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TANSPEC: TIFR-ARIES Near-infrared Spectrometer

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dc.contributor.author Sharma, Saurabh, et.al
dc.contributor.author Ghosh, Arpan
dc.contributor.author Reddy, B. Krishna
dc.contributor.author Nanjappa, Nandish
dc.contributor.author Pandey, Rakesh
dc.contributor.author Sinha, Tirthendu
dc.contributor.author Panwar, Neelam
dc.contributor.author Sahu, Sanjit
dc.contributor.author Bangia, Tarun
dc.date.accessioned 2024-05-06T09:33:57Z
dc.date.available 2024-05-06T09:33:57Z
dc.date.issued 2022-08
dc.identifier.uri https://doi.org/10.1088/1538-3873/ac81eb
dc.identifier.uri http://localhost:8080/xmlui/handle/123456789/1566
dc.description.abstract We present the design and performance of the TANSPEC, a medium-resolution 0.55–2.5 μm cryogenic spectrometer and imager, now in operation at the 3.6 m Devasthal Optical Telescope (DOT), Nainital, India. The TANSPEC provides three modes of operation, which include photometry with broad- and narrowband filters, spectroscopy with short slits of 20″ length and different widths (from 0 5 to 4 0) in cross-dispersed mode at a resolving power R of ∼2750, and spectroscopy with long slits of 60″ length and different widths (from 0 5 to 4 0) in prism mode at a resolving power R of ∼100–350. TANSPEC’s imager mode provides a field of view of 60″ × 60″ with a plate scale of 0 245 pixel−1 on the 3.6 m DOT. The TANSPEC was successfully commissioned during 2019 April–May, and the subsequent characterization and astronomical observations are presented here. The TANSPEC was made available to the worldwide astronomical community for science observations from 2020 October. en_US
dc.language.iso en en_US
dc.publisher Publications of the Astronomical Society of the Pacific en_US
dc.relation.ispartofseries 1897;pasp134-085002
dc.subject Spectrometers en_US
dc.subject Direct imaging en_US
dc.subject Near infrared astronomy en_US
dc.subject Optical observation en_US
dc.title TANSPEC: TIFR-ARIES Near-infrared Spectrometer en_US
dc.type Article en_US


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