Supernovae study: Context of the 4-m International Liquid Mirror Telescope

Kumar, B; Pandey, S. B; Pandey, Kanhaiya L; Anapuma, G. C; Surdej, J

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dc.contributor.author	Kumar, B
dc.contributor.author	Pandey, S. B
dc.contributor.author	Pandey, Kanhaiya L
dc.contributor.author	Anapuma, G. C
dc.contributor.author	Surdej, J
dc.date.accessioned	2020-11-11T01:13:38Z
dc.date.available	2020-11-11T01:13:38Z
dc.date.issued	2018-04
dc.identifier.citation	Bulletin de la Société Royale des Sciences de Liège, Vol. 87, Actes de colloques, 2018, p. 80 - 87	en_US
dc.identifier.issn	0037-9565
dc.identifier.uri	http://prints.iiap.res.in/handle/2248/6831
dc.description	Open Access ©Societe Royale des Sciences de Liege; https://popups.uliege.be/0037-9565/index.php?id=7520	en_US
dc.description.abstract	The 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.iso	en	en_US
dc.publisher	Societe Royale des Sciences de Liege	en_US
dc.subject	Astronomy	en_US
dc.subject	Astrophysics	en_US
dc.subject	Observatories	en_US
dc.subject	Instrumentation	en_US
dc.subject	Supernovae	en_US
dc.title	Supernovae study: Context of the 4-m International Liquid Mirror Telescope	en_US
dc.type	Article	en_US