dc.contributor.author |
Bordoloi, Swagat |
|
dc.contributor.author |
Shalima, P |
|
dc.contributor.author |
Gogoi, Rupjyoti |
|
dc.contributor.author |
Murthy, J |
|
dc.date.accessioned |
2024-12-05T05:54:36Z |
|
dc.date.available |
2024-12-05T05:54:36Z |
|
dc.date.issued |
2024-11 |
|
dc.identifier.citation |
Publications of the Astronomical Society of Australia, Vol. 41, e086 |
en_US |
dc.identifier.issn |
1323-3580 |
|
dc.identifier.uri |
http://hdl.handle.net/2248/8598 |
|
dc.description |
Restricted Access |
en_US |
dc.description.abstract |
The Ultra Violet Imaging Telescope (UVIT) onboard India’s first dedicated multiwavelength satellite AstroSat observed a significant fraction of the sky in the ultraviolet with a spatial resolution of 1.4. We present a catalogue of the point sources observed by UVIT in the far ultraviolet (FUV; 1 300–1 800 Å) and near ultraviolet (NUV; 2 000–3 000 Å). We carried out astrometry and photometry of 428 field pointings in the FUV and 54 field pointings in the NUV band, observed in 5 filter bands in each channel, respectively, covering an area of
about 63 square degrees. The final catalogue contains about 102 773 sources. The limiting magnitude(AB) of the F148W band filter, that has the largest number of detections is ∼21.3. For the NUV channel, we find the limiting magnitude at around ∼23. We describe the final catalogue and present the results of the statistical analysis. |
en_US |
dc.language.iso |
en |
en_US |
dc.publisher |
Cambridge University Press on behalf of Astronomical Society of Australia |
en_US |
dc.relation.uri |
https://doi.org/10.1017/pasa.2024.80 |
|
dc.rights |
© The Author(s), 2024 |
|
dc.subject |
Astrometry |
en_US |
dc.subject |
Catalogues |
en_US |
dc.title |
A sky survey of ultraviolet sources observed through AstroSat’s UVIT: A point source catalogue |
en_US |
dc.type |
Article |
en_US |