Gaia Data Release 2. Observations of solar system objects
F. Spoto, P. Tanga, F. Mignard, J. Berthier, B. Carry, A. Cellino, A. Dell’Oro, Daniel Hestroffer, K. Muinonen, T. Pauwels, JM Petit, Patrice David, F. De Angeli, M. Delbò, B. Frézouls, L. Galluccio, Mikael Granvik, J. Guiraud, J. Hernández, C. Ordénovic, J. Portell, E. Poujoulet, W. Thuillot, G. Walmsley, Aga Brown, A. Vallenari, T. Prusti, Jhj de Bruijne, C. Babusiaux, C. A. L. Bailer-Jones, M. Biermann, DW Evans, L. Eyer, F. Jansen, C. Jordi, SA Klioner, U. Lammers, L. Lindegren, X. Luri, C. Panem, D. Pourbaix, S. Randich, P. Sartoretti, HI Siddiqui, C. Soubiran, F. van Leeuwen, NA Walton, F. Arenou, U. Bastian, M. Cropper, R. Drimmel, D. Katz, MG Lattanzi, J. Bakker, C. Cacciari, J. Castañeda, L. Chaoul, N. Cheek, C. Fabricius, R. Guerra, B. Holl, E. Masana, R. Messineo, N. Mowlavï, K. Nienartowicz, P. Panuzzo, M. Riello, GM Seabroke, F. Thévenin, G. Gracia-Abril, G. Comoretto, M. Garcia-Reinaldos, D. Teyssier, M. Altmann, R. Andrae, M. Audard, I. Bellas-Velidis, K. Benson, R. Blomme, P. W. Burgess, G. Busso, G. Clementini, M. Clotet, O. L. Creevey, M. Davidson, J. De Ridder, L. Delchambre, C. Ducourant, J. Fernández-Hernández, M. Fouesneau, Y. Frémat, Miguel García-Torres, J. González-Núñez, J. J. González-Vidal, E. Gosset, LP Guy, J. L. Halbwachs, NC Hambly, DL Harrison, ST Hodgkin
Abstract
CONTEXT: The Gaia spacecraft of the European Space Agency (ESA) has been securing observations of solar system objects (SSOs) \nsince the beginning of its operations. Data Release 2 (DR2) contains the observations of a selected sample of 14,099 SSOs. These \nasteroids have been already identified and have been numbered by the Minor Planet Center repository. Positions are provided for each \nGaia observation at CCD level. As additional information, complementary to astrometry, the apparent brightness of SSOs in the unfiltered \nG band is also provided for selected observations. \nAIMS: We explain the processing of SSO data, and describe the criteria we used to select the sample published in Gaia DR2. We then \nexplore the data set to assess its quality. \nMETHODS: To exploit the main data product for the solar system in Gaia DR2, which is the epoch astrometry of asteroids, it is necessary \nto take into account the unusual properties of the uncertainty, as the position information is nearly one-dimensional. When this aspect \nis handled appropriately, an orbit fit can be obtained with post-fit residuals that are overall consistent with the a-priori error model that \nwas used to define individual values of the astrometric uncertainty. The role of both random and systematic errors is described. The \ndistribution of residuals allowed us to identify possible contaminants in the data set (such as stars). Photometry in the G band was \ncompared to computed values from reference asteroid shapes and to the flux registered at the corresponding epochs by the red and blue \nphotometers (RP and BP). \nRESULTS: The overall astrometric performance is close to the expectations, with an optimal range of brightness G ∼ 12 − 17. In this \nrange, the typical transit-level accuracy is well below 1 mas. For fainter asteroids, the growing photon noise deteriorates the performance. \nAsteroids brighter than G ∼ 12 are affected by a lower performance of the processing of their signals. The dramatic improvement \nbrought by Gaia DR2 astrometry of SSOs is demonstrated by comparisons to the archive data and by preliminary tests on the detection \nof subtle non-gravitational effects.