Galactic binary science with the new LISA design

@article{Cornish2017GalacticBS,
  title={Galactic binary science with the new LISA design},
  author={N. Cornish and T. Robson},
  journal={arXiv: Instrumentation and Methods for Astrophysics},
  year={2017},
  volume={840},
  pages={012024}
}
Building on the great success of the LISA Pathfinder mission, the outlines of a new LISA mission design were laid out at the 11th International LISA Symposium in Zurich. The revised design calls for three identical spacecraft forming an equilateral triangle with 2.5 million kilometer sides, and two laser links per side delivering full polarization sensitivity. With the demonstrated Pathfinder performance for the disturbance reduction system, and a well studied design for the laser metrology, it… Expand

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References

SHOWING 1-10 OF 14 REFERENCES
Laser Interferometer Space Antenna
Following the selection of The Gravitational Universe by ESA, and the successful flight of LISA Pathfinder, the LISA Consortium now proposes a 4 year mission in response to ESA's call for missionsExpand
Characterizing the galactic gravitational wave background with LISA
We present a Monte Carlo simulation for the response of the Laser Interferometer Space Antenna (LISA) to the galactic gravitational wave background. The simulated data streams are used to estimateExpand
Sub-Femto-g Free Fall for Space-Based Gravitational Wave Observatories: LISA Pathfinder Results.
We report the first results of the LISA Pathfinder in-flight experiment. The results demonstrate that two free-falling reference test masses, such as those needed for a space-based gravitational waveExpand
Prospects for observing ultracompact binaries with space-based gravitational wave interferometers and optical telescopes
ABSTRACT Space-based gravitational wave interferometers are sensitive to the galactic population ofultracompact binaries. An important subset of the ultracompact binary population are thosestars thatExpand
Reproducing GW150914: the first observation of gravitational waves from a binary black hole merger
TLDR
This is the first direct detection of gravitational waves and the first observation of a binary black hole merger, and these observations demonstrate the existence of binary stellar-mass black hole systems. Expand
Reconstructing the evolution of white dwarf binaries: further evidence for an alternative algorithm for the outcome of the common-envelope phase in close binaries
We determine the possible masses and radii of the progenitors of white dwarfs in binaries from fits to detailed stellar evolution models and use these to reconstruct the mass-transfer phase in whichExpand
Gravitational-wave Emission from Compact Galactic Binaries
Compact Galactic binaries where at least one member is a white dwarf (WD) or neutron star constitute the majority of individually detectable sources for future low-frequency space-basedExpand
Supernova Type Ia progenitors from merging double white dwarfs - Using a new population synthesis model
The study of Type Ia supernovae (SNIa) has lead to greatly improved insights into many fields in astrophysics, however a theoretical explanation of the origin of these events is still lacking. WeExpand
A search for the hidden population of AM CVn binaries in the Sloan Digital Sky Survey
We present the latest results from a spectroscopic survey designed to uncover the hidden population of AM Canum Venaticorum (AM CVn) binaries in the photometric data base of the Sloan Digital SkyExpand
Tests of Bayesian model selection techniques for gravitational wave astronomy
The analysis of gravitational wave data involves many model selection problems. The most important example is the detection problem of selecting between the data being consistent with instrumentExpand
...
1
2
...