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Upcoming 4m ILMT facility and data reduction pipeline testing

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dc.contributor.author Kumar, Brajesh, et.al.
dc.contributor.author negi, Vibhore
dc.contributor.author Ailawadhi, Bhavya
dc.contributor.author Misra, Kuntal
dc.date.accessioned 2024-05-20T06:30:06Z
dc.date.available 2024-05-20T06:30:06Z
dc.date.issued 2022-06
dc.identifier.uri https://doi.org/10.1007/s12036-021-09795-3S
dc.identifier.uri http://localhost:8080/xmlui/handle/123456789/1626
dc.description.abstract The 4m international liquid mirror telescope (ILMT) installation activities have recently been completed at the Devasthal observatory (Uttarakhand, India). The ILMT will perform continuous observa tion of a narrow strip of the sky ( 270 ) passing over the zenith in the SDSS g0 , r0 and i 0 bands. In combination with a highly efficient 4k 4k CCD camera and an optical corrector, the images will be secured at the prime focus of the telescope using the time delayed integration technique. The ILMT will reach 22.5 mag (g0 -band) in a single scan and this limiting magnitude can be further improved by co-adding the nightly images. The uniqueness of the one-day cadence and deeper imaging with the ILMT will make it possible to discover and study various galactic and extra-galactic sources, specially variable ones. Here, we present the latest updates of the ILMT facility and discuss the preparation for the first light, which is expected during early 2022. We also briefly explain different steps involved in the ILMT data reduction pipeline. en_US
dc.language.iso en en_US
dc.publisher Journal of Astrophysics & Astronomy en_US
dc.relation.ispartofseries 1846;jaa43-10
dc.subject Optical telescope en_US
dc.subject liquid mirror telescope en_US
dc.subject instrumentation en_US
dc.title Upcoming 4m ILMT facility and data reduction pipeline testing en_US
dc.type Article en_US


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