Effects of polarization aberrations in an unobscured off-axis space telescope on its PSF ellipticity Article Swipe
Jing Luo
,
Xu He
,
Kuo Chin Fan
,
Xiaohui Zhang
·
YOU?
·
· 2020
· Open Access
·
· DOI: https://doi.org/10.1364/oe.412413
YOU?
·
· 2020
· Open Access
·
· DOI: https://doi.org/10.1364/oe.412413
Polarization aberrations exist in almost all astronomical telescopes. Polarization aberrations would bring about asymmetric apodization in the exit pupil, leading to asymmetric PSFs. The shape of PSFs is critical to telescopes that are used to detect weak gravitational lensing (WGL) in the universe. In this paper, polarization aberrations and their connections with PSF ellipticity in an unobscured off-axis space telescope are analyzed. Together with the Jones pupil, cumulative diattenuation and retardance maps of the telescope are obtained via polarization ray tracing. Due to asymmetric apodization caused by polarization aberrations, the ellipticities of all four PSF components are found to be greater than zero. The PSF ellipticity of the telescope over the full FOV is obtained. Results show that polarization aberrations change PSF ellipticity in different degrees at different FOVs. The maximum variance of PSF ellipticity induced by polarization aberrations is 7.5e–3 and the average value is 2.7e–3. In addition, interpolation errors of PSF ellipticity would also be affected by polarization aberrations. It is found that there are 405 FOV points (about 4% of all FOV points involved in the calculations) whose variances of interpolation errors caused by polarization aberrations are greater than 1.4e–4. According to the results shown in this paper, polarization aberrations of telescopes play a significant role in WGL measurements.
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Metadata
- Type
- article
- Language
- en
- Landing Page
- https://doi.org/10.1364/oe.412413
- OA Status
- gold
- Cited By
- 13
- References
- 33
- Related Works
- 10
- OpenAlex ID
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All OpenAlex metadata
Raw OpenAlex JSON
- OpenAlex ID
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https://openalex.org/W3101012925Canonical identifier for this work in OpenAlex
- DOI
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https://doi.org/10.1364/oe.412413Digital Object Identifier
- Title
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Effects of polarization aberrations in an unobscured off-axis space telescope on its PSF ellipticityWork title
- Type
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articleOpenAlex work type
- Language
-
enPrimary language
- Publication year
-
2020Year of publication
- Publication date
-
2020-11-18Full publication date if available
- Authors
-
Jing Luo, Xu He, Kuo Chin Fan, Xiaohui ZhangList of authors in order
- Landing page
-
https://doi.org/10.1364/oe.412413Publisher landing page
- Open access
-
YesWhether a free full text is available
- OA status
-
goldOpen access status per OpenAlex
- OA URL
-
https://doi.org/10.1364/oe.412413Direct OA link when available
- Concepts
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Physics, Optics, Polarization (electrochemistry), Apodization, Telescope, Strehl ratio, Exit pupil, Optical telescope, Spitzer Space Telescope, Exoplanet, Optical aberration, Pupil, Wavefront, Astrophysics, Stars, Chemistry, Physical chemistryTop concepts (fields/topics) attached by OpenAlex
- Cited by
-
13Total citation count in OpenAlex
- Citations by year (recent)
-
2025: 1, 2024: 1, 2023: 6, 2022: 3, 2021: 2Per-year citation counts (last 5 years)
- References (count)
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33Number of works referenced by this work
- Related works (count)
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10Other works algorithmically related by OpenAlex
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| abstract_inverted_index.FOV | 112, 168, 174 |
| abstract_inverted_index.PSF | 52, 94, 104, 121, 133, 152 |
| abstract_inverted_index.The | 23, 103, 129 |
| abstract_inverted_index.WGL | 210 |
| abstract_inverted_index.all | 5, 92, 173 |
| abstract_inverted_index.and | 48, 69, 141 |
| abstract_inverted_index.are | 32, 60, 75, 96, 166, 189 |
| abstract_inverted_index.ray | 79 |
| abstract_inverted_index.the | 16, 41, 64, 73, 89, 107, 110, 142, 178, 195 |
| abstract_inverted_index.via | 77 |
