{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2011:N22M52OD7ZU6NBQRZ3MEMSIKG5","short_pith_number":"pith:N22M52OD","schema_version":"1.0","canonical_sha256":"6eb4cee9c3fe69e68611ced846490a37680fdae8600931aaf8a234cab5337b1d","source":{"kind":"arxiv","id":"1112.5595","version":3},"attestation_state":"computed","paper":{"title":"Planck Intermediate Results. I. Further validation of new Planck clusters with XMM-Newton","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"A. Balbi, A. Bonaldi, A. Catalano, A. Chamballu, A. Coulais, A. Da Silva, A. Gregorio, A. Gruppuso, A. Hempel, A. Hornstrup, A. J. Banday, A. L\\\"ahteenm\\\"aki, A. Lasenby, A. Liddle, A. Melchiorri, A. Mennella, A. Moneti, A. Zacchei, A. Zonca, B. D. Wandelt, B. M. Schaefer, B. P. Crill, B. Rusholme, B. Van Tent, C. Baccigalupi, C. Burigana, C. Hern\\'andez-Monteagudo, C. Renault, C. R. Lawrence, C. Rosset, D. Harrison, D. Herranz, D. J. Marshall, D. L. Clements, D. Maino, D. Mortlock, D. Munshi, D. Scott, D. Sutton, D. Yvon, E. Battaner, E. Keih\\\"anen, E. Mart\\'inez-Gonz\\'alez, E. Pierpaoli, E. Pointecouteau, F. Atrio-Barandela, F. Cuttaia, F. Finelli, F. K. Hansen, F. Marleau, F. Matthai, F. Noviello, F. Pasian, F. Perrotta, F. Piacentini, F. R. Bouchet, F. Stivoli, F. Villa, F.-X. D\\'esert, G. Chon, G. De Gasperis, G. de Zotti, G. F. Smoot, G. Hurier, G. Lagache, G. Luzzi, G. Morgante, G. Patanchon, G. Polenta, G. Rocha, G. Savini, G. W. Pratt, H. B\\\"ohringer, H. Bourdin, H. Dahle, H. Dole, H. K. Eriksen, H. Kurki-Suonio, H. U. N{\\o}rgaard-Nielsen, I. Flores-Cacho, I. Ristorcelli, J. A. Rubi\\~no-Mart\\'in, J. A. Tauber, J. Aumont, J.-B. Melin, J. Borrill, J. Delabrouille, J. D\\'emocl\\`es, J.-F. Cardoso, J. F. Mac\\'ias-P\\'erez, J.-F. Sygnet, J. G. Bartlett, J. Gonz\\'alez-Nuevo, J. Jasche, J. Knoche, J.-L. Puget, J.-L. Starck, J. M. Diego, J.-M. Lamarre, J.-P. Bernard, J. P. Rachen, J. R. Bond, J. Weller, K. Benabed, K. Dolag, K. Ganga, K. M. G\\'orski, K. M. Huffenberger, L. Cay\\'on, L. Knox, L. Mendes, L. Montier, L. Popa, 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. Juvela, M. L. Brown, M. L\\'opez-Caniego, M. Massardi, M. Reinecke, M. Remazeilles, M. Rossetti, M. Sandri, M. Tomasi, M. Tristram, N. Mandolesi, N. Ponthieu, N. Vittorio, O. Dor\\'e, O. Forni, O. Perdereau, P. B. Lilje, P. Cabella, P. Carvalho, P. De Bernardis, P. Fosalba, P. Mazzotta, P. Naselsky, P. Natoli, P. Platania, P. R. Christensen, P. R. Meinhold, P. Vielva, R. B. Barreiro, R. C. Butler, R. Gonz\\'alez-Riestra, R. J. Davis, R. Keskitalo, R. Kneissl, R. Leonardi, R. Mann, R.-R. Chary, R. Rebolo, R. Sunyaev, R. T. G\\'enova-Santos, S. Colafrancesco, S. Colombi, S. D. M. White, S. Donzelli, S. Fromenteau, S. Galeotta, S. Leach, S. Masi, S. Matarrese, S. Osborne, S. Plaszczynski, S. R. Hildebrandt, S. Ricciardi, T. A. En{\\ss}lin, The Planck Collaboration: N. Aghanim, T. Jagemann, T. Poutanen, T. Riller, T. S. Kisner, X. Dupac","submitted_at":"2011-12-23T14:36:37Z","abstract_excerpt":"We present further results from the ongoing XMM-Newton validation follow-up of Planck cluster candidates, detailing X-ray observations of eleven candidates detected at a signal-to-noise ratio of 4.5<S/N<5.3 in the same 10-month survey maps used in the construction of the Early