Please use this identifier to cite or link to this item: http://hdl.handle.net/2445/140071
Title: Gaia Data Release 2: observations of Solar System objects
Author: Gaia Collaboration
Jordi i Nebot, Carme
Luri Carrascoso, Xavier
Antoja Castelltort, M. Teresa
Castro Ginard, Alfred
Masana Fresno, Eduard
Farras Casas, Martí
Figueras Siñol, Francesca
Portell i de Mora, Jordi
Garralda Torre, Nora
Casamiquela Floriach, Laia
Balaguer Núñez, María de los Dolores
Cantat Gaudin, Tristan
Borrachero, Raul
Bartolomé Muñoz, Sergi
Julbe, Francesc
Clotet Altarriba, Marcial
González Vidal, Juan José
Carrasco Martínez, José Manuel
Torra Roca, Jorge
Antiche Garzón, Erika
Fabricius, Claus
Castañeda Pons, Javier Bernardo
Keywords: Astrometria
Asteroides
Processament de dades
Astrometry
Asteroids
Data processing
Issue Date: 10-Aug-2018
Publisher: EDP Sciences
Abstract: Context. The Gaia spacecraft of the European Space Agency (ESA) has been securing observations of Solar System Objects since the beginning of its operations. The Data Release 2 (DR2) contains the observations of a selected sample of 14,099 Solar System Objects, SSOs for brevity. These asteroids were already identified and numbered by the Minor Planet Center repository. Positions are provided for each Gaia observation, at CCD level. As additional information, complementary to astrometry, the apparent brightness of SSOs in the unfiltered G band is also provided for selected observations. Aims. We explain the processing of SSO data, and the criteria used to select the sample published in the Gaia DR2. We then explore the data set to assess its quality. Methods. To exploit the main data product for the Solar System in Gaia DR2, namely epoch astrometry of asteroids, it is necessary to take into account the unusual properties of the uncertainty, as the position information is nearly one-dimensional. Once this aspect is appropriately handled, an orbit fit can be obtained, with post-fit residuals that are overall consistent with the a-priori error model used to define individual values of the astrometric uncertainty. The role of both random and systematic errors is described. The distribution of residuals allows us to identify possible contaminants in the data set (such as stars). Photometry in the G band is compared to computed values from reference asteroid shapes and to the flux registered, at the corresponding epochs, by the red and blue photometers (RP and BP). Results. The overall astrometric performance is close to the expectations, with an optimal range of brightness G 12-17. In that range the typical transit-level accuracy is well below 1 milliarcsec (mas). For fainter asteroids, the growing photon noise deteriorates the performance. Asteroids brighter than G = 12 are aff ected by a lower performance of the processing of their signals. The dramatic improvement brought by Gaia DR2 astrometry of SSOs is demonstrated by comparisons to the archive data, and by preliminary tests on the detection of subtle non-gravitational effects.
Note: Reproducció del document publicat a: https://doi.org/10.1051/0004-6361/201832900
It is part of: Astronomy & Astrophysics, 2018, vol. 616, num. A13
URI: http://hdl.handle.net/2445/140071
Related resource: https://doi.org/10.1051/0004-6361/201832900
ISSN: 0004-6361
Appears in Collections:Articles publicats en revistes (Física Quàntica i Astrofísica)

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