Influence of a continuous plane gravitational wave on <i>Gaia</i>-like astrometry

Context. A gravitational wave (GW) passing through an astrometric observer causes periodic shifts of the apparent star positions measured by the observer. For a GW of sufficient amplitude and duration, at a suitable frequency, these shifts might be detected with a Gaia -like astrometric telescope. Aims. This paper is aimed at making a detailed analysis of the effects of GWs on an astrometric solution based on Gaia -like observations, which are one-dimensional and strictly differential between two widely separated fields of view, following a prescribed scanning law. Methods. We present a simple geometric model for the astrometric effects of a plane GW in terms of the time-dependent positional shifts. Using this model, we discuss the general interaction between the GW and a Gaia -like observation. Numerous Gaia -like astrometric solutions have been computed, taking as input simulated observations that include the effects of a continuous plain GW with constant parameters and periods ranging from ~50 days to 100 years. The resulting solutions have been analysed in terms of the systematic errors on astrometric and attitude parameters, as well as the observational residuals. Results. We found that a significant part of the GW signal is absorbed by the astrometric parameters, leading to astrometric errors of a magnitude (in radians) comparable to the strain parameters. These astrometric errors are generally impossible to detect because the true (unperturbed) astrometric parameters are not known with a corresponding level of accuracy. The astrometric errors are especially large for specific GW frequencies that are linear combinations of two characteristic frequencies of the scanning law. Nevertheless, for all GW periods smaller than the time span covered by the observations, significant parts of the GW signal also go into the astrometric residuals. This fosters the hope for a GW detection algorithm based on the residuals of standard Gaia -like astrometric solutions.

Authors

Institutions

Publication Details

Journal
Astronomy and Astrophysics
Published
2025-02-18
DOI
https://doi.org/10.1051/0004-6361/202453545
Citations
1
Primary Topic
Geophysics and Gravity Measurements
Type
article
Field-Weighted Citation Impact
1.79

Funders

Controls
|||
ALL TIME
JAN
FEB
MAR
APR
MAY
JUN
JUL
AUG
SEP
OCT
article

Influence of a continuous plane gravitational wave on Gaia-like astrometry

R. Geyer, Sergei A. Klioner, U. Lammers, L. Lindegren
1 citations
Astronomy and Astrophysics
Geophysics and Gravity Measurements
1.79
article

Influence of a continuous plane gravitational wave on Gaia-like astrometry

R. Geyer, Sergei A. Klioner, U. Lammers, L. Lindegren
article en
1 citations

Abstract

Context. A gravitational wave (GW) passing through an astrometric observer causes periodic shifts of the apparent star positions measured by the observer. For a GW of sufficient amplitude and duration, at a suitable frequency, these shifts might be detected with a Gaia -like astrometric telescope. Aims. This paper is aimed at making a detailed analysis of the effects of GWs on an astrometric solution based on Gaia -like observations, which are one-dimensional and strictly differential between two widely separated fields of view, following a prescribed scanning law. Methods. We present a simple geometric model for the astrometric effects of a plane GW in terms of the time-dependent positional shifts. Using this model, we discuss the general interaction between the GW and a Gaia -like observation. Numerous Gaia -like astrometric solutions have been computed, taking as input simulated observations that include the effects of a continuous plain GW with constant parameters and periods ranging from ~50 days to 100 years. The resulting solutions have been analysed in terms of the systematic errors on astrometric and attitude parameters, as well as the observational residuals. Results. We found that a significant part of the GW signal is absorbed by the astrometric parameters, leading to astrometric errors of a magnitude (in radians) comparable to the strain parameters. These astrometric errors are generally impossible to detect because the true (unperturbed) astrometric parameters are not known with a corresponding level of accuracy. The astrometric errors are especially large for specific GW frequencies that are linear combinations of two characteristic frequencies of the scanning law. Nevertheless, for all GW periods smaller than the time span covered by the observations, significant parts of the GW signal also go into the astrometric residuals. This fosters the hope for a GW detection algorithm based on the residuals of standard Gaia -like astrometric solutions.

Astronomy and AstrophysicsVol. 695
Lund University (SE), European Space Astronomy Centre (ES), Technische Universität Dresden (DE)
European Space Agency, Swedish National Space Agency, Deutsches Zentrum für Luft- und Raumfahrt, Technische Universität Dresden
Openalex Percentile: Top 20%
Geophysics and Gravity Measurements
1.79
AI Navigator

Ask Laika to Summarize, Analyze, and Connect papers live on the map.

Summarize Papers & Methodologies

Extract key findings, datasets, and comparative methods across publications.

Benchmark Rankings & Visual Analytics

Rank top research institutions, authors, funders, topics, and journals by Field-Weighted Citation Impact (FWCI) and paper volume with instant charts.

Connect Distant Disciplines

Bridge topological clusters on the map to find hidden collaborative intersections.