We present the motivation, aims and preliminary result from the Swift/VLT legacy survey on gamma-ray burst host galaxies. This survey will produce a homogeneous and well-understood host sample covering more than 95% of the lookback time to the Big Bang, and allow us to characterize their fundamental properties
We present observations and analysis of the host galaxies of 23 heavily dust-obscured gamma-ray burs...
We present a preliminary data release from our multi-year campaign at Keck Observatory to study the ...
We present simultaneous optical and near-infrared (NIR) spectroscopy of 19 Swift γ-ray burst (GRB) h...
We describe the current status and recent results from our Swift/VLT legacy survey, a VLT Large Prog...
We introduce the Swift Gamma-Ray Burst Host Galaxy Legacy Survey ("SHOALS"), a multi-observatory hig...
We introduce the Swift Gamma-Ray Burst Host Galaxy Legacy Survey (SHOALS), a multi-observatory high ...
We introduce the Swift Gamma-Ray Burst Host Galaxy Legacy Survey ("SHOALS"), a multi-observatory hig...
We introduce the Swift Gamma-Ray Burst Host Galaxy Legacy Survey (“SHOALS”), a multiobservatory high...
The Swift satellite allows us to use gamma-ray bursts (GRBs) to peer through the hearts of star form...
Aims. Long duration gamma-ray bursts (GRBs) allow us to explore the distant Universe, and are potent...
Long-duration gamma-ray bursts (GRBs) are powerful tracers of star-forming galaxies. We have defined...
International audienceAims. Long duration gamma-ray bursts (GRBs) allow us to explore the distant Un...
We present observations and analysis of the host galaxies of 23 heavily dust-obscured gamma-ray burs...
Gamma-ray bursts (GRBs) offer a route to characterizing star-forming galaxies and quantifying high-z...
We present data and initial results from VLT/X-Shooter emission-line spectroscopy of 96 galaxies sel...
We present observations and analysis of the host galaxies of 23 heavily dust-obscured gamma-ray burs...
We present a preliminary data release from our multi-year campaign at Keck Observatory to study the ...
We present simultaneous optical and near-infrared (NIR) spectroscopy of 19 Swift γ-ray burst (GRB) h...
We describe the current status and recent results from our Swift/VLT legacy survey, a VLT Large Prog...
We introduce the Swift Gamma-Ray Burst Host Galaxy Legacy Survey ("SHOALS"), a multi-observatory hig...
We introduce the Swift Gamma-Ray Burst Host Galaxy Legacy Survey (SHOALS), a multi-observatory high ...
We introduce the Swift Gamma-Ray Burst Host Galaxy Legacy Survey ("SHOALS"), a multi-observatory hig...
We introduce the Swift Gamma-Ray Burst Host Galaxy Legacy Survey (“SHOALS”), a multiobservatory high...
The Swift satellite allows us to use gamma-ray bursts (GRBs) to peer through the hearts of star form...
Aims. Long duration gamma-ray bursts (GRBs) allow us to explore the distant Universe, and are potent...
Long-duration gamma-ray bursts (GRBs) are powerful tracers of star-forming galaxies. We have defined...
International audienceAims. Long duration gamma-ray bursts (GRBs) allow us to explore the distant Un...
We present observations and analysis of the host galaxies of 23 heavily dust-obscured gamma-ray burs...
Gamma-ray bursts (GRBs) offer a route to characterizing star-forming galaxies and quantifying high-z...
We present data and initial results from VLT/X-Shooter emission-line spectroscopy of 96 galaxies sel...
We present observations and analysis of the host galaxies of 23 heavily dust-obscured gamma-ray burs...
We present a preliminary data release from our multi-year campaign at Keck Observatory to study the ...
We present simultaneous optical and near-infrared (NIR) spectroscopy of 19 Swift γ-ray burst (GRB) h...