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Table · dataset · 2026

Transit light curves of NGTS-5b

Listed in IVOA Registry (Virtual Observatory)

Transmission spectroscopy serves as a valuable tool for probing atmospheric absorption features in the terminator regions of exoplanets.

Description

Stellar surface heterogeneity can introduce wavelength-dependent contamination that complicates the interpretation of planetary spectra. We aim to investigate the atmosphere of the warm sub-Saturn NGTS-5b through optical transmission spectroscopy.

Two transits were observed with the low-resolution Optical System for Imaging and low-Intermediate-Resolution Integrated Spectroscopy (OSIRIS) on the 10.4 m Gran Telescopio Canarias (GTC). Chromatic transit light curves were modeled to derive optical transmission spectra, and multiple Bayesian spectral retrievals were performed to characterize the atmospheric properties. Model comparisons provide strong evidence for contamination from unocculted stellar spots.

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A joint retrieval of the transmission spectra, assuming equilibrium chemistry, indicates a relatively clear atmosphere with a subsolar C/O ratio of <0.22 (90% upper limit) and a low metallicity of 0.10^+0.34^_-0.05_solar. Retrievals assuming free chemistry yield strong evidence for the presence of H_2_O, with its abundance constrained to X_H2O_=-0.79^+0.14^_-0.17_. However, the abundances of other species remain unconstrained due to limited optical wavelength coverage.

The discrepancies between the two NGTS-5b transit spectra can be attributed to varying levels of stellar contamination. NGTS-5b thus appears to host a relatively clear, water-rich atmosphere, pending confi

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IVOA Registry (Virtual Observatory)ivo://cds.vizier/j/a+a/707/a3159 d agoJSON v1
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concepts[modality].local:modality:imagingenrichment · IVOA Registrykeyword-concept-rules@1.0.0title+description (75%)
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