The <i>M</i>_BH-<i>M</i>_∗ Relation up to <i>z</i> ∼ 2 through Decomposition of COSMOS-Web NIRCam Images

Our knowledge of relations between supermassive black holes and their host galaxies at z greater than or similar to 1 is still limited, even though being actively sought out to z similar to 6. Here, we use the high resolution and sensitivity of JWST to measure the host galaxy properties for 107 X-ray-selected type-I AGNs at 0.68