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Accessibility of the ILMT Survey Data

Kuntal MisraAryabhatta Research Institute of Observational sciencES (ARIES), Manora Peak, Nainital, 263001, IndiaBhavya AilawadhiAryabhatta Research Institute of Observational sciencES (ARIES), Manora Peak, Nainital, 263001, IndiaTalat AkhunovNational University of Uzbekistan, Department of Astronomy and Astrophysics, 100174 Tashkent, UzbekistanE. F. BorraDepartment of Physics, Université Laval, 2325, rue de l'Université, Québec, G1V 0A6, CanadaMonalisa DubeyAryabhatta Research Institute of Observational sciencES (ARIES), Manora Peak, Nainital, 263001, IndiaNaveen DukiyaAryabhatta Research Institute of Observational sciencES (ARIES), Manora Peak, Nainital, 263001, IndiaJiuyang FuDepartment of Physics and Astronomy, University of British Columbia, 6224 Agricultural Road, Vancouver, BC V6T 1Z1, CanadaBaldeep GrewalDepartment of Physics and Astronomy, University of British Columbia, 6224 Agricultural Road, Vancouver, BC V6T 1Z1, CanadaPaul HicksonDepartment of Physics and Astronomy, University of British Columbia, 6224 Agricultural Road, Vancouver, BC V6T 1Z1, CanadaBrajesh KumarAryabhatta Research Institute of Observational sciencES (ARIES), Manora Peak, Nainital, 263001, IndiaVibhore NegiDepartment of Physics, Deen Dayal Upadhyaya Gorakhpur University, Gorakhpur, 273009, IndiaKumar PranshuDepartment of Applied Optics and Photonics, University of Calcutta, Kolkata, 700106, IndiaEthen SunDepartment of Physics and Astronomy, University of British Columbia, 6224 Agricultural Road, Vancouver, BC V6T 1Z1, CanadaJean SurdejInstitute of Astrophysics and Geophysics, University of Liège, Allée du 6 Août 19c, 4000 Liège, Belgium
ABI

Abstract

The 4m International Liquid Mirror Telescope (ILMT) continuously scans a 22′ wide strip of the zenithal sky and records the images in three broadband filters (g’, r’ and i’) using a 4K×4K CCD camera. In about 10–12 hours of observations during a single night, ∼15 GB of data volume is generated. The raw images resulting from the observations in October–November 2022 have been pre-processed and astrometrically calibrated. In order to exploit the scientific capabilities of the ILMT survey data by the larger scientific community, we are disseminating the raw data (along with dark and flat fields) and the astrometrically calibrated data. These data sets can be downloaded by the users to conduct the scientific projects of their interest. In future, the data will be processed in near real-time and will be available via the ARIES data archive portal.

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