Deciphering the JWST Spectrum of a 'little Red Dot' at Z ∼ 4.53: an Obscured AGN and Its Star-Forming Host

JWST has revealed a class of numerous, extremely compact sources with rest-frame red optical/near-infrared (NIR) and blue ultraviolet (UV) colours nicknamed 'little red dots'. We present one of the highest signal-to-noise ratio JWST NIRSpec prism spectra of a little red dot, J0647_1045 at z = 4.5319 +/- 0.0001, and examine its NIRCam morphology to differentiate the origin of the UV and optical/NIR emission and elucidate the nature of the little red dot phenomenon. J0647_1045 is unresolved (r(e) less than or similar to 0.17 kpc) in the three NIRCam long-wavelength filters but significantly extended (r(e) = 0.45 +/- 0.06 kpc) in the three short-wavelength filters, indicating a red compact source in a blue star-forming galaxy. The spectral continuum shows a clear change in slope, from blue in the optical/UV to red in the rest-frame optical/NIR, which is consistent with two distinct components fit by power laws with different attenuations: A(V) = 0.38 +/- 0.01 (UV) and A(V) = 5.61 +/- 0.04 (optical/NIR). Fitting the H alpha line requires both broad (full width at half maximum of similar to 4300 +/- 100 km s(-1)) and narrow components, but none of the other emission lines, including H beta, show evidence of broadness. We calculated A(V) = 0.9 +/- 0.4 from the Balmer decrement using narrow H alpha and H beta and A(V) > 4.1 +/- 0.1 from broad H alpha and an upper limit on broad H beta, which is consistent with blue and red continuum attenuation, respectively. Based on a single-epoch H alpha line width, the mass of the central black hole is 8(-0.4)(+0.5) x 10(8) M-circle dot. Our findings are consistent with a multi-component model, in which the optical/NIR and broad lines arise from a highly obscured, spatially unresolved region, likely a relatively massive active galactic nucleus, while the less obscured UV continuum and narrow lines arise, at least partly, from a small but spatially resolved star-forming host galaxy.