Articles by Casey Barr in JoVE
用数字全息显微镜 (DHM) 定量化低浓度微生物 Manuel Bedrossian1, Casey Barr2, Chris A. Lindensmith3, Kenneth Nealson2, Jay L. Nadeau1 1Department of Medical Engineering, California Institute of Technology, 2Department of Earth Sciences, University of Southern California, 3Jet Propulsion Laboratory, California Institute of Technology 数字全息显微镜 (DHM) 是一种体积技术, 允许成像样品50-100X 厚比明显微镜在可比的分辨率, 与重点进行后处理。DHM 用于识别、计数和跟踪非常低密度的微生物, 并与光学密度测量、平板计数和直接计数相比较。
Other articles by Casey Barr on PubMed
Limits on Gravitational-wave Emission from Selected Pulsars Using LIGO Data Physical Review Letters. May, 2005 | Pubmed ID: 15904354 We place direct upper limits on the amplitude of gravitational waves from 28 isolated radio pulsars by a coherent multidetector analysis of the data collected during the second science run of the LIGO interferometric detectors. These are the first direct upper limits for 26 of the 28 pulsars. We use coordinated radio observations for the first time to build radio-guided phase templates for the expected gravitational-wave signals. The unprecedented sensitivity of the detectors allows us to set strain upper limits as low as a few times 10(-24). These strain limits translate into limits on the equatorial ellipticities of the pulsars, which are smaller than 10(-5) for the four closest pulsars.