Saurabh W. Jha
Department of Physics and Astronomy
Rutgers, the State University of New Jersey
136 Frelinghuysen Road
Piscataway, NJ 08854
office: Serin 315, Busch campus
tel: (732) 445-5500 ext. 6979
fax: (732) 445-4343
I joined the Rutgers astrophysics group in September 2007. Previously, I was a Panofsky Fellow at the Kavli Institute for Particle Astrophysics and Cosmology at the Stanford Linear Accelerator Center, a Miller Fellow in the University of California, Berkeley Department of Astronomy, and a graduate student at the Harvard-Smithsonian Center for Astrophysics.
Research interests and collaborations
My main research focus is the observational study of Type Ia supernovae (SN Ia). I am interested in understanding the properties of these exploding white dwarf stars: their progenitor systems, how they explode, and using this knowledge to turn them into tools with which to survey the Universe.
This work is done in collaboration with a variety of groups:
The High-z Supernova Search Team first published strong evidence from observations of distant SN Ia that we live in an accelerating Universe. Along with the results of the Supernova Cosmology Project, this work was called the Breakthrough of the Year by Science in 1998, and was awarded the 2007 Gruber Cosmology Prize. This discovery was recently honored with the 2011 Nobel Prize in Physics.
The ESSENCE project is following up this earlier work, in an attempt to characterize the dark energy that is driving the accelerating expansion of the Universe, by measuring its equation of state to 10% accuracy.
The SDSS-II Supernova Survey is filling a gap in previous work, by finding and analyzing hundreds of SN Ia in the redshift range between z=0.1 and z=0.3.
CLULESS (the CLUster and LEnsed Supernova Survey) is a project to find SN Ia in and behind galaxy clusters with the Magellan Telescopes in Chile.
In the future, the Large Synoptic Survey Telescope will find thousands of SN Ia. This huge number of objects means we (the LSST SN science collaboration, in particular) will need new methods to make best use of the data.
While distant SN Ia have driven our understanding of the history of the expansion of the Universe, nearby SN Ia are the crucial underpinning to this enterprise. Not only do they anchor the Hubble diagram for cosmology, they provide the samples which show the utility of SN Ia as distance indicators. They are also the ones which we can study the best, from observations at many wavelengths to data at late times when more distant objects are too faint to be measured.
The Lick Observatory SN Search is the most successful nearby (z < 0.1) SN search, using KAIT to repeatedly image nearby galaxies.
The CfA Supernova follow-up program spectroscopically classifies and produces optical and near-infrared light curves for many nearby SN. The CfA II sample of SN Ia, presented in my doctoral thesis, comprises 44 objects homogeneously observed and analyzed, including the largest collection of near-ultraviolet U-band light curves published.
MLCS2k2 is the development of the multi-color light curve shape method to turn SN Ia optical light curves into precise distances. This analysis tool continues to grow and be refined, and is in use by many SN Ia projects.
I am also interested in the detection and characterization of planets around other stars. With the AFOE group, we discovered the planetary companion to rho Coronae Borealis in 1997. In addition, colleagues and I have shown that a few of the transiting companions discovered by the OGLE survey are planets, including OGLE-TR-56b (the first planet discovered first by its transit), OGLE-TR-113b, and OGLE-TR-10b.