{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2012:GEP2GNIS4O6RHDA6EN56IJ2AQW","short_pith_number":"pith:GEP2GNIS","schema_version":"1.0","canonical_sha256":"311fa33512e3bd138c1e237be4274085bc1371edee78549fde4ecc7703ccfbc9","source":{"kind":"arxiv","id":"1209.6347","version":3},"attestation_state":"computed","paper":{"title":"Results and perspectives of the solar axion search with the CAST experiment","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"hep-ex","authors_text":"A. Belov, A. Gardikiotis, A. Liolios, A. Ljubi\\v{c}i\\'c, A. Nordt, A. Rodr\\'iguez, A. Tom\\'as, B. Laki\\'c, C. Eleftheriadis, C. Ezer, D. H. H. Hoffmann, E. Ferrer-Ribas, E. Gruber, E. N. Gazis, F. Haug, F. J. Iguaz, G. Cantatore, G. Fanourakis, G. Lutz, G. Luz\\'on, G. Raffelt, H. Br\\\"auninger, H. G\\'omez, H. Riege, I. Giomataris, I. G. Irastorza, I. Savvidis, J. A. Garc\\'ia, J. Gal\\'an, J. G. Garza, J. I. Collar, J. Jacoby, J. K. Vogel, J. M. Carmona, J. M. Laurent, J. Morales, J. Ruz, J. Villar, K. Barth, K. Jakov\\v{c}i\\'c, K. K\\\"onigsmann, K. van Bibber, K. Zioutas (CAST Collaboration), L. Stewart, M. Arik, M. Davenport, M. D. Hasinoff, M. J. Pivovaroff, M. Karuza, M. Kr\\v{c}mar, M. Kuster, M. Rosu, M. Tsagri, N. Elias, P. Friedrich, P. S. Silva, R. Hartmann, R. Kotthaus, S. A. Cetin, S. Aune, S. Borghi, S. C. Yildiz, S. Gninenko, S. K. Solanki, T. Dafni, T. Geralis, T. Guth\\\"orl, T. Niinikoski, T. Papaevangelou, T. Rashba, T. Vafeiadis, V. Lozza","submitted_at":"2012-09-27T19:52:42Z","abstract_excerpt":"The status of the solar axion search with the CERN Axion Solar Telescope (CAST) will be presented. Recent results obtained by the use of $^3$He as a buffer gas has allowed us to extend our sensitivity to higher axion masses than our previous measurements with $^4$He. With about 1 h of data taking at each of 252 different pressure settings we have scanned the axion mass range 0.39 eV$ \\le m_{a} \\le $ 0.64 eV. From the absence of an excess of x rays when the magnet was pointing to the Sun we set a typical upper limit on the axion-photon coupling of g$_{a\\gamma} \\le 2.3\\times 10^{-10}$ GeV$^{-1}$"},"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":"1209.6347","kind":"arxiv","version":3},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-ex","submitted_at":"2012-09-27T19:52:42Z","cross_cats_sorted":["astro-ph.CO"],"title_canon_sha256":"6f9c72aeb5b0a7f6d1a78f410d76f270efce044f5a3323141188626fafb03af9","abstract_canon_sha256":"ac367a56b541439ee2dfad1f8211d0068541f8da9bc8d26502ce96f63add8e39"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:09:26.314443Z","signature_b64":"aV7wodLhnrfIqw1RaAVCAU3AFUA9H9KqIxa12o+ALLh+N/PRj/AgyBAwMWHy0Ag//jh1JqwPvjY7EZBH9gslBg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"311fa33512e3bd138c1e237be4274085bc1371edee78549fde4ecc7703ccfbc9","last_reissued_at":"2026-05-18T01:09:26.313968Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:09:26.313968Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Results and perspectives of the solar axion search with the CAST experiment","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"hep-ex","authors_text":"A. Belov, A. Gardikiotis, A. Liolios, A. Ljubi\\v{c}i\\'c, A. Nordt, A. Rodr\\'iguez, A. Tom\\'as, B. Laki\\'c, C. Eleftheriadis, C. Ezer, D. H. H. Hoffmann, E. Ferrer-Ribas, E. Gruber, E. N. Gazis, F. Haug, F. J. Iguaz, G. Cantatore, G. Fanourakis, G. Lutz, G. Luz\\'on, G. Raffelt, H. Br\\\"auninger, H. G\\'omez, H. Riege, I. Giomataris, I. G. Irastorza, I. Savvidis, J. A. Garc\\'ia, J. Gal\\'an, J. G. Garza, J. I. Collar, J. Jacoby, J. K. Vogel, J. M. Carmona, J. M. Laurent, J. Morales, J. Ruz, J. Villar, K. Barth, K. Jakov\\v{c}i\\'c, K. K\\\"onigsmann, K. van