Long baseline stellar interferometry shares with other techniques the need for calibrator stars in order to correct for instrumental and atmospheric effects. We present a catalogue of 374 stars carefully selected to be used for that purpose in the near infrared. Owing to several convergent criteria with the work of Cohen et al. ([CITE]), this catalogue is in essence a subset of their self-consistent all-sky network of spectro-photometric calibrator stars. For every star, we provide the angular limb-darkened diameter, uniform disc angular diameters in the J, H and K bands, the Johnson photometry and other useful parameters. Most stars are type III giants with spectral types K or M0, magnitudes $V=3$–7 and $K=0$–3. Their angular lim...
International audienceABSTRACT A good knowledge of the angular diameters of stars used to calibrate ...
The availability of a number of new interferometric measurements of Main Sequence and subgiant stars...
Significant effort has been expended to locate and characterize small groups of stars for use as sta...
Long baseline stellar interferometry shares with other techniques the need for calibrator stars in ...
We present in this paper a catalog of reference stars suitable for calibrating infrared interferomet...
International audienceWe present in this paper a catalog of reference stars suitable for calibrating...
The calibration process of long baseline stellar interferometers requires the use of reference stars...
9 pagesWe present in this paper a catalog of reference stars suitable for calibrating infrared inter...
Reliable prediction of stellar diameters, particularly angular diameters, is a useful and necessary...
Context. In long-baseline interferometry, images or astrophysical parameters are obtained ...
In the framework of an ongoing series of high angular resolution observations by lunar occultations ...
By construction, optical (and near-infrared) interferometers typically have resolutions designed to ...
International audienceOver the last few years, a new generation of long baseline interferometers has...
The apparent size of stars is a crucial benchmark for fundamental stellar properties such as effecti...
In long baseline interferometry, the raw fringe contrast must be calibrated to obtain the true visib...
International audienceABSTRACT A good knowledge of the angular diameters of stars used to calibrate ...
The availability of a number of new interferometric measurements of Main Sequence and subgiant stars...
Significant effort has been expended to locate and characterize small groups of stars for use as sta...
Long baseline stellar interferometry shares with other techniques the need for calibrator stars in ...
We present in this paper a catalog of reference stars suitable for calibrating infrared interferomet...
International audienceWe present in this paper a catalog of reference stars suitable for calibrating...
The calibration process of long baseline stellar interferometers requires the use of reference stars...
9 pagesWe present in this paper a catalog of reference stars suitable for calibrating infrared inter...
Reliable prediction of stellar diameters, particularly angular diameters, is a useful and necessary...
Context. In long-baseline interferometry, images or astrophysical parameters are obtained ...
In the framework of an ongoing series of high angular resolution observations by lunar occultations ...
By construction, optical (and near-infrared) interferometers typically have resolutions designed to ...
International audienceOver the last few years, a new generation of long baseline interferometers has...
The apparent size of stars is a crucial benchmark for fundamental stellar properties such as effecti...
In long baseline interferometry, the raw fringe contrast must be calibrated to obtain the true visib...
International audienceABSTRACT A good knowledge of the angular diameters of stars used to calibrate ...
The availability of a number of new interferometric measurements of Main Sequence and subgiant stars...
Significant effort has been expended to locate and characterize small groups of stars for use as sta...