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Bulent Kiziltan Harvard LogoBulent Kiziltan Smithsonian LogoI am a postdoctoral fellow at Harvard-Smithsonian Center for Astrophysics where I am also affiliated with the Instutute for Theory and Computation.

My primary research focuses on compact objects; mainly neutron star, pulsars, supernova remnants and related phenomena. I develop Bayesian statistical methods and use them in conjunction with stellar population synthesis modules to constrain the bulk properties of the neutron star population.

I use multiwavelength pulsar observations to probe diverse aspects of their evolution. Recently, I have been interested in developing alternative time-series analysis techniques, particularly tailored for detecting very faint periodic fluctuations in astronomical data.

I am also a member of the Fermi-LAT (formerly GLAST) collaboration. The very high energy (γ-ray) emission from pulsars will hopefully help us finally understand the pulsar emission mechanism; a more than 40 year old jigsaw puzzle.

Talks & Presentations...

  • "The Neutron Star Mass Distribution", Kiziltan, Kottas & Thorsett, 2010 [...Details...]
  • "Millisecond Pulsar Ages: implications of Binary Evolution & a Maximum Spin Limit ", Kiziltan & Thorsett, 2009 [...Details...]
  • "Constraints on Pulsar Evolution: The Joint Period-Spindown Distribution of Millisecond Pulsars", Kiziltan & Thorsett, 2009, ADS, [...Detail...]
  • "Suprising Trove of Gamma-Ray Pulsars", an article in the Sky & Telescope magazine:
  • ...Bülent Kiziltan and Steve Thorsett (University of California, Santa Cruz) showed that different millisecond pulsars must form by at least two distinct processes. But the nature of the second process remains a mystery... [...Details...]

     

  • U. of California, Santa Cruz, Department of Astronomy & Astrophysics ranked 1st in the US., arXiv, [...Details...]