Suzanne Jacoby

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In the history of astronomy, major advances in our understanding of the Universe frequently arise from dramatic improvements in our ability to accurately measure astronomical quantities. Aided by rapid progress in information technology, current sky surveys are changing the way we view and study the Universe. Next-generation surveys will maintain this(More)
National Optical Astronomy Observatory, 950 N. Cherry Ave, Tucson, AZ 85719 Lawrence Livermore National Laboratory, 7000 East Avenue, Livermore, CA 94550 Physics Department, University of California, One Shields Avenue, Davis, CA 95616 Department of Astrophysical Sciences, Princeton University, Princeton, NJ 08544 U.S. Naval Observatory Flagstaff Station,(More)
Articles in this issue describe new capabilities with three instruments in different areas of the resolution–field of view–wavelength domain. Counter-clockwise from upper right: • 0.13” resolution with the Hokupa’a/ QUIRC adaptive optics camera at Gemini North. [Page 3] • 7.3’-square field with the four-color IR camera SQIID at Kitt Peak. [Page 36] • 0.8 ×(More)
e14624 Background: Carcinoid tumors are known to secrete neurohumoral substances resulting in the manifestation of carcinoid syndrome. There are only rare reports of severe psychiatric symptoms associated with carcinoid disease. We report our institutional experience of two pts with advanced carcinoid disease who developed significant psychiatric symptoms(More)
As our capacity to study ever-expanding domains of our science has increased (including the time domain, non-electromagnetic phenomena, magnetized plasmas, and numerous sky surveys in multiple wavebands with broad spatial coverage and unprecedented depths), so have the horizons of our understanding of the Universe been similarly expanding. This expansion is(More)
The six-band (ugrizy) LSST survey will yield a sample of ten billion galaxies (§ 3.7.2) over a huge volume. It will be the largest photometric galaxy sample of its time for studies of the largescale structure of the Universe, and will characterize the distribution and evolution of matter on extragalactic scales through observations of baryonic matter at a(More)
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