You have requested a machine translation of selected content from our databases. This functionality is provided solely for your convenience and is in no way intended to replace human translation. Neither SPIE nor the owners and publishers of the content make, and they explicitly disclaim, any express or implied representations or warranties of any kind, including, without limitation, representations and warranties as to the functionality of the translation feature or the accuracy or completeness of the translations.
Translations are not retained in our system. Your use of this feature and the translations is subject to all use restrictions contained in the Terms and Conditions of Use of the SPIE website.
13 December 2020Optical aspects of Near-Infrared Imager Spectrometer and Polarimeter instrument (NISP)
Archita Rai,1,2 Shashikiran Ganeshhttps://orcid.org/0000-0002-7721-3827,1 Sukamal K. Paul,3 Prashanth K. Kasarla,1 Prachi V. Prajapati,1 Deekshya R. Sarkar,1 Alka Singh,1 Pitambar S. Patwal,1 Hitesh K. L. Adalja,1 Satya N. Mathur,1 Sachindra Naik,1 Amish B. Shah,1 Kiran S. Baliyan1
1Physical Research Lab. (India) 2Indian Institute of Technology (India) 3Space Applications Ctr. (India)
As a Near- IR instrument to PRL's upcoming 2.5 m telescope, NISP is designed indigeniously at PRL to serve as a multifaceted instrument. Optical, Mechanical and Electronics subsystems are being designed and developed in-house at PRL. It will consist of imaging, spectroscopy and imaging-polarimetry mode in the wavelength bands Y, J, H, Ks i.e. 0.8 - 2.5 µm. The detector is an 2K x 2K H2RG (MCT) array detector from Teledyne, which will give a large FOV of 10' x 10' in the imaging mode. Spectroscopic modes with resolving power of R ~ 3000, will be achieved using grisms. Spectroscopy will be available in single order and a cross-dispersed mode shall be planned for simultaneous spectra. The instrument enables multi-wavelength imaging- polarimetry using Wedged-Double Wollaston (WeDoWo) prisms to get single shot Stokes parameters (I, Q, U) for linear polarisation simultaneously, thus increasing the efficiency of polarisation measurements and reducing observation time.
The alert did not successfully save. Please try again later.
Archita Rai, Shashikiran Ganesh, Sukamal K. Paul, Prashanth K. Kasarla, Prachi V. Prajapati, Deekshya R. Sarkar, Alka Singh, Pitambar S. Patwal, Hitesh K. L. Adalja, Satya N. Mathur, Sachindra Naik, Amish B. Shah, Kiran S. Baliyan, "Optical aspects of Near-Infrared Imager Spectrometer and Polarimeter instrument (NISP)," Proc. SPIE 11447, Ground-based and Airborne Instrumentation for Astronomy VIII, 1144765 (13 December 2020); https://doi.org/10.1117/12.2560988