'Background rate' presentation slideshows

Professor Julie Quinlivan University of Notre Dame Australia

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WELCOME!!

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THE BIOLOGICAL EFFECTS OF IONIZING RADIATION

THE BIOLOGICAL EFFECTS OF IONIZING RADIATION. Lesley Hines lhines@ehs.ufl.edu Environmental Health and Safety Radiation Control and Radiological Services. The Effects of Radiation. Time Scales. Physics 10 -15 seconds Initial ionization Chemistry 10 -9 seconds

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An Ultra-low-background detector for axion search

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The Very-Low Energy Neutrino Factory physics with a ? storage ring Alan Bross

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ACADs (08-006) Covered Keywords

Detector Efficiency. ACADs (08-006) Covered Keywords Efficiency, LLD, CPM, DPM, relative efficiency, absolute efficiency, standard deviation, confidence, count time. Description Supporting Material. Detector Efficiency. IRAD 2371 Week 3. Efficiency.

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cast

DE | GA | IA | LA | ME | MA | MI | MN | MO | NY | PA | UT | VT | WI.

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Prospects for the Use of Large Water-Based Anti-neutrino Detectors for Monitoring Fission Bomb Detonations

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Biodiversity Loss and Species Extinction

AP Environmental Science Mr. Grant Lesson 38. Biodiversity Loss and Species Extinction. Objectives:. Define the terms extinction , extirpation and mass extinction . Contrast background extinction rates and periods of mass extinction. Evaluate the primary causes of biodiversity loss.

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No Place Like Home Invasional Meltdown in the New Pangaea

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Collinear resonant ionization laser spectroscopy of rare francium isotopes

IPN Orsay, IKS Leuven, University of Manchester, New York University and University of Birmingham. Collinear resonant ionization laser spectroscopy of rare francium isotopes. The first dedicated ISCOOL experiment. This proposal aims at pushing the limits of laser spectroscopy sensitivity.

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Unit 6: Sustaining Biodiversity

Unit 6: Sustaining Biodiversity. January 8, 2012 AP Environmental Science Mr. Plowman. LT 6A : Discuss the role human activities play in extinction. Biological extinction: a species has disappeared from the earth. Background extinction is an historic, continuous, low level of extinction.

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Detecting Neutrino Transients with optical Follow-up Observations

Detecting Neutrino Transients with optical Follow-up Observations. Marek Kowalski Humboldt-University, Berlin TeV-III Venice , 2007. Gravitative collaps of a very massive, rotating star (>25 M ? ):. Simulation: MacFadyen (2000). Testing the Supernovae-GRB connection. Observation:

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Current Status of Experimental Requirement in Technical Document

Current Status of Experimental Requirement in Technical Document. Xin Qian Caltech. Introduction. Consistent plots for each configuration ( Z hiwen ) Two tables summarize key features and detector requirements We should clarify requirements vs. limitations. SoLID -PVDIS.

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Muon Experiment

Xinjun Guo Dec. 16, 2009. Muon Experiment. Cosmic Rays. Primary: protons( ), light nuclei Secondary: , , others Decay product: , , . Muons. Mean energy near the ground: Total flux crossing unit horizontal area:

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Calibration of the OMNIS-LPC Supernova Neutrino Detector

Calibration of the OMNIS-LPC Supernova Neutrino Detector. Outline OMNIS Experiment and Detectors Lead Slab & Plastic Scintillator Lead Perchlorate SNS2 OMNIS Calibration Experiment Goals LPC Module Event identification Event rate estimates Background rate estimates Conclusion.

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SPring-8 ??????? ???????? ????????????

?????? ???? 2000.4.1. SPring-8 ??????? ???????? ????????????. ????????? ?? ? LEPS collaboration. ????????? ????????? ?????????? ?????????? ?????????????????? ?????. Laser Electron Photon. Electron 8GeV. Laser 3.5eV. Backward Compton scattering. Scattered photon

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LOOC UP Seeking the EM counterparts to gravitational wave signal candidates

LOOC UP Seeking the EM counterparts to gravitational wave signal candidates. Jonah Kanner (University of Maryland) for the LIGO Scientific Collaboration and the Virgo Collaboration together with the TAROT, QUEST and Pi of the Sky teams. LIGO DCC: G0900951-v4.

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Pair-Symmetric Background Analysis

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San Miguel JF et al. Proc ASH 2011;Abstract 476.

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