posted on 2024-08-06, 10:27authored byC. Bonnett, M. A. Troxel, W. Hartley, A. Amara, B. Leistedt, M. R. Becker, G. M. Bernstein, S. L. Bridle, C. Bruderer, M. T. Busha, M. Carrasco Kind, M. J. Childress, F. J. Castander, C. Chang, M. Crocce, T. M. Davis, T. F. Eifler, J. Frieman, C. Gangkofner, E. Gaztanaga, Karl GlazebrookKarl Glazebrook, D. Gruen, T. Kacprzak, A. King, J. Kwan, O. Lahav, G. Lewis, C. Lidman, H. Lin, N. MacCrann, R. Miquel, C. R. O'Neill, A. Palmese, H. V. Peiris, A. Refregier, E. Rozo, E. S. Rykoff, I. Sadeh, C. Sánchez, E. Sheldon, S. Uddin, R. H. Wechsler, J. Zuntz, T. Abbott, F. B. Abdalla, S. Allam, R. Armstrong, M. Banerji, A. H. Bauer, A. Benoit-Lévy, E. Bertin, D. Brooks, E. Buckley-Geer, D. L. Burke, D. Capozzi, A. Carnero Rosell, J. Carretero, C. E. Cunha, C. B. D'Andrea, L. N. Da Costa, D. L. Depoy, S. Desai, H. T. Diehl, J. P. Dietrich, P. Doel, A. Fausti Neto, E. Fernandez, B. Flaugher, P. Fosalba, D. W. Gerdes, R. A. Gruendl, K. Honscheid, B. Jain, D. J. James, M. Jarvis, A. G. Kim, K. Kuehn, N. Kuropatkin, T. S. Li, M. Lima, M. A G Maia, M. March, J. L. Marshall, P. Martini, P. Melchior, C. J. Miller, E. Neilsen, R. C. Nichol, B. Nord, R. Ogando, A. A. Plazas, K. Reil, A. K. Romer, A. Roodman, M. Sako, E. Sanchez, B. Santiago, R. C. Smith, M. Soares-Santos, F. Sobreira, E. Suchyta, M. E C Swanson, G. Tarle, J. Thaler, D. Thomas, V. Vikram, A. R. Walker
We present photometric redshift estimates for galaxies used in the weak lensing analysis of the Dark Energy Survey Science Verification (DES SV) data. Four model- or machine learning-based photometric redshift methods—annz2, bpz calibrated against BCC-Ufig simulations, skynet, and tpz—are analyzed. For training, calibration, and testing of these methods, we construct a catalogue of spectroscopically confirmed galaxies matched against DES SV data. The performance of the methods is evaluated against the matched spectroscopic catalogue, focusing on metrics relevant for weak lensing analyses, with additional validation against COSMOS photo-z’s. From the galaxies in the DES SV shear catalogue, which have mean redshift 0.72±0.01 over the range 0.3
Funding
Research England
Deutsche Forschungsgemeinschaft
Science and Technology Facilities Council
Fermilab
United States Department of Energy
European Research Council
Office of Science
Directorate for Mathematical & Physical Sciences
Australian Research Council
Swiss National Science Foundation
Ministerio de Educación Cultura y Deporte
National Science Foundation
Alfred P. Sloan Foundation
National Council for Scientific and Technological Development
Financiadora de Estudos e Projetos
Fundação Carlos Chagas Filho de Amparo à Pesquisa do Estado do Rio de Janeiro