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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| Autori principali: | , , , , |
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| Natura: | Artigo |
| Lingua: | Inglês |
| Pubblicazione: |
IOP Publishing
2025-01-01
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| Serie: | The Astrophysical Journal Letters |
| Soggetti: | |
| Accesso online: | https://doi.org/10.3847/2041-8213/adb42b |
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