Reducing Ground-based Astrometric Errors with Gaia and Gaussian Processes

Fortino, W. F.; Bernstein, G. M.; Bernardinelli, P. H.; Aguena, M.; Allam, S.; Annis, J.; Bacon, D.; Bechtol, K.; Bhargava, S.; Brooks, D.; Burke, D. L.; Carretero, J.; Choi, A.; Costanzi, M.; da Costa, L. N.; Pereira, M. E. S.; De Vicente, J.; Desai, S.; Doel, P.; Drlica-Wagner, A.; Eckert, K.; Eifler, T. F.; Evrard, A. E.; Ferrero, I.; Frieman, J.; Garcia-Bellido, J.; Gaztanaga, E.; Gerdes, D. W.; Gruendl, R. A.; Gschwend, J.; Gutierrez, G.; Hartley, W. G.; Hinton, S. R.; Hollowood, D. L.; Honscheid, K.; James, D. J.; Jarvis, M.; Kent, S.; Kuehn, K.; Kuropatkin, N.; Maia, M. A. G.; Marshall, J. L.; Menanteau, F.; Miquel, R.; Morgan, R.; Myles, J.; Ogando, R. L. C.; Palmese, A.; Paz-Chinchon, F.; Plazas, A. A.; Roodman, A.; Rykoff, E. S.; Sanchez, E.; Santiago, B.; Scarpine, V.; Schubnell, M.; Serrano, S.; Sevilla-Noarbe, I.; Smith, M.; Suchyta, E.; Tarle, G.; To, C.; Tucker, D. L.; Varga, T. N.; Walker, A. R.; Weller, J. und Wester, W. (2021): Reducing Ground-based Astrometric Errors with Gaia and Gaussian Processes. In: Astronomical Journal, Bd. 162, Nr. 3, 106

Abstract

Stochastic field distortions caused by atmospheric turbulence are a fundamental limitation to the astrometric accuracy of ground-based imaging. This distortion field is measurable at the locations of stars with accurate positions provided by the Gaia DR2 catalog;we develop the use of Gaussian process regression (GPR) to interpolate the distortion field to arbitrary locations in each exposure. We introduce an extension to standard GPR techniques that exploits the knowledge that the 2D distortion field is curl-free. Applied to several hundred 90 s exposures from the Dark Energy Survey as a test bed, we find that the GPR correction reduces the variance of the turbulent astrometric distortions approximate to 12x , on average, with better performance in denser regions of the Gaia catalog. The rms per-coordinate distortion in the riz bands is typically approximate to 7 mas before any correction and approximate to 2 mas after application of the GPR model. The GPR astrometric corrections are validated by the observation that their use reduces, from 10 to 5 mas rms, the residuals to an orbit fit to riz-band observations over 5 yr of the r = 18.5 trans-Neptunian object Eris. We also propose a GPR method, not yet implemented, for simultaneously estimating the turbulence fields and the 5D stellar solutions in a stack of overlapping exposures, which should yield further turbulence reductions in future deep surveys.

• Dokumententyp: Zeitschriftenartikel
• Fakultät: Physik
• Themengebiete: 500 Naturwissenschaften und Mathematik > 530 Physik
• ISSN: 0004-6256
• Sprache: Englisch