{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2016:DNXMGM33X4XU4E3JNUXGM32RAM","short_pith_number":"pith:DNXMGM33","schema_version":"1.0","canonical_sha256":"1b6ec3337bbf2f4e13696d2e666f51032dfac9a94e23a8f34a69c571c15b3bdf","source":{"kind":"arxiv","id":"1611.10326","version":2},"attestation_state":"computed","paper":{"title":"Weak lensing magnification in the Dark Energy Survey Science Verification 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. E. Evrard, A. K. Romer, A. Roodman, A. R. Walker, B. Flaugher, B. Hoyle, C. B. D'Andrea, C. E. Cunha, D. Brooks, D. Gruen, D. J. James, D. Kirk, D. L. Burke, D. L. DePoy, D. Thomas, D. W. Gerdes, E. Bertin, E. Buckley-Geer, E. Fernandez, E. Gaztanaga, E. Krause, E. M. Huff, E. S\\'anchez, E. S. Rykoff, E. Suchyta, F. B. Abdalla, F. J. Castander, F. Sobreira, G. Gutierrez, G. M. Bernstein, G. Tarle, H. T. Diehl, I. Sevilla-Noarbe, J. Aleksi\\'c, J. Annis, J. Carretero, J. Frieman, J. Garc\\'ia-Bellido, J. Gschwend, J. J. Mohr, J. L. Marshall, K. Kuehn, L. N. da Costa, M. A. G. Maia, M. Carrasco Kind, M. Crocce, M. Garcia-Fernandez, M. Jarvis, M. Lima, M. March, M. Schubnell, M. Soares-Santos, N. Kuropatkin, N. MacCrann, O. Lahav, P. Fosalba, P. Melchior, R. A. Gruendl, R. C. Smith, R. Miquel, R. Ponce, S. Allam, S. Desai, T. F. Eifler, T. Giannantonio, T. M. C. Abbott, V. Scarpine, W. Wester","submitted_at":"2016-11-30T19:34:56Z","abstract_excerpt":"In this paper the effect of weak lensing magnification on galaxy number counts is studied by cross-correlating the positions of two galaxy samples, separated by redshift, using data from the Dark Energy Survey Science Verification dataset. The analysis is carried out for two photometrically-selected galaxy samples, with mean photometric redshifts in the $0.2 < z < 0.4$ and $0.7 < z < 1.0$ ranges, in the riz bands. A signal is detected with a $3.5\\sigma$ significance level in each of the bands tested, and is compatible with the magnification predicted by the $\\Lambda$CDM model. After an extensi"},"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":"1611.10326","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2016-11-30T19:34:56Z","cross_cats_sorted":[],"title_canon_sha256":"95bdce4933303bdc134ddf42b8bae9a4e76aeccbb3e46ab47d4a65563422aef2","abstract_canon_sha256":"62cc78422747b182da845881055d5a2ddf3c0682f7b1c3e1f0901aa8c226e8bc"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:24:35.487972Z","signature_b64":"45pFLcYq8ShLxM22BM7Owl9ZlPXgRQJWB866fF0wx/70S6e2rRjuIAP/qVWF6/FbcRAU05dBHuC6m/Te1mwzBQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"1b6ec3337bbf2f4e13696d2e666f51032dfac9a94e23a8f34a69c571c15b3bdf","last_reissued_at":"2026-05-18T00:24:35.487600Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:24:35.487600Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Weak lensing magnification in the Dark Energy Survey Science Verification 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. E. Evrard, A. K. Romer, A. Roodman, A. R. Walker, B. Flaugher, B. Hoyle, C. B. D'Andrea, C. E. Cunha, D. Brooks, D. Gruen, D. J. James, D. Kirk, D. L. Burke, D. L. DePoy, D. Thomas, D. W. Gerdes, E. Bertin, E. Buckley-Geer, E. Fernandez, E. Gaztanaga, E. Krause, E. M. Huff, E. S\\'anchez, E. S. Rykoff, E. Suchyta, F. B. Abdalla, F. J. Castander, F. Sobreira, G. Gutierrez, G. M. Bernstein, G. Tarle, H. T. Diehl, I. Sevilla-Noarbe, J. Aleksi\\'c, J. Annis, J. Carretero, J. Frieman, J. Garc\\'ia-Bellido, J. Gschwend, J. J. Mohr, J. L. Marshall, K. Kuehn, L. N. da