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Gaia Early Data Release 3 : Modelling and calibration of Gaia 's point and line spread functions

Rowell, N. ; Davidson, M. ; Lindegren, L. LU orcid ; Van Leeuwen, F. ; Castañeda, J. ; Fabricius, C. ; Bastian, U. ; Hambly, N. C. ; Hernández, J. and Bombrun, A. , et al. (2021) In Astronomy and Astrophysics 649.
Abstract

Context. The unprecedented astrometric precision of the Gaia mission relies on accurate estimates of the locations of sources in the Gaia data stream. This is ultimately performed by point spread function (PSF) fitting, which in turn requires an accurate reconstruction of the PSF, including calibrations of all the major dependences. These include a strong colour dependence due to Gaia's broad G band and a strong time dependence due to the evolving contamination levels and instrument focus. Accurate PSF reconstruction is also important for photometry. Gaia Early Data Release 3 (EDR3) will, for the first time, use a PSF calibration that models several of the strongest dependences, leading to signficantly reduced systematic errors. Aims.... (More)

Context. The unprecedented astrometric precision of the Gaia mission relies on accurate estimates of the locations of sources in the Gaia data stream. This is ultimately performed by point spread function (PSF) fitting, which in turn requires an accurate reconstruction of the PSF, including calibrations of all the major dependences. These include a strong colour dependence due to Gaia's broad G band and a strong time dependence due to the evolving contamination levels and instrument focus. Accurate PSF reconstruction is also important for photometry. Gaia Early Data Release 3 (EDR3) will, for the first time, use a PSF calibration that models several of the strongest dependences, leading to signficantly reduced systematic errors. Aims. We describe the PSF model and calibration pipeline implemented for Gaia EDR3, including an analysis of the calibration results over the 34 months of data. We include a discussion of the limitations of the current pipeline and directions for future releases. This will be of use both to users of Gaia data and as a reference for other precision astrometry missions. Methods. We develop models of the 1D line spread function (LSF) and 2D PSF profiles based on a linear combination of basis components. These are designed for flexibility and performance, as well as to meet several mathematical criteria such as normalisation. We fit the models to selected primary sources in independent time ranges, using simple parameterisations for the colour and other dependences. Variation in time is smoothed by merging the independent calibrations in a square root information filter, with resets at certain mission events that induce a discontinuous change in the PSF. Results. The PSF calibration shows strong time and colour dependences that accurately reproduce the varying state of the Gaia astrometric instrument. Analysis of the residuals reveals both the performance and the limitations of the current models and calibration pipeline, and indicates the directions for future development. Conclusions. The PSF modelling and calibration carried out for Gaia EDR3 represents a major step forwards in the data processing and will lead to reduced systematic errors in the core mission data products. Further significant improvements are expected in the future data releases.

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type
Contribution to journal
publication status
published
subject
keywords
Instrumentation: detectors, Methods: data analysis, Space vehicles: instruments
in
Astronomy and Astrophysics
volume
649
article number
A11
publisher
EDP Sciences
external identifiers
  • scopus:85104945749
ISSN
0004-6361
DOI
10.1051/0004-6361/202039448
language
English
LU publication?
yes
additional info
Publisher Copyright: © ESO 2021.
id
9ba39058-76d4-4967-9b5e-06fcbcb97d83
date added to LUP
2022-01-27 10:13:30
date last changed
2024-04-20 19:31:39
@article{9ba39058-76d4-4967-9b5e-06fcbcb97d83,
  abstract     = {{<p>Context. The unprecedented astrometric precision of the Gaia mission relies on accurate estimates of the locations of sources in the Gaia data stream. This is ultimately performed by point spread function (PSF) fitting, which in turn requires an accurate reconstruction of the PSF, including calibrations of all the major dependences. These include a strong colour dependence due to Gaia's broad G band and a strong time dependence due to the evolving contamination levels and instrument focus. Accurate PSF reconstruction is also important for photometry. Gaia Early Data Release 3 (EDR3) will, for the first time, use a PSF calibration that models several of the strongest dependences, leading to signficantly reduced systematic errors. Aims. We describe the PSF model and calibration pipeline implemented for Gaia EDR3, including an analysis of the calibration results over the 34 months of data. We include a discussion of the limitations of the current pipeline and directions for future releases. This will be of use both to users of Gaia data and as a reference for other precision astrometry missions. Methods. We develop models of the 1D line spread function (LSF) and 2D PSF profiles based on a linear combination of basis components. These are designed for flexibility and performance, as well as to meet several mathematical criteria such as normalisation. We fit the models to selected primary sources in independent time ranges, using simple parameterisations for the colour and other dependences. Variation in time is smoothed by merging the independent calibrations in a square root information filter, with resets at certain mission events that induce a discontinuous change in the PSF. Results. The PSF calibration shows strong time and colour dependences that accurately reproduce the varying state of the Gaia astrometric instrument. Analysis of the residuals reveals both the performance and the limitations of the current models and calibration pipeline, and indicates the directions for future development. Conclusions. The PSF modelling and calibration carried out for Gaia EDR3 represents a major step forwards in the data processing and will lead to reduced systematic errors in the core mission data products. Further significant improvements are expected in the future data releases. </p>}},
  author       = {{Rowell, N. and Davidson, M. and Lindegren, L. and Van Leeuwen, F. and Castañeda, J. and Fabricius, C. and Bastian, U. and Hambly, N. C. and Hernández, J. and Bombrun, A. and Evans, D. W. and De Angeli, F. and Riello, M. and Busonero, D. and Crowley, C. and Mora, A. and Lammers, U. and Gracia, G. and Portell, J. and Biermann, M. and Brown, A. G.A.}},
  issn         = {{0004-6361}},
  keywords     = {{Instrumentation: detectors; Methods: data analysis; Space vehicles: instruments}},
  language     = {{eng}},
  month        = {{05}},
  publisher    = {{EDP Sciences}},
  series       = {{Astronomy and Astrophysics}},
  title        = {{Gaia Early Data Release 3 : Modelling and calibration of Gaia 's point and line spread functions}},
  url          = {{http://dx.doi.org/10.1051/0004-6361/202039448}},
  doi          = {{10.1051/0004-6361/202039448}},
  volume       = {{649}},
  year         = {{2021}},
}