High-resolution M-band spectroscopy detects super-stellar SiO in TWA 5 B, implying no significant magnesium-silicate clouds and formation consistent with core accretion beyond the CO snowline or gravitational instability with solid enrichment.
W., Foreman-Mackey, D., Montet, B
2 Pith papers cite this work. Polarity classification is still indexing.
2
Pith papers citing it
fields
astro-ph.EP 2years
2026 2verdicts
UNVERDICTED 2representative citing papers
Generative spectral decomposition on NEID solar data recovers 238 of 500 injected planets (including 13 with K<0.3 m/s) versus 9 for traditional CCF detrending in calibrated injection-recovery tests.
citing papers explorer
-
The CRIMSON survey I: super-stellar SiO in the directly imaged companion TWA 5 B from high-resolution M-band spectroscopy
High-resolution M-band spectroscopy detects super-stellar SiO in TWA 5 B, implying no significant magnesium-silicate clouds and formation consistent with core accretion beyond the CO snowline or gravitational instability with solid enrichment.
-
AESTRA II: Generative Spectral Modeling of the Sun as a Star for Precise Radial Velocities
Generative spectral decomposition on NEID solar data recovers 238 of 500 injected planets (including 13 with K<0.3 m/s) versus 9 for traditional CCF detrending in calibrated injection-recovery tests.