NASA NTRS · 19820009161
Monitoring solar-type stars
Abstract
Old UBV and recent uvby photometry of solar-type dwarfs and other standard stars yield an upper limit of variability (determined by observational errors) of about 0.004 mag rms. A factor two improvement in this upper limit is achievable.
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Lockwood, G. W.. 1981-12-01. Monitoring solar-type stars. https://ntrs.nasa.gov/citations/19820009161
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