dc.contributor.author |
Kameswara Rao, N |
|
dc.date.accessioned |
2008-06-03T10:10:38Z |
|
dc.date.available |
2008-06-03T10:10:38Z |
|
dc.date.issued |
2003 |
|
dc.identifier.citation |
BASI, Vol. 31, No. 3&4, pp. 249 - 255 |
en |
dc.identifier.uri |
http://hdl.handle.net/2248/2390 |
|
dc.description.abstract |
Some of the significant areas of astronomy that would be persued by UVIT, one of the payloads on the proposed Indian multiwavelength astronomy satellite ASTROSAT, is described. Some of the considerations and uniqueness of the system are high lighted. UVIT aims to provide flux calibrated images of the sky at a spatial resolution of about a second of arc in the wavelength range 1250 to 3200Å along with optical bands. |
en |
dc.format.extent |
234815 bytes |
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dc.format.mimetype |
application/pdf |
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dc.language.iso |
en |
en |
dc.publisher |
Astronomical Society of India |
en |
dc.relation.uri |
http://adsabs.harvard.edu/abs/2003BASI...31..249K |
en |
dc.subject |
UVIT |
en |
dc.subject |
ASTROSAT |
en |
dc.title |
Ultra Violet Imaging Telescope (UVIT) Science* |
en |
dc.type |
Article |
en |