Problems of improvement of unambiguous radial velocity measurement in low PRF radar

Author(s):  
T.W. Brenner ◽  
A.P. Modrzewski ◽  
J.F. Pietrasinski ◽  
T. Rapacki
2014 ◽  
Author(s):  
Kai Zhang ◽  
Haijiao Jiang ◽  
Jin Tang ◽  
Hangxin Ji ◽  
Yongtian Zhu ◽  
...  

2013 ◽  
Vol 9 (S298) ◽  
pp. 444-444
Author(s):  
Fengfei Wang ◽  
Ali Luo ◽  
Haotong Zhang

AbstractWe select super high quality spectra of spectral type A, F, G, K, M stars from SDSS C DR7. We mix our spectra with noise and then measure their radial velocity. The analysis shows that the accuracy of K, M type stars is much better than A, F stars. With our relationship between the signal-to-noise and accuracy of radial velocity measurement of different spectral type, we provide a good reference for stellar study related to radial velocity.


2008 ◽  
Vol 60 (1) ◽  
pp. 45-53 ◽  
Author(s):  
Eiji Kambe ◽  
Hiroyasu Ando ◽  
Bun’ei Sato ◽  
Hideyuki Izumiura ◽  
Takashi Sekii ◽  
...  

1983 ◽  
Vol 62 ◽  
pp. 93-103
Author(s):  
C. D. Scarfe

AbstractThis review considers three main areas, leaving several others to be discussed in more detail in the contributed papers of this session.1.The need for spectrographs and measuring instruments of great stability for long-term projects such as radial velocity observations of visual binary stars.2.The use of cross-correlation devices, both analog (radial velocity scanners) and digital, for radial velocity measurement.3.The use of comparison spectra impressed directly onto the starlight and of polarisation instruments as means to very precise radial velocities.


2014 ◽  
Vol 562 ◽  
pp. A97 ◽  
Author(s):  
M. David ◽  
R. Blomme ◽  
Y. Frémat ◽  
Y. Damerdji ◽  
C. Delle Luche ◽  
...  

Sign in / Sign up

Export Citation Format

Share Document