Bibber, K. Zioutas (CAST Collaboration), L. Stewart, M. Arik, M. Davenport, M. D. Hasinoff, M. J. Pivovaroff, M. Karuza, M. Kr\\v{c}mar, M. Kuster, M. Rosu, M. Tsagri, N. Elias, P. Friedrich, P. S. Silva, R. Hartmann, R. Kotthaus, S. A. Cetin, S. Aune, S. Borghi, S. C. Yildiz, S. Gninenko, S. K. Solanki, T. Dafni, T. Geralis, T. Guth\\\"orl, T. Niinikoski, T. Papaevangelou, T. Rashba, T. Vafeiadis, V. Lozza","submitted_at":"2012-09-27T19:52:42Z","abstract_excerpt":"The status of the solar axion search with the CERN Axion Solar Telescope (CAST) will be presented. Recent results obtained by the use of $^3$He as a buffer gas has allowed us to extend our sensitivity to higher axion masses than our previous measurements with $^4$He. With about 1 h of data taking at each of 252 different pressure settings we have scanned the axion mass range 0.39 eV$ \\le m_{a} \\le $ 0.64 eV. From the absence of an excess of x rays when the magnet was pointing to the Sun we set a typical upper limit on the axion-photon coupling of g$_{a\\gamma} \\le 2.3\\times 10^{-10}$ GeV$^{-1}$"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1209.6347","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":"1209.6347","created_at":"2026-05-18T01:09:26.314039+00:00"},{"alias_kind":"arxiv_version","alias_value":"1209.6347v3","created_at":"2026-05-18T01:09:26.314039+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1209.6347","created_at":"2026-05-18T01:09:26.314039+00:00"},{"alias_kind":"pith_short_12","alias_value":"GEP2GNIS4O6R","created_at":"2026-05-18T12:27:06.952714+00:00"},{"alias_kind":"pith_short_16","alias_value":"GEP2GNIS4O6RHDA6","created_at":"2026-05-18T12:27:06.952714+00:00"},{"alias_kind":"pith_short_8","alias_value":"GEP2GNIS","created_at":"2026-05-18T12:27:06.952714+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/GEP2GNIS4O6RHDA6EN56IJ2AQW","json":"https://pith.science/pith/GEP2GNIS4O6RHDA6EN56IJ2AQW.json","graph_json":"https://pith.science/api/pith-number/GEP2GNIS4O6RHDA6EN56IJ2AQW/graph.json","events_json":"https://pith.science/api/pith-number/GEP2GNIS4O6RHDA6EN56IJ2AQW/events.json","paper":"https://pith.science/paper/GEP2GNIS"},"agent_actions":{"view_html":"https://pith.science/pith/GEP2GNIS4O6RHDA6EN56IJ2AQW","download_json":"https://pith.science/pith/GEP2GNIS4O6RHDA6EN56IJ2AQW.json","view_paper":"https://pith.science/paper/GEP2GNIS","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1209.6347&json=true","fetch_graph":"https://pith.science/api/pith-number/GEP2GNIS4O6RHDA6EN56IJ2AQW/graph.json","fetch_events":"https://pith.science/api/pith-number/GEP2GNIS4O6RHDA6EN56IJ2AQW/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/GEP2GNIS4O6RHDA6EN56IJ2AQW/action/timestamp_anchor","attest_storage":"https://pith.science/pith/GEP2GNIS4O6RHDA6EN56IJ2AQW/action/storage_attestation","attest_author":"https://pith.science/pith/GEP2GNIS4O6RHDA6EN56IJ2AQW/action/author_attestation","sign_citation":"https://pith.science/pith/GEP2GNIS4O6RHDA6EN56IJ2AQW/action/citation_signature","submit_replication":"https://pith.science/pith/GEP2GNIS4O6RHDA6EN56IJ2AQW/action/replication_record"}},"created_at":"2026-05-18T01:09:26.314039+00:00","updated_at":"2026-05-18T01:09:26.314039+00:00"}