Difference between revisions of "Members"

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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 GW background and data analysis techniques to detect primordial signals from the early universe with GW detectors.  
 
[[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 GW background and data analysis techniques to detect primordial signals from the early universe with GW detectors.  
 
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[[File:Francesca Badaracco.jpg|thumb|left|'''Francesca Badaracco'''. She is working on Newtonian noise mitigation for underground and surface detectors in order to improve their sensitivity. She also focuses on detector calibration. ]]

Revision as of 18:57, 30 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 GW background and data analysis techniques to detect primordial signals from the early universe with GW detectors.
Francesca Badaracco. She is working on Newtonian noise mitigation for underground and surface detectors in order to improve their sensitivity. She also focuses on detector calibration.
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