Description
Using data from the James Webb Space Telescope (JWST), the AGN Emission Lines Properties in the JWST-SUSPENSE Ultradeep Spectroscopic Program examines the spectral properties of active galactic nuclei (AGN). The investigation of emission lines, which are essential for understanding the dynamics and environment within AGN, is the primary objective of this work. We intend to classified observed spectral data into AGN, Non-AGN and composite.Then we will investigate the relationship between emission line characteristics and other AGN parameters, including luminosity, redshift, and host galaxy morphology, using the high sensitivity and spectral resolution of JWST. Our research will advance our knowledge of the evolution of AGNs and their function in galaxy formation. The findings, which emphasize the importance of ultradeep spectroscopy in astrophysics research, will be discussed in light of current theoretical models and observational data.
| Stream | Science |
|---|