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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/6831
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dc.contributor.authorKumar, B-
dc.contributor.authorPandey, S. B-
dc.contributor.authorPandey, Kanhaiya L-
dc.contributor.authorAnapuma, G. C-
dc.contributor.authorSurdej, J-
dc.date.accessioned2020-11-11T01:13:38Z-
dc.date.available2020-11-11T01:13:38Z-
dc.date.issued2018-04-
dc.identifier.citationBulletin de la Société Royale des Sciences de Liège, Vol. 87, Actes de colloques, 2018, p. 80 - 87en_US
dc.identifier.issn0037-9565-
dc.identifier.urihttp://prints.iiap.res.in/handle/2248/6831-
dc.descriptionOpen Access ©Societe Royale des Sciences de Liege; https://popups.uliege.be/0037-9565/index.php?id=7520en_US
dc.description.abstractThe upcoming 4-m International Liquid Mirror Telescope (ILMT) facility will perform deep imaging (in single scan g 0 ∼22 mag) of a narrow strip of sky each clear night in the Time Delayed Integration mode. A cadence of one day observation will provide unique opportunities to discover different types of supernovae (SNe) along with many other types of variable sources. We present the approach to discover SNe with the 4-m ILMT and discuss the follow-up strategy in the context of other existing observational facilities. The advantages of liquid mirror telescope observations over the traditional glass mirror telescopes are also discussed.en_US
dc.language.isoenen_US
dc.publisherSociete Royale des Sciences de Liegeen_US
dc.subjectAstronomyen_US
dc.subjectAstrophysicsen_US
dc.subjectObservatoriesen_US
dc.subjectInstrumentationen_US
dc.subjectSupernovaeen_US
dc.titleSupernovae study: Context of the 4-m International Liquid Mirror Telescopeen_US
dc.typeArticleen_US
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