We present the study of seven systems, three of which TOI-2295, TOI-2537, and TOI-5110 are newly discovered planetary systems.
TESS
NASA ROSES-24 Amendment 78: D.10 TESS General Investigator Program Final Text and Due Date
The Transiting Exoplanet Survey Satellite (TESS) General Investigator (GI) Program solicits proposals for the acquisition and analysis of scientific data from the TESS mission. The primary purpose of the TESS […]
Hot Neptune TOI-3261 b Is In A Tight Orbit Around Its Host Star
The Discovery A Neptune-sized planet, TOI-3261 b, makes a scorchingly close orbit around its host star. Only the fourth object of its kind ever found, the planet could reveal clues […]
OrCAS: Origins, Compositions, and Atmospheres of Sub-neptunes. I. Survey Definition
Sub-Neptunes – volatile-rich exoplanets smaller than Neptune – are intrinsically the most common type of planet known.
Validating the Orbital Periods of the Coolest TESS Exoplanet Candidates
When an exoplanet passes in front of its host star, the resulting eclipse causes an observable decrease in stellar flux, and when multiple such transits are detected, the orbital period […]
Precise Density Measurement of TOI-1430 b, A Young Planet With An Evaporating Atmosphere
Small-sized exoplanets in tight orbits around young stars (10-1000 Myr) give us the opportunity to investigate the mechanisms that led to their formation, the evolution of their physical and orbital […]
TIDYE-1b Is The Youngest Transiting Planet Yet Discovered
University of North Carolina at Chapel Hill researchers have made an exciting discovery of a 3-million-year-old planet, TIDYE-1b – on a human scale, the equivalent in age to a two-week-old […]
Preparing For The Early eVolution Explorer
Ultraviolet flare emission can drive photochemistry in exoplanet atmospheres and even serve as the primary source of uncertainty in atmospheric retrievals. Additionally, flare energy budgets are not well-understood due to […]
Gl 725A b: A Potential Super-Earth Detected With SOPHIE and SPIRou In An M Dwarf Binary System At 3.5 pc
We report the discovery of a super-Earth candidate orbiting the nearby mid M dwarf Gl 725A using the radial velocity (RV) method.
Examining The Rotation Of The Planet-hosting M Dwarf GJ 3942
Based on radial velocities, EXORAP photometry, and activity indicators, the HADES team reported a 16.3-day rotation period for the M dwarf GJ 3992. However, an RV–Hα magnitude-squared coherence estimate has […]
