dc.contributor.author |
Joshi, Y. C. |
|
dc.contributor.author |
Bangia, T. |
|
dc.contributor.author |
Jaiswar, M. K. |
|
dc.contributor.author |
Pant, J. |
|
dc.contributor.author |
Reddy, K. |
|
dc.contributor.author |
Yadav, S. |
|
dc.date.accessioned |
2024-02-23T05:41:08Z |
|
dc.date.available |
2024-02-23T05:41:08Z |
|
dc.date.issued |
2022-12 |
|
dc.identifier.uri |
10.1142/S2251171722400049 |
|
dc.identifier.uri |
http://localhost:8080/xmlui/handle/123456789/1459 |
|
dc.description.abstract |
This paper studies about the 130-cm Devasthal Fast Optical Telescope (DFOT) at Devasthal, India that
has been in operation for more than 10 years and is the main workhorse for the photometric observations for
a wide range of scientific programs carried out at ARIES, Nainital. Having a 2 k * 2 k pixel imager mounted
on the prime focus of the telescope, DFOT provides a field of view of about 18 * 18 arcmin2 in the sky.
Another frame transfer CCD imager of 512 * 512 pixel size enables monitoring transient sources with
millisecond temporal resolution. DFOT is equipped with a filter assembly having eight filters, an auto-guider, an All Sky Camera, and GPS-enabled weather monitoring system to support the observations in the
most optimum way. The telescope is capable of producing sub-milimag photometric stability which has
allowed us to detect many small-scale photometric variations. |
en_US |
dc.language.iso |
en |
en_US |
dc.publisher |
Journal of Astronomical Instrumentation |
en_US |
dc.relation.ispartofseries |
2007;jai11(4)-2240004 |
|
dc.subject |
Telescope |
en_US |
dc.subject |
instrumentation |
en_US |
dc.subject |
photometric observations |
en_US |
dc.title |
ARIES 130-cm Devasthal Fast Optical Telescope — Operation and Outcome |
en_US |
dc.type |
Article |
en_US |