LIGO-G040062-00-Z 18 March 2004Penn State University1 GravEn Simulation Engine Amber L. Stuver

Slides:

Advertisements

Similar presentations

Modeling Electrical Systems With EMTP-RV

Advertisements

LIGO-G Z Status and Plans for the LIGO-TAMA Joint Data Analysis Patrick Sutton LIGO Laboratory, Caltech, for the LIGO-TAMA Joint Working Group.

Goal: to rotate a figure around a central point

LIGO- G Z August 19, 2004August 2004 LSC Meeting 1 Towards an Astrophysics-Based Burst ETG Tuning Keith Thorne Penn State University Relativity.

1 Steps for Production Code Generation Wind Turbine Pitch Controller 1. Generate test data and extract controller 2. Discretize Change integrator blocks.

Dale E. Gary Professor, Physics, Center for Solar-Terrestrial Research New Jersey Institute of Technology 1 3/16/2012OVSA Preliminary Design Review.

Visual Traffic Simulation Thomas Fotherby. Objective To visualise traffic flow. –Using 2D animated graphics –Using simple models of microscopic traffic.

LIGO-G Z External Triggers Circulation only within LIGO I authorship list Status of the Triggered Burst Search (highlights from LIGO DCC# T Z,

Searching for pulsars using the Hough transform Badri Krishnan AEI, Golm (for the pulsar group) LSC meeting, Hanford November 2003 LIGO-G Z.

LIGO- G Z AJW, Caltech, LIGO Project1 Use of detector calibration info in the burst group

Frequency Response of LIGO Interferometers Andrew Weber University of Maryland (no relation) SURF Student Lecture Series Advisor: Andri Gretarsson.

LIGO Response to High Frequency Gravitational Waves Implications for Calibration Hunter Elliott Mentors: Rick Savage, Greg Mendell, Malik Rakhmanov.

Abstract In this project we expand our previous work entitled "Design of a Robotic Platform and Algorithms for Adaptive Control of Sensing Parameters".

Inputs to Signal Generation.vi: -Initial Distance (m) -Velocity (m/s) -Chirp Duration (s) -Sampling Info (Sampling Frequency, Window Size) -Original Signal.

LIGO-G Z Coherent Coincident Analysis of LIGO Burst Candidates Laura Cadonati Massachusetts Institute of Technology LIGO Scientific Collaboration.

Waveburst DSO: current state, testing on S2 hardware burst injections Sergei Klimenko Igor Yakushin LSC meeting, March 2003 LIGO-G Z.

Security and QoS Self-Optimization in Mobile Ad Hoc Networks ZhengMing Shen and Johnson P. Thomas Presented by: Sharanpal singh.

LIGO- G Z AJW, Caltech, LIGO Project1 Use of detector calibration info in the burst group

DelayRatio: A Gravitational Wave Event Physical Likelihood Estimator Based on Detection Delays and SNR Ratios Amber L. Stuver LIGO Livingston ObservatoryCalifornia.

LIGO- G Z 03/23/2005LSC Meeting March BlockNormal Near-Online S4 Burst Analysis Keith Thorne Penn State University Relativity Group (Shantanu.

A coherent null stream consistency test for gravitational wave bursts Antony Searle (ANU) in collaboration with Shourov Chatterji, Albert Lazzarini, Leo.

7 th SMOS Workshop, Frascati, October /17 AMIRAS campaign Fernando Martin-Porqueras.

The RIDGE pipeline as a method to search for gravitational waves associated with magnetar bursts LIGO-G Z Jason Lee, Tiffany Summerscales (Andrews.

Software Status  Last Software Workshop u Held at Fermilab just before Christmas. u Completed reconstruction testing: s MICE trackers and KEK tracker.

LIGO-G Z A Coherent Network Burst Analysis Patrick Sutton on behalf of Shourov Chatterji, Albert Lazzarini, Antony Searle, Leo Stein, Massimo.

EE 113D Fall 2008 Patrick Lundquist Ryan Wong

S.Klimenko, December 2003, GWDAW Performance of the WaveBurst algorithm on LIGO S2 playground data S.Klimenko (UF), I.Yakushin (LLO), G.Mitselmakher (UF),

9. What is the measure of angle b? What vocabulary words apply to this Figure? 1) 2) A.1,2,and 3 B.1 and 2 C.1 and 3 D.2 and A point is located at.

High Speed Digital Systems Lab. Agenda  High Level Architecture.  Part A.  DSP Overview. Matrix Inverse. SCD  Verification Methods. Verification Methods.

LSC-March  LIGO End to End simulation  Lock acquisition design »How to increase the threshold velocity under realistic condition »Hanford 2k simulation.

S.Klimenko, August 2005, LSC, G Z Constraint likelihood analysis with a network of GW detectors S.Klimenko University of Florida, in collaboration.

Provides an overview of the main components in the simulator. Shows the relation between functions, data and user-inputs. The design is broken up into.

S.Klimenko, July 14, 2007, Amaldi7,Sydney, G Z Detection and reconstruction of burst signals with networks of gravitational wave detectors S.Klimenko,

G030XXX-00-Z Excess power trigger generator Patrick Brady and Saikat Ray-Majumder University of Wisconsin-Milwaukee LIGO Scientific Collaboration.

A Waveform Consistency Test for Binary Inspirals using LIGO data LSC Inspiral Analysis Working Group LIGO-G Z LSC Meeting Andres C. Rodriguez.

Remcom Inc. 315 S. Allen St., Suite 416  State College, PA  USA Tel:  Fax:   ©

T.Akutsu, M.Ando, N.Kanda, D.Tatsumi, S.Telada, S.Miyoki, M.Ohashi and TAMA collaboration GWDAW10 UTB Texas 2005 Dec. 13.