SZ sample. The sample was selected in order to test internal SZ quality flags, and the pertinence of these flags is discussed in light of the validation results. Ten of the candidates are found to be bona fide clusters lying below the RASS flux limit. Redshift estimates are available for all confirmed systems via X-ray F"},"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":"1112.5595","kind":"arxiv","version":3},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2011-12-23T14:36:37Z","cross_cats_sorted":[],"title_canon_sha256":"ff82be75ef0f65c7709c1b151cfe8ea88ec8dc3853f5420873824a20241b9ec1","abstract_canon_sha256":"767e8856ed32617b8dc8d7fdcd3734c21298ca2842561099e88c21db1c4d4e8f"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:09:21.854306Z","signature_b64":"FJf9VZF8vSxvEAPiU8wgqrI2RHTbeZ15nVrK/f9C/LoSTliS+/+wHMzlJcGqFpgkSDSZlsG6Y46JpUOMHTPqAg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"6eb4cee9c3fe69e68611ced846490a37680fdae8600931aaf8a234cab5337b1d","last_reissued_at":"2026-05-18T01:09:21.853911Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:09:21.853911Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Planck Intermediate Results. I. Further validation of new Planck clusters with XMM-Newton","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"A. Balbi, A. Bonaldi, A. Catalano, A. Chamballu, A. Coulais, A. Da Silva, A. Gregorio, A. Gruppuso, A. Hempel, A. Hornstrup, A. J. Banday, A. L\\\"ahteenm\\\"aki, A. Lasenby, A. Liddle, A. Melchiorri, A. Mennella, A. Moneti, A. Zacchei, A. Zonca, B. D. Wandelt, B. M. Schaefer, B. P. Crill, B. Rusholme, B. Van Tent, C. Baccigalupi, C. Burigana, C. Hern\\'andez-Monteagudo, C. Renault, C. R. Lawrence, C. Rosset, D. Harrison, D. Herranz, D. J. Marshall, D. L. Clements, D. Maino, D. Mortlock, D. Munshi, D. Scott, D. Sutton, D. Yvon, E. Battaner, E. Keih\\\"anen, E. Mart\\'inez-Gonz\\'alez, E. Pierpaoli, E. Pointecouteau, F. Atrio-Barandela, F. Cuttaia, F. Finelli, F. K. Hansen, F. Marleau, F. Matthai, F. Noviello, F. Pasian, F. Perrotta, F. Piacentini, F. R. Bouchet, F. Stivoli, F. Villa, F.-X. D\\'esert, G. Chon, G. De Gasperis, G. de Zotti, G. F. Smoot, G. Hurier, G. Lagache, G. Luzzi, G. Morgante, G. Patanchon, G. Polenta, G. Rocha, G. Savini, G. W. Pratt, H. B\\\"ohringer, H. Bourdin, H. Dahle, H. Dole, H. K. Eriksen, H. Kurki-Suonio, H. U. N{\\o}rgaard-Nielsen, I. Flores-Cacho, I. Ristorcelli, J. A. Rubi\\~no-Mart\\'in, J. A. Tauber, J. Aumont, J.-B. Melin, J. Borrill, J. Delabrouille, J. D\\'emocl\\`es, J.-F. Cardoso, J. F. Mac\\'ias-P\\'erez, J.-F. Sygnet, J. G. Bartlett, J. Gonz\\'alez-Nuevo, J. Jasche, J. Knoche, J.-L. Puget, J.-L. Starck, J. M. Diego, J.-M. Lamarre, J.-P. Bernard, J. P. Rachen, J. R. Bond, J. Weller, K. Benabed, K. Dolag, K. Ganga, K. M. G\\'orski, K. M. Huffenberger, L. Cay\\'on, L. Knox, L. Mendes, L. Montier, L. Popa, 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. Juvela, M. L. Brown, M. L\\'opez-Caniego, M. Massardi, M. Reinecke, M. Remazeilles, M. Rossetti, M. Sandri, M. Tomasi, M. Tristram, N. Mandolesi, N. Ponthieu, N. Vittorio, O. Dor\\'e, O. Forni, O. Perdereau, P. B. Lilje, P. Cabella, P. Carvalho, P. De Bernardis, P. Fosalba, P. Mazzotta, P. Naselsky, P. Natoli, P. Platania, P. R. Christensen, P. R. Meinhold, P. Vielva, R. B. Barreiro, R. C. Butler, R. Gonz\\'alez-Riestra, R. J. Davis, R. Keskitalo, R. Kneissl, R. Leonardi, R. Mann, R.