Skip to search formSkip to main content
You are currently offline. Some features of the site may not work correctly.

SigSpec

SigSpec is an acronym of "SIGnificance SPECtrum" and addresses a statistical technique to provide the reliability of periodicities in a measured… Expand
Wikipedia

Papers overview

Semantic Scholar uses AI to extract papers important to this topic.
2017
2017
Context. Space photometric time series of the most massive members of the young open cluster NGC 2264 allow us to study their… Expand
2011
2011
The two pulsating pre-main sequence (PMS) stars V 588 Mon and V 589 Mon were observed by CoRoT for 23.4 days in 2008 March during… Expand
2011
2011
Context. The CoRoT- Convection Rotation and planetary Transits - space mission provides a unique opportunity to monitor RR Lyrae… Expand
  • figure 1
  • figure 3
  • figure 2
  • figure 5
  • figure 4
2010
2010
{\sc SigSpec} computes the spectral significance levels for the DFT amplitude spectrum of a time series at arbitrarily given… Expand
  • figure 1
  • figure 2
  • figure 3
  • figure 4
  • figure 5
2010
2010
Cinderella is a software solution for the quantitative comparison of time series in the frequency domain. It assigns… Expand
  • figure 1
2009
2009
It has also been suggested that the detection of a wealth of very low amplitude modes in Delta Sct stars was only a matter of… Expand
  • figure 1
  • figure 2
  • table 1
  • figure 3
  • figure 4
Highly Cited
2009
Highly Cited
2009
The Lomb-Scargle periodogram is a common tool in the frequency analysis of unequally spaced data equivalent to least-squares… Expand
  • table 1
  • figure 1
  • figure 4
  • figure 2
  • figure 3
Highly Cited
2008
Highly Cited
2008
Context: Several approaches to estimate frequency, phase and amplitude errors in time series analyses were reported in the… Expand
Highly Cited
2007
Highly Cited
2007
Identifying frequencies with low signal-to-noise ratios in time series of stellar photometry and spectroscopy, and measuring… Expand
  • figure 1
  • figure 2
  • figure 3
  • figure 4
  • figure 5
2004
2004
Context. Herbig Ae/Be stars are intermediate-mass pre-main sequence (PMS) stars showing signs of intense activity and strong… Expand
  • table 1
  • table 2
  • table 3
  • figure 2
  • figure 1