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“Reese” Haywood - Physics Department - University of Notre Dame

“Reese” Haywood - Physics Department - University of Notre Dame

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annual machine quality assurance, acceptance testing and commissioning.Responsibilities•Protection <strong>of</strong> the patient and others from potentially harmful or excessive radiationthrough monthly and annual Machine Calibration and Room Surveys•Establishment <strong>of</strong> adequate protocols to ensure accurate patient dosimetry, review <strong>of</strong>patient charts throughout entire treatment process•Measurement and characterization <strong>of</strong> radiation, determination <strong>of</strong> delivered dose,Measurements <strong>of</strong> IMRT Patient Plans on treatment machine using Mapcheck•Development <strong>of</strong> second check s<strong>of</strong>tware for Gamma Med Plus HDR afterloader•Development <strong>of</strong> Winston-Lutz analysis tool•Development <strong>of</strong> Portal Dosimetry Analysis toolEquipmentThe Cancer Care at Memorial Hospital is a comprehensive cancer center which housestwo Varian linear accelerators (Trilogy and 21-Ex δ), GE CT simulator and Gamma MedPlus HDR Afterloader. Trilogy is On-Board Imaging, Cone-Beam CT, Portal Vision,Respiratory Gating, IMRT and RapidArc. Treatment Planning is completed with Eclipseand paperless, film-less patient charting is accomplished using ARIA.Visiting Lecturer in <strong>Physics</strong> and Mathematics, 2006-2007, Indiana <strong>University</strong>Southeast, New Albany, INTeach Calculus Based <strong>Physics</strong> and Algebra Based <strong>Physics</strong> along with relevantLaboratoriesBinary Neutron Star Simulation, Grant Mathews, 2005-2006, <strong>University</strong> <strong>of</strong> <strong>Notre</strong><strong>Dame</strong>, <strong>Notre</strong> <strong>Dame</strong>, INRelativistic Hydrodynamic Simulation <strong>of</strong> Binary neutron stars in close orbits to predictthe gravitational radiation produced by the motion, main code written and updated usingFORTRAN 77, utility programs developed in Mathematica for solving the TOVequation, and IDL for making movies <strong>of</strong> the simulation.High Resolution Spectroscopy <strong>of</strong> Disks Around Proto-stars, Terry Rettig, 2002-2005, <strong>University</strong> <strong>of</strong> <strong>Notre</strong> <strong>Dame</strong>, <strong>Notre</strong> <strong>Dame</strong>, INTake and analyze high resolution near-infrared spectra <strong>of</strong> developing (proto-) stars andstar forming regions and exoplanets, using IDL for analysis and display <strong>of</strong> spectra andMathematica program for predicting the absorption coefficient <strong>of</strong> gases in the planetarydiscs.Semiconductor Research, Jacek Furdyna, Summer 2001, <strong>University</strong> <strong>of</strong> <strong>Notre</strong> <strong>Dame</strong>,<strong>Notre</strong> <strong>Dame</strong>, INSelf-organization <strong>of</strong> Ge Quantum Dots Grown by Molecular Beam Epitaxy, RobertNemanich, Summer 2000, North Carolina State <strong>University</strong>, Raleigh, NCHonors and Awards<strong>Department</strong> <strong>of</strong> <strong>Physics</strong> Graduate Student Fellowship for academic year 2005-2006<strong>University</strong> <strong>of</strong> <strong>Notre</strong> <strong>Dame</strong> Summer Grant Writing Fellowship, June 2003Outstanding Graduate Student Teacher Award for Excellence in Teaching, March 2003Graduated Magna Cumme Laude, King College, May 2001

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