Keck Week Video #16: Cosmic Explosions: Gamma Ray Bursts and Other Transient Events from Keck – Dr. Shrinivas Kulkarni

Gamma ray bursts are the brightest electromagnetic events known in the Universe. They emit a narrow beam of intense radiation during a supernova when a massive star collapses into a neutron star or a black hole.

Dr. Shrinivas Kulkarni from the California Institute of Technology gives an illuminating presentation on how spectroscopy from Keck Observatory gives insight into the most powerful forces in the Universe.

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UCLA observers will work with MOSFIRE tonight. And UCI/UCB observers will work with NIRC2-LGS/NIRC2-NGS. Sun set 05:59:00pm rise 06:12:00am
Observers from UCR will use MOSFIRE on Keck 1, while on Keck 2, UCI observers will use DEIMOS. Sun set 06:00:00pm rise 06:12:00am
On Keck 1, we have UCR observers using LRIS-ADC. On Keck 2, we have Swinburne observers using ESI. Sun set 06:00:00pm rise 06:11:00am
CIT observers will use LRISP-ADC on Keck 1, and UCSC observers will use ESI on Keck 2 tonight. Sun set 06:01:00pm rise 06:11:00am
Our guests tonight are observers from UCSC and Swinburne, using LRISP-ADC and DEIMOS respectively. Sun set 06:02:00pm rise 06:10:00am