{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2016:66L4MVFN7Q2LROC52A7MXVVNOH","short_pith_number":"pith:66L4MVFN","schema_version":"1.0","canonical_sha256":"f797c654adfc34b8b85dd03ecbd6ad71db8949ec8237360b045e6779b478e7ef","source":{"kind":"arxiv","id":"1602.07246","version":1},"attestation_state":"computed","paper":{"title":"Development of the Model of Galactic Interstellar Emission for Standard Point-Source Analysis of Fermi Large Area Telescope Data","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"A. Albert, A. B. Hill, A. Chekhtman, A. Cuoco, A. De Angelis, A. Franckowiak, A. K. Harding, A. Manfreda, A. Morselli, A. Reimer, A. Schulz, A. W. Strong, C. Cecchi, C. Favuzzi, C. Sgr\\`o, D. Bastieri, D. F. Torres, D. Gasparrini, D. Hadasch, D. Horan, D. J. Suson, D. J. Thompson, D. Landriu, D. Malyshev, D. Paneque, E. Bissaldi, E. Bottacini, E. Cavazzuti, E. C. Ferrara, E. Charles, E. D. Bloom, E. Hays, E. J. Siskind, E. Nuss, E. Orlando, E. Troja, F. Acero, F. D'Ammando, F. de Palma, F. Gargano, F. Giordano, F. Longo, F. Loparco, F. Piron, F. Spada, G. A. Caliandro, G. Barbiellini, G. Chiaro, G. Godfrey, G. J\\'ohannesson, G. Pivato, G. Spandre, G. Tosti, G. Vianello, G. Zaharijas, H. Tajima, H. Takahashi, I. A. Grenier, J. Ballet, J. Bregeon, J. B. Thayer, J. Chiang, J. Cohen-Tanugi, J. Conrad, J. E. McEnery, J. F. Ormes, J. Li, J. M. Casandjian, J.W. Hewitt, K. Hayashi, K. S. Wood, L. Baldini, L. Di Venere, L. Latronico, L. Li, L. Tibaldo, M. Ackermann, M. Ajello, M. Caragiulo, M. E. Monzani, M. Giroletti, M. Kuss, M. Mayer, M. N. Lovellette, M. N. Mazziotta, M. Orienti, M. Pesce-Rollins, M. Razzano, M. S\\'anchez-Conde, M. Schaal, M. Tinivella, M. Werner, M. Wood, N. Giglietto, N. Mirabal, N. Omodei, N. Renault, O. Reimer, P. A. Caraveo, P. Bruel, P. F. Michelson, P. Fusco, P. Lubrano, P. Martin, P. S. Drell, P. Spinelli, Q. Remy, R. A. Cameron, R. Bellazzini, R. Bonino, R. Buehler, R. Claus, R. Desiante, R. Rando, S. Buson, S. Ciprini, S. Cutini, S. Funk, S. Guiriec, S. J. Fegan, S. Larsson, S. Maldera, S. Rain\\`o, S. Razzaque, S. W. Digel, S. Zimmer, T. Glanzman, T. J. Brandt, T. Jogler, T. Kamae, T. Mizuno, T. Ohsugi, W. B. Focke, X. Hou","submitted_at":"2016-02-23T17:48:00Z","abstract_excerpt":"Most of the celestial gamma rays detected by the Large Area Telescope (LAT) aboard the Fermi Gamma-ray Space Telescope originate from the interstellar medium when energetic cosmic rays interact with interstellar nucleons and photons. Conventional point and extended source studies rely on the modeling of this diffuse emission for accurate characterization. We describe here the development of the Galactic Interstellar Emission Model (GIEM) that is the standard adopted by the LAT Collaboration and is publicly available. The model is based on a linear combination of maps for interstellar gas colum"},"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":"1602.07246","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2016-02-23T17:48:00Z","cross_cats_sorted":[],"title_canon_sha256":"3dd4271342d61d4b4fabdc6138fe8a2a2b0066c1533a90206d329fc95d6922cc","abstract_canon_sha256":"1afdae84fa09fc02354428fa28394424f4120fa30de27433cc2e863f0e102920"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:16:20.011952Z","signature_b64":"7SKhBNw9RiXV5PpSPONnVDRCVrf0fco6oOEyb5pTvSAfYMHv1sTzbqvY4v7xPbPfBSMi2VTaieiL7vEIKRMGAA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"f797c654adfc34b8b85dd03ecbd6ad71db8949ec8237360b045e6779b478e7ef","last_reissued_at":"2026-05-18T01:16:20.008491Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:16:20.008491Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Development of the Model of Galactic Interstellar Emission for Standard Point-Source Analysis of Fermi Large Area Telescope Data","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"A. Albert, A. B. Hill, A. Chekhtman, A. Cuoco, A. De Angelis, A. Franckowiak, A. K. Harding, A. Manfreda, A. Morselli, A. Reimer, A. Schulz, A. W. Strong, C. Cecchi, C. Favuzzi, C. Sgr\\`o, D. Bastieri, D. F. Torres, D. Gasparrini, D. Hadasch, D. Horan, D. J. Suson, D. J. Thompson, D. Landriu, D. Malyshev, D. Paneque, E. Bissaldi, E. Bottacini, E. Cavazzuti, E. C. Ferrara, E. Charles, E. D. Bloom, E. Hays, E. J. Siskind, E. Nuss, E. Orlando, E. Troja, F. Acero, F. D'Ammando, F. de Palma, F. Gargano, F. Giordano, F. Longo, F. Loparco, F. Piron, F. Spada, G. A. Caliandro, G. Barbiellini, G. Chiaro, G. Godfrey, G. J\\'ohannesson, G. Pivato, G. Spandre, G. Tosti, G. Vianello, G. Zaharijas, H. Tajima, H. Takahashi, I. A. Grenier, J. Ballet, J. Bregeon, J. B. Thayer, J. Chiang, J. Cohen-Tanugi, J. Conrad, J. E. McEnery, J. F. Ormes, J. Li, J. M. Casandjian, J.W. Hewitt, K. Hayashi, K. S. Wood, L. Baldini, L. Di