{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2014:TNSB4M4IJPJGJGI2WR5R6QD3PH","short_pith_number":"pith:TNSB4M4I","schema_version":"1.0","canonical_sha256":"9b641e33884bd264991ab47b1f407b79fb7ac86c293aedcccf8c254f77a92c98","source":{"kind":"arxiv","id":"1404.7853","version":1},"attestation_state":"computed","paper":{"title":"Doppler Imaging of Exoplanets and Brown Dwarfs","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.EP","astro-ph.IM"],"primary_cat":"astro-ph.SR","authors_text":"Ian J. M. Crossfield","submitted_at":"2014-04-30T19:56:32Z","abstract_excerpt":"Doppler Imaging produces 2D global maps of rotating objects using high-dispersion spectroscopy. When applied to brown dwarfs and extrasolar planets, this technique can constrain global atmospheric dynamics and/or magnetic effects on these objects in un- precedented detail. I present the first quantitative assessment of the prospects for Doppler Imaging of substellar objects with current facilities and with future giant ground-based telescopes. Observations will have the greatest sensitivity in K band, but the H and L bands will also be useful for these purposes. To assess the number and availa"},"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":"1404.7853","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2014-04-30T19:56:32Z","cross_cats_sorted":["astro-ph.EP","astro-ph.IM"],"title_canon_sha256":"4dda70ae8dc4147108ea2e2493098195ac79e644e38633b38708e5ccd451afdf","abstract_canon_sha256":"97c6945980ac55d1716d8ee6a2439fa4d06e54921e26b96eca5d6cbce8129cd9"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:48:36.027203Z","signature_b64":"Ko8+rwd84MqLIyqZcizdhAOkFzIFP7Fuc6FE7ELgxKZEK+02qoncWia7rrCpqyKeyalxm2vVt0FN1T/XQKhHDA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"9b641e33884bd264991ab47b1f407b79fb7ac86c293aedcccf8c254f77a92c98","last_reissued_at":"2026-05-18T02:48:36.026355Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:48:36.026355Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Doppler Imaging of Exoplanets and Brown Dwarfs","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.EP","astro-ph.IM"],"primary_cat":"astro-ph.SR","authors_text":"Ian J. M. Crossfield","submitted_at":"2014-04-30T19:56:32Z","abstract_excerpt":"Doppler Imaging produces 2D global maps of rotating objects using high-dispersion spectroscopy. When applied to brown dwarfs and extrasolar planets, this technique can constrain global atmospheric dynamics and/or magnetic effects on these objects in un- precedented detail. I present the first quantitative assessment of the prospects for Doppler Imaging of substellar objects with current facilities and with future giant ground-based telescopes. Observations will have the greatest sensitivity in K band, but the H and L bands will also be useful for these purposes. To assess the number and availa"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1404.7853","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":"1404.7853","created_at":"2026-05-18T02:48:36.026495+00:00"},{"alias_kind":"arxiv_version","alias_value":"1404.7853v1","created_at":"2026-05-18T02:48:36.026495+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1404.7853","created_at":"2026-05-18T02:48:36.026495+00:00"},{"alias_kind":"pith_short_12","alias_value":"TNSB4M4IJPJG","created_at":"2026-05-18T12:28:49.207871+00:00"},{"alias_kind":"pith_short_16","alias_value":"TNSB4M4IJPJGJGI2","created_at":"2026-05-18T12:28:49.207871+00:00"},{"alias_kind":"pith_short_8","alias_value":"TNSB4M4I","created_at":"2026-05-18T12:28:49.207871+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":2,"internal_anchor_count":2,"sample":[{"citing_arxiv_id":"2606.03824","citing_title":"The CRIMSON survey I: super-stellar SiO in the directly imaged companion TWA 5 B from high-resolution M-band spectroscopy","ref_index":240,"is_internal_anchor":true},{"citing_arxiv_id":"2606.11972","citing_title":"$^{13}$CO and potential variability in $\\beta$ Pictoris b with GRAVITY+","ref_index":32,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/TNSB4M4IJPJGJGI2WR5R6QD3PH","json":"https://pith.science/pith/TNSB4M4IJPJGJGI2WR5R6QD3PH.json","graph_json":"https://pith.science/api/pith-number/TNSB4M4IJPJGJGI2WR5R6QD3PH/graph.json","events_json":"https://pith.science/api/pith-number/TNSB4M4IJPJGJGI2WR5R6QD3PH/events.json","paper":"https://pith.science/paper/TNSB4M4I"},"agent_actions":{"view_html":"https://pith.science/pith/TNSB4M4IJPJGJGI2WR5R6QD3PH","download_json":"https://pith.science/pith/TNSB4M4IJPJGJGI2WR5R6QD3PH.json","view_paper":"https://pith.science/paper/TNSB4M4I","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1404.7853&json=true","fetch_graph":"https://pith.science/api/pith-number/TNSB4M4IJPJGJGI2WR5R6QD3PH/graph.json","fetch_events":"https://pith.science/api/pith-number/TNSB4M4IJPJGJGI2WR5R6QD3PH/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/TNSB4M4IJPJGJGI2WR5R6QD3PH/action/timestamp_anchor","attest_storage":"https://pith.science/pith/TNSB4M4IJPJGJGI2WR5R6QD3PH/action/storage_attestation","attest_author":"https://pith.science/pith/TNSB4M4IJPJGJGI2WR5R6QD3PH/action/author_attestation","sign_citation":"https://pith.science/pith/TNSB4M4IJPJGJGI2WR5R6QD3PH/action/citation_signature","submit_replication":"https://pith.science/pith/TNSB4M4IJPJGJGI2WR5R6QD3PH/action/replication_record"}},"created_at":"2026-05-18T02:48:36.026495+00:00","updated_at":"2026-05-18T02:48:36.026495+00:00"}