HARPS-N @ TNG, two year harvesting data: performances and results

R. Cosentino; C. Lovis; F. Pepe; A.C. Cameron; D.W. Latham; E. Molinari; S. Udry; N. Bezawada; N. Buchschacher; P. Figueira; M. Fleury; A. Ghedina; A.G. Glenday; M. Gonzalez; J. Guerra; D. Henry; I. Hughes; C. Maire; F. Motalebi; D.F. Phillips

doi:10.1117/12.2055813

HARPS-N @ TNG, two year harvesting data: performances and results

R. Cosentino, C. Lovis, F. Pepe, A.C. Cameron, D.W. Latham, E. Molinari, S. Udry, N. Bezawada, N. Buchschacher, P. Figueira, M. Fleury, A. Ghedina, A.G. Glenday, M. Gonzalez, J. Guerra, D. Henry, I. Hughes, C. Maire, F. Motalebi, D.F. Phillips

School of Physics and Astronomy

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

Abstract

The planet hunter HARPS-N[1], in operation at the Telescopio Nazionale Galileo (TNG)[13] from April 2012 is a highresolution spectrograph designed to achieve a very high radial velocity precision measurement thanks to an ultra stable environment and in a temperature-controlled vacuum. The main part of the observing time was devoted to Kepler field and achieved a very important result with the discovery of a terrestrial exoplanet. After two year of operation, we are able to show the performances and the results of the instrument.

Original language	English
Title of host publication	Ground-based and Airborne Instrumentation for Astronomy V
Editors	Suzanne K. Ramsay, Ian S. McLean, Hideki Takami
Publisher	SPIE
Volume	9147
ISBN (Print)	9780819496157
DOIs	https://doi.org/10.1117/12.2055813
Publication status	Published - 2014
Event	Ground-based and Airborne Instrumentation for Astronomy V - Montréal, United States Duration: 22 Jun 2014 → 22 Jun 2014

Publication series

Name	Proceedings of SPIE
Publisher	SPIE - The International Society for Optical Engineering
Volume	9147
ISSN (Print)	0277-786X

Conference

Conference	Ground-based and Airborne Instrumentation for Astronomy V
Country/Territory	United States
City	Montréal
Period	22/06/14 → 22/06/14

Access to Document

10.1117/12.2055813

Cameron_2015_SPIE_HARPS
Rosario Cosentino, Christophe Lovis, Francesco Pepe, Andrew C. Cameron, et al., "HARPS-N @ TNG, two year harvesting data: performances and results," Proc. SPIE 9147, Ground-based and Airborne Instrumentation for Astronomy V, 9147, 2014. Copyright 2014 Society of Photo Optical Instrumentation Engineers. One print or electronic copy may be made for personal use only. Systematic reproduction and distribution, duplication of any material in this paper for a fee or for commercial purposes, or modification of the content of the paper are prohibited.
Final published version, 2.22 MB

EU FP7 Space ETAEARTH: ETAEARTH
Cameron, A. C. (PI)
European Commission
1/01/13 → 31/12/17
Project: Standard
Astrophysics at St Andrews:2012 - 2014: Astrophysics at St Andrews: 2012 - 2014
Horne, K. D. (PI)
Science & Technology Facilities Council
1/10/11 → 31/03/12
Project: Standard

Cite this

Cosentino, R., Lovis, C., Pepe, F., Cameron, A. C., Latham, D. W., Molinari, E., Udry, S., Bezawada, N., Buchschacher, N., Figueira, P., Fleury, M., Ghedina, A., Glenday, A. G., Gonzalez, M., Guerra, J., Henry, D., Hughes, I., Maire, C., Motalebi, F., & Phillips, D. F. (2014). HARPS-N @ TNG, two year harvesting data: performances and results. In S. K. Ramsay, I. S. McLean, & H. Takami (Eds.), Ground-based and Airborne Instrumentation for Astronomy V (Vol. 9147). (Proceedings of SPIE; Vol. 9147). SPIE. https://doi.org/10.1117/12.2055813

