| DOI | Resolve DOI: https://doi.org/10.1117/12.2181397 |
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| Author | Search for: Anche, Ramya M.; Search for: Anupama, G. C.; Search for: Reddy, Krishna; Search for: Sen, Asoke; Search for: Sankarasubramanian, K.; Search for: Ramaprakash, A. N.; Search for: Sengupta, Sujan; Search for: Skidmore, Warren; Search for: Atwood, Jenny1; Search for: Tirupathi, Sivarani; Search for: Pandey, Shashi Bhushan |
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| Affiliation | - National Research Council of Canada. National Science Infrastructure
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| Format | Text, Article |
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| Conference | International Conference on Optics and Photonics 2015, ICOP 2015, February 20-22, 2015, Kolkata, India |
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| Subject | optical telescopes; photonics; polarimeters; polarization; telescopes; astronomical polarimetry; entire system; focal Plane; instrumental polarization; Mueller matrix; Thirty Meter Telescope; analytical models |
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| Abstract | The polarization introduced due to Thirty Meter Telescope (TMT) optics is calculated using an analytical model. Mueller matrices are also generated for each optical element using Zemax, based on which the instrumental polarization due to the entire system at the focal plane is estimated and compared with the analytical model. This study is significant in the estimation of the telescope sensitivity and also has great implications for future instruments. |
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| Publication date | 2015-06-15 |
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| Publisher | SPIE |
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| In | |
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| Series | |
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| Language | English |
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| Peer reviewed | Yes |
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| NPARC number | 21276967 |
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| Export citation | Export as RIS |
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| Report a correction | Report a correction (opens in a new tab) |
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| Record identifier | ce878911-d6b6-4183-8ca2-53a448dd64f6 |
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| Record created | 2015-11-10 |
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| Record modified | 2020-04-22 |
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