The VSPEC Collection: A suite of utilities to model spectroscopic phase curves of 3D exoplanet atmospheres in the presence of stellar variability

Ted M Johnson; Cameron Kelahan; Avi M. Mandell; Ashraf Dhahbi; Tobi Hammond; Thomas Barclay; Veselin B. Kostov; Geronimo L. Villanueva

arXiv · 2410.21190

The VSPEC Collection: A suite of utilities to model spectroscopic phase curves of 3D exoplanet atmospheres in the presence of stellar variability

Ted M Johnson·Cameron Kelahan·Avi M. Mandell·Ashraf Dhahbi·Tobi Hammond·Thomas Barclay·Veselin B. Kostov·Geronimo L. Villanueva

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Abstract

We present the Variable Star PhasE Curve (VSPEC) Collection, a set of Python packages for simulating combined-light spectroscopic observations of 3-dimensional exoplanet atmospheres in the presence of stellar variability and inhomogeneity. VSPEC uses the Planetary Spectrum Generator's Global Emission Spectra (PSG/GlobES) application along with a custom-built multi-component time-variable stellar model based on a user-defined grid of stellar photosphere models to produce spectroscopic light curves of the planet-host system. VSPEC can be a useful tool for modeling observations of exoplanets in transiting geometries (primary transit, secondary eclipse) as well as orbital phase curve measurements, and is built in a modular and flexible configuration for easy adaptability to new stellar and planetary model inputs. We additionally present a set of codes developed alongside the core VSPEC modules, including the stellar surface model generator vspec-vsm, the stellar spectral grid interpolation code GridPolator, and a Python interface for PSG, libpypsg.

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Ted M Johnson, Cameron Kelahan, Avi M. Mandell, Ashraf Dhahbi, Tobi Hammond, Thomas Barclay, Veselin B. Kostov, Geronimo L. Villanueva. 2024-10-28. The VSPEC Collection: A suite of utilities to model spectroscopic phase curves of 3D exoplanet atmospheres in the presence of stellar variability. https://arxiv.org/abs/2410.21190

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