dc.contributor.author |
Tandon, S. N |
|
dc.contributor.author |
Ghosh, S. K |
|
dc.contributor.author |
Hutchings, J |
|
dc.contributor.author |
Stalin, C. S |
|
dc.contributor.author |
Subramaniam, A |
|
dc.date.accessioned |
2020-11-10T02:32:31Z |
|
dc.date.available |
2020-11-10T02:32:31Z |
|
dc.date.issued |
2017-08 |
|
dc.identifier.citation |
Current Science, Vol. 113, No. 4, pp. 583 - 586 |
en_US |
dc.identifier.issn |
0011-3891 |
|
dc.identifier.uri |
http://prints.iiap.res.in/handle/2248/6735 |
|
dc.description |
Open Access © Current Science Association http://www.currentscience.ac.in/Volumes/113/04/0583.pdf |
en_US |
dc.description.abstract |
The AstroSat satellite is designed for multiwavelength astronomy for observations covering a
spectral range from soft and hard X-rays to the ultraviolet. The Ultraviolet Imaging Telescope (UVIT) is
the only non-X-ray telescope on AstroSat and it provides the long lever arm to the multi-wavelength observations. In addition to the simultaneous multiwavelength studies in coordination with the X-ray
telescopes on-board AstroSat, UVIT is used to study a
large variety of objects with arcsecond-level spatial
resolution. During the first year of observations,
UVIT has obtained images in many filter bands in the
wavelength range 130–300 nm over a field of ~28,
which are being used to study a variety of hot stars,
nebulae, stellar clusters and galaxies. |
en_US |
dc.language.iso |
en |
en_US |
dc.publisher |
Current Science Association |
en_US |
dc.subject |
Multi-wavelength astronomy |
en_US |
dc.subject |
Ultraviolet Imaging Telescope |
en_US |
dc.subject |
X-ray telescope |
en_US |
dc.title |
Ultraviolet Imaging Telescope on AstroSat |
en_US |
dc.type |
Article |
en_US |