4.6 Article

A Search of the Full Six Years of the Dark Energy Survey for Outer Solar System Objects

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出版社

IOP Publishing Ltd
DOI: 10.3847/1538-4365/ac3914

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资金

  1. National Science Foundation [AST-1515804, AST-2009210, AST-1138766, AST-1536171]
  2. Department of Energy [DE-SC0007901]
  3. U.S. Department of Energy
  4. U.S. National Science Foundation
  5. Ministry of Science and Education of Spain
  6. Science and Technology Facilities Council of the United Kingdom
  7. Higher Education Funding Council for England
  8. National Center for Supercomputing Applications at the University of Illinois at Urbana-Champaign
  9. Kavli Institute of Cosmological Physics at the University of Chicago
  10. Center for Cosmology and Astro-Particle Physics at the Ohio State University
  11. Mitchell Institute for Fundamental Physics and Astronomy at Texas AM University
  12. Financiadora de Estudos e Projetos
  13. Fundacao Carlos Chagas Filho de Amparo a Pesquisa do Estado do Rio de Janeiro
  14. Conselho Nacional de Desenvolvimento Cientifico e Tecnologico
  15. Ministerio da Ciencia, Tecnologia e Inovacao
  16. Deutsche Forschungsgemeinschaft
  17. MICINN [ESP2017-89838, PGC2018-094773, PGC2018-102021, SEV2016-0588, SEV-2016-0597, MDM-2015-0509]
  18. RDF funds from the European Union
  19. CERCA program of the Generalitat de Catalunya
  20. European Research Council under the European Union's Seventh Framework Program (FP7/2007-2013)
  21. ERC [240672, 291329, 306478]
  22. Brazilian Instituto Nacional de Ciencia e Tecnologia (INCT) do e-Universo (CNPq grant) [465376/2014-2]
  23. U.S. Department of Energy, Office of Science, Office of High Energy Physics [DE-AC02-07CH11359]
  24. Argonne National Laboratory
  25. University of California at Santa Cruz
  26. University of Cambridge, Centro de Investigaciones Energeticas, Medioambientales y Tecnologicas-Madrid
  27. University of Chicago
  28. University College London
  29. DES-Brazil Consortium
  30. University of Edinburgh
  31. Eidgenossische Technische Hochschule (ETH) Zurich
  32. Fermi National Accelerator Laboratory
  33. University of Illinois at UrbanaChampaign
  34. Institut de Ciencies de l'Espai (IEEC/CSIC)
  35. Institut de Fisica d'Altes Energies
  36. Lawrence Berkeley National Laboratory
  37. Ludwig-Maximilians Universitat Munchen
  38. associated Excellence Cluster Universe
  39. University of Michigan
  40. NSF's NOIRLab
  41. University of Nottingham
  42. Ohio State University
  43. University of Pennsylvania
  44. University of Portsmouth
  45. SLAC National Accelerator Laboratory
  46. Stanford University
  47. University of Sussex
  48. Texas AM University
  49. OzDES Membership Consortium

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In this study, we conducted a search for outer solar system objects using the data from Dark Energy Survey (DES) over a period of 6 years. We identified 812 trans-Neptunian objects (TNOs), one Centaur, and one Oort cloud comet, with 458 objects reported for the first time. Our methodology involved reprocessing all images and optimizing the detection pipeline, leading to significant improvements in completeness gain and catalog production. Visual inspection and sub-threshold significance were used for verification of all objects.
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 deg(2) of the southern sky with approximate to 80,000 3 deg(2) 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 approximate to 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 extreme TNOs (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.

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