},{"alias_kind":"pith_short_12","alias_value":"JTARML74LSFD","created_at":"2026-05-18T12:29:27.538025+00:00"},{"alias_kind":"pith_short_16","alias_value":"JTARML74LSFDVBTE","created_at":"2026-05-18T12:29:27.538025+00:00"},{"alias_kind":"pith_short_8","alias_value":"JTARML74","created_at":"2026-05-18T12:29:27.538025+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/JTARML74LSFDVBTEGLZHAFBNZD","json":"https://pith.science/pith/JTARML74LSFDVBTEGLZHAFBNZD.json","graph_json":"https://pith.science/api/pith-number/JTARML74LSFDVBTEGLZHAFBNZD/graph.json","events_json":"https://pith.science/api/pith-number/JTARML74LSFDVBTEGLZHAFBNZD/events.json","paper":"https://pith.science/paper/JTARML74"},"agent_actions":{"view_html":"https://pith.science/pith/JTARML74LSFDVBTEGLZHAFBNZD","download_json":"https://pith.science/pith/JTARML74LSFDVBTEGLZHAFBNZD.json","view_paper":"https://pith.science/paper/JTARML74","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1510.02165&json=true","fetch_graph":"https://pith.science/api/pith-number/JTARML74LSFDVBTEGLZHAFBNZD/graph.json","fetch_events":"https://pith.science/api/pith-number/JTARML74LSFDVBTEGLZHAFBNZD/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/JTARML74LSFDVBTEGLZHAFBNZD/action/timestamp_anchor","attest_storage":"https://pith.science/pith/JTARML74LSFDVBTEGLZHAFBNZD/action/storage_attestation","attest_author":"https://pith.science/pith/JTARML74LSFDVBTEGLZHAFBNZD/action/author_attestation","sign_citation":"https://pith.science/pith/JTARML74LSFDVBTEGLZHAFBNZD/action/citation_signature","submit_replication":"https://pith.science/pith/JTARML74LSFDVBTEGLZHAFBNZD/action/replication_record"}},"created_at":"2026-05-18T01:15:44.434452+00:00","updated_at":"2026-05-18T01:15:44.434452+00:00"}