ATTENZIONE! IL REPOSITORY E’ APERTO ESCLUSIVAMENTE ALL’IMMISSIONE DEI RAPPORTI TECNICI (COLLEZIONE 4.01). NON E’ POSSIBILE INSERIRE PRODOTTI IN TUTTE LE ALTRE COLLEZIONI, A CAUSA DI PROBLEMI TECNICI. THE REPOSITORY IS OPEN EXCLUSIVELY FOR THE SUBMISSION OF TECHNICAL REPORTS (COLLECTION 4.01). SUBMISSIONS TO ALL OTHER COLLECTIONS ARE TEMPORARILY UNAVAILABLE, DUE TO TECHNICAL ISSUES.
 

The Gaia-ESO Survey Astrophysical Calibration

Date Issued
2016
Author(s)
•
Gaia-ESO Survey Consortium
Abstract
The Gaia-ESO Survey is a wide field spectroscopic survey recently started with the FLAMES@VLT in Cerro Paranal, Chile. It will produce radial velocities more accurate than Gaia's for faint stars (down to V ≃ 18), and astrophysical parameters and abundances for approximately 100 000 stars, belonging to all Galactic populations. 300 nights were assigned in 5 years (with the last year subject to approval after a detailed report). In particular, to connect with other ongoing and planned spectroscopic surveys, a detailed calibration program — for the astrophysical parameters derivation — is planned, including well known clusters, Gaia benchmark stars, and special equatorial calibration fields designed for wide field/multifiber spectrographs.
Coverage
Calibration and standardization of missions and large surveys in astronomy and astrophysics
All editors
Deustua, S.; Allam, S.; Tucker, D.; Smith, J. A.
Series
Volume
503
Start page
275
Conferenece
Calibration and standardization of missions and large surveys in astronomy and astrophysics
Conferenece place
Batavia, Illinois (USA)
Conferenece date
16-19 April, 2012
Uri
Url
Issn Identifier
1050-3390
Ads BibCode
2016ASPC..503..275P
Rights
open.access
File(s)
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275.pdf

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605.36 KB

Format

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