Dark Energy Survey year 1 results: Galaxy-galaxy lensing
Physical review. D/Physical review. D.2018Vol. 98(4)
Citations Over TimeTop 1% of 2018 papers
J. Prat, C. Sánchez, Y Fang, D. Gruen, J. Elvin-Poole, Nickolas Kokron, L F Secco, Bhuvnesh Jain, R. Miquel, N. MacCrann, M. A. Troxel, A. Alarcon, David Bacon, G. M. Bernstein, J. Blazek, R. Cawthon, C. Chang, M. Crocce, C. Davis, J. De Vicente, J. P. Dietrich, A. Drlica-Wagner, O. Friedrich, M. Gatti, W. G. Hartley, B. Hoyle, Erica Huff, Mike Jarvis, Markus Michael Rau, R. P. Rollins, Ashley J. Ross, Eduardo Rozo, E. S. Rykoff, S. Samuroff, E. Sheldon, T. N. Varga, P Vielzeuf, J. Zuntz, T. M. C. Abbott, F. B. Abdalla, S. Allam, J. Annis, K. Bechtol, A. Benoit-Lévy, E. Bertin, D. Brooks, E. Buckley‐Geer, D. L. Burke, A. Carnero Rosell, M. Carrasco Kind, J. Carretero, F. J. Castander, C. E. Cunha, C. B. D’Andrea, L. N. da Costa, S. Desai, H. T. Diehl, Scott Dodelson, T. F. Eifler, E. Fernández, B. Flaugher, P. Fosalba, J. Frieman, J. García-Bellido, E. Gaztañaga, D. W. Gerdes, T. Giannantonio, D. A. Goldstein, R. A. Gruendl, J. Gschwend, G. Gutiérrez, K. Honscheid, D. J. James, T. Jeltema, M. W. G. Johnson, Michael D. Johnson, D. Kirk, E. Krause, K. Kuehn, S. E. Kuhlmann, O. Lahav, T. S. Li, M. Lima, M. A. G. Maia, M. March, J. L. Marshall, Paul Martini, P. Melchior, F. Menanteau, J. J. Mohr, R. C. Nichol, B. Nord, A. A. Plazas, A. K. Romer, A. Roodman, M. Šako, E. Sánchez, V. Scarpine, R. Schindler, M. Schubnell, I. Sevilla-Noarbe, M. Smith, Rory Smith, M. Soares-Santos, F. Sobreira, E. Suchyta, M. E. C. Swanson, G. Tarlé, D. Thomas, D. L. Tucker, V. Vikram, A. R. Walker, Risa H. Wechsler, B. Yanny, Y. Zhang
Abstract
We present galaxy-galaxy lensing measurements from 1321 sq. deg. of the Dark Energy Survey (DES) Year 1 (Y1) data. The lens sample consists of a selection of 660,000 red galaxies with high-precision photometric redshifts, known as redMaGiC, split into five tomographic bins in the redshift range 0.15 < z < 0.9. We use two different source samples, obtained from the METACALIBRATION (26 million galaxies) and IM3SHAPE (18 million galaxies) shear estimation codes, which are split into four photometric redshift bins in the range 0.2 < z < 1.3. We perform extensive testing of potential systematic effects that can bias the galaxy-galaxy lensing signal, including those from shear estimation, photometric redshifts, and
Related Papers
- → WHAT LIES BENEATH: USING p ( z ) TO REDUCE SYSTEMATIC PHOTOMETRIC REDSHIFT ERRORS(2009)44 cited
- → Calibrating photometric redshifts of luminous red galaxies(2005)105 cited
- → How Sensitive Are Weak Lensing Statistics to Dark Energy Content?(2003)21 cited
- → Constraints on the Physical Parameters of the Dark Energy Using a Model-Independent Approach(2005)3 cited
- → Calibrating Photometric Redshifts of Luminous Red Galaxies(2004)