James Webb Space Telescope Feed Post

UNCOVER: The growth of the first massive black holes from JWST/NIRSpec -- spectroscopic redshift confirmation of an X-ray luminous AGN at z=10.1

From top-left: NIRSpec/Prism MSA shutter positions for UHZ1 (see § 2), JWST/NIRCam images of UHZ1 in filters F115W, F150W, F200W, F277W, F356, F410M and F444W (photometric measurements from these calibrated data are presented in Fig. 2) and Chandra X-ray images in the 0.5-2 and 2-7 keV bands (smoothed with a 1 pixel width Gaussian filter). JWST cutout images are 1.5'' on a side, Chandra images are 5'' on a side. These are oriented in standard North-East convention. Abstract: The James Webb Space Telescope is now detecting early black holes (BHs) as they transition from "seeds" to supermassive BHs. Recently Bogdan et al. (2023) reported the detection of an X-ray luminous supermassive BH, UHZ-1, with a photometric redshift at z>10. Such an extreme source at this very high redshift provides new insights on seeding and growth models for BHs given the short time available for formation and growth. Harnessing the exquisite sensitivity of JWST/NIRSpec, here we report the spectroscopic confirmation of UHZ-1 at z=10.073±0.002. We find that the NIRSpec/Prism spectrum is typical of recently discovered z~10 galaxies, characterized primarily by star-formation features. We see no clear evidence of the powerful X-ray source in the rest-frame UV/optical spectrum, which may suggest heavy obscuration of the central BH, in line with the Compton-thick column density measured in the X-rays. We perform a stellar population fit simultaneously to the new NIRSpec spectroscopy and previously available photometry. The fit yields a stellar mass estimate for the host galaxy that is significantly better constrained than prior photometric estimates (M*~1.4+0.3-0.4×108M?). Given the predicted BH mass (MBH~107-108M?), the resulting ratio of MBH/M* remains two to three orders of magnitude higher than local values, thus lending support to the heavy seeding channel for the formation of supermassive BHs within the first billion years of cosmic evolution.