Name: GaiaNIR: next astrometric mission
Start: 2024-01-17T09:30:00+01:00
End: 2024-01-18T13:00:00+01:00
Location: Bologna, OAS

A new golden age for the proper motion anomaly technique with Gaia-NIR

Cepheids and RR Lyrae in the Gaia-NIR perspective

Characterization and occurrence rate of Jupiter and Saturn analogs to assess their impact on the formation of small and terrestrial inner planets. The crucial role of Gaia-NIR

Characterizing of long-period exoplanets with radial velocities and present and future high-precision astrometry

Discussion: Next steps & Actions

Discussion: Next steps & Actions-Part II

Euclid Early Release Observations - first results on Milky Way globular clusters

Exoplanet Demographics

From Gaia to Gaia-NIR: the INAF and Italian technological contribution.

Gaia Fireworks: the impact of Gaia on Eruptive Accretion and the crucial role of NIR-Gaia

Gaia-NIR: next astrometric mission

GaiaNIR: a pathway to the dark side of the Milky Way

Goal of the meeting

Low-mass young stellar populations in the Milky Way: the next frontier with Gaia NIR

Microlensing with exquisite astrometry

Revealing the disc of the Milky Way with Gaia NIR

Synergies with JWST/WFIRST

Synergies with LSST

Synergies with space-based transit surveys

The RR Lyrae in the disc as an interesting GAIA NIR scientific case.

The Gaia legacy: Gravitation and multi-messenger astronomy with Gaia NIR

The photometric heritage of Gaia missions

The structure and dynamics of ISM: spiral arms, molecular clouds and the earliest formation of stellar clusters.

The young supermassive star clusters: an opportunity to study stars and planets formation in starburst

Towards the innermost boundaries of the Galactic disc

Unveiling free-floating binary planets with Gaia-NIR astrometry

Unveiling the initial stages of star formation with Gaia-NIR

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GaiaNIR: next astrometric mission

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GaiaNIR: next astrometric mission

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