{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2017:KEXT2DRO7OGI7MHYRTRXNPXHAI","short_pith_number":"pith:KEXT2DRO","schema_version":"1.0","canonical_sha256":"512f3d0e2efb8c8fb0f88ce376bee70228faaadcd0604d0df501cdc0790697d4","source":{"kind":"arxiv","id":"1708.01360","version":2},"attestation_state":"computed","paper":{"title":"A Measurement of CMB Cluster Lensing with SPT and DES Year 1 Data","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"A. A. Plazas, A. Benoit-L\\'evy, A. Carnero Rosell, A. Drlica-Wagner, A. Fausti Neto, A. K. Romer, A. Manzotti, A. Roodman, A. R. Walker, A. Stark, A. T. Crites, A. T. Lee, B. A. Benson, B. Flaugher, B. Jain, B. Nord, C. B. D'Andrea, C. Davis, C. E. Cunha, C. J. Miller, C. L. Chang, C. L. Reichardt, C. Pryke, D. Gruen, D. J. James, D. L. Burke, D. Luong-Van, D. P. Marrone, D. Rapetti, D. Thomas, E. Bertin, E. Buckley-Geer, E. Gaztanaga, E. J. Baxter, E. Krause, E. M. George, E. M. Leitch, E. Rozo, E. Rykoff, E. Sanchez, E. Shirokoff, E. Suchyta, F. Menanteau, F. Z. Staniszewski, G. Gutierrez, G. P. Holder, G. Tarle, H-M. Cho, I. Sevilla-Noarbe, J. Annis, J. Carlstrom, J. Carretero, J. D. Hrubes, J. D. Vieira, J. E. Ruhl, J. Estrada, J. Frieman, J. Garc\\'ia-Bellido, J. Gschwend, J. J. McMahon, J. J. Mohr, J. L. Marshall, J. P. Dietrich, J. T. Sayre, J. Zuntz, K. Aylor, K. Honscheid, K. K. Schaffer, K. Kuehn, K. Story, K. Vanderlinde, L. Bleem, L. Knox, L. M. Mocanu, L. N. da Costa, M. A. Dobbs, M. A. Troxel, M. Carrasco Kind, M. Crocce, M. Jarvis, M. Lima, M. March, M. Sako, M. Schubnell, M. Smith, M. Soares-Santos, N. Kuropatkin, N. L. Harrington, N. W. Halverson, O. Lahav, P. Doel, P. Fosalba, P. Martini, P. Melchior, R. A. Gruendl, R. C. Smith, R. L. C. Ogando, R. Miquel, R. Schindler, R. Williamson, S. Desai, S. Dodelson, S. Kuhlmann, S. Padin, S. Patil, S. Raghunathan, S. S. Meyer, T. de Haan, T. Giannantonio, T. Jeltema, T. M. C. Abbott, T. M. Crawford, T. Natoli, T. S. Li, V. Scarpine, W. B. Everett, W. G. Hartley, W. L. Holzapfel, Y. Omori, Y. Zhang, Z. Hou","submitted_at":"2017-08-04T02:58:51Z","abstract_excerpt":"Clusters of galaxies gravitationally lens the cosmic microwave background (CMB) radiation, resulting in a distinct imprint in the CMB on arcminute scales. Measurement of this effect offers a promising way to constrain the masses of galaxy clusters, particularly those at high redshift. We use CMB maps from the South Pole Telescope Sunyaev-Zel'dovich (SZ) survey to measure the CMB lensing signal around galaxy clusters identified in optical imaging from first year observations of the Dark Energy Survey. The cluster catalog used in this analysis contains 3697 members with mean redshift of $\\bar{z}"},"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":"1708.01360","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2017-08-04T02:58:51Z","cross_cats_sorted":[],"title_canon_sha256":"736686977f319d4b0698fbddd10cee79a2698f1645b1ee80f1b9abab4020c752","abstract_canon_sha256":"7f987a93bf7f971eb5e503212a564a995a58135478114047e7bc6c89107781b3"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:22:28.720409Z","signature_b64":"TeCx7HfA1V1GAQyN+u1hKzwI1YLN3pO95LwCKIP2HoQwdQ+GbwO0Ei6pxaziKs+aU6IZOwbTpsQVXIPB+e4vBQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"512f3d0e2efb8c8fb0f88ce376bee70228faaadcd0604d0df501cdc0790697d4","last_reissued_at":"2026-05-18T00:22:28.719686Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:22:28.719686Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"A Measurement of CMB Cluster Lensing with SPT and DES Year 1 Data","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"A. A. Plazas, A. Benoit-L\\'evy, A. Carnero Rosell, A. Drlica-Wagner, A. Fausti