Shrinivas Kulkarni | |
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| Kulkarni in 2016 | |
| Born | 4 October 1956 Kurundwad, Maharashtra, India |
| Alma mater | |
| Awards |
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| Scientific career | |
| Fields | Astronomy
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| Institutions | California Institute of Technology |
| Doctoral advisor | |
| Notable students | |
Shrinivas Ramchandra Kulkarni (born 4 October 1956) is a US-based astronomer born and raised in India. [2] He is a professor of astronomy and planetary science at the California Institute of Technology (Caltech), [3] and was the director of the Caltech Optical Observatory (COO), overseeing the Palomar and Keck among other telescopes. [3]
Shrinivas Ramchandra Kulkarni was born on 4 October 1956 in the small town of Kurundwad in Maharashtra, into a Hindu family. His father, Dr. R. H. Kulkarni, was a surgeon based in Hubballi and his mother, Vimala Kulkarni, was a home-maker. He is one of four children and has three sisters, Sunanda Kulkarni, Sudha Murthy (educator, author, philanthropist and wife of one of the co-founders of Infosys) and Jaishree Deshpande (wife of Gururaj Deshpande). [4] [5] [6]
Kulkarni and his sisters grew up in Hubballi, Karnataka, and received their schooling at local schools there. [2] [4] [7] [5] He obtained his MS in applied physics from the Indian Institute of Technology, Delhi in 1978 and his PhD from the University of California, Berkeley in 1983. [3]
In 1987, Kulkarni obtained a position as faculty at the California Institute of Technology. [3] ADS shows that his papers cover following fields: (1) HI absorption studies of Milky Way Galaxy, (2) pulsars, millisecond pulsars, and globular cluster pulsars, (3) brown dwarfs and other sub-stellar objects, (4) soft gamma-ray repeaters, (5) gamma-ray bursts, and (6) optical transients.
Kulkarni started off his career as a radio astronomer. He studied the Milky Way Galaxy using HI absorption under the guidance of his advisor Carl Heiles, and observed its four arms. [8]
He discovered the first millisecond pulsar called PSR B1937+21 [9] with Donald Backer and colleagues, while he was a graduate student. In 1986, he found the first optical counterpart of binary pulsars, [10] while he was a Millikan Fellow at California Institute of Technology. He was instrumental in discovery of the first globular cluster pulsar in 1987 [11] using a supercomputer.
With Dale Frail at NRAO and Toshio Murakami and his colleagues at ISAS (predecessor of JAXA that was led by Yasuo Tanaka at that time), Kulkarni showed that soft gamma-ray repeaters are neutron stars associated with supernova remnants. [12] [13] This discovery eventually led to the understanding that neutron stars with extremely high magnetic field called magnetars are the soft gamma-ray repeaters. [14]
Caltech-NRAO team which he led showed in 1997 that gamma-ray bursts came from extra-galactic sources, [15] and identified optical counterparts. [16] Their research initiated the detailed studies of the sources of gamma-ray bursts along with the European team led by Jan van Paradijs.
He was also a member of the Caltech team that observed the first irrefutable brown dwarf in 1994 that orbited around a star called Gliese 229. [17]
His recent work involved Palomar Transient Factory which has succeeded in identifying the new groups of optical transients such as superluminous supernovae, [18] calcium-rich supernovae, [19] and luminous red novae. [20] [21]
Some of the awards he has received include the following:
In 2015, he received an honorary doctorate from Radboud University in the Netherlands. [27] In 2024, he was awarded the Shaw Prize in Astronomy. [28] [29]
Kulkarni has been the Jury Chair for the Infosys Prize for the discipline of Physical Sciences since 2009. [30] The prize is awarded by the Infosys Foundation, whose founder is Kulkarni's brother-in-law, Narayana Murthy.
Kulkarni is a member of four national academies. He was elected a Fellow of the Royal Society, London, in 2001, [1] [31] a member of the United States National Academy of Sciences in 2003, [32] an honorary fellow of Indian Academy of Sciences in 2012, [33] and a foreign member of the Royal Netherlands Academy of Arts and Sciences on 12 September 2016. [34] [35]
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