Building A Dedicated Radio Supernova Search Engine

Nair, Lekshmi M.; Balasubramanyam, R.

Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/7673

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DC Field	Value	Language
dc.contributor.author	Nair, Lekshmi M.	-
dc.contributor.author	Balasubramanyam, R.	-
dc.date.accessioned	2021-02-16T09:12:40Z	-
dc.date.available	2021-02-16T09:12:40Z	-
dc.date.issued	2019-06	-
dc.identifier.citation	URSI Asia-Pacific Radio Science Conference (AP-RASC), 2019, New Delhi, India,	en_US
dc.identifier.isbn	Electronic ISBN:978-908-25987-5-9	-
dc.identifier.isbn	USB ISBN:978-908-25987-4-2	-
dc.identifier.isbn	978-1-5386-8551-8	-
dc.identifier.uri	http://hdl.handle.net/2289/7673	-
dc.description	Restricted Access.	en_US
dc.description.abstract	Massive stars at the end of their lives explode as supernovae. The supernova rate in Milky Way is expected to be one in thirty years. Owing to interstellar opacity, they are likely to be visible in optical only if they happen within a few kilo parsec distance. In radio, they can be detected up to the end of the galaxy even with a modest sized telescope. To enable this we are building a dedicated radio Supernova Search Engine (SnSE).	en_US
dc.language.iso	en	en_US
dc.publisher	IEEE	en_US
dc.relation.uri	https://ieeexplore.ieee.org/document/8738267	en_US
dc.rights	2019, IEEE	en_US
dc.subject	Temperature measurement ,	en_US
dc.subject	Optical switches	en_US
dc.subject	Temperature sensors ,	en_US
dc.subject	Buildings ,	en_US
dc.subject	Search engines ,	en_US
dc.subject	Optical interferometry	en_US
dc.title	Building A Dedicated Radio Supernova Search Engine	en_US
dc.type	Article	en_US
dc.additional	Date of Conference: 9-15 March 2019, New Delhi, India	en_US
Appears in Collections:	Research Papers (A&A)

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