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Goddard Gravitational Wave Astrophysics Group

Goddard Gravitational Wave Astrophysics Group. G oddard G ravitational W ave A strophysics G roup (GGWAG) Joan Centrella Laboratory for High Energy Astrophysics NASA/Goddard Space Flight Center LIGO-G010274-00-Z. Gravitational Wave Astrophysics at NASA/Goddard.

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Goddard Gravitational Wave Astrophysics Group

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  1. Goddard Gravitational Wave Astrophysics Group Goddard Gravitational Wave Astrophysics Group (GGWAG) Joan Centrella Laboratory for High Energy Astrophysics NASA/Goddard Space Flight Center LIGO-G010274-00-Z

  2. Gravitational Wave Astrophysics at NASA/Goddard Gravitational Wave Astrophysics is located within the Laboratory for High Energy Astrophysics(LHEA) (Nicholas White, Lab Chief) http://lhea.gsfc.nasa.gov LHEA has 2 science branches: • X-Ray Astrophysics Branch(Rob Petre, Branch Head) • Relevant missions include Astro-E2, RXTE, and Constellation X • Gamma Ray, Cosmic Ray and Gravitational Wave Astrophysics Branch(Neil Gehrels, Branch Head) • Relevant missions include INTEGRAL, SWIFT, GLAST, ACE, and LISA • Gravitational Wave Astrophysics Group recently created in support of LISA mission

  3. Gravitational Wave Astrophysics Group Senior Members: • Jordan Camp • Joan Centrella • Stephen Merkowitz • Robin (Tuck) Stebbins (LISA Project Scientist) • Bonnard Teegarden NRC Senior Associate: • J. David Brown Postdocs: • John Baker • Dale Choi Graduate Students: • Orhan Donmez • Breno Imbiriba

  4. Gravitational Wave Astrophysics at Goddard Numerical Relativistic Astrophysics Group John BakerDale Choi J. David BrownOrhan Donmez Joan Centrella, group leader Breno Imbiriba • Large scale numerical simulations of astrophysical gravitational wave sources such as binary neutron star and black hole coalescences, stellar collapse, rotational instabilities … • Focus on sources of interest to LISA and ground-based detectors… • High performance computing, adaptive mesh refinement (AMR), Lazarus project … • Astrophysical source identification, data analysis…

  5. Goddard Gravitational Wave Astrophysics Group Current Members of GGWAG Senior PersonnelPostdoctoral Jordan Camp John Baker Joan Centrella Robin (Tuck) Stebbins Tod Strohmayer (X-Ray Astrophysics) Plus possible contributions from students and collaborators (non-LSC members)

  6. GGWAG contributions Joan Centrella and John Baker • Catalogs of Astrophysical Gravitational Waveforms Compile catalogs of computed gravitational waveforms from sources such as binary neutron star and black hole coalescence, rotational instabilities, gravitational collapse… Catalogs will be available online, and will be updated as new models become available. • Analysis of Model Calculations and Astrophysical Scenario Building Time-frequency analysis of the source models in the catalog will be carried out; noise and other detector characteristics will be added. Given assumed signals from the detectors, scenarios for astrophysical upper limits will be constructed. This work will be done in collaboration with the Bursts Upper Limits Group.

  7. GGWAG contributions Tod Strohmayer • Astrophysics of Gravitational Wave Sources Observations in the X-ray and other wavebands will be used to help model/determine/compute the strength and character of the gravitational wave signals expected from sources such as rotating neutron stars in LMXBs and black hole binaries. • Searches for Gravitational Radiation from Galactic Compact Objects Fast chirp transform (FCT) search strategies for transient (burst) GW signals in correlation with astrophysical triggers from compact objects such as X-ray bursts and accretion outbursts will be investigated. Strohmayer will also begin studying search strategies for coherent GW signals from rotating neutron stars in LMXBs.

  8. GGWAG contributions Jordan Camp • Detector Characterization Work will continue on characterization of detector noise, with emphasis on frequency noise, including prestabilized laser noise and frequency noise associated with the suspended cavities (both in and out of the LIGO signal band). Both Gaussian and non-Gaussian noise will be investigated. This work will take place in the binary inspiral and burst upper limit groups. • LIGO Core Optics Program Camp will be involved in the LIGO core optics program, including the use of commissioning data to diagnose the optical performance of the interferometers, and participation in the advanced LIGO optics R&D.

  9. GGWAG contributions R. Stebbins • Seismic Isolation Sytems • Participate in mechanical and system design and fabrication • Participate in prototype commissioning and testing • Access Goddard engineering expertise where appropriate

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