We present a characterization of CasPol, a dual-beam polarimeter mounted at the 2.15-m Jorge Sahade Telescope, located at the Complejo Astronómico El Leoncito, Argentina. The telescope is one of the few available meter-sized optical telescopes located in the southern hemisphere hosting a polarimeter. To carry out this work, we collected photopolarimetric data along five observing campaigns, the first one during January 2014, and the remaining ones spread between August 2017 and March 2018. The data were taken through the Johnson?Cousins V, R, and I filters. Along the campaigns, we observed eight unpolarized and four polarized standard stars. Our analysis began characterizing the impact of seeing and aperture into the polarimetric measuremen...
We present the design and science case for the Liverpool Telescope's fourth-generation polarimeter; ...
The daytime sky has recently been demonstrated as a useful calibration tool for deriving polarizatio...
The ability to accurately measure polarization changes at the part-per-million (ppm) level enables a...
We have designed and built a prototype imaging polarimeter for use on the PROMPT robotic telescopes ...
Aims: We present results of a polarimetric survey of main-belt asteroids at Complejo Astronómico El ...
Context. Optical polarimeters are typically calibrated using measurements of stars with known and st...
WALOP (Wide-Area Linear Optical Polarimeter)-South, to be mounted on the 1m SAAO telescope in South ...
We have built and used on several occasions an optical broadband stellar polarimeter, PlanetPol, whi...
Polarization plays an important role in various time-domain astrophysics to understand the magnetic ...
Context. The SPHERE "planet finder" is an extreme adaptive optics (AO) instrument for high resolutio...
Aims. Results of different polarimetric campaigns at Complejo Astronómico El Leoncito (Casleo), San ...
Even a brief glance at astronomical journals indicates the breadth and depth of observational projec...
We are currently in an era of precision cosmology. Study of the Cosmic Microwave Background (CMB) ha...
Many different methods exist for reducing data obtained when an astronomical source is studied with ...
Aims. We present the results of a polarimetric survey of main-belt asteroids at Complejo Astronómico...
We present the design and science case for the Liverpool Telescope's fourth-generation polarimeter; ...
The daytime sky has recently been demonstrated as a useful calibration tool for deriving polarizatio...
The ability to accurately measure polarization changes at the part-per-million (ppm) level enables a...
We have designed and built a prototype imaging polarimeter for use on the PROMPT robotic telescopes ...
Aims: We present results of a polarimetric survey of main-belt asteroids at Complejo Astronómico El ...
Context. Optical polarimeters are typically calibrated using measurements of stars with known and st...
WALOP (Wide-Area Linear Optical Polarimeter)-South, to be mounted on the 1m SAAO telescope in South ...
We have built and used on several occasions an optical broadband stellar polarimeter, PlanetPol, whi...
Polarization plays an important role in various time-domain astrophysics to understand the magnetic ...
Context. The SPHERE "planet finder" is an extreme adaptive optics (AO) instrument for high resolutio...
Aims. Results of different polarimetric campaigns at Complejo Astronómico El Leoncito (Casleo), San ...
Even a brief glance at astronomical journals indicates the breadth and depth of observational projec...
We are currently in an era of precision cosmology. Study of the Cosmic Microwave Background (CMB) ha...
Many different methods exist for reducing data obtained when an astronomical source is studied with ...
Aims. We present the results of a polarimetric survey of main-belt asteroids at Complejo Astronómico...
We present the design and science case for the Liverpool Telescope's fourth-generation polarimeter; ...
The daytime sky has recently been demonstrated as a useful calibration tool for deriving polarizatio...
The ability to accurately measure polarization changes at the part-per-million (ppm) level enables a...