Neto, A. K. Romer, A. Manzotti, A. Roodman, A. R. Walker, A. Stark, A. T. Crites, A. T. Lee, B. A. Benson, B. Flaugher, B. Jain, B. Nord, C. B. D'Andrea, C. Davis, C. E. Cunha, C. J. Miller, C. L. Chang, C. L. Reichardt, C. Pryke, D. Gruen, D. J. James, D. L. Burke, D. Luong-Van, D. P. Marrone, D. Rapetti, D. Thomas, E. Bertin, E. Buckley-Geer, E. Gaztanaga, E. J. Baxter, E. Krause, E. M. George, E. M. Leitch, E. Rozo, E. Rykoff, E. Sanchez, E. Shirokoff, E. Suchyta, F. Menanteau, F. Z. Staniszewski, G. Gutierrez, G. P. Holder, G. Tarle, H-M. Cho, I. Sevilla-Noarbe, J. Annis, J. Carlstrom, J. Carretero, J. D. Hrubes, J. D. Vieira, J. E. Ruhl, J. Estrada, J. Frieman, J. Garc\\'ia-Bellido, J. Gschwend, J. J. McMahon, J. J. Mohr, J. L. Marshall, J. P. Dietrich, J. T. Sayre, J. Zuntz, K. Aylor, K. Honscheid, K. K. Schaffer, K. Kuehn, K. Story, K. Vanderlinde, L. Bleem, L. Knox, L. M. Mocanu, L. N. da Costa, M. A. Dobbs, M. A. Troxel, M. Carrasco Kind, M. Crocce, M. Jarvis, M. Lima, M. March, M. Sako, M. Schubnell, M. Smith, M. Soares-Santos, N. Kuropatkin, N. L. Harrington, N. W. Halverson, O. Lahav, P. Doel, P. Fosalba, P. Martini, P. Melchior, R. A. Gruendl, R. C. Smith, R. L. C. Ogando, R. Miquel, R. Schindler, R. Williamson, S. Desai, S. Dodelson, S. Kuhlmann, S. Padin, S. Patil, S. Raghunathan, S. S. Meyer, T. de Haan, T. Giannantonio, T. Jeltema, T. M. C. Abbott, T. M. Crawford, T. Natoli, T. S. Li, V. Scarpine, W. B. Everett, W. G. Hartley, W. L. Holzapfel, Y. Omori, Y. Zhang, Z. Hou","submitted_at":"2017-08-04T02:58:51Z","abstract_excerpt":"Clusters of galaxies gravitationally lens the cosmic microwave background (CMB) radiation, resulting in a distinct imprint in the CMB on arcminute scales. Measurement of this effect offers a promising way to constrain the masses of galaxy clusters, particularly those at high redshift. We use CMB maps from the South Pole Telescope Sunyaev-Zel'dovich (SZ) survey to measure the CMB lensing signal around galaxy clusters identified in optical imaging from first year observations of the Dark Energy Survey. The cluster catalog used in this analysis contains 3697 members with mean redshift of $\\bar{z}"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1708.01360","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":"1708.01360","created_at":"2026-05-18T00:22:28.719797+00:00"},{"alias_kind":"arxiv_version","alias_value":"1708.01360v2","created_at":"2026-05-18T00:22:28.719797+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1708.01360","created_at":"2026-05-18T00:22:28.719797+00:00"},{"alias_kind":"pith_short_12","alias_value":"KEXT2DRO7OGI","created_at":"2026-05-18T12:31:24.725408+00:00"},{"alias_kind":"pith_short_16","alias_value":"KEXT2DRO7OGI7MHY","created_at":"2026-05-18T12:31:24.725408+00:00"},{"alias_kind":"pith_short_8","alias_value":"KEXT2DRO","created_at":"2026-05-18T12:31:24.725408+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/KEXT2DRO7OGI7MHYRTRXNPXHAI","json":"https://pith.science/pith/KEXT2DRO7OGI7MHYRTRXNPXHAI.json","graph_json":"https://pith.science/api/pith-number/KEXT2DRO7OGI7MHYRTRXNPXHAI/graph.json","events_json":"https://pith.science/api/pith-number/KEXT2DRO7OGI7MHYRTRXNPXHAI/events.json","paper":"https://pith.science/paper/KEXT2DRO"},"agent_actions":{"view_html":"https://pith.science/pith/KEXT2DRO7OGI7MHYRTRXNPXHAI","download_json":"https://pith.science/pith/KEXT2DRO7OGI7MHYRTRXNPXHAI.json","view_paper":"https://pith.science/paper/KEXT2DRO","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1708.01360&json=true","fetch_graph":"https://pith.science/api/pith-number/KEXT2DRO7OGI7MHYRTRXNPXHAI/graph.json","fetch_events":"https://pith.science/api/pith-number/KEXT2DRO7OGI7MHYRTRXNPXHAI/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/KEXT2DRO7OGI7MHYRTRXNPXHAI/action/timestamp_anchor","attest_storage":"https://pith.science/pith/KEXT2DRO7OGI7MHYRTRXNPXHAI/action/storage_attestation","attest_author":"https://pith.science/pith/KEXT2DRO7OGI7MHYRTRXNPXHAI/action/author_attestation","sign_citation":"https://pith.science/pith/KEXT2DRO7OGI7MHYRTRXNPXHAI/action/citation_signature","submit_replication":"https://pith.science/pith/KEXT2DRO7OGI7MHYRTRXNPXHAI/action/replication_record"}},"created_at":"2026-05-18T00:22:28.719797+00:00","updated_at":"2026-05-18T00:22:28.719797+00:00"}