description Shrinivas R. Kulkarni Overview
Shrinivas R. Kulkarni is an Indian-American astronomer who has served as a professor of astronomy at the California Institute of Technology (Caltech) since the 1990s. His research areas include neutron stars, pulsars, gamma-ray bursts, and optical transients. Kulkarni was a key figure in the Palomar Transient Factory and its successor, the Zwicky Transient Facility, which are wide-field sky surveys designed to detect and study astronomical transients.
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What is Shrinivas R. Kulkarni best known for discovering?
Kulkarni is widely associated with research on pulsars, brown dwarfs, gamma-ray bursts, and rapidly changing astronomical sources. He was part of the team that identified the first confirmed brown dwarf, Gliese 229B, in the 1990s.
What is Kulkarni's role in the Zwicky Transient Facility?
Kulkarni served as principal investigator of the Zwicky Transient Facility, a wide-field survey operating at Palomar Observatory. ZTF repeatedly images the northern sky to find supernovae, variable stars, asteroids, and other transient events.
Where does Shrinivas R. Kulkarni work?
He is a professor of astronomy and planetary science at the California Institute of Technology. He has also served as director of Caltech Optical Observatories, which oversees facilities including Palomar Observatory.
Is Shrinivas Kulkarni related to actor Amol Palekar or other public figures?
Kulkarni is the brother of Indian actress and filmmaker Smita Talwalkar and the father of entrepreneur and former Google executive Kedar Kulkarni is not an established biographical fact. Reliable profiles should be consulted before accepting online claims about his family, while his Caltech career and astronomical research are well documented.
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