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DC Field | Value | Language |
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dc.contributor.author | Singh, Kulinder Pal | - |
dc.date.accessioned | 2017-09-28T09:13:25Z | - |
dc.date.available | 2017-09-28T09:13:25Z | - |
dc.date.issued | 2015-11-17 | - |
dc.identifier.uri | http://hdl.handle.net/123456789/899 | - |
dc.description.abstract | AstroSat, India's first satellite for astromomy, was launched into a circular near-equatorial orbit, ~650 kms above the Earth by a polar satellite launch vecicle (PSLV) on september 28th, 2015, from SHAR. The satellite is designed to carry out simultaneous multi-wavelength observations in visible, near-ultraviolet (NUV), far-UV (FUV), soft X-rays and hard Xrays. There are five principal scientific payloads aboard the satellite for astronomical observations: (i) three Large Area Xenon Proportional Counters (LAXPCs) the largest space borne detectoes of thos kind, (ii) a Soft X-ray focusing Telescope (SXT), (iii) a Cadmium-Zinc-Telluride Imager (CZTI), (iv) two Ultra-Violet Imaging Telescopes (UVITs) one for visible and near-UV channels and another for far-UV, and (v) three Scanning Sky Monitors (SSMs). The first three of these and a charged particle monitor (CPM) were made in TIFR. All the X-ray telescopes have been switched on and are working very well. In the talk, I will review the history and development of X-ray astromomy to provide a rationale for Astrosat. A brief description of the design, construction, capabilities, scientific objectives of all the main scientific payloads. Results and images from the first light will be presented. | en_US |
dc.description.sponsorship | IISER-M | en_US |
dc.language.iso | en | en_US |
dc.publisher | IISER-M | en_US |
dc.title | India's First Astronomy Satellite | en_US |
dc.type | Other | en_US |
Appears in Collections: | Public Lectures |
Files in This Item:
File | Description | Size | Format | |
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Public Lecture, 17-10-2015.jpeg | 111.15 kB | JPEG | View/Open |
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