Skip to content
Review Open access

Predictions for astrometric microlensing in Gaia

Sep 2026 · Astronomy & Astrophysics · 0 citations · 6 references
Physics

Abstract

Gaia, the European Space Agency's astrometric mission, is uniquely positioned for microlensing studies thanks to its all-sky coverage and simultaneous astrometric and photometric observations. In Gaia Data Release 4 (DR4), astrometric time series will be published for the first time, providing a rich dataset for isolated stellar remnant searches. In anticipation of Gaia DR4, we have prepared tools for fitting photometric and one-dimensional astrometric measurements. We tested the recovery of true event parameters and population distributions with Gaia-like observations. We created a mock survey of microlensing events mirroring Gaia DR4's survey design. The events were generated using dedicated Galactic simulations to provide realistic expectations on stellar and dark lens yields. For selected events, we simulated observations following Gaia's scanning law and precision using the astromet package. Such simulations are needed to interpret forthcoming data ( i.e. to update Galactic models to match observed populations ) . They also enable testing of inference tools with known ground truth. We used nested sampling to infer full posterior distributions and compared them with the true lens parameters. Our simulation predicts 322 ± 70 microlensing events with astrometric signals above Gaia precision thresholds. Of these, 209 ± 57 have detectable photometric signals . Among the astrometric and astrometric+photometric events, 82 ± 9 and 49 ± 7 , respectively, have remnant lenses. To assess Gaia's capabilities in constraining remnant mass distributions, we modelled all remnant lens events with detectable astrometric and photometric signals. We recovered the true Einstein times (t_̊m E) and radii ( E) for most events. Microlensing parallax (π_̊m E) measurements are consistent with true values but uncertain, thus limiting mass determination. We recommend focusing on events with bright sources or anomalous five-parameter fits to optimise dark lens searches. We make available the mock Gaia time series dataset as well as a toolkit repository for working with the Gaia data format, fitting models, and visualising results.

Read PDF

Similar papers

Sep 2026

Probing extended dark objects through astrometric microlensing from Gaia

We present the first comprehensive study of astrometric microlensing by extended dark objects, focusing on two theoretically motivated models — Q-ball and boson star. We demonstrate that these extended objects generate distinctive signatures that depart markedly from point-mass lenses like primordial black holes. The s...

Lalit Singh Bhandari, Vikram Rentala, Arun M. Thalapillil et al. · 0 citations
Review Open access Sep 2026

A pilot study on the astrometric capability of CSST. Detecting astrometric binaries with Gaia synergy via simulated data

The China Space-station Survey Telescope (CSST) will provide deep, wide-field epoch astrometry over its 10-year mission. Accurate recovery of binary orbits requires both high-precision astrometry and sufficient orbital-phase coverage, enabling dynamical constraints on the masses of stellar and compact-object companions...

Shang-Yu Wen, Shi-Long Liao, Zhao-Xiang Qi et al. · 0 citations
Aug 2026

GECO: the galactic and extragalactic compact-object observatory

GECO is a mission concept recently proposed in response to a Small National Mission call jointly issued by INAF and ASI for a fast-track space mission, including a scientific payload not in excess of 100 kg and technologies with TRL ≥5. Launch of the selected mission is anticipated around 2033. GECO proposes an unprece...

M. Feroci, R. Campana, A. De Rosa et al. · 0 citations
Open access Aug 2026

Gaia DR3 Limits on Stellar Engine Technosignatures in Nearby Stars

An operating stellar engine that transfers momentum to its host star could produce an approximately persistent transverse acceleration during the Gaia Data Release 3 (DR3) observing epoch. We ask how common such stellar-engine-like accelerations could be among nearby stars. We define a quality-selected parent populatio...

Bo-Lun Huang, Z. Tao, Tong-Jie Zhang et al. · 0 citations
Review Open access Sep 2026

Euclid preparation. CXIII. Simulated galaxy catalogues for non-standard cosmological models

Stage-IV galaxy surveys will provide the opportunity to test cosmological models and the underlying theory of gravity with unparalleled precision. In this context, it is crucial for the Euclid mission to leverage its spectroscopic and photometric probes to systematically investigate and incorporate non-standard cosmolo...

M.-A. Breton, P. Fosalba, S. Ávila et al. · 0 citations
Preprint Sep 2026

Companion masses of Gaia DR3 AstroSpectroSB1 binaries: a Bayesian forward-modelling framework

Gaia Data Release 3 (DR3) has substantially expanded the study of unresolved binaries by providing combined astrometric and spectroscopic orbital solutions for a large sample of non-single stars. We present a Bayesian forward-modelling framework for estimating companion masses in Gaia DR3 \texttt{AstroSpectroSB1} syste...

Prasid Sandave, Raghuveer Garani · 0 citations

We use cookies to run the site and, with your consent, for analytics and to show ads. See our Cookie Policy.