TY - GEN
T1 - TODCOR - Two-dimensional correlation
AU - Zucker, Shay
PY - 2011/7
Y1 - 2011/7
N2 - TODCOR is a TwO-Dimensional CORrelation technique to measure radial velocities of the two components of a spectroscopic binary. Assuming the spectra of the two components are known, the technique correlates an observed binary spectrum against a combination of the two spectra with different shifts. TODCOR measures simultaneously the radial velocities of the two stars by finding the maximum correlation. The main use of the technique has been to turn single-lined binaries into double-lined systems. This helps to explore the binary mass-ratio distribution, especially the low-mass regime, where the secondaries are usually very faint and therefore hard to detect. The technique has been generalized to study multi-order spectra, and also triple- and quadruple-lined systems. It has several applications in studying extrasolar planets and in the future may even help to dynamically measure stellar masses of binaries through relativistc effects.
AB - TODCOR is a TwO-Dimensional CORrelation technique to measure radial velocities of the two components of a spectroscopic binary. Assuming the spectra of the two components are known, the technique correlates an observed binary spectrum against a combination of the two spectra with different shifts. TODCOR measures simultaneously the radial velocities of the two stars by finding the maximum correlation. The main use of the technique has been to turn single-lined binaries into double-lined systems. This helps to explore the binary mass-ratio distribution, especially the low-mass regime, where the secondaries are usually very faint and therefore hard to detect. The technique has been generalized to study multi-order spectra, and also triple- and quadruple-lined systems. It has several applications in studying extrasolar planets and in the future may even help to dynamically measure stellar masses of binaries through relativistc effects.
KW - Celestial mechanics
KW - binaries: spectroscopic
KW - brown dwarfs
KW - methods: data analysis
KW - planetary systems
KW - stars: low mass
KW - techniques: radial velocities
KW - techniques: spectroscopic
UR - http://www.scopus.com/inward/record.url?scp=84887376737&partnerID=8YFLogxK
U2 - 10.1017/S1743921311027852
DO - 10.1017/S1743921311027852
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AN - SCOPUS:84887376737
SN - 9781107019829
T3 - Proceedings of the International Astronomical Union
SP - 371
EP - 378
BT - From Interacting Binaries to Exoplanets
PB - Cambridge University Press
ER -