{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2024:AIFDECTB6YWPRTEYHWYACBCKD4","short_pith_number":"pith:AIFDECTB","schema_version":"1.0","canonical_sha256":"020a320a61f62cf8cc983db001044a1f33ac61ee8de92fa5d13e0bd3f6d059a1","source":{"kind":"arxiv","id":"2411.08092","version":1},"attestation_state":"computed","paper":{"title":"Preparing for the Early eVolution Explorer: Characterizing the photochemical inputs and transit detection efficiencies of young planets using multiwavelength flare observations by TESS and Swift","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.SR"],"primary_cat":"astro-ph.EP","authors_text":"Adina D. Feinstein, Ann Marie Cody, Jennifer A. Burt, Laura D. Vega, Laura Venuti, Meredith A. MacGregor, Neal J. Turner, Valerie J. Scott, Ward S. Howard","submitted_at":"2024-11-12T19:00:00Z","abstract_excerpt":"Ultraviolet flare emission can drive photochemistry in exoplanet atmospheres and even serve as the primary source of uncertainty in atmospheric retrievals. Additionally, flare energy budgets are not well-understood due to a paucity of simultaneous observations. We present new near-UV (NUV) and optical observations of flares from three M dwarfs obtained at 20 s cadence with Swift and TESS, along with a re-analysis of flares from two M dwarfs in order to explore the energy budget and timing of flares at NUV--optical wavelengths. We find a 9000 K blackbody underestimates the NUV flux by $\\geq$2$\\"},"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":"2411.08092","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.EP","submitted_at":"2024-11-12T19:00:00Z","cross_cats_sorted":["astro-ph.SR"],"title_canon_sha256":"681c59050ae960386e64555931b81d8e30ac8d255ac0ac9762706b94f29672e3","abstract_canon_sha256":"dd5d4cdbfe9fd9e1c119ef89d9b5e1c29201088704327b8d6dcdd86b36704368"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T09:34:41.410324Z","signature_b64":"eXvbk1aYQlO46NKm9GKibXiK972DtJHKPd21LetuaSdHfC2MSXQZvF+Qv6CG3lLuWNZPWwMSNZan7gfT3V/hCA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"020a320a61f62cf8cc983db001044a1f33ac61ee8de92fa5d13e0bd3f6d059a1","last_reissued_at":"2026-07-05T09:34:41.409817Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T09:34:41.409817Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Preparing for the Early eVolution Explorer: Characterizing the photochemical inputs and transit detection efficiencies of young planets using multiwavelength flare observations by TESS and Swift","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.SR"],"primary_cat":"astro-ph.EP","authors_text":"Adina D. Feinstein, Ann Marie Cody, Jennifer A. Burt, Laura D. Vega, Laura Venuti, Meredith A. MacGregor, Neal J. Turner, Valerie J. Scott, Ward S. Howard","submitted_at":"2024-11-12T19:00:00Z","abstract_excerpt":"Ultraviolet flare emission can drive photochemistry in exoplanet atmospheres and even serve as the primary source of uncertainty in atmospheric retrievals. Additionally, flare energy budgets are not well-understood due to a paucity of simultaneous observations. We present new near-UV (NUV) and optical observations of flares from three M dwarfs obtained at 20 s cadence with Swift and TESS, along with a re-analysis of flares from two M dwarfs in order to explore the energy budget and timing of flares at NUV--optical wavelengths. We find a 9000 K blackbody underestimates the NUV flux by $\\geq$2$\\"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2411.08092","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/2411.08092/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":"2411.08092","created_at":"2026-07-05T09:34:41.409876+00:00"},{"alias_kind":"arxiv_version","alias_value":"2411.08092v1","created_at":"2026-07-05T09:34:41.409876+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2411.08092","created_at":"2026-07-05T09:34:41.409876+00:00"},{"alias_kind":"pith_short_12","alias_value":"AIFDECTB6YWP","created_at":"2026-07-05T09:34:41.409876+00:00"},{"alias_kind":"pith_short_16","alias_value":"AIFDECTB6YWPRTEY","created_at":"2026-07-05T09:34:41.409876+00:00"},{"alias_kind":"pith_short_8","alias_value":"AIFDECTB","created_at":"2026-07-05T09:34:41.409876+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/AIFDECTB6YWPRTEYHWYACBCKD4","json":"https://pith.science/pith/AIFDECTB6YWPRTEYHWYACBCKD4.json","graph_json":"https://pith.science/api/pith-number/AIFDECTB6YWPRTEYHWYACBCKD4/graph.json","events_json":"https://pith.science/api/pith-number/AIFDECTB6YWPRTEYHWYACBCKD4/events.json","paper":"https://pith.science/paper/AIFDECTB"},"agent_actions":{"view_html":"https://pith.science/pith/AIFDECTB6YWPRTEYHWYACBCKD4","download_json":"https://pith.science/pith/AIFDECTB6YWPRTEYHWYACBCKD4.json","view_paper":"https://pith.science/paper/AIFDECTB","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2411.08092&json=true","fetch_graph":"https://pith.science/api/pith-number/AIFDECTB6YWPRTEYHWYACBCKD4/graph.json","fetch_events":"https://pith.science/api/pith-number/AIFDECTB6YWPRTEYHWYACBCKD4/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/AIFDECTB6YWPRTEYHWYACBCKD4/action/timestamp_anchor","attest_storage":"https://pith.science/pith/AIFDECTB6YWPRTEYHWYACBCKD4/action/storage_attestation","attest_author":"https://pith.science/pith/AIFDECTB6YWPRTEYHWYACBCKD4/action/author_attestation","sign_citation":"https://pith.science/pith/AIFDECTB6YWPRTEYHWYACBCKD4/action/citation_signature","submit_replication":"https://pith.science/pith/AIFDECTB6YWPRTEYHWYACBCKD4/action/replication_record"}},"created_at":"2026-07-05T09:34:41.409876+00:00","updated_at":"2026-07-05T09:34:41.409876+00:00"}