A Long Spin Period for a Sub-Neptune-mass Exoplanet

A Long Spin Period for a Sub-Neptune-mass Exoplanet

HIP 41378 f is a sub-Neptune exoplanet with an anomalously low density. Its long orbital period and deep transit make it an ideal candidate for detecting oblateness photometrically. We present a new cross-platform, GPU-enabled code, greenlantern , suitable for computing transit light curves of oblat...

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Bibliographic Details
Main Authors: Ellen M. Price, Juliette Becker, Zoë L. de Beurs, Leslie A. Rogers, Andrew Vanderburg
Format: Article
Language:English
Published: IOP Publishing 2025-01-01
Series:The Astrophysical Journal Letters
Subjects:
Oblateness
Exoplanet systems
Open source software
Online Access:https://doi.org/10.3847/2041-8213/adb42b
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