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title = "HARPS-N @ TNG, two year harvesting data: performances and results",

abstract = "The planet hunter HARPS-N[1], in operation at the Telescopio Nazionale Galileo (TNG)[13] from April 2012 is a highresolution spectrograph designed to achieve a very high radial velocity precision measurement thanks to an ultra stable environment and in a temperature-controlled vacuum. The main part of the observing time was devoted to Kepler field and achieved a very important result with the discovery of a terrestrial exoplanet. After two year of operation, we are able to show the performances and the results of the instrument.",

author = "R. Cosentino and C. Lovis and F. Pepe and A.C. Cameron and D.W. Latham and E. Molinari and S. Udry and N. Bezawada and N. Buchschacher and P. Figueira and M. Fleury and A. Ghedina and A.G. Glenday and M. Gonzalez and J. Guerra and D. Henry and I. Hughes and C. Maire and F. Motalebi and D.F. Phillips",

year = "2014",

doi = "10.1117/12.2055813",

language = "English",

isbn = "9780819496157",

volume = "9147",

series = "Proceedings of SPIE",

publisher = "SPIE",

editor = "Ramsay, {Suzanne K. } and McLean, {Ian S. } and Takami, {Hideki }",

booktitle = "Ground-based and Airborne Instrumentation for Astronomy V",

address = "United States",

note = "Ground-based and Airborne Instrumentation for Astronomy V ; Conference date: 22-06-2014 Through 22-06-2014",

}

Cosentino, R, Lovis, C, Pepe, F, Cameron, AC, Latham, DW, Molinari, E, Udry, S, Bezawada, N, Buchschacher, N, Figueira, P, Fleury, M, Ghedina, A, Glenday, AG, Gonzalez, M, Guerra, J, Henry, D, Hughes, I, Maire, C, Motalebi, F & Phillips, DF 2014, HARPS-N @ TNG, two year harvesting data: performances and results. in SK Ramsay, IS McLean & H Takami (eds), Ground-based and Airborne Instrumentation for Astronomy V. vol. 9147, Proceedings of SPIE, vol. 9147, SPIE, Ground-based and Airborne Instrumentation for Astronomy V, Montréal, United States, 22/06/14. https://doi.org/10.1117/12.2055813

TY - GEN

T1 - HARPS-N @ TNG, two year harvesting data

T2 - Ground-based and Airborne Instrumentation for Astronomy V

AU - Cosentino, R.

AU - Lovis, C.

AU - Pepe, F.

AU - Cameron, A.C.

AU - Latham, D.W.

AU - Molinari, E.

AU - Udry, S.

AU - Bezawada, N.

AU - Buchschacher, N.

AU - Figueira, P.

AU - Fleury, M.

AU - Ghedina, A.

AU - Glenday, A.G.

AU - Gonzalez, M.

AU - Guerra, J.

AU - Henry, D.

AU - Hughes, I.

AU - Maire, C.

AU - Motalebi, F.

AU - Phillips, D.F.

PY - 2014

Y1 - 2014

N2 - The planet hunter HARPS-N[1], in operation at the Telescopio Nazionale Galileo (TNG)[13] from April 2012 is a highresolution spectrograph designed to achieve a very high radial velocity precision measurement thanks to an ultra stable environment and in a temperature-controlled vacuum. The main part of the observing time was devoted to Kepler field and achieved a very important result with the discovery of a terrestrial exoplanet. After two year of operation, we are able to show the performances and the results of the instrument.

AB - The planet hunter HARPS-N[1], in operation at the Telescopio Nazionale Galileo (TNG)[13] from April 2012 is a highresolution spectrograph designed to achieve a very high radial velocity precision measurement thanks to an ultra stable environment and in a temperature-controlled vacuum. The main part of the observing time was devoted to Kepler field and achieved a very important result with the discovery of a terrestrial exoplanet. After two year of operation, we are able to show the performances and the results of the instrument.

U2 - 10.1117/12.2055813

DO - 10.1117/12.2055813

M3 - Conference contribution

AN - SCOPUS:84922676527

SN - 9780819496157

VL - 9147

T3 - Proceedings of SPIE

BT - Ground-based and Airborne Instrumentation for Astronomy V

A2 - Ramsay, Suzanne K.

A2 - McLean, Ian S.

A2 - Takami, Hideki

PB - SPIE

Y2 - 22 June 2014 through 22 June 2014

ER -

HARPS-N @ TNG, two year harvesting data: performances and results

Abstract

Publication series

Conference

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Projects

EU FP7 Space ETAEARTH: ETAEARTH

Astrophysics at St Andrews:2012 - 2014: Astrophysics at St Andrews: 2012 - 2014

Cite this