We describe the design and construction of a new novel optical polarimeter (RINGO2) for the Liverpool Telescope. The instrument is designed for rapid (< 3 minute) followup observations of Gamma Ray Bursts in order to measure the early time polarization and time evolution on timescales of about 1 − 10000 seconds. By using a fast rotating Polaroid whose rotation is synchronized to control the readout of an electron multiplying CCD eight times per revolution, we can rebin our data in the time domain after acquisition with little noise penalty, thereby allowing us to explore the polarization evolution of these rapidly variable objects for the first time
RINGO on the Liverpool Telescope has now measured the optical polarization of GRB 060418 (where a 2 ...
We present a status report on the study of gamma-ray bursts (GRBs) in the era of rapid followup usin...
The POLAR-2 Gamma-Ray Burst (GRB) Polarimetry mission is a follow-up to the successful POLAR mission...
We describe the design and construction of a new novel optical polarimeter (RINGO2) for the Liverpoo...
We describe the design and construction of a novel optical ring-polarimeter (RINGO) for the Liverpoo...
We describe the design and construction of a novel optical ring-polarimeter (RINGO) for the Liverpoo...
Following the start of science operations in 2004, it was quickly realised that the full robotic nat...
GRB jets contain rapidly moving electrons which will spiral around magnetic field lines. This causes...
We present a catalog of early-time (~10^2-10^4s) photometry and polarimetry of all Gamma-Ray Burst (...
Gamma-ray bursts are the most violent of known astrophysical events, with up to 10^53 ergs of energy...
We present a catalog of early-time (~10^2 - 10^4 s) photometry and polarimetry of all gamma-ray burs...
Gamma-ray bursts (GRBs) are extremely energetic events of cosmological origin. Observed GRBs have hi...
Optical polarimetry can play a key role in diagonistic of magnetic field strength/order/geometry in ...
Gamma-Ray Bursts (GRBs) are among the most powerful and violent events in the Universe. Despite half...
We present photometric and polarimetric measurements of gamma-ray burst (GRB) optical afterglows obs...
RINGO on the Liverpool Telescope has now measured the optical polarization of GRB 060418 (where a 2 ...
We present a status report on the study of gamma-ray bursts (GRBs) in the era of rapid followup usin...
The POLAR-2 Gamma-Ray Burst (GRB) Polarimetry mission is a follow-up to the successful POLAR mission...
We describe the design and construction of a new novel optical polarimeter (RINGO2) for the Liverpoo...
We describe the design and construction of a novel optical ring-polarimeter (RINGO) for the Liverpoo...
We describe the design and construction of a novel optical ring-polarimeter (RINGO) for the Liverpoo...
Following the start of science operations in 2004, it was quickly realised that the full robotic nat...
GRB jets contain rapidly moving electrons which will spiral around magnetic field lines. This causes...
We present a catalog of early-time (~10^2-10^4s) photometry and polarimetry of all Gamma-Ray Burst (...
Gamma-ray bursts are the most violent of known astrophysical events, with up to 10^53 ergs of energy...
We present a catalog of early-time (~10^2 - 10^4 s) photometry and polarimetry of all gamma-ray burs...
Gamma-ray bursts (GRBs) are extremely energetic events of cosmological origin. Observed GRBs have hi...
Optical polarimetry can play a key role in diagonistic of magnetic field strength/order/geometry in ...
Gamma-Ray Bursts (GRBs) are among the most powerful and violent events in the Universe. Despite half...
We present photometric and polarimetric measurements of gamma-ray burst (GRB) optical afterglows obs...
RINGO on the Liverpool Telescope has now measured the optical polarization of GRB 060418 (where a 2 ...
We present a status report on the study of gamma-ray bursts (GRBs) in the era of rapid followup usin...
The POLAR-2 Gamma-Ray Burst (GRB) Polarimetry mission is a follow-up to the successful POLAR mission...