Standard

The impact of red noise in radial velocity planet searches. / Baluev, Roman V.

From Interacting Binaries to Exoplanets: Essential Modeling Tools. ed. / Mercedes Richards; Ivan Hubeny. S282. ed. 2011. p. 119-120 (Proceedings of the International Astronomical Union; Vol. 7, No. S282).

Research output: Chapter in Book/Report/Conference proceedingConference contributionResearchpeer-review

Harvard

Baluev, RV 2011, The impact of red noise in radial velocity planet searches. in M Richards & I Hubeny (eds), From Interacting Binaries to Exoplanets: Essential Modeling Tools. S282 edn, Proceedings of the International Astronomical Union, no. S282, vol. 7, pp. 119-120. https://doi.org/10.1017/S1743921311027116

APA

Baluev, R. V. (2011). The impact of red noise in radial velocity planet searches. In M. Richards, & I. Hubeny (Eds.), From Interacting Binaries to Exoplanets: Essential Modeling Tools (S282 ed., pp. 119-120). (Proceedings of the International Astronomical Union; Vol. 7, No. S282). https://doi.org/10.1017/S1743921311027116

Vancouver

Baluev RV. The impact of red noise in radial velocity planet searches. In Richards M, Hubeny I, editors, From Interacting Binaries to Exoplanets: Essential Modeling Tools. S282 ed. 2011. p. 119-120. (Proceedings of the International Astronomical Union; S282). https://doi.org/10.1017/S1743921311027116

Author

Baluev, Roman V. / The impact of red noise in radial velocity planet searches. From Interacting Binaries to Exoplanets: Essential Modeling Tools. editor / Mercedes Richards ; Ivan Hubeny. S282. ed. 2011. pp. 119-120 (Proceedings of the International Astronomical Union; S282).

BibTeX

@inproceedings{15dc3b10d32b4604bf1cff4366841065,
title = "The impact of red noise in radial velocity planet searches",
abstract = "We demonstrate that moderate exoplanet radial velocity searches are often subject to the effect of the correlated (red) radial velocity noise. When disregarded, this effect may induce strong distortions in the results of the time series analysis and, ultimately, can even lead to false planet detections. We construct a maximum-likelihood algorithm, which is able to manage this issue rather efficiently.",
keywords = "methods: data analysis, methods: statistical, techniques: radial velocities",
author = "Baluev, {Roman V.}",
year = "2011",
month = jul,
day = "1",
doi = "10.1017/S1743921311027116",
language = "English",
isbn = "9781107019829",
series = "Proceedings of the International Astronomical Union",
number = "S282",
pages = "119--120",
editor = "Mercedes Richards and Ivan Hubeny",
booktitle = "From Interacting Binaries to Exoplanets",
edition = "S282",

}

RIS

TY - GEN

T1 - The impact of red noise in radial velocity planet searches

AU - Baluev, Roman V.

PY - 2011/7/1

Y1 - 2011/7/1

N2 - We demonstrate that moderate exoplanet radial velocity searches are often subject to the effect of the correlated (red) radial velocity noise. When disregarded, this effect may induce strong distortions in the results of the time series analysis and, ultimately, can even lead to false planet detections. We construct a maximum-likelihood algorithm, which is able to manage this issue rather efficiently.

AB - We demonstrate that moderate exoplanet radial velocity searches are often subject to the effect of the correlated (red) radial velocity noise. When disregarded, this effect may induce strong distortions in the results of the time series analysis and, ultimately, can even lead to false planet detections. We construct a maximum-likelihood algorithm, which is able to manage this issue rather efficiently.

KW - methods: data analysis

KW - methods: statistical

KW - techniques: radial velocities

UR - http://www.scopus.com/inward/record.url?scp=84887374214&partnerID=8YFLogxK

U2 - 10.1017/S1743921311027116

DO - 10.1017/S1743921311027116

M3 - Conference contribution

AN - SCOPUS:84887374214

SN - 9781107019829

T3 - Proceedings of the International Astronomical Union

SP - 119

EP - 120

BT - From Interacting Binaries to Exoplanets

A2 - Richards, Mercedes

A2 - Hubeny, Ivan

ER -

ID: 36295924