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A year-long representation of the ILMT observations in different coordinate systems

2023/11/08 by Monalisa Dubey, Dubey, Monalisa, Bhavya Ailawadhi +25
Physics and Astronomy · #Adaptive optics and wavefront sensing #Astronomy and Astrophysical Research #FOS: Physical sciences #Instrumentation and Methods for Astrophysics (astro-ph.IM) #Stellar, planetary, and galactic studies

paper · pdf · doi:10.48550/arxiv.2311.05616

openalex publication_date 2023/11/08 · openalex created_date 2023/11/11 · openalex updated_date 2026/07/28

Abstract

The 4m International Liquid Mirror Telescope (ILMT) is the first optical survey telescope in India that performs zenithal observations of a 22' wide strip of the sky. To determine the portion of the sky covered by the ILMT during the entire year, we represent the ILMT Field of View (FoV) in three different coordinate systems - galactic, ecliptic, and equatorial. We adopt a constant declination of +2921'41.4" and varying right ascension (RA) ranges corresponding to the Local Sidereal Time (LST). The observations from June to September are hampered due to the monsoon season. The handiness of such representations will allow us to locate a transient event in the ILMT FoV. This will enable prompt follow-up observations with other facilities.

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