High precision astrometry laboratory demonstration for exoplanet detection using a diffractive pupil telescope

Author(s):  
Eduardo A. Bendek ◽  
S. Mark Ammons ◽  
Ruslan Belikov ◽  
Eugene Pluzhnik ◽  
Olivier Guyon
Author(s):  
Fabien Malbet ◽  
Alexis Brandeker ◽  
Alain Léger ◽  
Bjorn Jakobsson ◽  
Renaud Goullioud ◽  
...  

2007 ◽  
Vol 471 (3) ◽  
pp. 1057-1067 ◽  
Author(s):  
P. F. Lazorenko ◽  
M. Mayor ◽  
M. Dominik ◽  
F. Pepe ◽  
D. Segransan ◽  
...  

1995 ◽  
Vol 166 ◽  
pp. 163-171 ◽  
Author(s):  
V. M. Kaspi

We present the technique of long-term, high-precision timing of millisecond pulsars as applied to precision astrometry. We provide a tutorial on pulsars and pulsar timing, as well as up-to-date results of long-term timing observations of two millisecond pulsars, PSRs B1855+09 and B1937+21. We consider the feasibility of tying the extragalactic and optical reference frames to that defined by solar system objects, and we conclude that precision astrometry from millisecond pulsar timing has a bright future.


2011 ◽  
Vol 34 (2) ◽  
pp. 385-413 ◽  
Author(s):  
Fabien Malbet ◽  
Alain Léger ◽  
Michael Shao ◽  
Renaud Goullioud ◽  
Pierre-Olivier Lagage ◽  
...  

1995 ◽  
Vol 166 ◽  
pp. 187-192
Author(s):  
J. Andersen

The state of the art in accurate mass determination for binary stars is reviewed, and the angular sizes and their errors are computed for a typical system from the existing high-precision sample. It appears that sub-μas (microarcsecond) absolute astrometry will be needed in order to improve the accuracy substantially by astrometry alone. The types of system, and the kinds of data, where precision astrometry appears most promising are outlined. Finally, astrophysical applications of such accurate stellar masses, and the auxiliary data required in them, are briefly reviewed.


1993 ◽  
Author(s):  
Jeffrey W. Yu ◽  
Stuart B. Shaklan ◽  
Michael Shao

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