{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2013:GJNQGKM6Z6QSSRD6M76WLPXJI6","short_pith_number":"pith:GJNQGKM6","schema_version":"1.0","canonical_sha256":"325b03299ecfa129447e67fd65bee9479d20aa0c2fb88d880dd6b9c1bcbe1e2d","source":{"kind":"arxiv","id":"1301.5839","version":2},"attestation_state":"computed","paper":{"title":"Planck intermediate results. XII: Diffuse Galactic components in the Gould Belt System","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"astro-ph.GA","authors_text":"A. Balbi, A. Beno\\^it, A. Bonaldi, A. Coulais, A. Gregorio, A. Gruppuso, A. H. Jaffe, A. Hornstrup, A. J. Banday, A. L\\\"ahteenm\\\"aki, A. Lasenby, A. Melchiorri, A. Mennella, A. Moneti, A.-S. Suur-Uski, A. Zacchei, A. Zonca, B. D. Wandelt, B. Maffei, B. Rusholme, B. Van Tent, C. A. Oxborrow, C. Baccigalupi, C. Burigana, C. Dickinson, C. Hern\\'andez-Monteagudo, C. Renault, C. R. Lawrence, C. Rosset, C. T. Tibbs, D. Harrison, D. J. Marshall, D. L. Clements, D. Maino, D. Mortlock, D. Munshi, D. Novikov, D. Paoletti, D. Pietrobon, D. Scott, D. Yvon, E. Battaner, E. Franceschi, E. Hivon, E. Keih\\\"anen, E. Mart\\'inez-Gonz\\'alez, E. Pierpaoli, E. Pointecouteau, E. Salerno, F. Atrio-Barandela, F. Boulanger, F. Cuttaia, F. Finelli, F. K. Hansen, F. Nati, F. Noviello, F. Pajot, F. Perrotta, F. Piacentini, F. R. Bouchet, F. Villa, G. De Gasperis, G. de Zotti, G. Dobler, G. Giardino, G. Lagache, G. Morgante, G. Polenta, G. Rocha, G. Savini, G. W. Pratt, H. Dole, H. Kurki-Suonio, H. U. N{\\o}rgaard-Nielsen, I. Novikov, I. Ristorcelli, J. A. Murphy, J. A. Rubi\\~no-Mart\\'in, J. A. Tauber, J. Aumont, J. Borrill, J. Delabrouille, J.-F. Cardoso, J. F. Mac\\'ias-P\\'erez, J.-F. Sygnet, J. G. Bartlett, J. Gonz\\'alez-Nuevo, J. Knoche, J.-L. Puget, J. M. Diego, J.-M. Lamarre, J.-P. Bernard, J. P. Rachen, J. R. Bond, J. Varis, K. Benabed, K. Ganga, K. M. G\\'orski, K. M. Huffenberger, L. A. Wade, L. Bedini, L. Montier, L. Perotto, L. P. L. Colombo, L. Popa, L. Spencer, L. Terenzi, L. Toffolatti, L. Valenziano, L.-Y Chiang, M.-A. Miville-Desch\\^enes, M. Arnaud, M. Ashdown, M. Bersanelli, M. Douspis, M. Frailis, M. Giard, M. Hobson, M. I. R. Alves, M. Juvela, M. Kunz, M. Linden-V{\\o}rnle, M. Maris, M. Massardi, M. Peel, M. Piat, M. Reinecke, M. Sandri, M. Tomasi, M. Tristram, N. Aghanim, N. Mandolesi, N. Vittorio, N. Ysard, O. Dor\\'e, O. Forni, P. B. Lilje, P. Cabella, P. De Bernardis, P. G. Martin, Planck Collaboration: P. A. R. Ade, P. Mazzotta, P. M. Lubin, P. Naselsky, P. Natoli, P. R. Christensen, P. Vielva, R. B. Barreiro, R. C. Butler, R. D. Davies, R. J. Davis, R. Keskitalo, R. Leonardi, R. Paladini, R. Rebolo, R. Sudiwala, R. T. G\\'enova-Santos, S. Colombi, S. Donzelli, S. Galeotta, S. Leach, S. Masi, S. Matarrese, S. Mitra, S. Osborne, S. Plaszczynski, S. Prunet, S. R. Hildebrandt, S. Ricciardi, T. A. En{\\ss}lin, T. Ghosh, T. Poutanen, T. R. Jaffe, T. S. Kisner, V. Stolyarov, W. A. Holmes, W. Hovest, W. T. Reach, X. Chen, X. Dupac, Y. Giraud-H\\'eraud","submitted_at":"2013-01-24T16:52:42Z","abstract_excerpt":"We perform an analysis of the diffuse low-frequency Galactic components in the Southern part of the Gould Belt system (130^\\circ\\leq l\\leq 230^\\circ and -50^\\circ\\leq b\\leq -10^\\circ). Strong ultra-violet (UV) flux coming from the Gould Belt super-association is responsible for bright diffuse foregrounds that we observe from our position inside the system and that can help us improve our knowledge of the Galactic emission. Free-free emission and anomalous microwave emission (AME) are the dominant components at low frequencies (\\nu < 40 GHz), while synchrotron emission is very smooth and faint."