-R. Chary, R. Rebolo, R. Sunyaev, R. T. G\\'enova-Santos, S. Colafrancesco, S. Colombi, S. D. M. White, S. Donzelli, S. Fromenteau, S. Galeotta, S. Leach, S. Masi, S. Matarrese, S. Osborne, S. Plaszczynski, S. R. Hildebrandt, S. Ricciardi, T. A. En{\\ss}lin, The Planck Collaboration: N. Aghanim, T. Jagemann, T. Poutanen, T. Riller, T. S. Kisner, X. Dupac","submitted_at":"2011-12-23T14:36:37Z","abstract_excerpt":"We present further results from the ongoing XMM-Newton validation follow-up of Planck cluster candidates, detailing X-ray observations of eleven candidates detected at a signal-to-noise ratio of 4.5<S/N<5.3 in the same 10-month survey maps used in the construction of the Early SZ sample. The sample was selected in order to test internal SZ quality flags, and the pertinence of these flags is discussed in light of the validation results. Ten of the candidates are found to be bona fide clusters lying below the RASS flux limit. Redshift estimates are available for all confirmed systems via X-ray F"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1112.5595","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":"1112.5595","created_at":"2026-05-18T01:09:21.853978+00:00"},{"alias_kind":"arxiv_version","alias_value":"1112.5595v3","created_at":"2026-05-18T01:09:21.853978+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1112.5595","created_at":"2026-05-18T01:09:21.853978+00:00"},{"alias_kind":"pith_short_12","alias_value":"N22M52OD7ZU6","created_at":"2026-05-18T12:26:37.096874+00:00"},{"alias_kind":"pith_short_16","alias_value":"N22M52OD7ZU6NBQR","created_at":"2026-05-18T12:26:37.096874+00:00"},{"alias_kind":"pith_short_8","alias_value":"N22M52OD","created_at":"2026-05-18T12:26:37.096874+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/N22M52OD7ZU6NBQRZ3MEMSIKG5","json":"https://pith.science/pith/N22M52OD7ZU6NBQRZ3MEMSIKG5.json","graph_json":"https://pith.science/api/pith-number/N22M52OD7ZU6NBQRZ3MEMSIKG5/graph.json","events_json":"https://pith.science/api/pith-number/N22M52OD7ZU6NBQRZ3MEMSIKG5/events.json","paper":"https://pith.science/paper/N22M52OD"},"agent_actions":{"view_html":"https://pith.science/pith/N22M52OD7ZU6NBQRZ3MEMSIKG5","download_json":"https://pith.science/pith/N22M52OD7ZU6NBQRZ3MEMSIKG5.json","view_paper":"https://pith.science/paper/N22M52OD","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1112.5595&json=true","fetch_graph":"https://pith.science/api/pith-number/N22M52OD7ZU6NBQRZ3MEMSIKG5/graph.json","fetch_events":"https://pith.science/api/pith-number/N22M52OD7ZU6NBQRZ3MEMSIKG5/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/N22M52OD7ZU6NBQRZ3MEMSIKG5/action/timestamp_anchor","attest_storage":"https://pith.science/pith/N22M52OD7ZU6NBQRZ3MEMSIKG5/action/storage_attestation","attest_author":"https://pith.science/pith/N22M52OD7ZU6NBQRZ3MEMSIKG5/action/author_attestation","sign_citation":"https://pith.science/pith/N22M52OD7ZU6NBQRZ3MEMSIKG5/action/citation_signature","submit_replication":"https://pith.science/pith/N22M52OD7ZU6NBQRZ3MEMSIKG5/action/replication_record"}},"created_at":"2026-05-18T01:09:21.853978+00:00","updated_at":"2026-05-18T01:09:21.853978+00:00"}