{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2016:IGFNBD724E3TFVA3SMQOPRSIAP","short_pith_number":"pith:IGFNBD72","canonical_record":{"source":{"id":"1612.07151","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.EP","submitted_at":"2016-12-21T14:48:37Z","cross_cats_sorted":["astro-ph.CO"],"title_canon_sha256":"4afc4d50e54765cbd5b1e2fe2c4dd9551b1941048995b72f10674ba8fa97a0ec","abstract_canon_sha256":"c67a8b1aa0266b48685329aff9d6533c16435e81063f9e317086d85d432916ed"},"schema_version":"1.0"},"canonical_sha256":"418ad08ffae13732d41b9320e7c64803ced8ec40fab6b088edbbae351aa21632","source":{"kind":"arxiv","id":"1612.07151","version":1},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1612.07151","created_at":"2026-05-18T00:29:31Z"},{"alias_kind":"arxiv_version","alias_value":"1612.07151v1","created_at":"2026-05-18T00:29:31Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1612.07151","created_at":"2026-05-18T00:29:31Z"},{"alias_kind":"pith_short_12","alias_value":"IGFNBD724E3T","created_at":"2026-05-18T12:30:22Z"},{"alias_kind":"pith_short_16","alias_value":"IGFNBD724E3TFVA3","created_at":"2026-05-18T12:30:22Z"},{"alias_kind":"pith_short_8","alias_value":"IGFNBD72","created_at":"2026-05-18T12:30:22Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2016:IGFNBD724E3TFVA3SMQOPRSIAP","target":"record","payload":{"canonical_record":{"source":{"id":"1612.07151","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.EP","submitted_at":"2016-12-21T14:48:37Z","cross_cats_sorted":["astro-ph.CO"],"title_canon_sha256":"4afc4d50e54765cbd5b1e2fe2c4dd9551b1941048995b72f10674ba8fa97a0ec","abstract_canon_sha256":"c67a8b1aa0266b48685329aff9d6533c16435e81063f9e317086d85d432916ed"},"schema_version":"1.0"},"canonical_sha256":"418ad08ffae13732d41b9320e7c64803ced8ec40fab6b088edbbae351aa21632","receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:29:31.151368Z","signature_b64":"1L5S0DvaleG5sE9Z/maa8+24uHFSAr1RuxsfwEazvg/N2VpR+C1W9EFV1xSXsy3ULPUPwPVYQ18Chxb1UGtBCw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"418ad08ffae13732d41b9320e7c64803ced8ec40fab6b088edbbae351aa21632","last_reissued_at":"2026-05-18T00:29:31.150624Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:29:31.150624Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"source_kind":"arxiv","source_id":"1612.07151","source_version":1,"attestation_state":"computed"},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-05-18T00:29:31Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"+Ih7tact7nIJSRoFXEByAjj5AuU+h48MAsVUxxAWNznvHttiOD/AlM0w+zs+p8/LmTnRR7x0VBw3bseFpwShCQ==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-25T20:35:56.856940Z"},"content_sha256":"d0b74a288601a2b4ecc52b719401eaa632d73bcafee699231cf02e04c00f16ee","schema_version":"1.0","event_id":"sha256:d0b74a288601a2b4ecc52b719401eaa632d73bcafee699231cf02e04c00f16ee"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2016:IGFNBD724E3TFVA3SMQOPRSIAP","target":"graph","payload":{"graph_snapshot":{"paper":{"title":"Planck intermediate results. LII. Planet flux densities","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"astro-ph.EP","authors_text":"A. A. Fraisse, A. Coulais, A. Curto, A. De Rosa, A. Ducout, A. Frolov, A. Gruppuso, A. H. Jaffe, A. J. Banday, A. Lasenby, A. Melchiorri, A. Mennella, A. Moneti, A. Renzi, A.