{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2018:7ORJT2NTIP743CYDFQDENF7OUT","short_pith_number":"pith:7ORJT2NT","schema_version":"1.0","canonical_sha256":"fba299e9b343ffcd8b032c064697eea4f1e6115c03c741ddb6e7e8e97c3fd1d5","source":{"kind":"arxiv","id":"1803.02094","version":1},"attestation_state":"computed","paper":{"title":"Developments of Multi-wavelength Spectro-Polarimeter on the Domeless Solar Telescope at Hida Observatory","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.SR"],"primary_cat":"astro-ph.IM","authors_text":"Goichi Kimura, Kiyoshi Ichimoto, Naoki Kaneda, Sanetaka Okada, Satoru UeNo, Shota Ninomiya, Tetsu Anan, Yoshikazu Nakatani, Yu Wei Huang","submitted_at":"2018-03-06T10:26:07Z","abstract_excerpt":"To obtain full Stokes spectra in multi-wavelength windows simultaneously, we developed a new spectro-polarimeter on the Domeless Solar Telescope at Hida Observatory. The new polarimeter consists of a 60 cm aperture vacuum telescope on an altazimuth mount, an image rotator, a high dispersion spectrograph, polarization modulator and analyzer composed of a continuously rotating waveplate with a retardation nearly constant around 127$^{circ}$ in 500 - 1100 nm and a polarizing beam splitter located closely behind the focus of the telescope, fast and large format CMOS cameras and an infrared camera."},"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":"1803.02094","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.IM","submitted_at":"2018-03-06T10:26:07Z","cross_cats_sorted":["astro-ph.SR"],"title_canon_sha256":"d13b4807f61f32bfc6e245e44fc4584a424f60921891728f75837b88ddf093f6","abstract_canon_sha256":"92cc6b8972cb3bcc6af4a256efda05d93004cbc65c6de4edd6ace3a80a83573a"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:13:27.286824Z","signature_b64":"Z7gO1+duv68XjLnBlvA7AvggUp3iyTgTJcYgxTlJRSVRaEHcjeNc+VTAkOuStPwTdU3Fw3wNimcjN/8+cG2jBw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"fba299e9b343ffcd8b032c064697eea4f1e6115c03c741ddb6e7e8e97c3fd1d5","last_reissued_at":"2026-05-18T00:13:27.286190Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:13:27.286190Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Developments of Multi-wavelength Spectro-Polarimeter on the Domeless Solar Telescope at Hida Observatory","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.SR"],"primary_cat":"astro-ph.IM","authors_text":"Goichi Kimura, Kiyoshi Ichimoto, Naoki Kaneda, Sanetaka Okada, Satoru UeNo, Shota Ninomiya, Tetsu Anan, Yoshikazu Nakatani, Yu Wei Huang","submitted_at":"2018-03-06T10:26:07Z","abstract_excerpt":"To obtain full Stokes spectra in multi-wavelength windows simultaneously, we developed a new spectro-polarimeter on the Domeless Solar Telescope at Hida Observatory. The new polarimeter consists of a 60 cm aperture vacuum telescope on an altazimuth mount, an image rotator, a high dispersion spectrograph, polarization modulator and analyzer composed of a continuously rotating waveplate with a retardation nearly constant around 127$^{circ}$ in 500 - 1100 nm and a polarizing beam splitter located closely behind the focus of the telescope, fast and large format CMOS cameras and an infrared camera."},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1803.02094","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":"1803.02094","created_at":"2026-05-18T00:13:27.286306+00:00"},{"alias_kind":"arxiv_version","alias_value":"1803.02094v1","created_at":"2026-05-18T00:13:27.286306+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1803.02094","created_at":"2026-05-18T00:13:27.286306+00:00"},{"alias_kind":"pith_short_12","alias_value":"7ORJT2NTIP74","created_at":"2026-05-18T12:32:11.075285+00:00"},{"alias_kind":"pith_short_16","alias_value":"7ORJT2NTIP743CYD","created_at":"2026-05-18T12:32:11.075285+00:00"},{"alias_kind":"pith_short_8","alias_value":"7ORJT2NT","created_at":"2026-05-18T12:32:11.075285+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/7ORJT2NTIP743CYDFQDENF7OUT","json":"https://pith.science/pith/7ORJT2NTIP743CYDFQDENF7OUT.json","graph_json":"https://pith.science/api/pith-number/7ORJT2NTIP743CYDFQDENF7OUT/graph.json","events_json":"https://pith.science/api/pith-number/7ORJT2NTIP743CYDFQDENF7OUT/events.json","paper":"https://pith.science/paper/7ORJT2NT"},"agent_actions":{"view_html":"https://pith.science/pith/7ORJT2NTIP743CYDFQDENF7OUT","download_json":"https://pith.science/pith/7ORJT2NTIP743CYDFQDENF7OUT.json","view_paper":"https://pith.science/paper/7ORJT2NT","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1803.02094&json=true","fetch_graph":"https://pith.science/api/pith-number/7ORJT2NTIP743CYDFQDENF7OUT/graph.json","fetch_events":"https://pith.science/api/pith-number/7ORJT2NTIP743CYDFQDENF7OUT/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/7ORJT2NTIP743CYDFQDENF7OUT/action/timestamp_anchor","attest_storage":"https://pith.science/pith/7ORJT2NTIP743CYDFQDENF7OUT/action/storage_attestation","attest_author":"https://pith.science/pith/7ORJT2NTIP743CYDFQDENF7OUT/action/author_attestation","sign_citation":"https://pith.science/pith/7ORJT2NTIP743CYDFQDENF7OUT/action/citation_signature","submit_replication":"https://pith.science/pith/7ORJT2NTIP743CYDFQDENF7OUT/action/replication_record"}},"created_at":"2026-05-18T00:13:27.286306+00:00","updated_at":"2026-05-18T00:13:27.286306+00:00"}