{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2016:QWO6VRN7YKQDCIOHMW6H6AF2OO","short_pith_number":"pith:QWO6VRN7","schema_version":"1.0","canonical_sha256":"859deac5bfc2a03121c765bc7f00ba73a69e23e54d75f62eda6c51d492c86a4a","source":{"kind":"arxiv","id":"1609.02042","version":3},"attestation_state":"computed","paper":{"title":"Polarimetry at millimeter wavelengths with the NIKA camera: calibration and performance","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["physics.ins-det"],"primary_cat":"astro-ph.IM","authors_text":"A. Beelen, A. Beno\\^it, A. Bideaud, A. Catalano, A. Maury, A. Monfardini, A. Ritacco, A. Sievers, B. Comis, C. Kramer, C. Romero, C. Thum, C. Tucker, E. Pascale, F. Mayet, F. Pajot, F. Ruppin, F.-X. D\\'esert, G. Coiffard, G. Pisano, G. Savini, J.F. Mac\\'ias-P\\'erez, J. Goupy, K. Schuster, L. Perotto, L. Rodriguez, M. Calvo, M. Rebolo-Iglesias, N. Billot, N. Ponthieu, O. Bourrion, P. Ade, P. Andr\\'e, P. Mauskopf, R. Adam, R. Zylka, S. Doyle, S. Leclercq, S. Triqueneaux, V. Rev\\'eret","submitted_at":"2016-09-07T16:04:49Z","abstract_excerpt":"Magnetic fields, which play a major role in a large number of astrophysical processes from galactic to cosmological scales, can be traced via observations of dust polarization as demonstrated by the Planck satellite results. In particular, low-resolution observations of dust polarization have demonstrated that Galactic filamentary structures, where star formation takes place, are associated to well organized magnetic fields. A better understanding of this process requires detailed observations of galactic dust polarization on scales of 0.01 to 0.1 pc. Such high-resolution polarization observat"},"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":"1609.02042","kind":"arxiv","version":3},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.IM","submitted_at":"2016-09-07T16:04:49Z","cross_cats_sorted":["physics.ins-det"],"title_canon_sha256":"3187652815dd4cb9d9556f83255a65f4a659af14c38ffbe1ed572154ff664303","abstract_canon_sha256":"ca0c2eb304fc8d92037b5a0de67efa634183ef3187a29ac285d5763d5d49130a"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:50:04.261529Z","signature_b64":"ldCZw8pXvYnAjAWT/VHV2i8ta0KWPQ02BesTjK7ZLdylD505biYpJXy2KjqWXXbc3nRduKyZ/UCrVArOr3ulCQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"859deac5bfc2a03121c765bc7f00ba73a69e23e54d75f62eda6c51d492c86a4a","last_reissued_at":"2026-05-18T00:50:04.260693Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:50:04.260693Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Polarimetry at millimeter wavelengths with the NIKA camera: calibration and performance","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["physics.ins-det"],"primary_cat":"astro-ph.IM","authors_text":"A. Beelen, A. Beno\\^it, A. Bideaud, A. Catalano, A. Maury, A. Monfardini, A. Ritacco, A. Sievers, B. Comis, C. Kramer, C. Romero, C. Thum, C. Tucker, E. Pascale, F. Mayet, F. Pajot, F. Ruppin, F.-X. D\\'esert, G. Coiffard, G. Pisano, G. Savini, J.F. Mac\\'ias-P\\'erez, J. Goupy, K. Schuster, L. Perotto, L. Rodriguez, M. Calvo, M. Rebolo-Iglesias, N. Billot, N. Ponthieu, O. Bourrion, P. Ade, P. Andr\\'e, P. Mauskopf, R. Adam, R. Zylka, S. Doyle, S. Leclercq, S. Triqueneaux, V. Rev\\'eret","submitted_at":"2016-09-07T16:04:49Z","abstract_excerpt":"Magnetic fields, which play a major role in a large number of astrophysical processes from galactic to cosmological scales, can be traced via observations of dust polarization as demonstrated by the Planck satellite results. In particular, low-resolution observations of dust polarization have demonstrated that Galactic filamentary structures, where star formation takes place, are associated to well organized magnetic fields. A better understanding of this process requires detailed observations of galactic dust polarization on scales of 0.01 to 0.1 pc. Such high-resolution polarization observat"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1609.02042","kind":"arxiv","version":3},"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":"1609.02042","created_at":"2026-05-18T00:50:04.260838+00:00"},{"alias_kind":"arxiv_version","alias_value":"1609.02042v3","created_at":"2026-05-18T00:50:04.260838+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1609.02042","created_at":"2026-05-18T00:50:04.260838+00:00"},{"alias_kind":"pith_short_12","alias_value":"QWO6VRN7YKQD","created_at":"2026-05-18T12:30:41.710351+00:00"},{"alias_kind":"pith_short_16","alias_value":"QWO6VRN7YKQDCIOH","created_at":"2026-05-18T12:30:41.710351+00:00"},{"alias_kind":"pith_short_8","alias_value":"QWO6VRN7","created_at":"2026-05-18T12:30:41.710351+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/QWO6VRN7YKQDCIOHMW6H6AF2OO","json":"https://pith.science/pith/QWO6VRN7YKQDCIOHMW6H6AF2OO.json","graph_json":"https://pith.science/api/pith-number/QWO6VRN7YKQDCIOHMW6H6AF2OO/graph.json","events_json":"https://pith.science/api/pith-number/QWO6VRN7YKQDCIOHMW6H6AF2OO/events.json","paper":"https://pith.science/paper/QWO6VRN7"},"agent_actions":{"view_html":"https://pith.science/pith/QWO6VRN7YKQDCIOHMW6H6AF2OO","download_json":"https://pith.science/pith/QWO6VRN7YKQDCIOHMW6H6AF2OO.json","view_paper":"https://pith.science/paper/QWO6VRN7","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1609.02042&json=true","fetch_graph":"https://pith.science/api/pith-number/QWO6VRN7YKQDCIOHMW6H6AF2OO/graph.json","fetch_events":"https://pith.science/api/pith-number/QWO6VRN7YKQDCIOHMW6H6AF2OO/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/QWO6VRN7YKQDCIOHMW6H6AF2OO/action/timestamp_anchor","attest_storage":"https://pith.science/pith/QWO6VRN7YKQDCIOHMW6H6AF2OO/action/storage_attestation","attest_author":"https://pith.science/pith/QWO6VRN7YKQDCIOHMW6H6AF2OO/action/author_attestation","sign_citation":"https://pith.science/pith/QWO6VRN7YKQDCIOHMW6H6AF2OO/action/citation_signature","submit_replication":"https://pith.science/pith/QWO6VRN7YKQDCIOHMW6H6AF2OO/action/replication_record"}},"created_at":"2026-05-18T00:50:04.260838+00:00","updated_at":"2026-05-18T00:50:04.260838+00:00"}