Artículos de revistas
A Search of the Full Six Years of the Dark Energy Survey for Outer Solar System Objects
Fecha
2022-01-01Registro en:
Astrophysical Journal, Supplement Series, v. 258, n. 2, 2022.
0067-0049
10.3847/1538-4365/ac3914
2-s2.0-85125691286
Autor
University of Pennsylvania
Fermi National Accelerator Laboratory
Laboratório Interinstitucional de E-Astronomia - LIneA
Universidade Estadual Paulista (UNESP)
Institut d'Astrophysique de Paris
University College London
University of Chicago
Stanford University
SLAC National Accelerator Laboratory
National Center for Supercomputing Applications
University of Illinois at Urbana-Champaign
The Barcelona Institute of Science and Technology
University of Manchester
School of Physics and Astronomy
University of Trieste
INAF-Osservatorio Astronomico di Trieste
Institute for Fundamental Physics of the Universe
Observatório Nacional
Medioambientales y Tecnológicas (CIEMAT)
IIT Hyderabad
Ludwig-Maximilians-Universität
Santa Cruz Institute for Particle Physics
University of Oslo
Institut d'Estudis Espacials de Catalunya (IEEC)
CSIC)
Universidad Autonoma de Madrid
University of Michigan
University of Queensland
The Ohio State University
60 Garden Street
Macquarie University
Lowell Observatory
Institució Catalana de Recerca i Estudis Avançats
University of Wisconsin-Madison
University of Cambridge
Princeton University
University of Sussex
University of Southampton
Oak Ridge National Laboratory
Max Planck Institute for Extraterrestrial Physics
Ludwig-Maximilians Universität München
NSFs NOIRLab
Institución
Resumen
We present a search for outer solar system objects in the 6 yr of data from the Dark Energy Survey (DES). The DES covered a contiguous 5000 deg2 of the southern sky with ≈80,000 3 deg2 exposures in the grizY filters between 2013 and 2019. This search yielded 812 trans-Neptunian objects (TNOs), one Centaur and one Oort cloud comet, 458 reported here for the first time. We present methodology that builds upon our previous search on the first 4 yr of data. All images were reprocessed with an optimized detection pipeline that leads to an average completeness gain of 0.47 mag per exposure, as well as improved transient catalog production and algorithms for linkage of detections into orbits. All objects were verified by visual inspection and by the sub-threshold significance,the signal-to-noise ratio in the stack of images in which its presence is indicated by the orbit, but no detection was reported. This yields a pure catalog complete to r ≈ 23.8 mag and distances 29 < d < 2500 au. The TNOs have minimum (median) of 7 (12) nights' detections and arcs of 1.1 (4.2) yr, and will have grizY magnitudes available in a further publication. We present software for simulating our observational biases for comparisons of models to our detections. Initial inferences demonstrating the catalog's statistical power are: the data are inconsistent with the CFEPS-L7 model for the classical Kuiper Belt; the 16 extremeTNOs (a > 150 au, q > 30 au) are consistent with the null hypothesis of azimuthal isotropy; and nonresonant TNOs with q > 38 au, a > 50 au show a significant tendency to be sunward of major mean-motion resonances.