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Flaring activities of fast rotating stars
The dynamo theory has always been one of the biggest mysteries in stellar physics. One key reason for its uncertainty is poor knowledge of the dynamo process on stars except the... -
Detached eclipsing binaries lifetime of starspots
Tidal deformation breaks the axisymmetric structure of stars, and this may affect stellar activity. This effect has been demonstrated in theoretical analyses and simulations,... -
Exoplanets parameters
The number of discovered exoplanets now exceeds 5500, allowing statistical analyses of planetary systems. Multi-planet systems are mini-laboratories of planet formation and... -
X-Shooting ULLYSES. Project Description
Observations of individual massive stars, super-luminous supernovae, gamma-ray bursts, and gravitational wave events involving spectacular black hole mergers indicate that the... -
Dwarfs & giants surface brightness-colour relations
Surface brightness-colour relations (SBCRs) are used to derive the stellar angular diameters from photometric observations. They have various astrophysical applications, such as... -
Active red giants asteroseismic & rotation param.
Oscillating red-giant stars have provided a wealth of asteroseismic information regarding their interiors and evolutionary states, and access to their fundamental properties... -
Slow-rotator sequence radii
Average stellar radii in open clusters can be estimated from rotation periods and projected rotational velocities under the assumption of random orientation of the spin axis.... -
NGC 2264, NGC 2547 and NGC 2516 stellar radii
Rapidly rotating, low-mass members of eclipsing binary systems have measured radii that are significantly larger than predicted by standard evolutionary models. It has been... -
ESO VLTI Calibrators Program
The ESO Very Large Telescope Interferometer (VLTI) is one of the leading interferometric facilities. It is equiped with several 8.2 and 1.8m telescopes, a large number of... -
Cepheid radii
We have refined the CORS method, introduced in 1980 for the computation of the Cepheid radii, in order to extend its applicability to recent and extensive sets of observations.... -
Teff and angular diameters from IRFM
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MDFC Version 10
We present the Mid-infrared stellar Diameters and Fluxes compilation Catalogue (MDFC) dedicated to long-baseline interferometry at mid-infrared wavelengths (3-13um). It gathers... -
JMDC : JMMC Measured Stellar Diameters Catalogue
This catalog lists all measurements of stellar apparent diameters made with "direct" techniques: optical interferometry, intensity interferometry and lunar occultations that... -
JMMC Stellar Diameters Catalogue - JSDC
This catalogue contains stellar angular diameter estimate for bright stars, complete for all stars with Hipparcos parallaxes. The JMMC Calibrator Workgroup has long developed... -
Catalogue of Stellar Diameters (CADARS)
For 9733 stars this catalog lists all values of the apparent and absolute radii from the literature. Data were compiled beginning 1950 up to 1997. The stars are listed according... -
Apparent Diameters and Absolute Radii of Stars
For 7255 stars this catalog lists all values of the apparent and absolute radii from the literature. Data were compiled beginning 1950 up to 1985, including some data from 1986... -
Contact binaries from CSS DR2
With the continuous development of large optical surveys, a large number of light curves of late-type contact binary systems (CBs) have been released. Deriving parameters for... -
ASAS-SN eclipsing contact binaries with Gaia DR3
Starting from more than 11200 short-period (less than 0.5 days) EW-type eclipsing binary candidates with the All-Sky Automated Survey for Supernovae V-band light curves, we use... -
Solar-like oscillators using TESS 2min cadence LCs
Based on all 2 minute cadence TESS light curves from Sector 1 to 60, we provide a catalog of 8651 solar-like oscillators, including frequency at maximum power ({nu}max, with its... -
Masses of OB-type stars from LAMOST DR5
The measurements of masses and luminosities of massive stars play an important role in understanding the formation and evolution of their host galaxies. In this work, we present...
