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Related papers: The 3.6 meter Devasthal Optical Telescope: From in…

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A very unique strength of the Devasthal Observatory is its capability of detecting optical transients with the 4-m International Liquid Mirror Telescope (ILMT) and to rapidly follow them up using the 1.3-m Devasthal Fast Optical Telescope…

India reached a major milestone in the area of space astronomy with the successful launch and post-launch operations of its first space observatory, AstroSat. The success of this space observatory and the lessons learned must be utilized…

Instrumentation and Methods for Astrophysics · Physics 2022-06-09 Annapurni Subramaniam

The present article is based upon an invited talk delivered at the occasion of the inauguration of the 4m International Liquid Mirror Telescope (ILMT) which took place in Devasthal (ARIES, Uttarakhand, India) on 21st of March 2023. We…

The International Liquid Mirror Telescope (ILMT) project was motivated by the need for an inexpensive 4 metre diameter optical telescope that could be devoted entirely to astronomical surveys. Its scientific programmes include the detection…

A low dispersion spectrograph-cum-imager has been developed and assembled in ARIES, Nainital. The optical design of the spectrograph consists of a collimator and a focal reducer converting the f/9 beam from the 3.6-m Devasthal optical…

Instrumentation and Methods for Astrophysics · Physics 2022-04-20 Amitesh Omar , T. S. Kumar , B. Krishna Reddy , Jayshreekar Pant , Manoj Mahto

Ultra Violet Imaging Telescope on ASTROSAT Satellite mission is a suite of Far Ultra Violet (FUV 130 to 180 nm), Near Ultra Violet (NUV 200 to 300 nm) and Visible band (VIS 320 to 550nm) imagers. ASTROSAT is the first multi wavelength…

Instrumentation and Methods for Astrophysics · Physics 2015-06-11 Amit Kumar , S. K. Ghosh , J. Hutchings , P. U. Kamath , S. Kathiravan , P. K. Mahesh , J. Murthy , Nagbhushana. S , A. K. Pati , M. N. Rao , N. K. Rao , S. Sriram , S. N. Tandon

Conventional ground-based optical telescopes, even those with large apertures, primarily observe stars, close binaries, and multiple systems as unresolved point sources through photometric measurements. Spectroscopy can identify multiple…

Instrumentation and Methods for Astrophysics · Physics 2025-12-10 Km Nitu Rai , Neelam Panwar , Jeewan C Pandey , T S Kumar , Subrata Sarangi , Prasenjit Saha

As an in-house instrument developmental activity at ARIES, the 4Kx4K CCD Imager is designed and developed as a first-light instrument for the axial port of the 3.6m DOT. The f/9 beam of the telescope having a plate-scale of ~ 6.4 arc-sec/mm…

Instrumentation and Methods for Astrophysics · Physics 2017-11-16 S. B. Pandey , R. K. S. Yadav , Nandish Nanjappa , Shobhit Yadav , B. Krishna Reddey , Sanjeet Sahu , R. Srinivasan

We present the design and performance of the TANSPEC, a medium-resolution $0.55-2.5~\mu$m cryogenic spectrometer and imager, now in operation at the 3.6-m Devasthal Optical Telescope (DOT), Nainital, India. The TANSPEC provides three modes…

Ultra Violet Imaging Telescope on ASTROSAT Satellite mission is a suite of Far Ultra Violet (FUV; 130 to 180 nm), Near Ultra Violet (NUV; 200 to 300 nm) and Visible band (VIS; 320 to 550nm) imagers. ASTROSAT is a first multi wavelength…

Instrumentation and Methods for Astrophysics · Physics 2015-06-11 Amit Kumar , S. K. Ghosh , P. U. Kamath , Joe Postma , S. Kathiravan , P. K. Mahesh , Nagbhushana. S , K. H. Navalgund , N Rajkumar , M. N. Rao , K. S. Sarma , S. Sriram , C. S. Stalin , S. N. Tandon

We present here the information on the design and performance of the recently commissioned 2.5-meter telescope at the PRL Mount Abu Observatory, located at Gurushikhar, Mount Abu, India. The telescope has been successfully installed at the…

The Five-hundred-meter Aperture Spherical radio Telescope (FAST) is by far the largest telescope of any kind ever built. FAST produced its first light in September 2016 and it is now under commissioning, with normal operation to commence in…

Instrumentation and Methods for Astrophysics · Physics 2019-04-15 Di Li , John M. Dickey , Shu Liu

We report on 26 lunar occultation events observed in the context of a program started at Devasthal in 2017. In addition to the customary observations with the 1.3-m telescope, we report here also the first attempts performed with the…

Solar and Stellar Astrophysics · Physics 2020-09-09 A. Richichi , Saurabh Sharma , T. Sinha , R. Pandey , A. Ghosh , D. K. Ojha , A. K. Pandey , M. B. Naik

The Ultra-Violet Imaging Telescope (UVIT) is one of the five payloads onboard the first Indian multiwavelength astronomical observatory, AstroSat, launched by the Indian Space Research Organisation on 28 September 2015. UVIT, designed for…

Instrumentation and Methods for Astrophysics · Physics 2026-01-01 Akanksha Dagore , Prajwel Joseph , S. N. Tandon , Annapurni Subramaniam , S. K. Ghosh , C. S. Stalin

In this article, we present a detailed analysis of the statistical properties of seeing for the Muztagh-ata site which is the candidate site for hosting future Chinese Large Optical/infrared Telescope (LOT) project. The measurement was…

The 4-m International Liquid Mirror Telescope (ILMT) will soon become operational at the newly developed Devasthal observatory near Nainital (Uttarakhand, India). Coupled with a 4k $\times$ 4k pixels CCD detector and TDI optical corrector,…

Instrumentation and Methods for Astrophysics · Physics 2018-02-21 Brajesh Kumar , Kanhaiya L. Pandey , S. B. Pandey , P. Hickson , E. F. Borra , G. C. Anupama , J. Surdej

In the present work, recent characterization results of the 4K$\times$4K CCD Imager (a first light instrument of the 3.6m Devasthal Optical Telescope; DOT) and photometric calibrations are discussed, along with measurements of the…

Instrumentation and Methods for Astrophysics · Physics 2022-05-31 Amit Kumar , S. B. Pandey , Avinash Singh , R. K. S. Yadav , B. K. Reddy , N. Nanjappa , S. Yadav , R. Srinivasan

The Ultra-Violet Imaging Telescope (UVIT) is one of the payloads in ASTROSAT, the first Indian Space Observatory. The UVIT instrument has two 375mm telescopes: one for the far-ultraviolet (FUV) channel (1300--1800\AA), and the other for the…