{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2016:6PLFEL5KQUMTRGFXWUTRVMFTPW","short_pith_number":"pith:6PLFEL5K","schema_version":"1.0","canonical_sha256":"f3d6522faa85193898b7b5271ab0b37d98e828f27dac5f7f41807a0ff552c366","source":{"kind":"arxiv","id":"1601.00405","version":3},"attestation_state":"computed","paper":{"title":"Galaxy bias from the Dark Energy Survey Science Verification data: combining galaxy density maps and weak lensing maps","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"A. Amara, A. A. Plazas, A. Benoit-Levy, A. Carnero Rosell, A. E. Evrard, A. J. Ross, A. K. Romer, A. Pujol, A. Refregier, A. Roodman, A. R. Walker (The DES Collaboration), B. Flaugher, B. Jain, B. Nord, C. B. D'Andrea, C. Bonnett, C. Chang, C. E. Cunha, C. J. Miller, D. A. Goldstein, D. Bacon, D. Brooks, D. Capozzi, D. Gruen, D. J. James, D. L. Burke, D. Thomas, E. Bertin, E. Buckley-Geer, E. Gaztanaga, E. Sanchez, E. Sheldon, E. S. Rykoff, E. Suchyta, F. B. Abdalla, F. J. Castander, F. Sobreira, G. Gutierrez, G. Tarle, H. T. Diehl, I. Sevilla-Noarbe, J. Annis, J. Carretero, J. Estrada, J. Frieman, J. J. Mohr, J. L. Marshall, J. P. Dietrich, J. Zuntz, K. Honscheid, K. Kuehn, K. Reil, L. N. da Costa, M. A. Troxel, M. Carrasco Kind, M. Crocce, M. E. C. Swanson, M. Jarvis, M. Lima, M. R. Becker, M. Schubnell, M. Soares-Santos, N. Kuropatkin, O. Lahav, P. Doel, P. Fosalba, P. Martini, P. Melchior, R. A. Gruendl, R. C. Nichol, R. C. Smith, R. Miquel, R. Ogando, S. Allam, S. Desai, T. F. Eifler, T. Giannantonio, T. Kacprzak, T. M. C. Abbott, T. S. Li, V. Scarpine, V. Vikram, W. Hartley","submitted_at":"2016-01-04T08:03:28Z","abstract_excerpt":"We measure the redshift evolution of galaxy bias for a magnitude-limited galaxy sample by combining the galaxy density maps and weak lensing shear maps for a $\\sim$116 deg$^{2}$ area of the Dark Energy Survey (DES) Science Verification data. This method was first developed in Amara et al. (2012) and later re-examined in a companion paper (Pujol et al. 2016) with rigorous simulation tests and analytical treatment of tomographic measurements. In this work we apply this method to the DES SV data and measure the galaxy bias for a i$<$22.5 galaxy sample. We find the galaxy bias and 1$\\sigma$ error "},"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":"1601.00405","kind":"arxiv","version":3},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2016-01-04T08:03:28Z","cross_cats_sorted":[],"title_canon_sha256":"88351905adc567611967811d8c56a9d9260df129f5887767533c77c5fc39c398","abstract_canon_sha256":"6cc1d6711279d7b6b9843bdd399267f52036a2d5abde3d2943a792108eaf352e"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:13:15.792575Z","signature_b64":"MBvSPU01xymrM+i9p3GzEytA/m3Sfxb5VqoSCRGU/s4MIDx3fcArlOO5ACTApOsPWEP+VwPoppodVVte3xsuAA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"f3d6522faa85193898b7b5271ab0b37d98e828f27dac5f7f41807a0ff552c366","last_reissued_at":"2026-05-18T01:13:15.792065Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:13:15.792065Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Galaxy bias from the Dark Energy Survey Science Verification data: combining galaxy density maps and weak lensing maps","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"A. Amara, A. A. Plazas, A. Benoit-Levy, A. Carnero Rosell, A. E. Evrard, A. J. Ross, A. K. Romer, A. Pujol, A. Refregier, A. Roodman, A. R. Walker (The DES