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We describe the model for the mapping from sky brightness to the digital output of the Dark Energy Camera, and the algorithms adopted by the Dark Energy Survey (DES) for inverting this model to obtain photometric measures of celestial…

Instrumentation and Methods for Astrophysics · Physics 2017-09-20 G. M. Bernstein , T. M. C. Abbott , S. Desai , D. Gruen , R. A. Gruendl , M. D. Johnson , H. Lin , F. Menanteau , E. Morganson , E. Neilsen , K. Paech , A. R. Walker , W. Wester , B. Yanny

We describe the Dark Energy Survey (DES) photometric data set assembled from the first three years of science operations to support DES Year 3 cosmology analyses, and provide usage notes aimed at the broad astrophysics community. Y3 Gold…

Cosmology and Nongalactic Astrophysics · Physics 2021-05-28 I. Sevilla-Noarbe , K. Bechtol , M. Carrasco Kind , A. Carnero Rosell , M. R. Becker , A. Drlica-Wagner , R. A. Gruendl , E. S. Rykoff , E. Sheldon , B. Yanny , A. Alarcon , S. Allam , A. Amon , A. Benoit-Lévy , G. M. Bernstein , E. Bertin , D. L. Burke , J. Carretero , A. Choi , H. T. Diehl , S. Everett , B. Flaugher , E. Gaztanaga , J. Gschwend , I. Harrison , W. G. Hartley , B. Hoyle , M. Jarvis , M. D. Johnson , R. Kessler , R. Kron , N. Kuropatkin , B. Leistedt , T. S. Li , F. Menanteau , E. Morganson , R. L. C. Ogando , A. Palmese , F. Paz-Chinchón , A. Pieres , C. Pond , M. Rodriguez-Monroy , J. Allyn-Smith , K. M. Stringer , M. A. Troxel , D. L. Tucker , J. de Vicente , W. Wester , Y. Zhang , T. M. C. Abbott , M. Aguena , J. Annis , S. Avila , S. Bhargava , S. L. Bridle , D. Brooks , D. Brout , F. J. Castander , R. Cawthon , C. Chang , C. Conselice , M. Costanzi , M. Crocce , L. N. da Costa , M. E. E. Pereira , T. M. Davis , S. Desai , J. P. Dietrich , P. Doel , K. Eckert , A. E. Evrard , I. Ferrero , P. Fosalba , J. García-Bellido , D. W. Gerdes , T. Giannantonio , D. Gruen , G. Gutierrez , S. R. Hinton , D. L. Hollowood , K. Honscheid , E. M. Huff , D. Huterer , D. J. James , T. Jeltema , K. Kuehn , O. Lahav , C. Lidman , M. Lima , H. Lin , M. A. G. Maia , J. L. Marshall , P. Martini , P. Melchior , R. Miquel , J. J. Mohr , R. Morgan , E. Neilsen , A. A. Plazas , A. K. Romer , A. Roodman , E. Sanchez , V. Scarpine , M. Schubnell , S. Serrano , M. Smith , E. Suchyta , G. Tarle , D. Thomas , C. To , T. N. Varga , R. H. Wechsler , J. Weller , R. D. Wilkinson

Synthetic source injection (SSI), the insertion of sources into pixel-level on-sky images, is a powerful method for characterizing object detection and measurement in wide-field, astronomical imaging surveys. Within the Dark Energy Survey…

In this paper we present the testing of a back-illuminated development Euclid Visible Instrument (VIS) Charge-Coupled Device (CCD) to measure the intrinsic CCD Point Spread Function (PSF) characteristics using a novel modelling technique.…

Instrumentation and Methods for Astrophysics · Physics 2015-06-23 Sami-Matias Niemi , Mark Cropper , Magdalena Szafraniec , Thomas Kitching

The weak distortions produced by gravitational lensing in the images of background galaxies provide a method to measure directly the distribution of mass in the universe. However this technique requires high precision measurements of the…

Astrophysics · Physics 2009-10-31 Jason Rhodes , Alexandre Refregier , Ed Groth

We present the theoretical and analytical bases of optimal techniques to measure weak gravitational shear from images of galaxies. We first characterize the geometric space of shears and ellipticity, then use this geometric interpretation…

Astrophysics · Physics 2009-11-06 G. M. Bernstein , M. Jarvis

The ability to accurately measure the shapes of faint objects in images taken with the Advanced Camera for Surveys(ACS) on the Hubble Space Telescope (HST) depends upon detailed knowledge of the Point Spread Function (PSF). We show that…

Point Spread Function (PSF) engineering is used in single emitter localization to measure the emitter position in 3D and possibly other parameters such as the emission color or dipole orientation as well. Advanced PSF models such as spline…

X-ray cone-beam computed tomography (CT) has the notable features such as high efficiency and precision, and is widely used in the fields of medical imaging and industrial non-destructive testing, but the inherent imaging degradation…

Optics · Physics 2015-06-19 Hua Zhang , Kuidong Huang , Yikai Shi , Zhe Xu

In a previous work we have demonstrated a novel numerical model for the point spread function (PSF) of an optical system that can efficiently model both experimental measurements and lens design simulations of the PSF. The novelty lies in…

