# Galactic astronomy and small telescopes

**Authors:** Toma\v{z} Zwitter

arXiv: 1812.06461 · 2018-12-18

## TL;DR

The paper discusses how small telescopes can complement Gaia's data by conducting ground-based photometric surveys to obtain detailed stellar chemistry, enhancing galactic archaeology efforts.

## Contribution

It introduces a method for small telescopes to measure stellar metallicity and alpha enhancement, complementing Gaia's data for galactic archaeology.

## Key findings

- Small telescopes can measure metallicity and alpha enhancement at ~0.1 dex.
- Ground-based photometric surveys can provide unique chemical information.
- Complementary data enhances understanding of stellar populations.

## Abstract

The second data release of ESA's Gaia satellite (Gaia DR2) revolutionised astronomy by providing accurate distances, proper motions, apparent magnitudes, and in many cases temperatures and radial velocities for an unprecedented number of stars. These new results, which are freely available, need to be considered in virtually any stellar research project, as they provide crucial information on luminosity, position, motion, orbit, and colours of observed targets. Ground-based spectroscopic surveys, like RAVE, Gaia-ESO, Apogee, LAMOST, and GALAH, are adding more measurements of radial velocities and, most importantly, chemistry of stellar atmospheres, including abundances of individual elements. We briefly describe the new information trove, together with some warnings against blind-folded use.   Even though it may seem that Gaia is already providing any information that could be collected by small telescopes, the opposite is true. In particular, we discuss a possible reach of a ground-based photometric survey using a custom filter set. We demonstrate that it can provide valuable information on chemistry of observed stars, which is not provided by Gaia or other sky surveys. A survey conducted with a small telescope has the potential to measure both the metallicity and alpha enhancement at a ~0.1 dex level for a large fraction of Gaia targets, a valuable goal for galactic archaeology.

## Full text

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## Figures

2 figures with captions in the complete paper: https://tomesphere.com/paper/1812.06461/full.md

## References

32 references — full list in the complete paper: https://tomesphere.com/paper/1812.06461/full.md

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Source: https://tomesphere.com/paper/1812.06461