In-orbit Performance of UVIT and First Results
arXiv:1612.00612 · doi:10.1007/s12036-017-9445-x
Abstract
The performance of the ultraviolet telescope (UVIT) on-board ASTROSAT is reported. The performance in orbit is also compared with estimates made from the calibrations done on the ground. The sensitivity is found to be within ~15% of the estimates, and the spatial resolution in the NUV is found to exceed significantly the design value of 1.8 arcsec and it is marginally better in the FUV. Images obtained from UVIT are presented to illustrate the details revealed by the high spatial resolution. The potential of multi-band observations in the ultraviolet with high spatial resolution is illustrated by some results.
arXiv commentComment: Accepted for publication in JAA on December 1, 2016
References in corpus (11)
- The Galaxy Evolution Explorer: A Space Ultraviolet Survey Mission
- The Swift Ultra-Violet/Optical Telescope
- The propagation of uncertainties in stellar population synthesis modeling I: The relevance of uncertain aspects of stellar evolution and the IMF to the derived physical properties of galaxies
- The XMM-Newton Optical/UV Monitor Telescope
- Ultra Violet Imaging Telescope (UVIT) on ASTROSAT
- The Ultraviolet Imaging Telescope: Instrument and Data Characteristics
- Calibration and performance of the photon-counting detectors for the Ultraviolet Imaging Telescopes (UVIT) of the Astrosat observatory
- In-orbit Performance of UVIT on ASTROSAT
- Mapping Distortion of Detectors in UVIT Onboard AstroSat Observatory
- Studying the Imaging Characteristics of Ultra Violet Imaging Telescope (UVIT) through Numerical Simulations
- Tests & Calibration on Ultra Violet Imaging Telescope (UVIT)
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