Parents

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Stefan L. Piotrowski grad student 1964 University of Warsaw (Astronomy Tree)

Children

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Tomasz Stepinski grad student
Shude Mao grad student 1990-1992 Princeton
James Rhoads grad student 1992-1993 (Astronomy Tree)
Thulsi Wickramasinghe grad student 1989-1994 Penn
Krzysztof Z. Stanek grad student 1996 Princeton (Astronomy Tree)
Li-Xin Li grad student 2001 Princeton
Przemyslaw R. Wozniak grad student 2001 Princeton
Laurent Eyer post-doc 2000-2002 Princeton
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Publications

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Gaudi BS, Bennett DP, Udalski A, et al. (2008) Discovery of a Jupiter/Saturn analog with gravitational microlensing. Science (New York, N.Y.). 319: 927-30
Paczyński B, Sienkiewicz R, Szczygieł DM. (2007) A model of AW UMa Monthly Notices of the Royal Astronomical Society. 378: 961-965
Subo D, Udalski A, Gould A, et al. (2007) First space-based microlens parallax measurement: Spitzer observations of OGLE-2005-SMC-001 Astrophysical Journal. 664: 862-878
Shabun K, Richichi A, Munari U, et al. (2007) The VLTI as a tool to study eclipsing binaries for an improved distance scale Proceedings of the International Astronomical Union. 3: 118-119
Beaulieu JP, Bennett DP, Fouqué P, et al. (2006) Discovery of a cool planet of 5.5 Earth masses through gravitational microlensing. Nature. 439: 437-40
Paczyński B, Szczygieł DM, Pilecki B, et al. (2006) Eclipsing binaries in the All Sky Automated Survey catalogue Monthly Notices of the Royal Astronomical Society. 368: 1311-1318
Li L, Paczynski B. (2006) Improved correlation between the variability and peak luminosity of gamma-ray bursts Monthly Notices of the Royal Astronomical Society. 366: 219-226
Paczyński B. (2006) Astronomy with Small Telescopes Publications of the Astronomical Society of the Pacific. 118: 1621-1625
Gould A, Udalski A, An D, et al. (2006) Microlens OGLE-2005-BLG-169 Implies That Cool Neptune-like Planets Are Common The Astrophysical Journal. 644: L37-L40
Sumi T, Woźniak PR, Udalski A, et al. (2006) Microlensing Optical Depth toward the Galactic Bulge Using Bright Sources from OGLE-II The Astrophysical Journal. 636: 240-260
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