The European Southern Observatory Faint Object Spectrograph and Camera v2 is one of the workhorse instruments on ESO’s New Technology Telescope, and is one of the most popular instruments at La Silla observatory. It is mounted at a Nasmyth focus, and therefore exhibits strong, wavelength and pointing-direction-dependent instrumental polarisation. In this document, we describe our efforts to calibrate the broadband imaging polarimetry mode, and provide a calibration for broadband B, V, and R filters to a level that satisfies most use cases (i.e. polarimetric calibration uncertainty ~0.1%). We make our calibration codes public. This calibration effort can be used to enhance the yield of future polarimetric programmes with the European Souther...
Aims.We present the first lab and sky validation of spectro-polarimetric equipment put at the combi...
EST, the European Solar Telescope, is a 4-m class solar telescope, which will be located at the Cana...
We present a system-level description of the Low Frequency Instrument (LFI) considered as a differen...
The European Southern Observatory Faint Object Spectrograph and Camera v2 is one of the workhorse in...
Context. Polarimetry is a very powerful tool for uncovering various properties of astronomical objec...
Polarised light from astronomical targets can yield a wealth of information about their source radia...
The Wide-Area Linear Optical Polarimeter (WALOP)-South instrument is an upcoming wide-field and high...
Polarised light from astronomical targets can yield a wealth of information about their source radia...
International audienceAims.We present the first lab and sky validation of spectro-polarimetric equip...
Polarised light from astronomical targets can yield a wealth of information about their source radia...
The process of data taking, reduction and calibration of near-infrared imaging polarimetry data tak...
Received date; accepted date The ∼39-m European Extremely Large Telescope (E-ELT) will be the larges...
"We test the performance of the FOcal Reducer and low dispersion Spectrograph (FORS2) instrument mou...
Context. We report on the results of calibrating and simulating the instrumental polarizat...
We report the development of a semi-automatic pipeline for the calibration of 86 GHz full-polarizati...
Aims.We present the first lab and sky validation of spectro-polarimetric equipment put at the combi...
EST, the European Solar Telescope, is a 4-m class solar telescope, which will be located at the Cana...
We present a system-level description of the Low Frequency Instrument (LFI) considered as a differen...
The European Southern Observatory Faint Object Spectrograph and Camera v2 is one of the workhorse in...
Context. Polarimetry is a very powerful tool for uncovering various properties of astronomical objec...
Polarised light from astronomical targets can yield a wealth of information about their source radia...
The Wide-Area Linear Optical Polarimeter (WALOP)-South instrument is an upcoming wide-field and high...
Polarised light from astronomical targets can yield a wealth of information about their source radia...
International audienceAims.We present the first lab and sky validation of spectro-polarimetric equip...
Polarised light from astronomical targets can yield a wealth of information about their source radia...
The process of data taking, reduction and calibration of near-infrared imaging polarimetry data tak...
Received date; accepted date The ∼39-m European Extremely Large Telescope (E-ELT) will be the larges...
"We test the performance of the FOcal Reducer and low dispersion Spectrograph (FORS2) instrument mou...
Context. We report on the results of calibrating and simulating the instrumental polarizat...
We report the development of a semi-automatic pipeline for the calibration of 86 GHz full-polarizati...
Aims.We present the first lab and sky validation of spectro-polarimetric equipment put at the combi...
EST, the European Solar Telescope, is a 4-m class solar telescope, which will be located at the Cana...
We present a system-level description of the Low Frequency Instrument (LFI) considered as a differen...