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Ping-Shine Shaw (Fed)

Dr. Shaw received his Ph.D in physics from Columbia University in 1989 at the Microelectronics Sciences Laboratories studying surface adsorbed layers on semiconductors. He was an Associate Research Scientist at Columbia Astrophysics Laboratory, Columbia University, from 1989 to 1993. While there, he was a co-investigator on the Stellar X-Ray Polarimeter for the Spectrum-X-Gamma satellite mission. Dr. Shaw joined NIST in 1993 as a National Research Council Postdoctoral Research Associate working primarily on x-ray technology and synchrotron radiation. Since 1995 he has been a physicist at NIST studying ultraviolet and visible radiometry.

Awards:

  • National Research Council Postdoctoral Research Fellowship, 1993
  • Department of Commerce Silver Medal, 2008

Research Interests:

  • Synchrotron radiation based radiometry
  • UV optical metrology
  • UV-Visible material characterization

Publications

CALIBRATION OF SPECTRORADIOMETERS USING TUNABLE LASERS

Author(s)
Yuqin Zong, Ping-Shine Shaw, Joseph Rice, C Cameron Miller
To shorten the long calibration chain when using the conventional source-based approach and therefore to reduce spectroradiometer's calibration uncertainty, we

SURF III: A flexible Synchrotron Radiation Source for Radiometry and Research

Author(s)
Uwe Arp, Charles W. Clark, Lu Deng, Nadir S. Faradzhev, Alex P. Farrell, Mitchell L. Furst, Steven E. Grantham, Edward W. Hagley, Shannon B. Hill, Thomas B. Lucatorto, Ping-Shine Shaw, Charles S. Tarrio, Robert E. Vest
The calculability of synchrotron radiation (SR) makes electron storage rings wonderful light sources for radiometry. The broadband nature of SR allows coverage
Created March 26, 2019, Updated June 15, 2021