CORAVEL

Francisco Diego; Roger F. Griffin; Juan Echevarria; Richard G. Bingham; David D. Walker

doi:10.1117/12.19129

CORAVEL

Francisco Diego, Roger F. Griffin, Juan Echevarria, Richard G. Bingham, David D. Walker

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution › peer-review

4 Citations (Scopus)

Abstract

CORAVEL is a very useful tool to measure stellar Doppler shifts directly. It was originally conceived at the Observatories of Marseilles and Geneve. Its operation is based on the hard cross-correlation of an echelle stellar spectrum with a suitable template. This paper describes the characteristics of an updated version of the instrument, under development at the Optical Science Laboratory (OSL) of University College London (UCL) for the University of Cambridge 36-inch telescope.

Original language	English
Title of host publication	Instrumentation in Astronomy VII
Editors	David L. Crawford
Publisher	SPIE
Pages	662-672
Number of pages	11
Volume	1235, Part 2
ISBN (Print)	0819402796, 9780819402790
DOIs	https://doi.org/10.1117/12.19129
Publication status	Published - 1 Jul 1990
Externally published	Yes
Event	SPIE Astronomical Telescopes and Instrumentation for the 21st Century - Tucson, United States Duration: 11 Feb 1990 → 16 Feb 1990 Conference number: 7

Publication series

Name	Proceedings of SPIE - The International Society for Optical Engineering
Publisher	SPIE
Volume	1235
ISSN (Print)	0277-786X
ISSN (Electronic)	1996-756X

Conference

Conference	SPIE Astronomical Telescopes and Instrumentation for the 21st Century
Country/Territory	United States
City	Tucson
Period	11/02/90 → 16/02/90

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10.1117/12.19129Licence: Unspecified

Cite this

@inproceedings{0589057760c748de885784c8868eb5b1,

title = "CORAVEL",

abstract = "CORAVEL is a very useful tool to measure stellar Doppler shifts directly. It was originally conceived at the Observatories of Marseilles and Geneve. Its operation is based on the hard cross-correlation of an echelle stellar spectrum with a suitable template. This paper describes the characteristics of an updated version of the instrument, under development at the Optical Science Laboratory (OSL) of University College London (UCL) for the University of Cambridge 36-inch telescope.",

keywords = "Data Processing, Data Acquisition, Image Sensors, Mathematical Techniques, Correlation Methods, Photons, Detectors, Telescopes, CORAVEL Guiding System",

author = "Francisco Diego and Griffin, {Roger F.} and Juan Echevarria and Bingham, {Richard G.} and Walker, {David D.}",

year = "1990",

month = jul,

day = "1",

doi = "10.1117/12.19129",

language = "English",

isbn = "0819402796",

volume = "1235, Part 2",

series = "Proceedings of SPIE - The International Society for Optical Engineering",

publisher = "SPIE",

pages = "662--672",

editor = "Crawford, {David L.}",

booktitle = "Instrumentation in Astronomy VII",

address = "United States",

note = "SPIE Astronomical Telescopes and Instrumentation for the 21st Century ; Conference date: 11-02-1990 Through 16-02-1990",

}

Diego, F, Griffin, RF, Echevarria, J, Bingham, RG & Walker, DD 1990, CORAVEL. in DL Crawford (ed.), Instrumentation in Astronomy VII. vol. 1235, Part 2, Proceedings of SPIE - The International Society for Optical Engineering, vol. 1235, SPIE, pp. 662-672, SPIE Astronomical Telescopes and Instrumentation for the 21st Century, Tucson, Arizona, United States, 11/02/90. https://doi.org/10.1117/12.19129

TY - GEN

T1 - CORAVEL

AU - Diego, Francisco

AU - Griffin, Roger F.

AU - Echevarria, Juan

AU - Bingham, Richard G.

AU - Walker, David D.

N1 - Conference code: 7

PY - 1990/7/1

Y1 - 1990/7/1

N2 - CORAVEL is a very useful tool to measure stellar Doppler shifts directly. It was originally conceived at the Observatories of Marseilles and Geneve. Its operation is based on the hard cross-correlation of an echelle stellar spectrum with a suitable template. This paper describes the characteristics of an updated version of the instrument, under development at the Optical Science Laboratory (OSL) of University College London (UCL) for the University of Cambridge 36-inch telescope.

AB - CORAVEL is a very useful tool to measure stellar Doppler shifts directly. It was originally conceived at the Observatories of Marseilles and Geneve. Its operation is based on the hard cross-correlation of an echelle stellar spectrum with a suitable template. This paper describes the characteristics of an updated version of the instrument, under development at the Optical Science Laboratory (OSL) of University College London (UCL) for the University of Cambridge 36-inch telescope.

KW - Data Processing

KW - Data Acquisition

KW - Image Sensors

KW - Mathematical Techniques

KW - Correlation Methods

KW - Photons

KW - Detectors

KW - Telescopes

KW - CORAVEL Guiding System

UR - http://www.scopus.com/inward/record.url?scp=0025589013&partnerID=8YFLogxK

U2 - 10.1117/12.19129

DO - 10.1117/12.19129

M3 - Conference contribution

AN - SCOPUS:0025589013

SN - 0819402796

SN - 9780819402790

VL - 1235, Part 2

T3 - Proceedings of SPIE - The International Society for Optical Engineering

SP - 662

EP - 672

BT - Instrumentation in Astronomy VII

A2 - Crawford, David L.

PB - SPIE

T2 - SPIE Astronomical Telescopes and Instrumentation for the 21st Century

Y2 - 11 February 1990 through 16 February 1990

ER -

CORAVEL

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