# Time-Series Analysis of Broadband Photometry of Neptune from K2

## TL;DR

This study analyzed nearly continuous 49-day broadband photometry of Neptune from the K2 mission to detect intrinsic global oscillations, developing new correction methods and finding no evidence of such oscillations within the sensitivity limits.

## Contribution

The paper introduces new techniques to correct for instrumental effects in K2 photometry and applies them to search for planetary oscillations in Neptune, setting upper limits on detectable signals.

## Key findings

- No evidence of Neptune's global oscillations was found.
- The photometric precision was sufficient to detect signals down to ~5 ppm at 1000 μHz.
- Reflected sunlight and atmospheric variability dominate the observed photometric signals.

## Abstract

We report here on our search for excess power in photometry of Neptune collected by the K2 mission that may be due to intrinsic global oscillations of the planet Neptune. To conduct this search, we developed new methods to correct for instrumental effects such as intrapixel variability and gain variations. We then extracted and analyzed the time-series photometry of Neptune from 49 days of nearly continuous broadband photometry of the planet. We find no evidence of global oscillations and place an upper limit of $\sim$5 ppm at 1000 \uhz\ for the detection of a coherent signal. With an observed cadence of 1-minute and point-to-point scatter less than 0.01\%, the photometric signal is dominated by reflected light from the Sun, which is in turn modulated by atmospheric variability of Neptune at the 2\% level. A change in flux is also observed due to the increasing distance between Neptune and the K2 spacecraft, and solar variability with convection-driven solar p modes present.