332 citations · 2.7k across the 53 of their papers we have counts for
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A Correlation Between Lyα Spectral Line Profile and Rest-Frame UV Morphology
Vivian U, Shoubaneh Hemmati, Behnam Darvish +6
We explore the relationship between the spectral shape of the Lyα emission and the UV morphology of the host galaxy using a sample of 304 Lyα-emitting BV i-dropouts at 3 < z < 7 in…
Spectroscopic Study of Star-forming Galaxies in Filaments and the Field at 0.5: Evidence for Environmental Dependence of Electron Density
Behnam Darvish, Bahram Mobasher, David Sobral +3
We study the physical properties of a spectroscopic sample of 28 star-forming galaxies in a large filamentary structure in the COSMOS field at 0.53, with spectroscopic data…
Nebular and Stellar Dust Extinction Across the Disk of Emission-Line Galaxies on Small (KPC) Scales
Shoubaneh Hemmati, Bahram Mobasher, Behnam Darvish +3
We investigate resolved kpc-scale stellar and nebular dust distribution in eight star-forming galaxies at z~0.4 in the GOODS fields. Constructing the observed Spectral Energy Distr…
Evidence for PopIII-like stellar populations in the most luminous Lyman- emitters at the epoch of re-ionisation: spectroscopic confirmation
David Sobral, Jorryt Matthee, Behnam Darvish +5
Faint Lyman- (Ly) emitters become increasingly rarer towards the re-ionisation epoch (z~6-7). However, observations from a very large (~5deg) Ly survey at z=6.6 (Matth…
A Comparative Study of Density Field Estimation for Galaxies: New Insights into the Evolution of Galaxies with Environment in COSMOS out to z~3
Behnam Darvish, Bahram Mobasher, David Sobral +2
It is well-known that galaxy environment has a fundamental effect in shaping its properties. We study the environmental effects on galaxy evolution, with an emphasis on the environ…
Identification of the brightest Lyα emitters at z=6.6: implications for the evolution of the luminosity function in the re-ionisation era
Jorryt Matthee, David Sobral, Sérgio Santos +3
Using wide field narrow-band surveys, we provide a new measurement of the Lyman- Emitter (LAE) luminosity function (LF), which constraints the bright end for the first t…