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- lisa. nasa. gov
The LISA web site (http: lisa nasa gov) describes the science objectives of the mission; the proposed mission itself, the spacecraft and instruments; some of the technology challenges that must be met; and a background primer on gravitational waves
- Microsoft Word - RFI. doc - lisa. nasa. gov
The LISA web site (http: lisa nasa gov) describes the science objectives of the mission; the proposed mission itself, the spacecraft and instruments; some of the technology challenges that must be met; and a background primer on gravitational waves
- ASTRO2020 DECADAL SCIENCE WHITE PAPER - lisa. nasa. gov
ected through-out the galaxy by LISA Thanks to their high SNR, these short-period UCBs will be identi ed early in a GW mission (within a few weeks of observing) and well localized, making them ex-cellent candid
- LISA Frequently Asked Questions (FAQs) - NASA
LISA's goal is not limited to discovering low frequency gravitational waves, but to use them as a new window into astrophysical and physical phenomena that cannot be studied any other way
- Top Level Requirements for the LISA Pathfinder Mission
LISA, a joint ESA Horizons 2000+ Cornerstone NASA Beyond Einstein Great Observatory mission, is designed to detect low frequency gravitational waves emitted from the most energetic events in the known universe The technologies required for LISA are many and extremely challenging
- Multimessenger science opportunities with mHz gravitational waves
LISA will open the mHz band of gravitational waves (GWs) to the astronomy community The strong gravity which powers the variety of GW sources in this band is also crucial in a number of important astrophysical processes at the current frontiers of astronomy
- Overview of LISA Pathfinder - NASA
LISA Path nder, the second of the European Space Agency's Small Missions for Advanced Research in Technology (SMART), is a dedicated technology demonstra-tor for the joint ESA NASA Laser Interferometer Space Antenna (LISA) mission [1]
- BUILDING A FIELD - lisa. nasa. gov
The data analysis challenges for the lower frequency bands of Pulsar Timing and LISA will require expertise from across the elds of astronomy, physics, and data science, and present an exciting opportunity for innovative data analysis techniques in signal identi ca-tion, parameter estimation, data access, source catalogs, and multimessenger
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