An Adolescent, Near-Resonant Planetary System Near the End of Photoevaporation

These datasets include the data that can reproduce the main figures in paper titled: "An Adolescent, Near-Resonant Planetary System Near the End of Photoevaporation". - The CSV files starts with "TESS", "LCO", and "CHEOPS" are the photometric light curves that are used for photodynamical modeling. - The CSV files ends with _atm.csv are the simulated atmospheric evolution of TOI-2076 planets under photoevaporation. First column: log10(time/yr), Second column: planet radius (Earth radii), Third column: Envelope mass fraction (m_env/m_core).