{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2020:5C6JFSD5BNZF3BBXG32H2DIKIA","short_pith_number":"pith:5C6JFSD5","schema_version":"1.0","canonical_sha256":"e8bc92c87d0b725d843736f47d0d0a4012091cb67a462953b9b5dfec9e742978","source":{"kind":"arxiv","id":"2007.02702","version":2},"attestation_state":"computed","paper":{"title":"Detection of the magnetar XTE J1810-197 at 150 and 260 GHz with the NIKA2 Kinetic Inductance Detector camera","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE"],"primary_cat":"astro-ph.IM","authors_text":"A. Ritacco, B. Ladjelate, D. John, G. Desvignes, G. Paubert, J. Mac\\'ias-P\\'erez, J. Pe\\~nalver, K. Schuster, M. Calvo, M. Kramer, M. S\\'anchez-Portal, P. Torne, R. Karuppusamy, S. Berta, S. Navarro, S. S\\'anchez","submitted_at":"2020-07-06T12:48:25Z","abstract_excerpt":"The investigation of pulsars between millimetre and optical wavelengths is challenging due to the faintness of the pulsar signals and the relative low sensitivity of the available facilities compared to 100-m class telescopes operating in the centimetre band. The Kinetic Inductance Detector (KID) technology offers large instantaneous bandwidths and a high sensitivity that can help to substantially increase the ability of existing observatories at short wavelengths to detect pulsars and transient emission. To investigate the feasibility of detecting pulsars with KIDs, we observed the anomalous "},"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":"2007.02702","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.IM","submitted_at":"2020-07-06T12:48:25Z","cross_cats_sorted":["astro-ph.HE"],"title_canon_sha256":"a3d5ccc30ee660d4f9617383410478b53cb535958fb0a9e83b2da21b52d2a755","abstract_canon_sha256":"e1e9734a54f86b4ca6ac7286192ceee3370aec6cf63402fe150327ffbf5cdf3e"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T01:23:06.358655Z","signature_b64":"IQpr7p+SeMEZEeEjt5uNOpLICo4RpVNNXfeG34XvRaxGPHmg56U9pj3gjMTzlkMBOXEW1LgsuEJz8uT/O4OeDw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"e8bc92c87d0b725d843736f47d0d0a4012091cb67a462953b9b5dfec9e742978","last_reissued_at":"2026-07-05T01:23:06.358135Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T01:23:06.358135Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Detection of the magnetar XTE J1810-197 at 150 and 260 GHz with the NIKA2 Kinetic Inductance Detector camera","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE"],"primary_cat":"astro-ph.IM","authors_text":"A. Ritacco, B. Ladjelate, D. John, G. Desvignes, G. Paubert, J. Mac\\'ias-P\\'erez, J. Pe\\~nalver, K. Schuster, M. Calvo, M. Kramer, M. S\\'anchez-Portal, P. Torne, R. Karuppusamy, S. Berta, S. Navarro, S. S\\'anchez","submitted_at":"2020-07-06T12:48:25Z","abstract_excerpt":"The investigation of pulsars between millimetre and optical wavelengths is challenging due to the faintness of the pulsar signals and the relative low sensitivity of the available facilities compared to 100-m class telescopes operating in the centimetre band. The Kinetic Inductance Detector (KID) technology offers large instantaneous bandwidths and a high sensitivity that can help to substantially increase the ability of existing observatories at short wavelengths to detect pulsars and transient emission. To investigate the feasibility of detecting pulsars with KIDs, we observed the anomalous "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2007.02702","kind":"arxiv","version":2},"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/2007.02702/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":"2007.02702","created_at":"2026-07-05T01:23:06.358199+00:00"},{"alias_kind":"arxiv_version","alias_value":"2007.02702v2","created_at":"2026-07-05T01:23:06.358199+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2007.02702","created_at":"2026-07-05T01:23:06.358199+00:00"},{"alias_kind":"pith_short_12","alias_value":"5C6JFSD5BNZF","created_at":"2026-07-05T01:23:06.358199+00:00"},{"alias_kind":"pith_short_16","alias_value":"5C6JFSD5BNZF3BBX","created_at":"2026-07-05T01:23:06.358199+00:00"},{"alias_kind":"pith_short_8","alias_value":"5C6JFSD5","created_at":"2026-07-05T01:23:06.358199+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/5C6JFSD5BNZF3BBXG32H2DIKIA","json":"https://pith.science/pith/5C6JFSD5BNZF3BBXG32H2DIKIA.json","graph_json":"https://pith.science/api/pith-number/5C6JFSD5BNZF3BBXG32H2DIKIA/graph.json","events_json":"https://pith.science/api/pith-number/5C6JFSD5BNZF3BBXG32H2DIKIA/events.json","paper":"https://pith.science/paper/5C6JFSD5"},"agent_actions":{"view_html":"https://pith.science/pith/5C6JFSD5BNZF3BBXG32H2DIKIA","download_json":"https://pith.science/pith/5C6JFSD5BNZF3BBXG32H2DIKIA.json","view_paper":"https://pith.science/paper/5C6JFSD5","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2007.02702&json=true","fetch_graph":"https://pith.science/api/pith-number/5C6JFSD5BNZF3BBXG32H2DIKIA/graph.json","fetch_events":"https://pith.science/api/pith-number/5C6JFSD5BNZF3BBXG32H2DIKIA/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/5C6JFSD5BNZF3BBXG32H2DIKIA/action/timestamp_anchor","attest_storage":"https://pith.science/pith/5C6JFSD5BNZF3BBXG32H2DIKIA/action/storage_attestation","attest_author":"https://pith.science/pith/5C6JFSD5BNZF3BBXG32H2DIKIA/action/author_attestation","sign_citation":"https://pith.science/pith/5C6JFSD5BNZF3BBXG32H2DIKIA/action/citation_signature","submit_replication":"https://pith.science/pith/5C6JFSD5BNZF3BBXG32H2DIKIA/action/replication_record"}},"created_at":"2026-07-05T01:23:06.358199+00:00","updated_at":"2026-07-05T01:23:06.358199+00:00"}