{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2009:G5E6Q6WOVBGPRHVCX7YPC2EDWV","short_pith_number":"pith:G5E6Q6WO","schema_version":"1.0","canonical_sha256":"3749e87acea84cf89ea2bff0f16883b552748b44eafb524b0e7937d18bad7454","source":{"kind":"arxiv","id":"0904.3788","version":1},"attestation_state":"computed","paper":{"title":"Calibration and Performance of the AKARI Far-Infrared Surveyor (FIS) -- Slow-Scan Observation Mode for Point Sources","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.IM","authors_text":"Hidehiro Kaneda, Hiroshi Shibai, Issei Yamamura, Mai Shirahata, Martin Cohen, Mitsunobu Kawada, Shuji Matsuura, Sin'itirou Makiuti, Sunao Hasegawa, Takafumi Ootsubo, Takao Nakagawa, Thomas Muller, Toyoaki Suzuki, Yasuo Doi","submitted_at":"2009-04-24T03:27:59Z","abstract_excerpt":"We present the characterization and calibration of the Slow-Scan observation mode of the Far-Infrared Surveyor (FIS) onboard the AKARI satellite. The FIS, one of the two focal-plane instruments on AKARI, has four photometric bands between 50--180 um with two types of Ge:Ga array detectors. In addition to the All-Sky Survey, FIS has also taken detailed far-infrared images of selected targets by using the Slow-Scan mode. The sensitivity of the Slow-Scan mode is one to two orders of magnitude better than that of the All-Sky Survey, because the exposure time on a targeted source is much longer. Th"},"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":"0904.3788","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.IM","submitted_at":"2009-04-24T03:27:59Z","cross_cats_sorted":[],"title_canon_sha256":"25427ca6b395013d83c92ed6bcd57197f9f160a6dde77a004f449bd57cfb7a0a","abstract_canon_sha256":"c16de124ca5143dea8a6058319e18b774a8501bc7ff5106b7b1eed1e76894329"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:13:57.654634Z","signature_b64":"lWPZNeY/JhkDycWVpQA1bftLNOvDPZsS/IK9kUG8vd8RIbhQN3pRwVCrFst8j0vFPZiPuFwg2e++izMJRPUkAg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"3749e87acea84cf89ea2bff0f16883b552748b44eafb524b0e7937d18bad7454","last_reissued_at":"2026-05-18T02:13:57.653931Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:13:57.653931Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Calibration and Performance of the AKARI Far-Infrared Surveyor (FIS) -- Slow-Scan Observation Mode for Point Sources","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.IM","authors_text":"Hidehiro Kaneda, Hiroshi Shibai, Issei Yamamura, Mai Shirahata, Martin Cohen, Mitsunobu Kawada, Shuji Matsuura, Sin'itirou Makiuti, Sunao Hasegawa, Takafumi Ootsubo, Takao Nakagawa, Thomas Muller, Toyoaki Suzuki, Yasuo Doi","submitted_at":"2009-04-24T03:27:59Z","abstract_excerpt":"We present the characterization and calibration of the Slow-Scan observation mode of the Far-Infrared Surveyor (FIS) onboard the AKARI satellite. The FIS, one of the two focal-plane instruments on AKARI, has four photometric bands between 50--180 um with two types of Ge:Ga array detectors. In addition to the All-Sky Survey, FIS has also taken detailed far-infrared images of selected targets by using the Slow-Scan mode. The sensitivity of the Slow-Scan mode is one to two orders of magnitude better than that of the All-Sky Survey, because the exposure time on a targeted source is much longer. Th"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"0904.3788","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":"0904.3788","created_at":"2026-05-18T02:13:57.654047+00:00"},{"alias_kind":"arxiv_version","alias_value":"0904.3788v1","created_at":"2026-05-18T02:13:57.654047+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.0904.3788","created_at":"2026-05-18T02:13:57.654047+00:00"},{"alias_kind":"pith_short_12","alias_value":"G5E6Q6WOVBGP","created_at":"2026-05-18T12:25:59.703012+00:00"},{"alias_kind":"pith_short_16","alias_value":"G5E6Q6WOVBGPRHVC","created_at":"2026-05-18T12:25:59.703012+00:00"},{"alias_kind":"pith_short_8","alias_value":"G5E6Q6WO","created_at":"2026-05-18T12:25:59.703012+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/G5E6Q6WOVBGPRHVCX7YPC2EDWV","json":"https://pith.science/pith/G5E6Q6WOVBGPRHVCX7YPC2EDWV.json","graph_json":"https://pith.science/api/pith-number/G5E6Q6WOVBGPRHVCX7YPC2EDWV/graph.json","events_json":"https://pith.science/api/pith-number/G5E6Q6WOVBGPRHVCX7YPC2EDWV/events.json","paper":"https://pith.science/paper/G5E6Q6WO"},"agent_actions":{"view_html":"https://pith.science/pith/G5E6Q6WOVBGPRHVCX7YPC2EDWV","download_json":"https://pith.science/pith/G5E6Q6WOVBGPRHVCX7YPC2EDWV.json","view_paper":"https://pith.science/paper/G5E6Q6WO","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=0904.3788&json=true","fetch_graph":"https://pith.science/api/pith-number/G5E6Q6WOVBGPRHVCX7YPC2EDWV/graph.json","fetch_events":"https://pith.science/api/pith-number/G5E6Q6WOVBGPRHVCX7YPC2EDWV/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/G5E6Q6WOVBGPRHVCX7YPC2EDWV/action/timestamp_anchor","attest_storage":"https://pith.science/pith/G5E6Q6WOVBGPRHVCX7YPC2EDWV/action/storage_attestation","attest_author":"https://pith.science/pith/G5E6Q6WOVBGPRHVCX7YPC2EDWV/action/author_attestation","sign_citation":"https://pith.science/pith/G5E6Q6WOVBGPRHVCX7YPC2EDWV/action/citation_signature","submit_replication":"https://pith.science/pith/G5E6Q6WOVBGPRHVCX7YPC2EDWV/action/replication_record"}},"created_at":"2026-05-18T02:13:57.654047+00:00","updated_at":"2026-05-18T02:13:57.654047+00:00"}