-S. Suur-Uski, A. Zacchei, B. Comis, B. Partridge, B. P. Crill, B. Racine, B. Ruiz-Granados, C. A. Oxborrow, C. Baccigalupi, C. Burigana, C. Dickinson, C. R. Lawrence, C. Rosset, D. Herranz, D. Maino, D. Molinari, D. Paoletti, D. Scott, D. Tavagnacco, E. Calabrese, E. Di Valentino, E. Falgarone, E. Franceschi, E. Hivon, E. Keih\\\"anen, E. Lellouch, E. Mart\\'inez-Gonz\\'alez, E. Romelli, F. Boulanger, F. Couchot, F. Cuttaia, F. Elsner, F. Finelli, F. K. Hansen, F. Levrier, F. Piacentini, F. R. Bouchet, F. Van Tent, F. Villa, G. de Zotti, G. Helou, G. Lagache, G. Maggio, G. Morgante, G. Patanchon, G. Polenta, G. Rocha, G. Roudier, G. Sirri, H. C. Chiang, H. K. Eriksen, H. Kurki-Suonio, I. K. Wehus, J. A. Rubi\\~no-Mart\\'in, J. A. Tauber, J. Aumont, J. Borrill, J. Carron, J. Delabrouille, J. D. McEwen, J. E. Gudmundsson, J.-F. Cardoso, J. F. Mac\\'ias-P\\'erez, J. Gonz\\'alez-Nuevo, J. Kim, J. M. Diego, J.-M. Lamarre, J.-P. Bernard, J. P. Rachen, J. R. Bond, J. Valiviita, K. Benabed, K. Ganga, K. Kiiveri, K. M. G\\'orski, L. Bonavera, L. D. Spencer, L. Montier, L. Patrizii, L. P. L. Colombo, L. Salvati, L. Toffolatti, M.-A. Miville-Desch\\^enes, M. Ashdown, M. Ballardini, M. Bersanelli, M. Bucher, M. Frailis, M. Gerbino, M. Kunz, M. Lattanzi, M. Le Jeune, M. Liguori, M. L\\'opez-Caniego, M. Maris, M. Migliaccio, M. Reinecke, M. Remazeilles, M. Sandri, M. Savelainen, M. Tenti, M. Tomasi, M. Tristram, N. Bartolo, N. Krachmalnicoff, N. Mandolesi, N. Mauri, O. Dor\\'e, O. Perdereau, P. Bielewicz, P. B. Lilje, P. De Bernardis, P. G. Martin, Planck Collaboration: Y. Akrami, P. Natoli, P. Vielva, R. B. Barreiro, R. C. Butler, R. Keskitalo, R. Moreno, R. T. G\\'enova-Santos, S. Basak, S. Galeotta, S. Galli, S. Henrot-Versill\\'e, S. Matarrese, S. Plaszczynski, T. A. En{\\ss}lin, T. S. Kisner, T. Trombetti, V. Lindholm, W. C. Jones, X. Dupac, Y. Fantaye, Y.-Z. Ma","submitted_at":"2016-12-21T14:48:37Z","abstract_excerpt":"Measurements of flux density are described for five planets, Mars, Jupiter, Saturn, Uranus, and Neptune, across the six Planck High Frequency Instrument frequency bands (100-857 GHz) and these are then compared with models and existing data. In our analysis, we have also included estimates of the brightness of Jupiter and Saturn at the three frequencies of the Planck Low Frequency Instrument (30, 44, and 70 GHz). The results provide constraints on the intrinsic brightness and the brightness time-variability of these planets. The majority of the planet flux density estimates are limited by syst"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1612.07151","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"},"verdict_id":null},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-05-18T00:29:31Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"H9P+ugS4v7/A/lm8WaDxhr0CLviC/hXB8U1pVDH7UlH305WOru+3ngiXjiekzOBv9wrUuYWQDoNQGmIIRg+bCw==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-25T20:35:56.857623Z"},"content_sha256":"615102e3ebd63ea36d026110f4acc18fad039f73b589b29ada69f2ef381a55e4","schema_version":"1.0","event_id":"sha256:615102e3ebd63ea36d026110f4acc18fad039f73b589b29ada69f2ef381a55e4"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/IGFNBD724E3TFVA3SMQOPRSIAP/bundle.json","state_url":"https://pith.science/pith/IGFNBD724E3TFVA3SMQOPRSIAP/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/IGFNBD724E3TFVA3SMQOPRSIAP/bundle.json","status":"primary"}],"public_keys":[{"key_id":"pith-v1-2026-05","algorithm":"ed25519","format":"raw","public_key_b64":"stVStoiQhXFxp4s2pdzPNoqVNBMojDU/fJ2db5S3CbM=","public_key_hex":"b2d552b68890857171a78b36a5dccf368a953413288c353f7c9d9d6f94b709b3","fingerprint_sha256_b32_first128bits":"RVFV5Z2OI2J3ZUO7ERDEBCYNKS","fingerprint_sha256_hex":"8d4b5ee74e4693bcd1df2446408b0d54","rotates_at":null,"url":"https://pith.science/pith-signing-key.json","notes":"Pith uses this Ed25519 key to sign canonical record SHA-256 digests. Verify with: ed25519_verify(public_key, message=canonical_sha256_bytes, signature=base64decode(signature_b64))."