Disentangling telluric lines in stellar spectra

被引:18
作者
Hadrava, P [1 ]
机构
[1] Akad Ved Ceske Republ, Astron Ustav, Ondrejov 25165, Czech Republic
关键词
atmospheric effects; techniques : spectroscopic; techniques : radial velocities; line : profiles; stars : atmospheres; stars : planetary systems;
D O I
10.1051/0004-6361:20054209
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The use of a method of spectra disentangling for telluric lines is explained in detail, with a particular emphasis on high-precision radial-velocity measurements for the search for extrasolar planets. New improvements to the method are introduced.
引用
收藏
页码:1149 / 1152
页数:4
相关论文
共 17 条
[1]  
Adelman SJ, 1996, ASTR SOC P, V108, P293
[2]   Attaining Doppler precision of 3 m s(-1) [J].
Butler, RP ;
Marcy, GW ;
Williams, E ;
McCarthy, C ;
Dosanjh, P ;
Vogt, SS .
PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF THE PACIFIC, 1996, 108 (724) :500-509
[3]  
Greimel R, 1999, ASTR SOC P, V185, P48
[4]   POSSIBILITY OF DETERMINING STELLAR RADIAL-VELOCITIES TO O.OIKM S-1 [J].
GRIFFIN, R ;
GRIFFIN, R .
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 1973, 162 (03) :243-253
[5]   The detection and measurement of telluric ozone from stellar spectra [J].
Griffin, RE .
PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF THE PACIFIC, 2005, 117 (834) :885-894
[6]  
Hadrava P, 2004, ASTR SOC P, V318, P86
[7]   Relative line photometry of eclipsing binaries [J].
Hadrava, P .
ASTRONOMY & ASTROPHYSICS SUPPLEMENT SERIES, 1997, 122 (03) :581-584
[8]  
Hadrava P, 1995, ASTRON ASTROPHYS SUP, V114, P393
[9]  
HADRAVA P, 2005, UNPUB AP SS
[10]  
Hadrava P., 2004, PUBL ASTRON I ASCR, V92, P15