{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2015:AQY3ZWFWYQYFR2EPNB35QTDEBH","short_pith_number":"pith:AQY3ZWFW","schema_version":"1.0","canonical_sha256":"0431bcd8b6c43058e88f6877d84c6409d35f41db6114644ec027436d5308b01f","source":{"kind":"arxiv","id":"1507.06758","version":1},"attestation_state":"computed","paper":{"title":"Study of the diffuse gamma-ray emission from the Galactic plane with ARGO-YBJ","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE","hep-ph"],"primary_cat":"astro-ph.IM","authors_text":"A. Budano, A. D'Amone, A.F. Yuan, A. Surdo, B. Bartoli, B. D'Ettorre Piazzoli, B.Z. Dai, C.C. Ning, C.F. Feng, C. Liu, C. Vigorito, C.Y. Wu, Danzengluobu, D. Martello, F. Ruggieri, F.R. Zhu, F. Shi, G. Di Sciascio, G. Liguori, G. Mancarella, G. Marsella, G. Zizzi, Haibing Hu, H.H. He, H.J. Li, H. Lu, H.M. Zhang, Hongbo Hu, H.R. Wu, H. Wang, H.Y. Jia, I. De Mitri, J. Liu, J. Zhao, Labaciren, L.L. Ma, L. Perrone, L. Xue, L. Zhang, M. Iacovacci, M. Panareo, M.Y. Liu, M. Zha, P. Bernardini, P. Branchini, P. Camarri, P. Creti, P. Montini, P. Pistilli, P.R. Shen, P. Salvini, P. Vallania, Q.B. Gou, Q.Q. Zhu, Q.Y. Yang, R. Cardarelli, R. Iuppa, R. Santonico, S. Catalanotti, S. Mastroianni, S.M. Mari, S. Vernetto, S.W. Cui, S.Z. Chen, T. Di Girolamo, T.L. Chen, X.C. Yang, X.D. Sheng, X.H. Ma, X.J. Bi, X.X. Zhou, X.Y. Zhang, Y.H. Tan, Y.Q. Guo, Y. Zhang, Z. Cao, Z.G. Yao, Zhaoyang Feng, Zhaxiciren, Zhaxisangzhu, Zhenyong Feng","submitted_at":"2015-07-24T06:48:56Z","abstract_excerpt":"The events recorded by ARGO-YBJ in more than five years of data collection have been analyzed to determine the diffuse gamma-ray emission in the Galactic plane at Galactic longitudes 25{\\deg} < l < 100{\\deg} and Galactic latitudes . The energy range covered by this analysis, from ~350 GeV to ~2 TeV, allows the connection of the region explored by Fermi with the multi-TeV measurements carried out by Milagro. Our analysis has been focused on two selected regions of the Galactic plane, i.e., 40{\\deg} < l < 100{\\deg} and 65{\\deg} < l < 85{\\deg} (the Cygnus region), where Milagro observed an excess"},"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":"1507.06758","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.IM","submitted_at":"2015-07-24T06:48:56Z","cross_cats_sorted":["astro-ph.HE","hep-ph"],"title_canon_sha256":"828674c30272d4711f0aab66cab1e2717fd11e56a6cec688416b882ff40ea4f5","abstract_canon_sha256":"bd61f78a6816a4ec0dcc823118eb3e97dd1d75bb9e023ef9b74c0ddd58ecaec0"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:36:22.455764Z","signature_b64":"lTqNlm5K9vRRnNEiFwILNK8/qVLTWpoo8HmVhLa/fKPI9x+PCjRSqHeLsl2WhXkEotc+My6X59UJ0paS6Qo5DQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"0431bcd8b6c43058e88f6877d84c6409d35f41db6114644ec027436d5308b01f","last_reissued_at":"2026-05-18T01:36:22.455229Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:36:22.455229Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Study of the diffuse gamma-ray emission from the Galactic plane with ARGO-YBJ","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE","hep-ph"],"primary_cat":"astro-ph.IM","authors_text":"A. Budano, A. D'Amone, A.F. Yuan, A. Surdo, B. Bartoli, B. D'Ettorre Piazzoli, B.Z. Dai, C.C. Ning, C.F. Feng, C. Liu, C. Vigorito, C.Y. Wu, Danzengluobu, D. Martello, F. Ruggieri, F.R. Zhu, F. Shi, G. Di Sciascio, G. Liguori, G. Mancarella, G. Marsella, G. Zizzi, Haibing Hu, H.H. He, H.J. Li, H. Lu, H.M. Zhang, Hongbo Hu, H.R. Wu, H. Wang, H.Y. Jia, I. De