Add to ORKGWe report {\em JWST}/NIRCam measurements of quasar host galaxy emissions and supermassive black hole (SMBH) masses for six quasars at $5.9<z<7.1$ in the \textit{Emission-line galaxies and Intergalactic Gas in the Epoch of Reionization} (EIGER) project. We obtain deep NIRCam imaging in the F115W, F200W, and F356W bands, as well as F356W grism spectroscopy of the quasars. We use bright unsaturated stars to construct models of the point spread function (PSF) and estimate the errors of these PSFs. We then measure or constrain the fluxes and morphology of the quasar host galaxies by fitting the quasar images as a point source plus an exponential disk. We successfully detect the host galaxy of three quasars, which have host-to-quasar flux ratios ...
We have used far-infrared data from IRAS, Infrared Space Observatory (ISO), Spitzer Wide-Area Infrar...
We investigate the star-forming main sequence of the host galaxies of a large, well-defined sample o...
Here we explore the infrared (IR) properties of the progenitors of high-z quasar host galaxies. Adop...
The properties of quasar-host galaxies might be determined by the growth and feedback of their super...
We present rest-frame ultraviolet (UV) images of six luminous quasars at $z \sim 4.8$ obtained with ...
We present measurements of black hole masses and Eddington ratios for a sample of 38 bright (M$_{145...
There are only five radio-loud quasars currently known within 1 Gyr from the Big Bang ($z>6$) and th...
We present rest-frame ultraviolet (UV) images of six luminous quasars at $z \sim 4.8$ obtained with ...
State-of-the-art models of massive black hole formation postulate that quasars at z > 6 reside in...
State-of-the-art models of massive black hole formation postulate that quasars at z > 6 reside in...
Over 60 years after the discovery of the first quasar, more than $275$ such sources are identified i...
We study the dependence of the M-BH-M-host relation on the redshift up to z = 3 for a sample of 96 q...
open12siState-of-the-art models of massive black hole formation postulate that quasars at z > 6 r...
The most distant known quasar recently discovered by Bañados et al. (2018) is at z=7.5 (690 Myr aft...
Integral Field Spectroscopy (IFS) with JWST NIRSpec will significantly improve our understanding of ...
We have used far-infrared data from IRAS, Infrared Space Observatory (ISO), Spitzer Wide-Area Infrar...
We investigate the star-forming main sequence of the host galaxies of a large, well-defined sample o...
Here we explore the infrared (IR) properties of the progenitors of high-z quasar host galaxies. Adop...
The properties of quasar-host galaxies might be determined by the growth and feedback of their super...
We present rest-frame ultraviolet (UV) images of six luminous quasars at $z \sim 4.8$ obtained with ...
We present measurements of black hole masses and Eddington ratios for a sample of 38 bright (M$_{145...
There are only five radio-loud quasars currently known within 1 Gyr from the Big Bang ($z>6$) and th...
We present rest-frame ultraviolet (UV) images of six luminous quasars at $z \sim 4.8$ obtained with ...
State-of-the-art models of massive black hole formation postulate that quasars at z > 6 reside in...
State-of-the-art models of massive black hole formation postulate that quasars at z > 6 reside in...
Over 60 years after the discovery of the first quasar, more than $275$ such sources are identified i...
We study the dependence of the M-BH-M-host relation on the redshift up to z = 3 for a sample of 96 q...
open12siState-of-the-art models of massive black hole formation postulate that quasars at z > 6 r...
The most distant known quasar recently discovered by Bañados et al. (2018) is at z=7.5 (690 Myr aft...
Integral Field Spectroscopy (IFS) with JWST NIRSpec will significantly improve our understanding of ...
We have used far-infrared data from IRAS, Infrared Space Observatory (ISO), Spitzer Wide-Area Infrar...
We investigate the star-forming main sequence of the host galaxies of a large, well-defined sample o...
Here we explore the infrared (IR) properties of the progenitors of high-z quasar host galaxies. Adop...