Add to ORKGOld 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
Smoothing solar UV data on rotational timescale (approx. 27 days) improves identification of solar m...
The daily variation of the solar photocenter over some 11 yr is derived from the Mount Wilson data r...
The Shuttle SBUV (SSBUV) and NOAA-11 SBUV/2 instruments measured solar spectral UV irradiance during...
Since 1984, researchers have made more than 1500 differential photometric b (471 nm) and y (551 nm) ...
Recently published precise stellar photometry of 72 Sun-like stars obtained at the Fairborn Observat...
We present 14 years of contemporaneous photometric and spectroscopic observations of 28 solar analog...
We examine patterns of variation of 32 primarily main-sequence Sun-like stars [selected at project o...
In this paper, a summary of optical time-series photometry of 125 ultracool dwarfs is given. The ob...
Context. A recent paper by Shapiro and colleagues (2011, A&A, 529, A67) reconstructs spectral and t...
Context. A recent paper by Shapiro and colleagues (2011, A&A, 529, A67) reconstructs spectral and t...
Context. Ultracool dwarfs (≲2500 K) are known to display photometric variability in short timescales...
The Sun’s net radiative output varies on timescales of minutes to gigayears. Direct measurements of ...
The Sun’s net radiative output varies on timescales of minutes to gigayears. Direct measurements of ...
The Sun’s net radiative output varies on timescales of minutes to gigayears. Direct measurements of ...
Context. A recent paper by Shapiro and colleagues (2011, A&A, 529, A67) reconstructs spectral and to...
Smoothing solar UV data on rotational timescale (approx. 27 days) improves identification of solar m...
The daily variation of the solar photocenter over some 11 yr is derived from the Mount Wilson data r...
The Shuttle SBUV (SSBUV) and NOAA-11 SBUV/2 instruments measured solar spectral UV irradiance during...
Since 1984, researchers have made more than 1500 differential photometric b (471 nm) and y (551 nm) ...
Recently published precise stellar photometry of 72 Sun-like stars obtained at the Fairborn Observat...
We present 14 years of contemporaneous photometric and spectroscopic observations of 28 solar analog...
We examine patterns of variation of 32 primarily main-sequence Sun-like stars [selected at project o...
In this paper, a summary of optical time-series photometry of 125 ultracool dwarfs is given. The ob...
Context. A recent paper by Shapiro and colleagues (2011, A&A, 529, A67) reconstructs spectral and t...
Context. A recent paper by Shapiro and colleagues (2011, A&A, 529, A67) reconstructs spectral and t...
Context. Ultracool dwarfs (≲2500 K) are known to display photometric variability in short timescales...
The Sun’s net radiative output varies on timescales of minutes to gigayears. Direct measurements of ...
The Sun’s net radiative output varies on timescales of minutes to gigayears. Direct measurements of ...
The Sun’s net radiative output varies on timescales of minutes to gigayears. Direct measurements of ...
Context. A recent paper by Shapiro and colleagues (2011, A&A, 529, A67) reconstructs spectral and to...
Smoothing solar UV data on rotational timescale (approx. 27 days) improves identification of solar m...
The daily variation of the solar photocenter over some 11 yr is derived from the Mount Wilson data r...
The Shuttle SBUV (SSBUV) and NOAA-11 SBUV/2 instruments measured solar spectral UV irradiance during...