Venere, L. Latronico, L. Li, L. Tibaldo, M. Ackermann, M. Ajello, M. Caragiulo, M. E. Monzani, M. Giroletti, M. Kuss, M. Mayer, M. N. Lovellette, M. N. Mazziotta, M. Orienti, M. Pesce-Rollins, M. Razzano, M. S\\'anchez-Conde, M. Schaal, M. Tinivella, M. Werner, M. Wood, N. Giglietto, N. Mirabal, N. Omodei, N. Renault, O. Reimer, P. A. Caraveo, P. Bruel, P. F. Michelson, P. Fusco, P. Lubrano, P. Martin, P. S. Drell, P. Spinelli, Q. Remy, R. A. Cameron, R. Bellazzini, R. Bonino, R. Buehler, R. Claus, R. Desiante, R. Rando, S. Buson, S. Ciprini, S. Cutini, S. Funk, S. Guiriec, S. J. Fegan, S. Larsson, S. Maldera, S. Rain\\`o, S. Razzaque, S. W. Digel, S. Zimmer, T. Glanzman, T. J. Brandt, T. Jogler, T. Kamae, T. Mizuno, T. Ohsugi, W. B. Focke, X. Hou","submitted_at":"2016-02-23T17:48:00Z","abstract_excerpt":"Most of the celestial gamma rays detected by the Large Area Telescope (LAT) aboard the Fermi Gamma-ray Space Telescope originate from the interstellar medium when energetic cosmic rays interact with interstellar nucleons and photons. Conventional point and extended source studies rely on the modeling of this diffuse emission for accurate characterization. We describe here the development of the Galactic Interstellar Emission Model (GIEM) that is the standard adopted by the LAT Collaboration and is publicly available. The model is based on a linear combination of maps for interstellar gas colum"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1602.07246","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":"1602.07246","created_at":"2026-05-18T01:16:20.011335+00:00"},{"alias_kind":"arxiv_version","alias_value":"1602.07246v1","created_at":"2026-05-18T01:16:20.011335+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1602.07246","created_at":"2026-05-18T01:16:20.011335+00:00"},{"alias_kind":"pith_short_12","alias_value":"66L4MVFN7Q2L","created_at":"2026-05-18T12:30:01.593930+00:00"},{"alias_kind":"pith_short_16","alias_value":"66L4MVFN7Q2LROC5","created_at":"2026-05-18T12:30:01.593930+00:00"},{"alias_kind":"pith_short_8","alias_value":"66L4MVFN","created_at":"2026-05-18T12:30:01.593930+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":4,"internal_anchor_count":4,"sample":[{"citing_arxiv_id":"2605.23489","citing_title":"A comparison between Galactic magnetic field models and polarized synchrotron emission with C-BASS at 4.76 GHz and S-PASS at 2.3 GHz","ref_index":9,"is_internal_anchor":true},{"citing_arxiv_id":"1907.07737","citing_title":"The Southern Wide-Field Gamma-Ray Observatory (SWGO): A Next-Generation Ground-Based Survey Instrument for VHE Gamma-Ray Astronomy","ref_index":51,"is_internal_anchor":true},{"citing_arxiv_id":"2404.15944","citing_title":"IceCube Results and Perspective for Neutrinos from LHAASO Sources","ref_index":84,"is_internal_anchor":true},{"citing_arxiv_id":"2605.15986","citing_title":"Temporal evolution of the periodic GeV signal from 4FGL J1913.2+0512 and analysis of the SS 433 / W50 lobes","ref_index":64,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/66L4MVFN7Q2LROC52A7MXVVNOH","json":"https://pith.science/pith/66L4MVFN7Q2LROC52A7MXVVNOH.json","graph_json":"https://pith.science/api/pith-number/66L4MVFN7Q2LROC52A7MXVVNOH/graph.json","events_json":"https://pith.science/api/pith-number/66L4MVFN7Q2LROC52A7MXVVNOH/events.json","paper":"https://pith.science/paper/66L4MVFN"},"agent_actions":{"view_html":"https://pith.science/pith/66L4MVFN7Q2LROC52A7MXVVNOH","download_json":"https://pith.science/pith/66L4MVFN7Q2LROC52A7MXVVNOH.json","view_paper":"https://pith.science/paper/66L4MVFN","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1602.07246&json=true","fetch_graph":"https://pith.science/api/pith-number/66L4MVFN7Q2LROC52A7MXVVNOH/graph.json","fetch_events":"https://pith.science/api/pith-number/66L4MVFN7Q2LROC52A7MXVVNOH/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/66L4MVFN7Q2LROC52A7MXVVNOH/action/timestamp_anchor","attest_storage":"https://pith.science/pith/66L4MVFN7Q2LROC52A7MXVVNOH/action/storage_attestation","attest_author":"https://pith.science/pith/66L4MVFN7Q2LROC52A7MXVVNOH/action/author_attestation","sign_citation":"https://pith.science/pith/66L4MVFN7Q2LROC52A7MXVVNOH/action/citation_signature","submit_replication":"https://pith.science/pith/66L4MVFN7Q2LROC52A7MXVVNOH/action/replication_record"}},"created_at":"2026-05-18T01:16:20.011335+00:00","updated_at":"2026-05-18T01:16:20.011335+00:00"}