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Type Preview Title Media Description Date
The universe in the gravitational wave range (long) Sound file from the Mock Data Challenge that contains several easy-to-hear coalescences...
Jan 17, 2013
DA Spectrogram Data Analysis Spectrogram
May 01, 2013
Fundamental physics: GW_Notes_04_fundamental_physics.pdf GW Notes was born from the need for a journal where the distinct communities involved in...
May 24, 2013
University of Glasgow University of Glasgow The University of Glasgow is the fourth-oldest university in the english-speaking world...
Jun 27, 2013
LISA sensitivity: strain sensitivity with instrumental and confusion noise, two arm configuration. This is the sensitivity in units of strain per sqrt(Hz). It contains the instrumental...
Jan 07, 2014
Hubble Constant Hubble Constant Spitzer refines the value of Hubble's constant to 97 percent accuracy.
Oct 22, 2012
GRS Vacuum Chamber
Apr 30, 2013
Shocktest Shocktest The LISA Pathfinder spacecraft composite (science module above, propulsion module below)...
May 21, 2013
ICE Group ICE Group A group of the Institute of Space Sciences, Spain (ICE).
Jun 24, 2013
LISA sensitivity: PSD for the TDI X-Michelson combination This is the power spectral density (PSD) for the TDI X-Michelson combination. It...
Jan 06, 2014
Pulsar and Star Remnant Pulsar and Star Remnant
Oct 19, 2012
LPF - Noise Breakdown LPF - Noise Breakdown
Apr 29, 2013
eLISA - payload LISA - Payload
May 17, 2013
Galaxy - NGC 1277 Galaxy - NGC 1277 Invisible gravitational trap: the centre of the NGC 1277 disk galaxy harbours a black...
Jun 10, 2013
LPF optical bench prepared for integration into core assembly 2 The LPF optical bench is being prepared for integration into core assembly.
Sep 01, 2013
LISA - Consortium Structure LISA - Consortium Structure
Jan 12, 2013
History of the Universe History of the Universe LISA will measure the gravitational wave cosmic background where WMAP measures the cosmic...
May 30, 2013
AEI Hannover, Germany AEI Hannover - Germany Max Planck Institute for Gravitational Physics (Albert Einstein Institute), Potsdam and...
Jun 25, 2013
Neutron Star - Merger Neutron Star - Merger Two neutron stars merge in a few milliseconds to form a black hole. A large magnetic...
Jun 18, 2013
LPF - AEI Optical Bench Tests LPF - AEI Optical Bench Tests Before being declared spaceworthy, the LISA Pathfinder optical bench underwent a series...
Jun 28, 2013
LISA - Triple Orbit LISA - Triple Orbit One of LISA´s key features is the set of three orbits in a near-equilateral triangular...
Aug 23, 2012
LISA will observe gravitational waves in space LISA - Observing Gravitational Waves LISA will observe gravitational waves in space
Feb 05, 2013
M31 Spiral Galaxy Galaxy - M31 The Andromeda Galaxy is a spiral galaxy approximately 2.5 million light-years (2.4×1019 ...
May 01, 2013
LPF - IABG LPF ready to enter test chamber LISA Pathfinder at the IABG test facilities in Ottobrunn, GermanyFinal preparation work...
May 25, 2013
Soyuz launch Soyuz launch
Jun 27, 2013
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Apr 02, 2014
Dust-bound supermassive black hole Black Hole - Dust-bound supermassive black hole "Black holes lurk at the centres of active galaxies in environments not unlike those...
Jun 10, 2013
LPF - Laser Modulator Unit LPF - Laser Modulator Unit
May 01, 2013
Data Analysis: GW_Notes_01_data_analysis.pdf GW Notes was born from the need for a journal where the distinct communites involved in...
May 24, 2013
LISA sensitivity: strain sensitivity with instrumental noise only, two arm configuration.   This is the sensitivity in units of strain per sqrt(Hz). It contains the instrumental...
Jan 07, 2014

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