Discovery of a binary quasar at z~0.2 with 430 pc separation indicating a bound SMBH pair each >4e8 Msun, with 2.5 Gyr upper limit on merger timescale and implications for the PTA gravitational wave background.
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JADES is a 770-hour JWST Cycle 1 survey delivering deep multi-band NIRCam imaging over ~209 arcmin² and NIRSpec spectroscopy of over 5000 sources in the GOODS-S and GOODS-N fields to study galaxy evolution from high redshift to cosmic noon.
Half of strong CIII] emitters at z=5-7 show secure AGN signatures, with median equivalent width rising 0.67 dex relative to z=3-4 galaxies.
IllustrisTNG simulations link filament density to galaxy morphology trends across redshifts and predict that Roman's planned HLWAS survey needs greater depth to accurately map the z=1 cosmic web.
citing papers explorer
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Discovery of a close-separation binary quasar at the heart of a z~0.2 merging galaxy and its implications for low-frequency gravitational waves
Discovery of a binary quasar at z~0.2 with 430 pc separation indicating a bound SMBH pair each >4e8 Msun, with 2.5 Gyr upper limit on merger timescale and implications for the PTA gravitational wave background.
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Overview of the JWST Advanced Deep Extragalactic Survey (JADES)
JADES is a 770-hour JWST Cycle 1 survey delivering deep multi-band NIRCam imaging over ~209 arcmin² and NIRSpec spectroscopy of over 5000 sources in the GOODS-S and GOODS-N fields to study galaxy evolution from high redshift to cosmic noon.
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The AGN nature of strong CIII emitters in the Early Universe with JWST
Half of strong CIII] emitters at z=5-7 show secure AGN signatures, with median equivalent width rising 0.67 dex relative to z=3-4 galaxies.
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Impact of Cosmic Filaments on Galaxy Morphological Evolution and Predictions of Early Cosmic Web Structure for Roman
IllustrisTNG simulations link filament density to galaxy morphology trends across redshifts and predict that Roman's planned HLWAS survey needs greater depth to accurately map the z=1 cosmic web.