}],"merge_version":"pith-open-graph-merge-v1","built_at":"2026-05-25T20:35:56Z","links":{"resolver":"https://pith.science/pith/IGFNBD724E3TFVA3SMQOPRSIAP","bundle":"https://pith.science/pith/IGFNBD724E3TFVA3SMQOPRSIAP/bundle.json","state":"https://pith.science/pith/IGFNBD724E3TFVA3SMQOPRSIAP/state.json","well_known_bundle":"https://pith.science/.well-known/pith/IGFNBD724E3TFVA3SMQOPRSIAP/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2016:IGFNBD724E3TFVA3SMQOPRSIAP","merge_version":"pith-open-graph-merge-v1","event_count":2,"valid_event_count":2,"invalid_event_count":0,"equivocation_count":0,"current":{"canonical_record":{"metadata":{"abstract_canon_sha256":"c67a8b1aa0266b48685329aff9d6533c16435e81063f9e317086d85d432916ed","cross_cats_sorted":["astro-ph.CO"],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.EP","submitted_at":"2016-12-21T14:48:37Z","title_canon_sha256":"4afc4d50e54765cbd5b1e2fe2c4dd9551b1941048995b72f10674ba8fa97a0ec"},"schema_version":"1.0","source":{"id":"1612.07151","kind":"arxiv","version":1}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1612.07151","created_at":"2026-05-18T00:29:31Z"},{"alias_kind":"arxiv_version","alias_value":"1612.07151v1","created_at":"2026-05-18T00:29:31Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1612.07151","created_at":"2026-05-18T00:29:31Z"},{"alias_kind":"pith_short_12","alias_value":"IGFNBD724E3T","created_at":"2026-05-18T12:30:22Z"},{"alias_kind":"pith_short_16","alias_value":"IGFNBD724E3TFVA3","created_at":"2026-05-18T12:30:22Z"},{"alias_kind":"pith_short_8","alias_value":"IGFNBD72","created_at":"2026-05-18T12:30:22Z"}],"graph_snapshots":[{"event_id":"sha256:615102e3ebd63ea36d026110f4acc18fad039f73b589b29ada69f2ef381a55e4","target":"graph","created_at":"2026-05-18T00:29:31Z","signer":{"key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signer_id":"pith.science","signer_type":"pith_registry"},"payload":{"graph_snapshot":{"author_claims":{"count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","strong_count":0},"builder_version":"pith-number-builder-2026-05-17-v1","claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"paper":{"abstract_excerpt":"Measurements of flux density are described for five planets, Mars, Jupiter, Saturn, Uranus, and Neptune, across the six Planck High Frequency Instrument frequency bands (100-857 GHz) and these are then compared with models and existing data. In our analysis, we have also included estimates of the brightness of Jupiter and Saturn at the three frequencies of the Planck Low Frequency Instrument (30, 44, and 70 GHz). The results provide constraints on the intrinsic brightness and the brightness time-variability of these planets. The majority of the planet flux density estimates are limited by syst","authors_text":"A. A. Fraisse, A. Coulais, A. Curto, A. De Rosa, A. Ducout, A. Frolov, A. Gruppuso, A. H. Jaffe, A. J. Banday, A. Lasenby, A. Melchiorri, A. Mennella, A. Moneti, A. Renzi, A.-S. Suur-Uski, A. Zacchei, B. Comis, B. Partridge, B. P. Crill, B. Racine, B. Ruiz-Granados, C. A. Oxborrow, C. Baccigalupi, C. Burigana, C. Dickinson, C. R. Lawrence, C. Rosset, D. Herranz, D. Maino, D. Molinari, D. Paoletti, D. Scott, D. Tavagnacco, E. Calabrese, E. Di Valentino, E. Falgarone, E. Franceschi, E. Hivon, E. Keih\\\"anen, E. Lellouch, E. Mart\\'inez-Gonz\\'alez, E. Romelli, F. Boulanger, F. Couchot, F. Cuttaia, F. Elsner, F. Finelli, F. K. Hansen, F. Levrier, F. Piacentini, F. R. Bouchet, F. Van Tent, F. Villa, G. de Zotti, G. Helou, G. Lagache, G. Maggio, G. Morgante, G. Patanchon, G. Polenta, G. Rocha, G. Roudier, G. Sirri, H. C. Chiang, H. K. Eriksen, H. Kurki-Suonio, I. K. Wehus, J. A. Rubi\\~no-Mart\\'in, J. A. Tauber, J. Aumont, J. Borrill, J. Carron, J. Delabrouille, J. D. McEwen, J. E. Gudmundsson, J.