# A ground-based NUV secondary eclipse observation of KELT-9b

## TL;DR

This study used a ground-based telescope to observe the secondary eclipse of exoplanet KELT-9b in the near-ultraviolet, constraining its atmospheric temperature and albedo despite not detecting the eclipse signal.

## Contribution

First ground-based NUV secondary eclipse observation of KELT-9b, providing constraints on its atmospheric properties and demonstrating the feasibility of such studies from Earth.

## Key findings

- No eclipse detection, upper limit of 181 ppm on depth.
- Dayside temperature constrained to 4995 K at ~30 mbar pressure.
- Albedo likely very low, consistent with similar hot Jupiters.

## Abstract

KELT-9b is a recently discovered exoplanet with a 1.49 d orbit around a B9.5/A0-type star. The unparalleled levels of UV irradiation it receives from its host star put KELT-9b in its own unique class of ultra-hot Jupiters, with an equilibrium temperature > 4000 K. The high quantities of dissociated hydrogen and atomic metals present in the dayside atmosphere of KELT-9b bear more resemblance to a K-type star than a gas giant. We present a single observation of KELT-9b during its secondary eclipse, taken with the Wide Field Camera on the Isaac Newton Telescope (INT). This observation was taken in the U-band, a window particularly sensitive to Rayleigh scattering. We do not detect a secondary eclipse signal, but our 3$\sigma$ upper limit of 181 ppm on the depth allows us to constrain the dayside temperature of KELT-9b at pressures of ~30 mbar to 4995 K (3$\sigma$). Although we can place an observational constraint of $A_g<$ 0.14, our models suggest that the actual value is considerably lower than this due to H$^-$ opacity. This places KELT-9b squarely in the albedo regime populated by its cooler cousins, almost all of which reflect very small components of the light incident on their daysides. This work demonstrates the ability of ground-based 2m-class telescopes like the INT to perform secondary eclipse studies in the NUV, which have previously only been conducted from space-based facilities.