A Galactic-scale extreme-precision radial velocity survey
Abstract
We describe the first Galactic-scale extreme-precision radial velocity (EPRV) survey and outline our goals of measuring Galactic accelerations and deriving constraints on the dark matter distribution in our Galaxy. We are targeting quiet subgiant stars within a kiloparsec in radius of the Sun and about 2 kiloparsec in vertical height relative to the Galactic mid-plane. The observations described here were carried out using the Echelle SPectrograph for Rocky Exoplanets and Stable Spectroscopic Observations (ESPRESSO) at the Very Large Telescope (VLT), between 2021-2025. We began by operating at a typical RV precision of ∼ 70 cm/s to select quiet stars from stellar activity indicators, and are now operating at ∼ 50 cm/s. We selected stars with low stellar jitter (determined from their RV scatter as a function of epoch) with the goal that they yield a measurement of the Galactic acceleration on approximately a decade timescale. We refer to this as our ``gold" sample. We also identify stars with possible companions (either brown dwarfs or planetary companions) or hitherto unknown stellar binaries that we have culled from our survey. For a few cases, we present initial constraints on the companion mass and orbital period. We also present the photospheric and fundamental stellar parameters for our ``gold" sample of sub-giant stars. This first Galactic-scale EPRV survey provides a pathfinder for next-generation surveys with extremely large telescopes, opening the possibility of directly mapping the gravitational acceleration field across the Milky Way and potentially beyond.
Related
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- The GAPS programme at TNG. LXXIX. New mass constraints for the infant planets in the V1298,Tau system through a long-term radial-velocity monitoring with HARPS-N
- The contact frontier in Galactic civilization networks: radial structure and the Galactic habitable zone
BibTeX
@misc{chakrabarti2026galacticscale,
title = {{A Galactic-scale extreme-precision radial velocity survey}},
author = {Sukanya Chakrabarti and Jack Wagner and Robert J. de Rosa and Henrique Reggiani and Jason T. Wright and Peter A. Craig and Jacob K. Luhn and Francesco Pepe and Paul Robertson and Xavier Dumuesque and Massimiliano Bonamente},
howpublished = {arXiv},
year = {2026},
month = sep,
doi = {10.48550/arxiv.2609.23874},
eprint = {2609.23874},
archivePrefix = {arXiv},
url = {https://arxiv.org/abs/2609.23874},
note = {CC BY 4.0},
}
RIS
TY - UNPB
TI - A Galactic-scale extreme-precision radial velocity survey
AU - Sukanya Chakrabarti
AU - Jack Wagner
AU - Robert J. de Rosa
AU - Henrique Reggiani
AU - Jason T. Wright
AU - Peter A. Craig
AU - Jacob K. Luhn
AU - Francesco Pepe
AU - Paul Robertson
AU - Xavier Dumuesque
AU - Massimiliano Bonamente
PY - 2026
DA - 2026/09/20
PB - arXiv
DO - 10.48550/arxiv.2609.23874
UR - https://arxiv.org/abs/2609.23874
AB - We describe the first Galactic-scale extreme-precision radial velocity (EPRV) survey and outline our goals of measuring Galactic accelerations and deriving constraints on the dark matter distribution in our Galaxy. We are targeting quiet subgiant stars within a kiloparsec in radius of the Sun and about 2 kiloparsec in vertical height relative to the Galactic mid-plane. The observations described here were carried out using the Echelle SPectrograph for Rocky Exoplanets and Stable Spectroscopic Observations (ESPRESSO) at the Very Large Telescope (VLT), between 2021-2025. We began by operating at a typical RV precision of ∼ 70 cm/s to select quiet stars from stellar activity indicators, and are now operating at ∼ 50 cm/s. We selected stars with low stellar jitter (determined from their RV scatter as a function of epoch) with the goal that they yield a measurement of the Galactic acceleration on approximately a decade timescale. We refer to this as our ``gold" sample. We also identify stars with possible companions (either brown dwarfs or planetary companions) or hitherto unknown stellar binaries that we have culled from our survey. For a few cases, we present initial constraints on the companion mass and orbital period. We also present the photospheric and fundamental stellar parameters for our ``gold" sample of sub-giant stars. This first Galactic-scale EPRV survey provides a pathfinder for next-generation surveys with extremely large telescopes, opening the possibility of directly mapping the gravitational acceleration field across the Milky Way and potentially beyond.
ER -