| DOI | Trouver le DOI : https://doi.org/10.1117/12.2181397 |
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| Auteur | Rechercher : Anche, Ramya M.; Rechercher : Anupama, G. C.; Rechercher : Reddy, Krishna; Rechercher : Sen, Asoke; Rechercher : Sankarasubramanian, K.; Rechercher : Ramaprakash, A. N.; Rechercher : Sengupta, Sujan; Rechercher : Skidmore, Warren; Rechercher : Atwood, Jenny1; Rechercher : Tirupathi, Sivarani; Rechercher : Pandey, Shashi Bhushan |
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| Affiliation | - Conseil national de recherches du Canada. Infrastructure scientifique nationale
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| Format | Texte, Article |
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| Conférence | International Conference on Optics and Photonics 2015, ICOP 2015, February 20-22, 2015, Kolkata, India |
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| Sujet | 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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| Résumé | 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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| Date de publication | 2015-06-15 |
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| Maison d’édition | SPIE |
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| Dans | |
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| Série | |
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| Langue | anglais |
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| Publications évaluées par des pairs | Oui |
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| Numéro NPARC | 21276967 |
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| Exporter la notice | Exporter en format RIS |
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| Signaler une correction | Signaler une correction (s'ouvre dans un nouvel onglet) |
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| Identificateur de l’enregistrement | ce878911-d6b6-4183-8ca2-53a448dd64f6 |
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| Enregistrement créé | 2015-11-10 |
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| Enregistrement modifié | 2020-04-22 |
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