SIMBAD references

2012ApJS..200...15A - Astrophys. J., Suppl. Ser., 200, 15 (2012/June-0)

The HARPS-TERRA project. I. Description of the algorithms, performance, and new measurements on a few remarkable stars observed by HARPS.

ANGLADA-ESCUDE G. and BUTLER R.P.

Abstract (from CDS):

Doppler spectroscopy has uncovered or confirmed all the known planets orbiting nearby stars. Two main techniques are used to obtain precision Doppler measurements at optical wavelengths. The first approach is the gas cell method, which consists of least-squares matching of the spectrum of iodine imprinted on the spectrum of the star. The second method relies on the construction of a stabilized spectrograph externally calibrated in wavelength. The most precise stabilized spectrometer in operation is the High Accuracy Radial velocity Planet Searcher (HARPS), operated by the European Southern Observatory in La Silla Observatory, Chile. The Doppler measurements obtained with HARPS are typically obtained using the cross-correlation function (CCF) technique. This technique consists of multiplying the stellar spectrum by a weighted binary mask and finding the minimum of the product as a function of the Doppler shift. It is known that CCF is suboptimal in exploiting the Doppler information in the stellar spectrum. Here we describe an algorithm to obtain precision radial velocity measurements using least-squares matching of each observed spectrum to a high signal-to-noise ratio template derived from the same observations. This algorithm is implemented in our software HARPS-TERRA (Template-Enhanced Radial velocity Re-analysis Application). New radial velocity measurements on a representative sample of stars observed by HARPS are used to illustrate the benefits of the proposed method. We show that, compared with CCF, template matching provides a significant improvement in accuracy, especially when applied to M dwarfs.

Abstract Copyright:

Journal keyword(s): methods: data analysis - planetary systems - stars: individual (Tau Ceti, HD 85512, Barnard's star, Proxima, Kapteyn's star, GJ676A, Epsilon Eridani, HD 69830) - techniques: radial velocities

VizieR on-line data: <Available at CDS (J/ApJS/200/15): stars.dat table5.dat table6.dat table7.dat table10.dat>

Simbad objects: 16

goto Full paper

goto View the reference in ADS

To bookmark this query, right click on this link: simbad:2012ApJS..200...15A and select 'bookmark this link' or equivalent in the popup menu


2019.09.15-16:55:19

© Université de Strasbourg/CNRS

    • Contact