| abstract_inverted_index.PSFs | 26 |
| abstract_inverted_index.also | 155 |
| abstract_inverted_index.exit | 17 |
| abstract_inverted_index.four | 93 |
| abstract_inverted_index.full | 111 |
| abstract_inverted_index.maps | 71 |
| abstract_inverted_index.over | 109 |
| abstract_inverted_index.play | 205 |
| abstract_inverted_index.role | 208 |
| abstract_inverted_index.show | 116 |
| abstract_inverted_index.than | 101, 191 |
| abstract_inverted_index.that | 31, 117, 164 |
| abstract_inverted_index.this | 44, 199 |
| abstract_inverted_index.used | 33 |
| abstract_inverted_index.weak | 36 |
| abstract_inverted_index.with | 51, 63 |
| abstract_inverted_index.(WGL) | 39 |
| abstract_inverted_index.FOVs. | 128 |
| abstract_inverted_index.Jones | 65 |
| abstract_inverted_index.PSFs. | 22 |
| abstract_inverted_index.about | 12 |
| abstract_inverted_index.bring | 11 |
| abstract_inverted_index.exist | 2 |
| abstract_inverted_index.found | 97, 163 |
| abstract_inverted_index.shape | 24 |
| abstract_inverted_index.shown | 197 |
| abstract_inverted_index.space | 58 |
| abstract_inverted_index.their | 49 |
| abstract_inverted_index.there | 165 |
| abstract_inverted_index.value | 144 |
| abstract_inverted_index.whose | 180 |
| abstract_inverted_index.would | 10, 154 |
| abstract_inverted_index.zero. | 102 |
| abstract_inverted_index.(about | 170 |
| abstract_inverted_index.almost | 4 |
| abstract_inverted_index.caused | 85, 185 |
| abstract_inverted_index.change | 120 |
| abstract_inverted_index.detect | 35 |
| abstract_inverted_index.errors | 150, 184 |
| abstract_inverted_index.paper, | 45, 200 |
| abstract_inverted_index.points | 169, 175 |
| abstract_inverted_index.pupil, | 18, 66 |
| abstract_inverted_index.Results | 115 |
| abstract_inverted_index.average | 143 |
| abstract_inverted_index.degrees | 125 |
| abstract_inverted_index.greater | 100, 190 |
| abstract_inverted_index.induced | 135 |
| abstract_inverted_index.leading | 19 |
| abstract_inverted_index.lensing | 38 |
| abstract_inverted_index.maximum | 130 |
| abstract_inverted_index.results | 196 |
| abstract_inverted_index.7.5e–3 | 140 |
| abstract_inverted_index.Together | 62 |
| abstract_inverted_index.affected | 157 |
| abstract_inverted_index.critical | 28 |
| abstract_inverted_index.involved | 176 |
| abstract_inverted_index.obtained | 76 |
| abstract_inverted_index.off-axis | 57 |
| abstract_inverted_index.tracing. | 80 |
| abstract_inverted_index.variance | 131 |
| abstract_inverted_index.1.4e–4. | 192 |
| abstract_inverted_index.2.7e–3. | 146 |
| abstract_inverted_index.According | 193 |
| abstract_inverted_index.addition, | 148 |
| abstract_inverted_index.analyzed. | 61 |
| abstract_inverted_index.different | 124, 127 |
| abstract_inverted_index.obtained. | 114 |
| abstract_inverted_index.telescope | 59, 74, 108 |
| abstract_inverted_index.universe. | 42 |
| abstract_inverted_index.variances | 181 |
| abstract_inverted_index.asymmetric | 13, 21, 83 |
| abstract_inverted_index.components | 95 |
| abstract_inverted_index.cumulative | 67 |
| abstract_inverted_index.retardance | 70 |
| abstract_inverted_index.telescopes | 30, 204 |
| abstract_inverted_index.unobscured | 56 |
| abstract_inverted_index.aberrations | 1, 9, 47, 119, 138, 188, 202 |
| abstract_inverted_index.apodization | 14, 84 |
| abstract_inverted_index.connections | 50 |
| abstract_inverted_index.ellipticity | 53, 105, 122, 134, 153 |
| abstract_inverted_index.significant | 207 |
| abstract_inverted_index.telescopes. | 7 |
| abstract_inverted_index.Polarization | 0, 8 |
| abstract_inverted_index.aberrations, | 88 |
| abstract_inverted_index.aberrations. | 160 |
| abstract_inverted_index.astronomical | 6 |
| abstract_inverted_index.polarization | 46, 78, 87, 118, 137, 159, 187, 201 |
| abstract_inverted_index.calculations) | 179 |
| abstract_inverted_index.diattenuation | 68 |
| abstract_inverted_index.ellipticities | 90 |
| abstract_inverted_index.gravitational | 37 |
| abstract_inverted_index.interpolation | 149, 183 |
| abstract_inverted_index.measurements. | 211 |
| cited_by_percentile_year.max | 98 |
| cited_by_percentile_year.min | 90 |
| countries_distinct_count | 0 |
| institutions_distinct_count | 4 |
| citation_normalized_percentile.value | 0.85139552 |
| citation_normalized_percentile.is_in_top_1_percent | False |
| citation_normalized_percentile.is_in_top_10_percent | False |