Abstract Details

Name: Saurabh
Affiliation: ARIES
Conference ID: ASI2015_812
Title : TIFR-ARIES Near Infrared Spectrometer (TANSPEC)
Authors and Co-Authors : D K Ojha (TIFR) A K Pandey (ARIES) S K Ghosh (TIFR) TANSPCE TEAM (ARIES+TIFR)
Abstract Type : Oral
Abstract Category : Instrumentation and Techniques
Abstract : Through this project, TIFR-DAA and ARIES will bring together their resource pools for the development of a 0.8 to 2.5 micron Medium Resolution Spectrograph to be used on the main Cassegrain port of 3.6 metre Devasthal Optical Telescope. The instrument called TANSPEC, will provide unique medium resolution (R ~ 2000) spectroscopy capability to the telescope in a broad waveband range of 0.8 to 2.5 microns. It will also have low resolution prism mode (R~200) and a slit viewer with field of view of 1 x 1 arcmin square. This instrument will be extremely sensitive to low temperature stellar photospheres (T · 2500 K) and objects surrounded by warm dust envelopes or embedded in dust/molecular clouds. It is therefore particularly suited to the study of low and very low mass stellar populations (M/Ldwarfs, brown dwarfs), strong mass-losing stars on the asymptotic giant branch (AGB), young stellar objects (YSOs) still in their proto-stellar envelopes and active galactic nuclei (AGN). In this talk, I will discuss about the specification and science goal of this instrument along with some recent updates.