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http://hdl.handle.net/123456789/5216
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DC Field | Value | Language |
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dc.contributor.author | Singh, Kulinder Pal | - |
dc.date.accessioned | 2023-08-26T19:58:22Z | - |
dc.date.available | 2023-08-26T19:58:22Z | - |
dc.date.issued | 2021 | - |
dc.identifier.citation | Journal of Astrophysics and Astronomy, 42(2). | en_US |
dc.identifier.uri | https://doi.org/10.1007/s12036-020-09678-z | - |
dc.identifier.uri | http://hdl.handle.net/123456789/5216 | - |
dc.description | Only IISER Mohali authors are available in the record. | en_US |
dc.description.abstract | The Soft X-ray Telescope (SXT) aboard the AstroSat satellite is the first Indian X-ray telescope in space. It is a modest size X-ray telescope with a charge coupled device (CCD) camera in the focal plane, which provides X-ray images in the ∼0.3–8.0 keV band. A forte of SXT is in providing undistorted spectra of relatively bright X-ray sources, in which it excels over some current large CCD-based X-ray telescopes. Here, we highlight some of the published spectral and timing results obtained using the SXT data to demonstrate the capabilities and overall performance of this telescope. | en_US |
dc.language.iso | en_US | en_US |
dc.publisher | Springer Nature | en_US |
dc.subject | telescopes | en_US |
dc.subject | X-rays: stars | en_US |
dc.subject | X-rays: binaries | en_US |
dc.title | Science with the AstroSat Soft X-ray telescope: An overview. | en_US |
dc.type | Article | en_US |
Appears in Collections: | Research Articles |
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