Hubble Space Telescope observations of the Kepler-field cluster NGC 6819. I. The bottom of the white dwarf cooling sequence

TL;DR

This study uses Hubble Space Telescope observations to determine the white dwarf cooling sequence in NGC 6819, deriving an age consistent with main-sequence turn-off estimates and providing valuable high-resolution data for the Kepler field.

Contribution

First detailed measurement of the white dwarf cooling sequence in NGC 6819 using HST, confirming cluster age and releasing comprehensive source catalogues for the Kepler field.

Findings

White dwarf cooling sequence drops sharply at mF606W=26.05

Cluster age estimated at 2.25 Gyr from WD cooling sequence

High-resolution images and catalogs released for Kepler field

Abstract

We use Hubble Space Telescope (HST) to reach the end of the white dwarf (WD) cooling sequence (CS) in the solar-metallicity open cluster NGC 6819. Our photometry and completeness tests show a sharp drop in the number of WDs along the CS at magnitudes fainter than mF606W = 26.050+/- 0.075. This implies an age of 2.25+/-0.20 Gyr, consistent with the age of 2.25+/-0.30 Gyr obtained from fits to the main-sequence turn-off. The use of different WD cooling models and initial-final-mass relations have a minor impact the WD age estimate, at the level of ~0.1 Gyr. As an important by-product of this investigation we also release, in electronic format, both the catalogue of all the detected sources and the atlases of the region (in two filters). Indeed, this patch of sky studied by HST (of size ~70 arcmin sq.) is entirely within the main Kepler-mission field, so the high-resolution images and deep catalogues will be particularly useful.