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Finding Optical Transients with LIGO and Virgo Data

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Presentation on theme: "Finding Optical Transients with LIGO and Virgo Data"— Presentation transcript:

1 Locating and Observing Optical Counterparts to Unmodeled Pulses in Gravitational Waves
Finding Optical Transients with LIGO and Virgo Data Jonah Kanner University of Maryland LOOC UP LIGO-G Z /12/2008

2 Introduction to LOOC UP
GW Bursts are associated with cosmic violence Likely emission in EM as well as GW spectrum Analyze GW data in real time Actively seek EM counterparts to candidate GW events S6/VSR2 Starts in 2009! LOOC UP EGM /12/2008

3 Orphan Afterglow Model
SH GRB GW X-Ray/Optical/Radio/IR Gamma Rays LOOC UP EGM /12/2008

4 Global IFO Network (LIGO/Virgo) Global Telescope Network (TBA)
Identification Verification Reconstruction Scheduling Images of Virgo, LIGO, ROTSE, SWIFT, and Palomar Transient Factory

5 Interesting Challenges
Online Analysis Months to minutes, data transfer, vetoes Position Reconstruction Timing, Penalty factors, “Bayesian”, Gal. Catalog Network Definition Coverage in angle, depth, and frequency Scheduling SNR, location, time, weather, past  when & where Image Processing/Data Analysis How to spot a transient, How to set ULs and FARs LOOC UP EGM /12/2008

6 Pilot Study LIGO S5 DNS Pos-avg. range ~15 Mpc
Catalog: Globular clusters & galaxies 20 Mpc cut-off Modified version of CBC catalog 2766 Objects LOOC UP EGM /12/2008

7 Pilot Study For each candidate event, we seek galaxies within the error box of the estimated source location. These galaxies are then imaged for transients. LOOC UP EGM /12/2008

8 LOOC UP Thank you !! Columbia Univ Szabolcs Marka, Jennifer Piscionere
Univ. of Maryland Jonah Kanner, Peter Shawhan, Tracy Huard Carnegie Instit. of Washington David Murphy Thank you !! LOOC UP EGM /12/2008


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