{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2025:WDYWXMF5XEQIL2G5NJ4VWJ5BH5","short_pith_number":"pith:WDYWXMF5","schema_version":"1.0","canonical_sha256":"b0f16bb0bdb92085e8dd6a795b27a13f7df2aa6dcf454607e561ed08b4047fc7","source":{"kind":"arxiv","id":"2507.03524","version":1},"attestation_state":"computed","paper":{"title":"Design, Fabrication and Characterization of the Thermal Filter Assembly on the Solar Ultraviolet Imaging Telescope (SUIT) on-board Aditya- L1","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["astro-ph.SR"],"primary_cat":"astro-ph.IM","authors_text":"Aafaque R. Khan, Abhay Kohok, Abhijit Adoni, Akshay Kulkarni, Avyarthana Ghosh, Bhargava Ram B.S., Chaitanya Rajarshi, Deepa Modi, Durgesh Tripathi, Girish M. Gouda, Janmejoy Sarkar, Ketan Patel, Melvin James, Mintu Karmakar, Pravin Khodade, Ramaprakash A.N., Ravi Kesharwani, R. Venkateshwaran, Sajjade F. Mustafa, Sreejith Padinhatteeri","submitted_at":"2025-07-04T12:21:15Z","abstract_excerpt":"The Solar Ultraviolet Imaging Telescope (SUIT) observes the Sun in the near-ultraviolet regime on board the Aditya-L1 satellite, India's dedicated mission to study the Sun. SUIT will image the Sun in the wavelength range of 200-400 nm using 11 science bandpasses with varying spectral bandwidths between 0.1-58 nm. Within this range, the Sun provides huge incoming solar flux to the telescope that also varies by a factor of ~ 20 from the lower end to the upper end of the wavelength band of interest. Thermal Filter Assembly (TFA) is an optical component at the SUIT entrance aperture, directly faci"},"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":"2507.03524","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.IM","submitted_at":"2025-07-04T12:21:15Z","cross_cats_sorted":["astro-ph.SR"],"title_canon_sha256":"94f6bcaad98777fc6747f2eabbf3ea1acf073ffefef5e95391dc46648140ef0c","abstract_canon_sha256":"a76bf3674b196e2b198fd00390ead18af0dfd15045f0349bbfa9440dee5c12be"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T11:32:00.941945Z","signature_b64":"W3HWU/hgPAfU0/xj+VtBsMOg3cPzbaWnguhDasaqTOc3z+2QNKqcptUn3iWNZe7MIf6N8X7s5F0ANRtBb1euAA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"b0f16bb0bdb92085e8dd6a795b27a13f7df2aa6dcf454607e561ed08b4047fc7","last_reissued_at":"2026-07-05T11:32:00.941379Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T11:32:00.941379Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Design, Fabrication and Characterization of the Thermal Filter Assembly on the Solar Ultraviolet Imaging Telescope (SUIT) on-board Aditya- L1","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["astro-ph.SR"],"primary_cat":"astro-ph.IM","authors_text":"Aafaque R. Khan, Abhay Kohok, Abhijit Adoni, Akshay Kulkarni, Avyarthana Ghosh, Bhargava Ram B.S., Chaitanya Rajarshi, Deepa Modi, Durgesh Tripathi, Girish M. Gouda, Janmejoy Sarkar, Ketan Patel, Melvin James, Mintu Karmakar, Pravin Khodade, Ramaprakash A.N., Ravi Kesharwani, R. Venkateshwaran, Sajjade F. Mustafa, Sreejith Padinhatteeri","submitted_at":"2025-07-04T12:21:15Z","abstract_excerpt":"The Solar Ultraviolet Imaging Telescope (SUIT) observes the Sun in the near-ultraviolet regime on board the Aditya-L1 satellite, India's dedicated mission to study the Sun. SUIT will image the Sun in the wavelength range of 200-400 nm using 11 science bandpasses with varying spectral bandwidths between 0.1-58 nm. Within this range, the Sun provides huge incoming solar flux to the telescope that also varies by a factor of ~ 20 from the lower end to the upper end of the wavelength band of interest. Thermal Filter Assembly (TFA) is an optical component at the SUIT entrance aperture, directly faci"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2507.03524","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/2507.03524/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":"2507.03524","created_at":"2026-07-05T11:32:00.941446+00:00"},{"alias_kind":"arxiv_version","alias_value":"2507.03524v1","created_at":"2026-07-05T11:32:00.941446+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2507.03524","created_at":"2026-07-05T11:32:00.941446+00:00"},{"alias_kind":"pith_short_12","alias_value":"WDYWXMF5XEQI","created_at":"2026-07-05T11:32:00.941446+00:00"},{"alias_kind":"pith_short_16","alias_value":"WDYWXMF5XEQIL2G5","created_at":"2026-07-05T11:32:00.941446+00:00"},{"alias_kind":"pith_short_8","alias_value":"WDYWXMF5","created_at":"2026-07-05T11:32:00.941446+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/WDYWXMF5XEQIL2G5NJ4VWJ5BH5","json":"https://pith.science/pith/WDYWXMF5XEQIL2G5NJ4VWJ5BH5.json","graph_json":"https://pith.science/api/pith-number/WDYWXMF5XEQIL2G5NJ4VWJ5BH5/graph.json","events_json":"https://pith.science/api/pith-number/WDYWXMF5XEQIL2G5NJ4VWJ5BH5/events.json","paper":"https://pith.science/paper/WDYWXMF5"},"agent_actions":{"view_html":"https://pith.science/pith/WDYWXMF5XEQIL2G5NJ4VWJ5BH5","download_json":"https://pith.science/pith/WDYWXMF5XEQIL2G5NJ4VWJ5BH5.json","view_paper":"https://pith.science/paper/WDYWXMF5","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2507.03524&json=true","fetch_graph":"https://pith.science/api/pith-number/WDYWXMF5XEQIL2G5NJ4VWJ5BH5/graph.json","fetch_events":"https://pith.science/api/pith-number/WDYWXMF5XEQIL2G5NJ4VWJ5BH5/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/WDYWXMF5XEQIL2G5NJ4VWJ5BH5/action/timestamp_anchor","attest_storage":"https://pith.science/pith/WDYWXMF5XEQIL2G5NJ4VWJ5BH5/action/storage_attestation","attest_author":"https://pith.science/pith/WDYWXMF5XEQIL2G5NJ4VWJ5BH5/action/author_attestation","sign_citation":"https://pith.science/pith/WDYWXMF5XEQIL2G5NJ4VWJ5BH5/action/citation_signature","submit_replication":"https://pith.science/pith/WDYWXMF5XEQIL2G5NJ4VWJ5BH5/action/replication_record"}},"created_at":"2026-07-05T11:32:00.941446+00:00","updated_at":"2026-07-05T11:32:00.941446+00:00"}