LIGO- G Z August 17, 2005August LSC Meeting – ASIS Session 1 Recovering Hardware Injection Waveforms with Maximum Entropy Tiffany Summerscales.

S.Klimenko, LSC, August 2004, G Z BurstMon S.Klimenko, A.Sazonov University of Florida l motivation & documentation l description & results l.

LIGO-G Z Confidence Test for Waveform Consistency of LIGO Burst Candidate Events Laura Cadonati LIGO Laboratory Massachusetts Institute of Technology.

S.Klimenko, March 2003, LSC Burst Analysis in Wavelet Domain for multiple interferometers LIGO-G Z Sergey Klimenko University of Florida l Analysis.

LIGO-G Z GWDAW9 December 17, Search for Gravitational Wave Bursts in LIGO Science Run 2 Data John G. Zweizig LIGO / Caltech for the LIGO.

Peter Shawhan The University of Maryland & The LIGO Scientific Collaboration Penn State CGWP Seminar March 27, 2007 LIGO-G Z Reaching for Gravitational.

LIGO-G Z Status of the LIGO-TAMA Joint Bursts Search Patrick Sutton LIGO Laboratory, Caltech, for the LIGO-TAMA Joint Working Group.

LIGO- G Z AJW, Caltech, LIGO Project1 First look at Injection of Burst Waveforms prior to S1 Alan Weinstein Caltech Burst UL WG LSC meeting, 8/21/02.

LIGO-G Z TFClusters Tuning for the LIGO-TAMA Search Patrick Sutton LIGO-Caltech.

LIGO- G Z March 23, 2005March LSC Meeting – ASIS Session 1 Extracting Supernova Information from a LIGO Detection Tiffany Summerscales Penn State.

S5 First Epoch BNS Inspiral Results Drew Keppel 1 representing the Inspiral Group 1 California Institute of Technology Nov LSC Meeting MIT, 4 November.

1 MONALISA Compact Straightness Monitor Simulation and Calibration Week 2 Report By Patrick Gloster.

LIGO-G E Data Simulation for the DMT John Zweizig LIGO/Caltech.

LIGO-G Z 23 October 2002LIGO Laboratory NSF Review1 Searching for Gravitational Wave Bursts: An Overview Sam Finn, Erik Katsavounidis and Peter.

LIGO-G Z Status of the LIGO-TAMA Joint Bursts Search Patrick Sutton LIGO Laboratory, Caltech, for the LIGO-TAMA Joint Working Group.

Import and Implement QuartusII Megawizard library to modelsim simulation.

LIGO-G Z S5 calibration: time dependent coefficients  Myungkee Sung, Gabriela González, Mike Landry, Brian O’Reilly, Xavier Siemens,…

Searching for pulsars using the Hough transform

A.M. Sintes for the pulgroup

Waveform Generator Update– September ‘06

Maria Principe University of Sannio, Benevento, Italy

Targeted Searches using Q Pipeline

SLOPE: A MATLAB Revival

University of Wisconsin-Milwaukee

You need: Pencil Agenda Scrap Paper AP log Math book Calculator

First look at Injection of Burst Waveforms prior to S1

M Ashley - LSC Meeting – LIGO Hanford, 12 Nov 2003

Status of the LIGO-TAMA Joint Data Analyses

Recovering Hardware Injection Waveforms with Maximum Entropy

Status and Plans for the LIGO-TAMA Joint Data Analysis

Performance of the WaveBurst algorithm on LIGO S2 playground data

IMPLEMENTATION OF SMART ANTENNA USING

Presentation transcript:

LIGO-G Z 18 March 2004Penn State University1 GravEn Simulation Engine Amber L. Stuver

LIGO-G Z 18 March 2004Penn State University2 Capabilities Full sky Population simulations Simulates both  and  polarizations Projects onto antenna pattern Calibrated Multi-detector »MATLAB »Documentation available in DCC: LIGO-T Z »Code to become available

LIGO-G Z 18 March 2004Penn State University3 How does GravEn work? Developed in MATLAB Compiles to stand alone using the MATLAB Compiler Toolbox Does not need MATLAB toolboxes Driver function »Flexible usage modes »Process input through list function »Loop through the list: –Generate waveform –Project onto antenna pattern –Transform to AS_Q for given IFO –Save result and write info to log file

LIGO-G Z 18 March 2004Penn State University4 Simulation Controls # sims, type, amplitude, start time, internal and external angles Amplitude can be fixed or chosen from a random logarithmic or linear distribution Source sky location (external) »Randomly choose location on sky or chose to be zenith to IFO »Draw from file containing a population Source orientation (internal) »Chose a random or optimal orientation (optimal = no rotations) »Fixed

LIGO-G Z 18 March 2004Penn State University5 Waveform Generation Specify perturbation as a function of time Generates metric perturbation in TT gauge given a source’s orientation to line of sight Code can be adapted to accept previously generated waveforms (ZM, etc.) »This adaptation will be implemented soon

LIGO-G Z 18 March 2004Penn State University6 Multiple Detectors All calculations done at the center of the earth »Common coordinate origin »Start time of signal adjusted for GW’s time of flight Multi-detector (including TAMA, GEO, etc.) »Detectors other than LIGO will be added before code release »Sampling rate adjusted for appropriate IFO IFO’s response function used to transform strain into AS_Q

LIGO-G Z 18 March 2004Penn State University7 For the Future Expand available waveforms Working on galactic population »Will be available with engine as data set Undergo code review »Code will meet PSU MATLAB coding standard; T Z Will be used for LIGO/TAMA simulations with BlockNormal Code will become available after code review »Will be available on WWW until central code distribution available