ASCL Code Record
[ascl:2504.013]
VSPEC: Variable Star PhasE Curve
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Johnson, Ted M.; Kelahan, Cameron; Mandell, Avi M.; Dhahbi, Ashraf; Hammond, Tobi; Barclay, Thomas; Kostov, Veselin B.; Villanueva, Geronimo L.
VSPEC (Variable Star PhasE Curve) simulates exoplanet observations. It combines NASA’s Planetary Spectrum Generator (PSG) with a custom variable star model. Originally built to simulate the infrared excess of non-transiting planets, VSPEC supports transit, eclipse, phase curve geometries as well as spots, faculae, flares, granulation, and the transit light source effect.
- Code site:
- https://github.com/VSPEC-collab/VSPEC
- Described in:
- https://ui.adsabs.harvard.edu/abs/2025A%2526C....5000890J
- EMAC link:
- https://emac.gsfc.nasa.gov/?cid=2401-001
- Bibcode:
- 2025ascl.soft04013J
- Preferred citation method:
- https://ui.adsabs.harvard.edu/abs/2025A%2526C....5000890J ; also see https://github.com/VSPEC-collab/VSPEC/blob/main/CITATION.cff
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