},"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":"1301.5839","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2013-01-24T16:52:42Z","cross_cats_sorted":["astro-ph.CO"],"title_canon_sha256":"38798d78efdfcdce830885da299a32e0696e8db5a56dbfdf82f3dd84220f4eab","abstract_canon_sha256":"31ba6747ae275581c11888266c21d4f8d9d6cf7ea38bfd82ecb049170ea37ca8"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:51:58.870308Z","signature_b64":"fLrS+sgAeOGA8DGxprv6mEJYH/IZ6uOOdyNIYpMdlh3k/ydHaR/STa5f30qPT/p0WNHvFZdooXggnjebU4nkDQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"325b03299ecfa129447e67fd65bee9479d20aa0c2fb88d880dd6b9c1bcbe1e2d","last_reissued_at":"2026-05-18T01:51:58.869789Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:51:58.869789Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Planck intermediate results. XII: Diffuse Galactic components in the Gould Belt System","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"astro-ph.GA","authors_text":"A. Balbi, A. Beno\\^it, A. Bonaldi, A. Coulais, A. Gregorio, A. Gruppuso, A. H. Jaffe, A. Hornstrup, A. J. Banday, A. L\\\"ahteenm\\\"aki, A. Lasenby, A. Melchiorri, A. Mennella, A. Moneti, A.-S. Suur-Uski, A. Zacchei, A. Zonca, B. D. Wandelt, B. Maffei, B. Rusholme, B. Van Tent, C. A. Oxborrow, C. Baccigalupi, C. Burigana, C. Dickinson, C. Hern\\'andez-Monteagudo, C. Renault, C. R. Lawrence, C. Rosset, C. T. Tibbs, D. Harrison, D. J. Marshall, D. L. Clements, D. Maino, D. Mortlock, D. Munshi, D. Novikov, D. Paoletti, D. Pietrobon, D. Scott, D. Yvon, E. Battaner, E. Franceschi, E. Hivon, E. Keih\\\"anen, E. Mart\\'inez-Gonz\\'alez, E. Pierpaoli, E. Pointecouteau, E. Salerno, F. Atrio-Barandela, F. Boulanger, F. Cuttaia, F. Finelli, F. K. Hansen, F. Nati, F. Noviello, F. Pajot, F. Perrotta, F. Piacentini, F. R. Bouchet, F. Villa, G. De Gasperis, G. de Zotti, G. Dobler, G. Giardino, G. Lagache, G. Morgante, G. Polenta, G. Rocha, G. Savini, G. W. Pratt, H. Dole, H. Kurki-Suonio, H. U. N{\\o}rgaard-Nielsen, I. Novikov, I. Ristorcelli, J. A. Murphy, J. A. Rubi\\~no-Mart\\'in, J. A. Tauber, J. Aumont, J. Borrill, J. Delabrouille, J.-F. Cardoso, J. F. Mac\\'ias-P\\'erez, J.-F. Sygnet, J. G. Bartlett, J. Gonz\\'alez-Nuevo, J. Knoche, J.-L. Puget, J. M. Diego, J.-M. Lamarre, J.-P. Bernard, J. P. Rachen, J. R. Bond, J. Varis, K. Benabed, K. Ganga, K. M. G\\'orski, K. M. Huffenberger, L. A. Wade, L. Bedini, L. Montier, L. Perotto, L. P. L. Colombo, L. Popa, L. Spencer, L. Terenzi, L. Toffolatti, L. Valenziano, L.-Y Chiang, M.