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A Spatially Resolved [CII] Survey of 31 $z\sim7$ Massive Galaxies Hosting Luminous Quasars by Wang, Feige; Yang, Jinyi; Fan, Xiaohui; Venemans, Bram; Decarli, Roberto; Bañados, Eduardo; Walter, Fabian; Barth, Aaron J.; Bian, Fuyan; Davies, Frederick B.; Eilers, Anna-Christina; Farina, Emanuele Paolo; Hennawi, Joseph F.; Li, Jiang-Tao; Mazzucchelli, Chiara; Wang, Ran; Wu, Xue-Bing; Yue, Minghao is a scholarly article available to read on EtoBox.
What is A Spatially Resolved [CII] Survey of 31 $z\sim7$ Massive Galaxies Hosting Luminous Quasars about?
The [CII] 158 $\mu$m emission line and the underlying far-infrared (FIR) dust continuum are important tracers for studying star formation and kinematic properties of early galaxies. We present a survey of the [CII] emission lines and FIR continua of 31 luminous quasars at $z>6.5$ using the Atacama Large Millimeter Array (ALMA) and the NOrthern Extended Millimeter Array (NOEMA) at sub-arcsec resolution. This survey more than doubles the number of quasars with [CII] and FIR observations at these redshifts and enables statistical studies of quasar host galaxies deep into the epoch of reionization. We detect [CII] emission in 27 quasar hosts with a luminosity range of $L_{\rm [CII]}=(0.3-5.5)\times10^9~L_\odot$ and detect the FIR continuum of 28 quasar hosts with a luminosity range of $L_{\rm FIR}=(0.5-13.0)\times10^{12}~L_\odot$. Both $L_{\rm [CII]}$ and $L_{\rm FIR}$ are correlated ($\rho\simeq0.4$) with the quasar bolometric luminosity, albeit with substantial scatter. The quasar hosts detected by ALMA are clearly resolved with a median diameter of $\sim$5 kpc. About 40% of the quasar host galaxies show a velocity gradient in [CII] emission, while the rest show either dispersion-dom
- Author
- Wang, Feige; Yang, Jinyi; Fan, Xiaohui; Venemans, Bram; Decarli, Roberto; Bañados, Eduardo; Walter, Fabian; Barth, Aaron J.; Bian, Fuyan; Davies, Frederick B.; Eilers, Anna-Christina; Farina, Emanuele Paolo; Hennawi, Joseph F.; Li, Jiang-Tao; Mazzucchelli, Chiara; Wang, Ran; Wu, Xue-Bing; Yue, Minghao
- Published
- 2024
- Language
- EN