Difference between revisions of "Members"

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[[File:JanHarms.jpg|'''Jan Harms''' (loves pizza Hawai'i). Working on instrument modelling, environmental-noise mitigation, and data analysis with emphasize on compact-binary parameter estimation and primordial GW searches.|thumb|400px|left]]
 
[[File:JanHarms.jpg|'''Jan Harms''' (loves pizza Hawai'i). Working on instrument modelling, environmental-noise mitigation, and data analysis with emphasize on compact-binary parameter estimation and primordial GW searches.|thumb|400px|left]]
  
[[File:Ashish Sharma.jpg|'''Ashish Sharma'''. Working on stochastic cosmological gravitational-wave background and data analysis techniques to detect primordial signals from the early universe with GW detectors.
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[[File:Ashish Sharma.jpg|'''Ashish Sharma'''. I am working on how gravitational-wave (GW) detectors can be used to understand the cosmological phenomenon. Currently, I am focused on stochastic cosmological gravitational-wave background and data analysis techniques to detect primordial signals from the early universe with GW detectors.  
 
|thumb|400px|left]]
 
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Revision as of 22:21, 29 August 2019

Jan Harms (loves pizza Hawai'i). Working on instrument modelling, environmental-noise mitigation, and data analysis with emphasize on compact-binary parameter estimation and primordial GW searches.
Ashish Sharma. I am working on how gravitational-wave (GW) detectors can be used to understand the cosmological phenomenon. Currently, I am focused on stochastic cosmological gravitational-wave background and data analysis techniques to detect primordial signals from the early universe with GW detectors.