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Gaia Data Release 3: Gaia scan-angle-dependent signals and spurious periods

Authors :
Holl, Berry
Fabricius, Claus
Portell, Jordi
Lindegren, Lennart
Panuzzo, Pasquale
Bernet, M.
Castañeda, Javier
Jevardat De Fombelle, Grégory
Audard, Marc
Ducourant, Christine
Harrison, D.L.
Evans, Dafydd D.W.
Busso, Giorgia
Sozzetti, Alessandro
Gosset, Eric
Arenou, F.
De Angeli, Francesca
Riello, Marco
Eyer, Laurent
Rimoldini, Lorenzo
Gavras, Panagiotis
Mowlavi, Nami
Nienartowicz, Krzysztof
Lecoeur-Taibi, Isabelle
García-Lario, Pedro
Pourbaix, Dimitri
Holl, Berry
Fabricius, Claus
Portell, Jordi
Lindegren, Lennart
Panuzzo, Pasquale
Bernet, M.
Castañeda, Javier
Jevardat De Fombelle, Grégory
Audard, Marc
Ducourant, Christine
Harrison, D.L.
Evans, Dafydd D.W.
Busso, Giorgia
Sozzetti, Alessandro
Gosset, Eric
Arenou, F.
De Angeli, Francesca
Riello, Marco
Eyer, Laurent
Rimoldini, Lorenzo
Gavras, Panagiotis
Mowlavi, Nami
Nienartowicz, Krzysztof
Lecoeur-Taibi, Isabelle
García-Lario, Pedro
Pourbaix, Dimitri
Source :
Astronomy & astrophysics, 674
Publication Year :
2023

Abstract

Context. Gaia Data Release 3 (Gaia DR3) time series data may contain spurious signals related to the time-dependent scan angle. Aims. We aim to explain the origin of scan-angle-dependent signals and how they can lead to spurious periods, provide statistics to identify them in the data, and suggest how to deal with them in Gaia DR3 data and in future releases. Methods. Using real Gaia (DR3) data alongside numerical and analytical models, we visualise and explain the features observed in the data. Results. We demonstrated with Gaia (DR3) data that source structure (multiplicity or extendedness) or pollution from close-by bright objects can cause biases in the image parameter determination from which photometric, astrometric, and (indirectly) radial velocity time series are derived. These biases are a function of the time-dependent scan direction of the instrument and thus can introduce scan-angle-dependent signals, which due to the scanning-law-induced sampling of Gaia can result in specific spurious periodic signals. Numerical simulations in which a period search is performed on Gaia time series with a scan-angle-dependent signal qualitatively reproduce the general structure observed in the spurious period distribution of photometry and astrometry, and the associated spatial distributions on the sky. A variety of statistics allows for the deeper understanding and identification of affected sources. Conclusions. The origin of the scan-angle-dependent signals and subsequent spurious periods is well understood and is mostly caused by fixed-orientation optical pairs with a separation < 0.5'' (including binaries with P ≈ 5 y) and (cores of) distant galaxies. Although most of the sources with affected derived parameters have been filtered out from the Gaia archive nss-two-body-orbit and several vari-tables, Gaia DR3 data remain that should be treated with care (no sources were filtered from gaia-source). Finally, the various statistics discussed in the paper can be used to<br />SCOPUS: ar.j<br />info:eu-repo/semantics/published

Details

Database :
OAIster
Journal :
Astronomy & astrophysics, 674
Notes :
1 full-text file(s): application/pdf, English
Publication Type :
Electronic Resource
Accession number :
edsoai.on1435876675
Document Type :
Electronic Resource