Image and Video Processing · Electrical Eng. & Systems 2018-06-25 Matthias Lehmann , Christian Wittpahl , Hatem Ben Zakour , Alexander Braun

The Dark Energy Survey collaboration will study cosmic acceleration with a 5000 deg2 griZY survey in the southern sky over 525 nights from 2011-2016. The DES data management (DESDM) system will be used to process and archive these data and…

In this work, we derive and calibrate the redshift distribution of the MagLim++ lens galaxy sample used in the Dark Energy Survey Year 6 (DES Y6) 3x2pt cosmology analysis. The 3x2pt analysis combines galaxy clustering from the lens galaxy…

We present our cosmic shear analysis of GEMS, one of the largest wide-field surveys ever undertaken by the Hubble Space Telescope. Imaged with the Advanced Camera for Surveys (ACS), GEMS spans 795 square arcmin in the Chandra Deep Field…

Modeling the intrinsic alignment (IA) of galaxies poses a challenge to weak lensing analyses. The Dark Energy Survey is expected to be less impacted by IA when limited to blue, star-forming galaxies. The cosmological parameter constraints…

Cosmology and Nongalactic Astrophysics · Physics 2026-05-07 J. McCullough , A. Amon , E. Legnani , D. Gruen , A. Roodman , O. Friedrich , N. MacCrann , M. R. Becker , J. Myles , S. Dodelson , S. Samuroff , J. Blazek , J. Prat , K. Honscheid , A. Pieres , A. Ferté , A. Alarcon , A. Drlica-Wagner , A. Choi , A. Navarro-Alsina , A. Campos , A. A. Plazas Malagón , A. Porredon , A. Farahi , A. J. Ross , A. Carnero Rosell , B. Yin , B. Flaugher , B. Yanny , C. Sánchez , C. Chang , C. Davis , C. To , C. Doux , D. Brooks , D. J. James , D. Sanchez Cid , D. L. Hollowood , D. Huterer , E. S. Rykoff , E. Gaztanaga , E. M. Huff , E. Suchyta , E. Sheldon , E. Sanchez , F. Tarsitano , F. Andrade-Oliveira , F. J. Castander , G. M. Bernstein , G. Gutierrez , G. Giannini , G. Tarle , H. T. Diehl , H. Huang , I. Harrison , I. Sevilla-Noarbe , I. Tutusaus , I. Ferrero , J. Elvin-Poole , J. L. Marshall , J. Muir , J. Weller , J. Zuntz , J. Carretero , J. DeRose , J. Frieman , J. Cordero , J. De Vicente , J. García-Bellido , J. Mena-Fernández , K. Eckert , A. K. Romer , K. Bechtol , K. Herner , K. Kuehn , L. F. Secco , L. N. da Costa , M. Paterno , 21 M. Soares-Santos , M. Gatti , M. Raveri , M. Yamamoto , M. Smith , M. Carrasco Kind , M. A. Troxel , M. Aguena , M. Jarvis , M. E. C. Swanson , N. Weaverdyck , O. Lahav , P. Doel , P. Wiseman , R. Miquel , R. A. Gruendl , R. Cawthon , S. Allam , S. R. Hinton , S. L. Bridle , S. Bocquet , S. Desai , S. Pandey , S. Everett , S. Lee , T. Shin , A. Palmese , C. Conselice , D. L. Burke , E. Buckley-Geer , M. Lima , M. Vincenzi , M. E. S. Pereira , M. Crocce , M. Schubnell , N. Jeffrey , O. Alves , V. Vikram , Y. Zhang , DES Collaboration

Neglecting the second order corrections in weak lensing measurements can lead to a few percent uncertainties on cosmic shears, and becomes more important for cluster lensing mass reconstructions. Existing methods which claim to measure the…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-18 Jun Zhang

Weak lensing by large-scale structure is a powerful probe of cosmology if the apparent alignments in the shapes of distant galaxies can be accurately measured. We study the performance of a fully data-driven approach, based on…

Cosmology and Nongalactic Astrophysics · Physics 2021-12-15 Henk Hoekstra

We present clustering redshift measurements for Dark Energy Survey (DES) lens sample galaxies to be used in weak gravitational lensing and galaxy clustering studies. To perform this measurement, we cross-correlate with spectroscopic…

The three-point correlation function (3PCF) of a weak lensing shear field contains information that is complementary to that in the two-point correlation function (2PCF), which can help improve the cosmological parameters and calibrate…

Cosmology and Nongalactic Astrophysics · Physics 2024-07-03 Sunao Sugiyama , Rafael C. H. Gomes , Mike Jarvis

Weak lensing studies typically require excellent seeing conditions for the purpose of maximizing the number density of well-resolved galaxy images. It is interesting to ask to what extent the seeing size limits the usefulness of the…

Cosmology and Nongalactic Astrophysics · Physics 2022-09-14 Jun Zhang , Cong Liu , Pedro Alonso Vaquero , Hekun Li , Haoran Wang , Zhi Shen , Fuyu Dong