Brian P. Schmidt

University of Washington, Seattle, Seattle, WA 
Visual perception
"Brian Schmidt"
Mean distance: 16.6 (cluster 17)


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Andrea Megela Simmons research assistant 2008-2009 Brown
Florian Eichler research assistant 2009-2011 Mass General Hospital
Jay Neitz grad student 2011-2015 University of Washington
Austin Roorda post-doc 2016- UC Berkeley
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Wolf C, Hon WJ, Bian F, et al. (2020) Ultra-luminous quasars at redshift z > 4.5 from SkyMapper Monthly Notices of the Royal Astronomical Society. 491: 1970-1979
Schmidt BP, Boehm AE, Tuten WS, et al. (2019) Spatial summation of individual cones in human color vision. Plos One. 14: e0211397
Boehm AE, Privitera CM, Schmidt BP, et al. (2019) Transverse chromatic offsets with pupil displacements in the human eye: sources of variability and methods for real-time correction. Biomedical Optics Express. 10: 1691-1706
Schmidt B, Boehm A, Roorda A. (2019) Predicting the appearance of light targeted to spectrally identified cones Journal of Vision. 19: 13
Nordlander T, Bessell MS, Da Costa GS, et al. (2019) The lowest detected stellar Fe abundance: the halo star SMSS J160540.18−144323.1 Monthly Notices of the Royal Astronomical Society: Letters. 488: L109-L113
Marino AF, Da Costa GS, Casey AR, et al. (2019) Keck HIRES spectroscopy of SkyMapper commissioning survey candidate extremely metal-poor stars Monthly Notices of the Royal Astronomical Society. 485: 5153-5167
Schmidt BP, Boehm AE, Foote KG, et al. (2018) The spectral identity of foveal cones is preserved in hue perception. Journal of Vision. 18: 19
Schmidt BP, Sabesan R, Tuten WS, et al. (2018) Sensations from a single M-cone depend on the activity of surrounding S-cones. Scientific Reports. 8: 8561
Contreras C, Phillips MM, Burns CR, et al. (2018) SN 2012fr: Ultraviolet, Optical, and Near-infrared Light Curves of a Type Ia Supernova Observed within a Day of Explosion The Astrophysical Journal. 859: 24
Inserra C, Smartt SJ, Gall EEE, et al. (2018) On the nature of hydrogen-rich superluminous supernovae Monthly Notices of the Royal Astronomical Society. 475: 1046-1072
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