| 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 |