S. S. Antor A. K. Alif · BRAC University
We detect faint exoplanets in JWST/MIRI imagery via contrastive learning, separating planetary signals from bright host stars and recovering 92% of injected planets at a false-positive rate below 0.1 per frame.
Figure 1: JWST/MIRI direct imaging of a faint exoplanet (b).
Real-time co-authoring, instant compiles, every template — free to start.
Already have an account?
By continuing, you agree to our Terms and Privacy Policy.