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The clustering of typical Ly emitters from : host halo masses depend on Ly and UV luminosities
Ali Ahmad Khostovan, David Sobral, Bahram Mobasher +7
We investigate the clustering and halo properties of Ly-selected emission line galaxies (LAEs) from the Slicing COSMOS 4K (SC4K) and from archival NB497 imaging of S…
Confirmation of double peaked Lyman-alpha emission at z=6.593: Witnessing a galaxy directly contributing to the reionisation of the Universe
Jorryt Matthee, David Sobral, Max Gronke +3
Distant luminous Lyman-alpha emitters (LAEs) are excellent targets for spectroscopic observations of galaxies in the epoch of reionisation (EoR). We present deep high-resolution (R…
The origin of scatter in the star formation rate - stellar mass relation
Jorryt Matthee, Joop Schaye
Observations have revealed that the star formation rate (SFR) and stellar mass (M) of star-forming galaxies follow a tight relation known as the galaxy main sequence.…
The nature of luminous Lyman-alpha emitters at z~2-3: maximal dust-poor starbursts and highly ionising AGN
David Sobral, Jorryt Matthee, Behnam Darvish +8
Deep narrow-band surveys have revealed a large population of faint Lyman-alpha (Lya) emitters (LAEs) in the distant Universe, but relatively little is known about the most luminous…
Predicting Lyman-alpha escape fractions with a simple observable: Lyman-alpha in emission as an empirically calibrated star formation rate indicator
David Sobral, Jorryt Matthee
Lyman-alpha (Lya) is intrinsically the brightest line emitted from active galaxies. While it originates from many physical processes, for star-forming galaxies the intrinsic Lya lu…
Star-forming galaxies are predicted to lie on a fundamental plane of mass, star formation rate and α-enhancement
Jorryt Matthee, Joop Schaye
Observations show that star-forming galaxies reside on a tight three-dimensional plane between mass, gas-phase metallicity and star formation rate (SFR), which can be explained by…