1992
DOI: 10.1016/0020-0891(92)90002-b
|View full text |Cite
|
Sign up to set email alerts
|

High efficiency half-wave plates for submillimetre polarimetry

Help me understand this report

Search citation statements

Order By: Relevance

Paper Sections

Select...
2
2
1

Citation Types

1
12
0

Year Published

1992
1992
2022
2022

Publication Types

Select...
8
1

Relationship

0
9

Authors

Journals

citations
Cited by 22 publications
(13 citation statements)
references
References 13 publications
1
12
0
Order By: Relevance
“…More specifically, in the field of experimental cosmology, the detection of the polarisation of the Cosmic Microwave Background radiation (CMB) requires extremely sensitive broadband instruments with very low-loss and low cross-polarisation HWPs in front of these instruments. In the past these devices were realised using combinations of birefringent plates following the well-known Pancharatnam recipes [5][6][7][8]. However, nowadays CMB experiments aiming to the detection of the very faint polarisation B-modes require very large arrays and modulating devices with diameters that cannot be achieved using commercially available birefringent materials.…”
Section: Introductionmentioning
confidence: 99%
“…More specifically, in the field of experimental cosmology, the detection of the polarisation of the Cosmic Microwave Background radiation (CMB) requires extremely sensitive broadband instruments with very low-loss and low cross-polarisation HWPs in front of these instruments. In the past these devices were realised using combinations of birefringent plates following the well-known Pancharatnam recipes [5][6][7][8]. However, nowadays CMB experiments aiming to the detection of the very faint polarisation B-modes require very large arrays and modulating devices with diameters that cannot be achieved using commercially available birefringent materials.…”
Section: Introductionmentioning
confidence: 99%
“…The polarization calibration sources were Jupiter and Uranus, assumed to be unpolarized. The polarization efficiency is 0.95, and a correction was applied for this e †ect (Murray et al 1992).…”
Section: Jcmt Observationsmentioning
confidence: 99%
“…The biggest inefficiency comes from the HWP, which has 5-10 % absorption due to the half-wave plate 25 and another 2% loss due to imperfections in the a/r coatings.…”
Section: Throughputmentioning
confidence: 99%