Collaboration), B. Flaugher, B. Jain, B. Nord, C. B. D'Andrea, C. Bonnett, C. Chang, C. E. Cunha, C. J. Miller, D. A. Goldstein, D. Bacon, D. Brooks, D. Capozzi, D. Gruen, D. J. James, D. L. Burke, D. Thomas, E. Bertin, E. Buckley-Geer, E. Gaztanaga, E. Sanchez, E. Sheldon, E. S. Rykoff, E. Suchyta, F. B. Abdalla, F. J. Castander, F. Sobreira, G. Gutierrez, G. Tarle, H. T. Diehl, I. Sevilla-Noarbe, J. Annis, J. Carretero, J. Estrada, J. Frieman, J. J. Mohr, J. L. Marshall, J. P. Dietrich, J. Zuntz, K. Honscheid, K. Kuehn, K. Reil, L. N. da Costa, M. A. Troxel, M. Carrasco Kind, M. Crocce, M. E. C. Swanson, M. Jarvis, M. Lima, M. R. Becker, M. Schubnell, M. Soares-Santos, N. Kuropatkin, O. Lahav, P. Doel, P. Fosalba, P. Martini, P. Melchior, R. A. Gruendl, R. C. Nichol, R. C. Smith, R. Miquel, R. Ogando, S. Allam, S. Desai, T. F. Eifler, T. Giannantonio, T. Kacprzak, T. M. C. Abbott, T. S. Li, V. Scarpine, V. Vikram, W. Hartley","submitted_at":"2016-01-04T08:03:28Z","abstract_excerpt":"We measure the redshift evolution of galaxy bias for a magnitude-limited galaxy sample by combining the galaxy density maps and weak lensing shear maps for a $\\sim$116 deg$^{2}$ area of the Dark Energy Survey (DES) Science Verification data. This method was first developed in Amara et al. (2012) and later re-examined in a companion paper (Pujol et al. 2016) with rigorous simulation tests and analytical treatment of tomographic measurements. In this work we apply this method to the DES SV data and measure the galaxy bias for a i$<$22.5 galaxy sample. We find the galaxy bias and 1$\\sigma$ error "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1601.00405","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":"1601.00405","created_at":"2026-05-18T01:13:15.792144+00:00"},{"alias_kind":"arxiv_version","alias_value":"1601.00405v3","created_at":"2026-05-18T01:13:15.792144+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1601.00405","created_at":"2026-05-18T01:13:15.792144+00:00"},{"alias_kind":"pith_short_12","alias_value":"6PLFEL5KQUMT","created_at":"2026-05-18T12:30:01.593930+00:00"},{"alias_kind":"pith_short_16","alias_value":"6PLFEL5KQUMTRGFX","created_at":"2026-05-18T12:30:01.593930+00:00"},{"alias_kind":"pith_short_8","alias_value":"6PLFEL5K","created_at":"2026-05-18T12:30:01.593930+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/6PLFEL5KQUMTRGFXWUTRVMFTPW","json":"https://pith.science/pith/6PLFEL5KQUMTRGFXWUTRVMFTPW.json","graph_json":"https://pith.science/api/pith-number/6PLFEL5KQUMTRGFXWUTRVMFTPW/graph.json","events_json":"https://pith.science/api/pith-number/6PLFEL5KQUMTRGFXWUTRVMFTPW/events.json","paper":"https://pith.science/paper/6PLFEL5K"},"agent_actions":{"view_html":"https://pith.science/pith/6PLFEL5KQUMTRGFXWUTRVMFTPW","download_json":"https://pith.science/pith/6PLFEL5KQUMTRGFXWUTRVMFTPW.json","view_paper":"https://pith.science/paper/6PLFEL5K","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1601.00405&json=true","fetch_graph":"https://pith.science/api/pith-number/6PLFEL5KQUMTRGFXWUTRVMFTPW/graph.json","fetch_events":"https://pith.science/api/pith-number/6PLFEL5KQUMTRGFXWUTRVMFTPW/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/6PLFEL5KQUMTRGFXWUTRVMFTPW/action/timestamp_anchor","attest_storage":"https://pith.science/pith/6PLFEL5KQUMTRGFXWUTRVMFTPW/action/storage_attestation","attest_author":"https://pith.science/pith/6PLFEL5KQUMTRGFXWUTRVMFTPW/action/author_attestation","sign_citation":"https://pith.science/pith/6PLFEL5KQUMTRGFXWUTRVMFTPW/action/citation_signature","submit_replication":"https://pith.science/pith/6PLFEL5KQUMTRGFXWUTRVMFTPW/action/replication_record"}},"created_at":"2026-05-18T01:13:15.792144+00:00","updated_at":"2026-05-18T01:13:15.792144+00:00"}