Costa, M. A. G. Maia, M. Carrasco Kind, M. Crocce, M. Garcia-Fernandez, M. Jarvis, M. Lima, M. March, M. Schubnell, M. Soares-Santos, N. Kuropatkin, N. MacCrann, O. Lahav, P. Fosalba, P. Melchior, R. A. Gruendl, R. C. Smith, R. Miquel, R. Ponce, S. Allam, S. Desai, T. F. Eifler, T. Giannantonio, T. M. C. Abbott, V. Scarpine, W. Wester","submitted_at":"2016-11-30T19:34:56Z","abstract_excerpt":"In this paper the effect of weak lensing magnification on galaxy number counts is studied by cross-correlating the positions of two galaxy samples, separated by redshift, using data from the Dark Energy Survey Science Verification dataset. The analysis is carried out for two photometrically-selected galaxy samples, with mean photometric redshifts in the $0.2 < z < 0.4$ and $0.7 < z < 1.0$ ranges, in the riz bands. A signal is detected with a $3.5\\sigma$ significance level in each of the bands tested, and is compatible with the magnification predicted by the $\\Lambda$CDM model. After an extensi"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1611.10326","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":"1611.10326","created_at":"2026-05-18T00:24:35.487663+00:00"},{"alias_kind":"arxiv_version","alias_value":"1611.10326v2","created_at":"2026-05-18T00:24:35.487663+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1611.10326","created_at":"2026-05-18T00:24:35.487663+00:00"},{"alias_kind":"pith_short_12","alias_value":"DNXMGM33X4XU","created_at":"2026-05-18T12:30:12.583610+00:00"},{"alias_kind":"pith_short_16","alias_value":"DNXMGM33X4XU4E3J","created_at":"2026-05-18T12:30:12.583610+00:00"},{"alias_kind":"pith_short_8","alias_value":"DNXMGM33","created_at":"2026-05-18T12:30:12.583610+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/DNXMGM33X4XU4E3JNUXGM32RAM","json":"https://pith.science/pith/DNXMGM33X4XU4E3JNUXGM32RAM.json","graph_json":"https://pith.science/api/pith-number/DNXMGM33X4XU4E3JNUXGM32RAM/graph.json","events_json":"https://pith.science/api/pith-number/DNXMGM33X4XU4E3JNUXGM32RAM/events.json","paper":"https://pith.science/paper/DNXMGM33"},"agent_actions":{"view_html":"https://pith.science/pith/DNXMGM33X4XU4E3JNUXGM32RAM","download_json":"https://pith.science/pith/DNXMGM33X4XU4E3JNUXGM32RAM.json","view_paper":"https://pith.science/paper/DNXMGM33","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1611.10326&json=true","fetch_graph":"https://pith.science/api/pith-number/DNXMGM33X4XU4E3JNUXGM32RAM/graph.json","fetch_events":"https://pith.science/api/pith-number/DNXMGM33X4XU4E3JNUXGM32RAM/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/DNXMGM33X4XU4E3JNUXGM32RAM/action/timestamp_anchor","attest_storage":"https://pith.science/pith/DNXMGM33X4XU4E3JNUXGM32RAM/action/storage_attestation","attest_author":"https://pith.science/pith/DNXMGM33X4XU4E3JNUXGM32RAM/action/author_attestation","sign_citation":"https://pith.science/pith/DNXMGM33X4XU4E3JNUXGM32RAM/action/citation_signature","submit_replication":"https://pith.science/pith/DNXMGM33X4XU4E3JNUXGM32RAM/action/replication_record"}},"created_at":"2026-05-18T00:24:35.487663+00:00","updated_at":"2026-05-18T00:24:35.487663+00:00"}