-F. Cardoso, J. F. Mac\\'ias-P\\'erez, J. Gonz\\'alez-Nuevo, J. Kim, J. M. Diego, J.-M. Lamarre, J.-P. Bernard, J. P. Rachen, J. R. Bond, J. Valiviita, K. Benabed, K. Ganga, K. Kiiveri, K. M. G\\'orski, L. Bonavera, L. D. Spencer, L. Montier, L. Patrizii, L. P. L. Colombo, L. Salvati, L. Toffolatti, M.-A. Miville-Desch\\^enes, M. Ashdown, M. Ballardini, M. Bersanelli, M. Bucher, M. Frailis, M. Gerbino, M. Kunz, M. Lattanzi, M. Le Jeune, M. Liguori, M. L\\'opez-Caniego, M. Maris, M. Migliaccio, M. Reinecke, M. Remazeilles, M. Sandri, M. Savelainen, M. Tenti, M. Tomasi, M. Tristram, N. Bartolo, N. Krachmalnicoff, N. Mandolesi, N. Mauri, O. Dor\\'e, O. Perdereau, P. Bielewicz, P. B. Lilje, P. De Bernardis, P. G. Martin, Planck Collaboration: Y. Akrami, P. Natoli, P. Vielva, R. B. Barreiro, R. C. Butler, R. Keskitalo, R. Moreno, R. T. G\\'enova-Santos, S. Basak, S. Galeotta, S. Galli, S. Henrot-Versill\\'e, S. Matarrese, S. Plaszczynski, T. A. En{\\ss}lin, T. S. Kisner, T. Trombetti, V. Lindholm, W. C. Jones, X. Dupac, Y. Fantaye, Y.-Z. Ma","cross_cats":["astro-ph.CO"],"headline":"","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.EP","submitted_at":"2016-12-21T14:48:37Z","title":"Planck intermediate results. LII. Planet flux densities"},"references":{"count":0,"internal_anchors":0,"resolved_work":0,"sample":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1612.07151","kind":"arxiv","version":1},"verdict":{"created_at":null,"id":null,"model_set":{},"one_line_summary":"","pipeline_version":null,"pith_extraction_headline":"","strongest_claim":"","weakest_assumption":""}},"verdict_id":null}}],"author_attestations":[],"timestamp_anchors":[],"storage_attestations":[],"citation_signatures":[],"replication_records":[],"corrections":[],"mirror_hints":[],"record_created":{"event_id":"sha256:d0b74a288601a2b4ecc52b719401eaa632d73bcafee699231cf02e04c00f16ee","target":"record","created_at":"2026-05-18T00:29:31Z","signer":{"key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signer_id":"pith.science","signer_type":"pith_registry"},"payload":{"attestation_state":"computed","canonical_record":{"metadata":{"abstract_canon_sha256":"c67a8b1aa0266b48685329aff9d6533c16435e81063f9e317086d85d432916ed","cross_cats_sorted":["astro-ph.CO"],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.EP","submitted_at":"2016-12-21T14:48:37Z","title_canon_sha256":"4afc4d50e54765cbd5b1e2fe2c4dd9551b1941048995b72f10674ba8fa97a0ec"},"schema_version":"1.0","source":{"id":"1612.07151","kind":"arxiv","version":1}},"canonical_sha256":"418ad08ffae13732d41b9320e7c64803ced8ec40fab6b088edbbae351aa21632","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"418ad08ffae13732d41b9320e7c64803ced8ec40fab6b088edbbae351aa21632","first_computed_at":"2026-05-18T00:29:31.150624Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-05-18T00:29:31.150624Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"1L5S0DvaleG5sE9Z/maa8+24uHFSAr1RuxsfwEazvg/N2VpR+C1W9EFV1xSXsy3ULPUPwPVYQ18Chxb1UGtBCw==","signature_status":"signed_v1","signed_at":"2026-05-18T00:29:31.151368Z","signed_message":"canonical_sha256_bytes"},"source_id":"1612.07151","source_kind":"arxiv","source_version":1}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:d0b74a288601a2b4ecc52b719401eaa632d73bcafee699231cf02e04c00f16ee","sha256:615102e3ebd63ea36d026110f4acc18fad039f73b589b29ada69f2ef381a55e4"],"state_sha256":"37b9b5ba5ee7b12cae60968d70644cca804ee6552ce83eb3d4dd790e21eda50f"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"i17bhmbq90y6G9iceCIEBnQUgOo7KaWma4ye7sUY5GIlRRm7U1eKmp9irqLY1tDwGAQv/2LZTKbr2KmCdZshCQ==","signed_message":"bundle_sha256_bytes","signed_at":"2026-05-25T20:35:56.861154Z","bundle_sha256":"4e6c847eee34891523dd50889cdfad5b6e68a8e5a2e2e33b895b8609820fdd2e"}}