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dc.contributor.authorSpoto, F
dc.contributor.authorTanga, P
dc.contributor.authorMignard, F
dc.contributor.authorBerthier, J
dc.contributor.authorCarry, B
dc.contributor.authorCellino, A
dc.contributor.authorDell'Oro, A
dc.contributor.authorHestroffer, D
dc.contributor.authorMuinonen, K
dc.contributor.authorPauwels, T
dc.contributor.authorPetit, JM
dc.contributor.authorDavid, P
dc.contributor.authorDe Angeli, Francesca
dc.contributor.authorDelbo, M
dc.contributor.authorFrézouls, B
dc.contributor.authorGalluccio, L
dc.contributor.authorGranvik, M
dc.contributor.authorGuiraud, J
dc.contributor.authorHernández, J
dc.contributor.authorOrdénovic, C
dc.contributor.authorPortell, J
dc.contributor.authorPoujoulet, E
dc.contributor.authorThuillot, W
dc.contributor.authorWalmsley, G
dc.contributor.authorBrown, AGA
dc.contributor.authorVallenari, A
dc.contributor.authorPrusti, T
dc.contributor.authorDe Bruijne, JHJ
dc.contributor.authorBabusiaux, C
dc.contributor.authorBailer-Jones, CAL
dc.contributor.authorBiermann, M
dc.contributor.authorEvans, Dafydd
dc.contributor.authorEyer, L
dc.contributor.authorJansen, F
dc.contributor.authorJordi, C
dc.contributor.authorKlioner, SA
dc.contributor.authorLammers, U
dc.contributor.authorLindegren, L
dc.contributor.authorLuri, X
dc.contributor.authorPanem, C
dc.contributor.authorPourbaix, D
dc.contributor.authorRandich, S
dc.contributor.authorSartoretti, P
dc.contributor.authorSiddiqui, HI
dc.contributor.authorSoubiran, C
dc.contributor.authorvan Leeuwen, Floor
dc.contributor.authorWalton, Nicholas
dc.contributor.authorArenou, F
dc.contributor.authorBastian, U
dc.contributor.authorCropper, M
dc.contributor.authorDrimmel, R
dc.contributor.authorKatz, D
dc.contributor.authorLattanzi, MG
dc.contributor.authorBakker, J
dc.contributor.authorCacciari, C
dc.contributor.authorCastañeda, J
dc.contributor.authorChaoul, L
dc.contributor.authorCheek, N
dc.contributor.authorFabricius, C
dc.contributor.authorGuerra, R
dc.contributor.authorHoll, B
dc.contributor.authorMasana, E
dc.contributor.authorMessineo, R
dc.contributor.authorMowlavi, N
dc.contributor.authorNienartowicz, K
dc.contributor.authorPanuzzo, P
dc.contributor.authorRiello, Marco
dc.contributor.authorSeabroke, GM
dc.contributor.authorThévenin, F
dc.contributor.authorGracia-Abril, G
dc.contributor.authorComoretto, G
dc.contributor.authorGarcia-Reinaldos, M
dc.contributor.authorTeyssier, D
dc.contributor.authorAltmann, M
dc.contributor.authorAndrae, R
dc.contributor.authorAudard, M
dc.contributor.authorBellas-Velidis, I
dc.contributor.authorBenson, K
dc.contributor.authorBlomme, R
dc.contributor.authorBurgess, Patrick
dc.contributor.authorBusso, Giorgia
dc.contributor.authorClementini, G
dc.contributor.authorClotet, M
dc.contributor.authorCreevey, O
dc.contributor.authorDavidson, M
dc.contributor.authorDe Ridder, J
dc.contributor.authorDelchambre, L
dc.contributor.authorDucourant, C
dc.contributor.authorFernández-Hernández, J
dc.contributor.authorFouesneau, M
dc.contributor.authorFrémat, Y
dc.contributor.authorGarcía-Torres, M
dc.date.accessioned2018-09-19T11:12:11Z
dc.date.available2018-09-19T11:12:11Z
dc.date.issued2018-08-10
dc.identifier.issn1432-0746
dc.identifier.urihttps://www.repository.cam.ac.uk/handle/1810/280343
dc.description.abstractContext. The Gaia spacecraft of the European Space Agency (ESA) has been securing observations of solar system objects (SSOs) since the beginning of its operations. Data Release 2 (DR2) contains the observations of a selected sample of 14,099 SSOs. These asteroids have been already identified and have been 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 describe the criteria we used to select the sample published in 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, which is the 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. When this aspect is handled appropriately, an orbit fit can be obtained with post-fit residuals that are overall consistent with the a-priori error model that was used to define individual values of the astrometric uncertainty. The role of both random and systematic errors is described. The distribution of residuals allowed us to identify possible contaminants in the data set (such as stars). Photometry in the G band was 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 this range, the typical transit-level accuracy is well below 1 mas. For fainter asteroids, the growing photon noise deteriorates the performance. Asteroids brighter than G ∼ 12 are affected 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.
dc.description.sponsorshipMultiple funders, including STFC, ERC and Horizon 2020.
dc.publisherEDP Sciences
dc.rightsAttribution 4.0 International
dc.rights.urihttp://creativecommons.org/licenses/by/4.0/
dc.subjectastrometry
dc.subjectminor planets, asteroids: general
dc.subjectmethods: data analysis
dc.subjectspace vehicles: instruments
dc.titleObservations of solar system objects
dc.typeArticle
prism.numberA13
prism.publicationNameAstronomy & Astrophysics
prism.volume616
dc.identifier.doi10.17863/CAM.27713
dcterms.dateAccepted2018-04-10
rioxxterms.versionofrecord10.1051/0004-6361/201832900
rioxxterms.versionVoR
rioxxterms.licenseref.urihttp://creativecommons.org/licenses/by/4.0/
rioxxterms.licenseref.startdate2018-04-10
dc.contributor.orcidEvans, Dafydd [0000-0002-6685-5998]
dc.contributor.orcidvan Leeuwen, Floor [0000-0003-1781-4441]
dc.contributor.orcidWalton, Nicholas [0000-0003-3983-8778]
dc.contributor.orcidRiello, Marco [0000-0002-3134-0935]
dc.identifier.eissn1432-0746
rioxxterms.typeJournal Article/Review
pubs.funder-project-idSTFC (ST/K000756/1)
pubs.funder-project-idSTFC (ST/N000641/1)
pubs.funder-project-idSTFC (PP/D006546/1)
pubs.funder-project-idSTFC (ST/I000542/1)
pubs.funder-project-idSTFC (ST/J005045/1)
pubs.funder-project-idPPARC (PP/C000757/1)
pubs.funder-project-idScience and Technology Facilities Council (ST/L006553/1)
pubs.funder-project-idSTFC (ST/P000975/1)
pubs.funder-project-idSTFC (ST/S000089/1)
pubs.funder-project-idScience and Technology Facilities Council (ST/N000927/1)
pubs.funder-project-idEuropean Commission (264895)
pubs.funder-project-idEuropean Research Council (320360)
pubs.funder-project-idEuropean Commission (606740)
cam.issuedOnline2018-08-10


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Attribution 4.0 International
Except where otherwise noted, this item's licence is described as Attribution 4.0 International