‘The definitive version is available at www.blackwell-synergy.com.’ Copyright Blackwell Publishing DOI: 10.1111/j.1365-2966.2008.13061.xPeer reviewe
High-precision radial-velocimetry (RV) is until now the more efficient way to discover planetary sys...
Context. The detection and characterisation of Earth-like planets with Doppler signals of the order ...
We have been using the Keck I High Resolution Spectrograph to search for planetary companions in the...
One of the most promising methods of discovering nearby, low-mass planets in the habitable zones of ...
‘The definitive version is available at www3.interscience.wiley.com '. Copyright Blackwell Publishin...
Radial velocity (RV) detection of planets is hampered by astrophysical processes on the surfaces of ...
The radial velocity (RV), or Doppler, technique is one of the most successful methods in the search ...
There has been tremendous progress in observing oscillations in solar-type stars. In a few short yea...
Accounting for stellar activity is a crucial component of the search for ever-smaller planets orbiti...
The Radial Velocity (RV) method, measuring the Doppler Shifts from stellar spectra, is widely used f...
Researchers are measuring small changes in the line-of-sight velocities of stars to detect the oscil...
Future generations of precise radial velocity (RV) surveys aim to achieve sensitivity sufficient to ...
ACC acknowledges support from the Science and Technology Facilities Council (STFC) consolidated gran...
Context. Stellar noise produced by oscillations, granulation phenomena (granulation, mesogranulation...
The Kepler Space Telescope observed over 15,000 stars for asteroseismic studies. Of these, 75% of dw...
High-precision radial-velocimetry (RV) is until now the more efficient way to discover planetary sys...
Context. The detection and characterisation of Earth-like planets with Doppler signals of the order ...
We have been using the Keck I High Resolution Spectrograph to search for planetary companions in the...
One of the most promising methods of discovering nearby, low-mass planets in the habitable zones of ...
‘The definitive version is available at www3.interscience.wiley.com '. Copyright Blackwell Publishin...
Radial velocity (RV) detection of planets is hampered by astrophysical processes on the surfaces of ...
The radial velocity (RV), or Doppler, technique is one of the most successful methods in the search ...
There has been tremendous progress in observing oscillations in solar-type stars. In a few short yea...
Accounting for stellar activity is a crucial component of the search for ever-smaller planets orbiti...
The Radial Velocity (RV) method, measuring the Doppler Shifts from stellar spectra, is widely used f...
Researchers are measuring small changes in the line-of-sight velocities of stars to detect the oscil...
Future generations of precise radial velocity (RV) surveys aim to achieve sensitivity sufficient to ...
ACC acknowledges support from the Science and Technology Facilities Council (STFC) consolidated gran...
Context. Stellar noise produced by oscillations, granulation phenomena (granulation, mesogranulation...
The Kepler Space Telescope observed over 15,000 stars for asteroseismic studies. Of these, 75% of dw...
High-precision radial-velocimetry (RV) is until now the more efficient way to discover planetary sys...
Context. The detection and characterisation of Earth-like planets with Doppler signals of the order ...
We have been using the Keck I High Resolution Spectrograph to search for planetary companions in the...
DOI
Add to ORKG