An Imaging Polarimeter(IMPOL) for multi-wavelength observations
| dc.contributor.author | Ramaprakash, A.N | |
| dc.contributor.author | Gupta, Ranjan | |
| dc.contributor.author | Sen, A.K. | |
| dc.contributor.author | et.al | |
| dc.date.accessioned | 2012-07-30T15:13:16Z | |
| dc.date.available | 2012-07-30T15:13:16Z | |
| dc.date.issued | 2008-02-02 | |
| dc.description.abstract | Taking advantage of the advances in array detector technology, an imaging polarimeter (IMPOL) has been constructed for measuring linear polarization in the wavelength band from 400-800 nm. It makes use of a Wollaston prism as the analyser to measure simultaneously the two orthogonal polarization components that define a Stoke’s parameter. An achromatic half-wave plate is used to rotate the plane of polarization with respect to the axis of the analyser so that the second Stoke’s parameter also can be determined. With a field of view correponding to about 30 × 30 mm2 for a / 1.2 m, f/13 telescope, a sensitive, liquid-N2 cooled CCD camera as the detector and a built-in acquisition and guidance unit, the instrument can be used for studying stellar fields or extended objects with an angular resolution of ∼2′′ . The instrumental polarization is less than 0.05% and the accuracies of measurement are primarily limited by photon noise for typical observations. | en_US |
| dc.identifier.uri | http://hdl.handle.net/11007/1890 | |
| dc.language.iso | en | en_US |
| dc.publisher | Astron. Astrophys. Suppl. Ser | en_US |
| dc.subject | Instrumention: polarimeters | en_US |
| dc.subject | Techniques: polarimetry | en_US |
| dc.subject | Polarization | en_US |
| dc.title | An Imaging Polarimeter(IMPOL) for multi-wavelength observations | en_US |
| dc.type | Article | en_US |