We present Keck-MOSFIRE H and K spectra for a sample of 24 candidate quiescent galaxies at 3 3, and offer the first insights on their formation histories
We combine Hubble Space Telescope (HST) G102 and G141 near-IR (NIR) grism spectroscopy with HST/WFC3...
A key issue in astronomy today is understanding the star-formation and assembly history of massive g...
Redshift of z ~ 2 is an important era in the history of the universe, as it contains the peak of sta...
We present Keck-MOSFIRE H and K spectra for a sample of 24 candidate quiescent galaxies at 3 3, and...
We present Keck–MOSFIRE H and K spectra for a sample of 24 candidate quiescent galaxies at 3 < z < 4...
The epoch of z~2-3 is a noticeably more active time in our universe for galaxies, with the global st...
We present Keck-I MOSFIRE near-infrared spectroscopy for a sample of 13 compact star-forming galaxie...
We present deep near-infrared Keck Near-Infrared Camera (NIRC) imaging of a recently discovered z = ...
We present our spectroscopic study of quenching/quiescent galaxies at z~4, resulted in the confirmat...
Using the MOSFIRE Deep Evolution Field (MOSDEF) rest-frame optical spectroscopic survey, we investig...
We performed a comprehensive stacking analysis on ∼14, 200 quiescent galaxy (QG) candidates at z = 0...
International audienceWe performed a comprehensive stacking analysis on similar to 14,200 quiescent ...
We present preliminary results from a programme to obtain multi-object near-infrared spectroscopy of...
The physical properties inferred from the spectral energy distributions (SEDs) of z > 3 galaxies hav...
We combine Hubble Space Telescope (HST) G102 and G141 near-IR (NIR) grism spectroscopy with HST/WFC3...
We combine Hubble Space Telescope (HST) G102 and G141 near-IR (NIR) grism spectroscopy with HST/WFC3...
A key issue in astronomy today is understanding the star-formation and assembly history of massive g...
Redshift of z ~ 2 is an important era in the history of the universe, as it contains the peak of sta...
We present Keck-MOSFIRE H and K spectra for a sample of 24 candidate quiescent galaxies at 3 3, and...
We present Keck–MOSFIRE H and K spectra for a sample of 24 candidate quiescent galaxies at 3 < z < 4...
The epoch of z~2-3 is a noticeably more active time in our universe for galaxies, with the global st...
We present Keck-I MOSFIRE near-infrared spectroscopy for a sample of 13 compact star-forming galaxie...
We present deep near-infrared Keck Near-Infrared Camera (NIRC) imaging of a recently discovered z = ...
We present our spectroscopic study of quenching/quiescent galaxies at z~4, resulted in the confirmat...
Using the MOSFIRE Deep Evolution Field (MOSDEF) rest-frame optical spectroscopic survey, we investig...
We performed a comprehensive stacking analysis on ∼14, 200 quiescent galaxy (QG) candidates at z = 0...
International audienceWe performed a comprehensive stacking analysis on similar to 14,200 quiescent ...
We present preliminary results from a programme to obtain multi-object near-infrared spectroscopy of...
The physical properties inferred from the spectral energy distributions (SEDs) of z > 3 galaxies hav...
We combine Hubble Space Telescope (HST) G102 and G141 near-IR (NIR) grism spectroscopy with HST/WFC3...
We combine Hubble Space Telescope (HST) G102 and G141 near-IR (NIR) grism spectroscopy with HST/WFC3...
A key issue in astronomy today is understanding the star-formation and assembly history of massive g...
Redshift of z ~ 2 is an important era in the history of the universe, as it contains the peak of sta...