Building A Dedicated Radio Supernova Search Engine
| dc.additional | Date of Conference: 9-15 March 2019, New Delhi, India | en_US |
| 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.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.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.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 |