pith:6ZY4U7GG
The NUV transit of XO-3 b
NUV transit of hot Jupiter XO-3b is 30-70% deeper than optical and arrives 22 minutes late.
arxiv:2605.05068 v2 · 2026-05-06 · astro-ph.EP
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Claims
We find a NUV transit depth of Rp,NUV/R⋆ = 0.1371+0.016−0.019, which is 30-70% deeper than the optical transit. The transit center in the NUV is 22+13−11 minutes late compared to the optical ephemeris.
That the observed NUV depth increase and late timing offset arise from atmospheric or bow-shock effects, given that the derived mass-loss rate is extremely small (~10^4 g/s) and the analytic magnetic model predicts an early rather than late transit.
XO-3 b exhibits a 30-70% deeper NUV transit depth of 0.1371 and a 22-minute late center relative to the optical ephemeris, with an extremely low estimated mass-loss rate and a bow-shock model that predicts the opposite timing direction.
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| First computed | 2026-05-25T02:01:21.773281Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
f671ca7cc65e07a60069df4c931cd52c783316584a784af9f03df79f0b6e5cb0
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Canonical record JSON
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