TIFR Treasures for Astronomy from Ground to Space
arXiv:2112.04877 · doi:10.1007/s12036-022-09800-3
Abstract
The infrared astronomy group of Department of Astronomy and Astrophysics at Tata Institute of Fundamental Research has been pursuing astronomical instrumentation activities since its inception. The group has been routinely involved in balloon-borne astronomy programs from the field station at Hyderabad with indigenously developed payloads. Ground-based astronomical activities began with a single element infrared detector. Later, over time, larger format array detectors are being used in the cameras. These astronomy cameras have been routinely used at observatories across India. Recently, the group has also developed a laboratory model of the Infrared Spectroscopic Imaging Survey payload, targeted for the small satellite mission of the Indian Space Research Organisation, which will carry out spectroscopic measurements in the wavelength range 1.7 to 6.4 m seamlessly
10 pages, 6 figures, accepted for publication in Special Issue of Journal of Astrophysics & Astronomy, 2022, Astrophysical jets and observational facilities: National perspective, 05 - 09 April 2021, ARIES, Nainital
References in corpus (10)
- The disintegrating old open cluster Czernik 3
- Star formation around mid-infrared bubble N37: Evidence of cloud-cloud collision
- Post-Outburst Phase of McNeil's Nebula (V1647 Orionis)
- Understanding Physical Properties of Young M-dwarfs: NIR spectroscopic studies
- TIRCAM2: The TIFR Near Infrared Imaging Camera
- Optical and NIR spectroscopy of cool CEMP stars to probe the nucleosynthesis in low mass AGB binary system
- Further milliarcsecond resolution results on cool giants and binary stars from lunar occultations at Devashtal
- [CII] emission properties of the massive star-forming region RCW36 in a filamentary molecular cloud
- PAH and nbL Features Detection in Planetary Nebulae NGC 7027 and BD +303639 with TIRCAM2 Instrument on 3.6m DOT
- Spectroscopic and photometric monitoring of a poorly known high-luminous OH/IR star: IRAS 18278+0931