12-24-2025, 08:40 PM
I'm an astronomy graduate student focusing on exoplanet detection methods, and I'm analyzing data from a transit survey that has several promising candidate signals. I'm currently working through the process of ruling out false positives like eclipsing binaries, which is more complex than I anticipated. For researchers experienced with transit photometry, what specific statistical tools or follow-up observation strategies (like radial velocity or high-resolution imaging) have you found most critical for confidently validating a terrestrial-sized exoplanet candidate in a crowded stellar field?