9 pagesWe present in this paper a catalog of reference stars suitable for calibrating infrared interferometric observations. In the K band, visibilities can be calibrated with a precision of 1 % on baselines up to 200 meters for the whole sky, and up to 300 meters for some part of the sky. This work, extending to longer baselines a previous catalog compiled by Bordé et al. (2002), is particularly well adapted to hectometric-class interferometers such as the Very Large Telescope Interferometer (VLTI, Glindemann et al. 2003) or the CHARA array (ten Brummelaar et al. 2003) when one is observing well-resolved, high-surface brightness objects (
The Palomar Testbed Interferometer (PTI) archive of observations between 1998 and 2005 is examined f...
Five new absolutely calibrated continuous stellar spectra from 1.2 to 35 microns are presented. The ...
4 pages, 4 figuresLong baseline interferometry is now able to resolve the pulsational change of the ...
9 pagesWe present in this paper a catalog of reference stars suitable for calibrating infrared inter...
International audienceWe present in this paper a catalog of reference stars suitable for calibrating...
We present in this paper a catalog of reference stars suitable for calibrating infrared interferomet...
The calibration process of long baseline stellar interferometers requires the use of reference stars...
In long baseline interferometry, the raw fringe contrast must be calibrated to obtain the true visib...
Long baseline stellar interferometry shares with other techniques the need for calibrator stars in ...
Context. In long-baseline interferometry, images or astrophysical parameters are obtained ...
In long baseline interferometry, the raw fringe contrast must be calibrated to obtain the true visib...
The near-infrared instruments in the upcoming Thirty Meter Telescope (TMT) will be assisted by a mul...
Long baseline optical/infrared interferometers, such as the Mark III Stellar Interferometer on Mt. W...
Reliable prediction of stellar diameters, particularly angular diameters, is a useful and necessary...
We present high-precision JHK photometry with the 3.8m UK Infrared Telescope (UKIRT) of 83 standard ...
The Palomar Testbed Interferometer (PTI) archive of observations between 1998 and 2005 is examined f...
Five new absolutely calibrated continuous stellar spectra from 1.2 to 35 microns are presented. The ...
4 pages, 4 figuresLong baseline interferometry is now able to resolve the pulsational change of the ...
9 pagesWe present in this paper a catalog of reference stars suitable for calibrating infrared inter...
International audienceWe present in this paper a catalog of reference stars suitable for calibrating...
We present in this paper a catalog of reference stars suitable for calibrating infrared interferomet...
The calibration process of long baseline stellar interferometers requires the use of reference stars...
In long baseline interferometry, the raw fringe contrast must be calibrated to obtain the true visib...
Long baseline stellar interferometry shares with other techniques the need for calibrator stars in ...
Context. In long-baseline interferometry, images or astrophysical parameters are obtained ...
In long baseline interferometry, the raw fringe contrast must be calibrated to obtain the true visib...
The near-infrared instruments in the upcoming Thirty Meter Telescope (TMT) will be assisted by a mul...
Long baseline optical/infrared interferometers, such as the Mark III Stellar Interferometer on Mt. W...
Reliable prediction of stellar diameters, particularly angular diameters, is a useful and necessary...
We present high-precision JHK photometry with the 3.8m UK Infrared Telescope (UKIRT) of 83 standard ...
The Palomar Testbed Interferometer (PTI) archive of observations between 1998 and 2005 is examined f...
Five new absolutely calibrated continuous stellar spectra from 1.2 to 35 microns are presented. The ...
4 pages, 4 figuresLong baseline interferometry is now able to resolve the pulsational change of the ...