email: akhil.krishna@iiap.res.in
Feel free to reach out if you have any ideas on how we can use UVIT to study specific phenomena.
Bright PAH emission regions were identified in the JWST images, and their corresponding UV emission was estimated using the UVIT images. We quantified the star formation properties of these PAH-emitting regions using the UVIT images.
More updates are coming soon.