-A. Miville-Desch\\^enes, M. Arnaud, M. Ashdown, M. Bersanelli, M. Douspis, M. Frailis, M. Giard, M. Hobson, M. I. R. Alves, M. Juvela, M. Kunz, M. Linden-V{\\o}rnle, M. Maris, M. Massardi, M. Peel, M. Piat, M. Reinecke, M. Sandri, M. Tomasi, M. Tristram, N. Aghanim, N. Mandolesi, N. Vittorio, N. Ysard, O. Dor\\'e, O. Forni, P. B. Lilje, P. Cabella, P. De Bernardis, P. G. Martin, Planck Collaboration: P. A. R. Ade, P. Mazzotta, P. M. Lubin, P. Naselsky, P. Natoli, P. R. Christensen, P. Vielva, R. B. Barreiro, R. C. Butler, R. D. Davies, R. J. Davis, R. Keskitalo, R. Leonardi, R. Paladini, R. Rebolo, R. Sudiwala, R. T. G\\'enova-Santos, S. Colombi, S. Donzelli, S. Galeotta, S. Leach, S. Masi, S. Matarrese, S. Mitra, S. Osborne, S. Plaszczynski, S. Prunet, S. R. Hildebrandt, S. Ricciardi, T. A. En{\\ss}lin, T. Ghosh, T. Poutanen, T. R. Jaffe, T. S. Kisner, V. Stolyarov, W. A. Holmes, W. Hovest, W. T. Reach, X. Chen, X. Dupac, Y. Giraud-H\\'eraud","submitted_at":"2013-01-24T16:52:42Z","abstract_excerpt":"We perform an analysis of the diffuse low-frequency Galactic components in the Southern part of the Gould Belt system (130^\\circ\\leq l\\leq 230^\\circ and -50^\\circ\\leq b\\leq -10^\\circ). Strong ultra-violet (UV) flux coming from the Gould Belt super-association is responsible for bright diffuse foregrounds that we observe from our position inside the system and that can help us improve our knowledge of the Galactic emission. Free-free emission and anomalous microwave emission (AME) are the dominant components at low frequencies (\\nu < 40 GHz), while synchrotron emission is very smooth and faint."},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1301.5839","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":""},"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":"1301.5839","created_at":"2026-05-18T01:51:58.869879+00:00"},{"alias_kind":"arxiv_version","alias_value":"1301.5839v2","created_at":"2026-05-18T01:51:58.869879+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1301.5839","created_at":"2026-05-18T01:51:58.869879+00:00"},{"alias_kind":"pith_short_12","alias_value":"GJNQGKM6Z6QS","created_at":"2026-05-18T12:27:45.050594+00:00"},{"alias_kind":"pith_short_16","alias_value":"GJNQGKM6Z6QSSRD6","created_at":"2026-05-18T12:27:45.050594+00:00"},{"alias_kind":"pith_short_8","alias_value":"GJNQGKM6","created_at":"2026-05-18T12:27:45.050594+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/GJNQGKM6Z6QSSRD6M76WLPXJI6","json":"https://pith.science/pith/GJNQGKM6Z6QSSRD6M76WLPXJI6.json","graph_json":"https://pith.science/api/pith-number/GJNQGKM6Z6QSSRD6M76WLPXJI6/graph.json","events_json":"https://pith.science/api/pith-number/GJNQGKM6Z6QSSRD6M76WLPXJI6/events.json","paper":"https://pith.science/paper/GJNQGKM6"},"agent_actions":{"view_html":"https://pith.science/pith/GJNQGKM6Z6QSSRD6M76WLPXJI6","download_json":"https://pith.science/pith/GJNQGKM6Z6QSSRD6M76WLPXJI6.json","view_paper":"https://pith.science/paper/GJNQGKM6","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1301.5839&json=true","fetch_graph":"https://pith.science/api/pith-number/GJNQGKM6Z6QSSRD6M76WLPXJI6/graph.json","fetch_events":"https://pith.science/api/pith-number/GJNQGKM6Z6QSSRD6M76WLPXJI6/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/GJNQGKM6Z6QSSRD6M76WLPXJI6/action/timestamp_anchor","attest_storage":"https://pith.science/pith/GJNQGKM6Z6QSSRD6M76WLPXJI6/action/storage_attestation","attest_author":"https://pith.science/pith/GJNQGKM6Z6QSSRD6M76WLPXJI6/action/author_attestation","sign_citation":"https://pith.science/pith/GJNQGKM6Z6QSSRD6M76WLPXJI6/action/citation_signature","submit_replication":"https://pith.science/pith/GJNQGKM6Z6QSSRD6M76WLPXJI6/action/replication_record"}},"created_at":"2026-05-18T01:51:58.869879+00:00","updated_at":"2026-05-18T01:51:58.869879+00:00"}