Mitri, J. Liu, J. Zhao, Labaciren, L.L. Ma, L. Perrone, L. Xue, L. Zhang, M. Iacovacci, M. Panareo, M.Y. Liu, M. Zha, P. Bernardini, P. Branchini, P. Camarri, P. Creti, P. Montini, P. Pistilli, P.R. Shen, P. Salvini, P. Vallania, Q.B. Gou, Q.Q. Zhu, Q.Y. Yang, R. Cardarelli, R. Iuppa, R. Santonico, S. Catalanotti, S. Mastroianni, S.M. Mari, S. Vernetto, S.W. Cui, S.Z. Chen, T. Di Girolamo, T.L. Chen, X.C. Yang, X.D. Sheng, X.H. Ma, X.J. Bi, X.X. Zhou, X.Y. Zhang, Y.H. Tan, Y.Q. Guo, Y. Zhang, Z. Cao, Z.G. Yao, Zhaoyang Feng, Zhaxiciren, Zhaxisangzhu, Zhenyong Feng","submitted_at":"2015-07-24T06:48:56Z","abstract_excerpt":"The events recorded by ARGO-YBJ in more than five years of data collection have been analyzed to determine the diffuse gamma-ray emission in the Galactic plane at Galactic longitudes 25{\\deg} < l < 100{\\deg} and Galactic latitudes . The energy range covered by this analysis, from ~350 GeV to ~2 TeV, allows the connection of the region explored by Fermi with the multi-TeV measurements carried out by Milagro. Our analysis has been focused on two selected regions of the Galactic plane, i.e., 40{\\deg} < l < 100{\\deg} and 65{\\deg} < l < 85{\\deg} (the Cygnus region), where Milagro observed an excess"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1507.06758","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":"1507.06758","created_at":"2026-05-18T01:36:22.455320+00:00"},{"alias_kind":"arxiv_version","alias_value":"1507.06758v1","created_at":"2026-05-18T01:36:22.455320+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1507.06758","created_at":"2026-05-18T01:36:22.455320+00:00"},{"alias_kind":"pith_short_12","alias_value":"AQY3ZWFWYQYF","created_at":"2026-05-18T12:29:10.953037+00:00"},{"alias_kind":"pith_short_16","alias_value":"AQY3ZWFWYQYFR2EP","created_at":"2026-05-18T12:29:10.953037+00:00"},{"alias_kind":"pith_short_8","alias_value":"AQY3ZWFW","created_at":"2026-05-18T12:29:10.953037+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":2,"internal_anchor_count":2,"sample":[{"citing_arxiv_id":"2606.23476","citing_title":"TeV-PeV Gamma-ray and Neutrino Emission in the Galactic Plane","ref_index":144,"is_internal_anchor":true},{"citing_arxiv_id":"2404.15944","citing_title":"IceCube Results and Perspective for Neutrinos from LHAASO Sources","ref_index":88,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/AQY3ZWFWYQYFR2EPNB35QTDEBH","json":"https://pith.science/pith/AQY3ZWFWYQYFR2EPNB35QTDEBH.json","graph_json":"https://pith.science/api/pith-number/AQY3ZWFWYQYFR2EPNB35QTDEBH/graph.json","events_json":"https://pith.science/api/pith-number/AQY3ZWFWYQYFR2EPNB35QTDEBH/events.json","paper":"https://pith.science/paper/AQY3ZWFW"},"agent_actions":{"view_html":"https://pith.science/pith/AQY3ZWFWYQYFR2EPNB35QTDEBH","download_json":"https://pith.science/pith/AQY3ZWFWYQYFR2EPNB35QTDEBH.json","view_paper":"https://pith.science/paper/AQY3ZWFW","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1507.06758&json=true","fetch_graph":"https://pith.science/api/pith-number/AQY3ZWFWYQYFR2EPNB35QTDEBH/graph.json","fetch_events":"https://pith.science/api/pith-number/AQY3ZWFWYQYFR2EPNB35QTDEBH/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/AQY3ZWFWYQYFR2EPNB35QTDEBH/action/timestamp_anchor","attest_storage":"https://pith.science/pith/AQY3ZWFWYQYFR2EPNB35QTDEBH/action/storage_attestation","attest_author":"https://pith.science/pith/AQY3ZWFWYQYFR2EPNB35QTDEBH/action/author_attestation","sign_citation":"https://pith.science/pith/AQY3ZWFWYQYFR2EPNB35QTDEBH/action/citation_signature","submit_replication":"https://pith.science/pith/AQY3ZWFWYQYFR2EPNB35QTDEBH/action/replication_record"}},"created_at":"2026-05-18T01:36:22.455320+00:00","updated_at":"2026-05-18T01:36:22.455320+00:00"}