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J/A+A/527/A136 HD 116956 V-band differential light curve (Lehtinen+, 2011)
The following files can be converted to FITS (extension .fit or fit.gz)
hd116956.dat results.dat
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Query from: http://vizier.cds.unistra.fr/viz-bin/VizieR?-source=J/A+A/527/A136
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Beginning of ReadMe :J/A+A/527/A136 HD 116956 V-band differential light curve (Lehtinen+, 2011)
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The continuous period search method and its application to the young solar
analogue HD 116956.
Lehtinen J., Jetsu L., Hackman T., Kajatkari P., Henry G.W.
<Astron. Astrophys. 527, A136 (2011)>
=2011A&A...527A.136L
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ADC_Keywords: Stars, variable
Keywords: methods: data analysis - stars: activity - starspots -
stars: individual: HD 116956 - stars: rotation
Abstract:
We formulate an improved time series analysis method for the analysis
of photometry of active stars. This new continuous period search (CPS)
method is applied to 12 years of V band photometry of the young solar
analogue HD 116956 (NQ UMa).
Description:
The included files present the numerical data of our CPS analysis of
the young solar analogue HD 116956 photometry. The data consists of
differential Johnson V-band photometry using the star HD 114446 as the
comparison star.
The CPS method is described in detail in our present paper. For a
thorough description of the formatting of the numerical results
provided by the CPS, see the appendix A of our paper.
Objects:
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RA (2000) DE Designation(s)
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13 25 45.5 +56 58 14 HD 116956 = V* NQ UMa
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