2022A&A...666A.120G


Query : 2022A&A...666A.120G

2022A&A...666A.120G - Astronomy and Astrophysics, volume 666A, 120 (2022/10-1)

The Gaia-ESO Public Spectroscopic Survey: Motivation, implementation, GIRAFFE data processing, analysis, and final data products.

GILMORE G., RANDICH S., WORLEY C.C., HOURIHANE A., GONNEAU A., SACCO G.G., LEWIS J.R., MAGRINI L., FRANCOIS P., JEFFRIES R.D., KOPOSOV S.E., BRAGAGLIA A., ALFARO E.J., ALLENDE PRIETO C., BLOMME R., KORN A.J., LANZAFAME A.C., PANCINO E., RECIO-BLANCO A., SMILJANIC R., VAN ECK S., ZWITTER T., BENSBY T., FLACCOMIO E., IRWIN M.J., FRANCIOSINI E., MORBIDELLI L., DAMIANI F., BONITO R., FRIEL E.D., VINK J.S., PRISINZANO L., ABBAS U., HATZIDIMITRIOU D., HELD E.V., JORDI C., PAUNZEN E., SPAGNA A., JACKSON R.J., MAIZ APELLANIZ J., ASPLUND M., BONIFACIO P., FELTZING S., BINNEY J., DREW J., FERGUSON A.M.N., MICELA G., NEGUERUELA I., PRUSTI T., RIX H.-W., VALLENARI A., BERGEMANN M., CASEY A.R., DE LAVERNY P., FRASCA A., HILL V., LIND K., SBORDONE L., SOUSA S.G., ADIBEKYAN V., CAFFAU E., DAFLON S., FEUILLET D.K., GEBRAN M., GONZALEZ HERNANDEZ J.I., GUIGLION G., HERRERO A., LOBEL A., MERLE T., MIKOLAITIS S., MONTES D., MOREL T., RUCHTI G., SOUBIRAN C., TABERNERO H.M., TAUTVAISIENE G., TRAVEN G., VALENTINI M., VAN DER SWAELMEN M., VILLANOVA S., VISCASILLAS VAZQUEZ C., BAYO A., BIAZZO K., CARRARO G., EDVARDSSON B., HEITER U., JOFRE P., MARCONI G., MARTAYAN C., MASSERON T., MONACO L., WALTON N.A., ZAGGIA S., AGUIRRE BORSEN-KOCH V., ALVES J., BALAGUER-NUNEZ L., BARKLEM P.S., BARRADO D., BELLAZZINI M., BERLANAS S.R., BINKS A.S., BRESSAN A., CAPUZZO-DOLCETTA R., CASAGRANDE L., CASAMIQUELA L., COLLINS R.S., D'ORAZI V., DANTAS M.L.L., DEBATTISTA V.P., DELGADO-MENA E., DI MARCANTONIO P., DRAZDAUSKAS A., EVANS N.W., FAMAEY B., FRANCHINI M., FREMAT Y., FU X., GEISLER D., GERHARD O., GONZALEZ SOLARES E.A., GREBEL E.K., GUTIERREZ ALBARRAN M.L., JIMENEZ-ESTEBAN F., JONSSON H., KHACHATURYANTS T., KORDOPATIS G., KOS J., LAGARDE N., LUDWIG H.-G., MAHY L., MAPELLI M., MARFIL E., MARTELL S.L., MESSINA S., MIGLIO A., MINCHEV I., MOITINHO A., MONTALBAN J., MONTEIRO M.J.P.F.G., MOROSSI C., MOWLAVI N., MUCCIARELLI A., MURPHY D.N.A., NARDETTO N., ORTOLANI S., PALETOU F., PALOUS J., PICKERING J.C., QUIRRENBACH A., RE FIORENTIN P., READ J.I., ROMANO D., RYDE N., SANNA N., SANTOS W., SEABROKE G.M., SPINA L., STEINMETZ M., STONKUTE E., SUTORIUS E., THEVENIN F., TOSI M., TSANTAKI M., WRIGHT N., WYSE R.F.G., ZOCCALI M., ZOREC J. and ZUCKER D.B.

Abstract (from CDS):


Context. The Gaia-ESO Public Spectroscopic Survey is an ambitious project designed to obtain astrophysical parameters and elemental abundances for 100 000 stars, including large representative samples of the stellar populations in the Galaxy, and a well-defined sample of 60 (plus 20 archive) open clusters. We provide internally consistent results calibrated on benchmark stars and star clusters, extending across a very wide range of abundances and ages. This provides a legacy data set of intrinsic value, and equally a large wide-ranging dataset that is of value for the homogenisation of other and future stellar surveys and Gaia's astrophysical parameters.
Aims. This article provides an overview of the survey methodology, the scientific aims, and the implementation, including a description of the data processing for the GIRAFFE spectra. A companion paper introduces the survey
Results.
Methods. Gaia-ESO aspires to quantify both random and systematic contributions to measurement uncertainties. Thus, all available spectroscopic analysis techniques are utilised, each spectrum being analysed by up to several different analysis pipelines, with considerable effort being made to homogenise and calibrate the resulting parameters. We describe here the sequence of activities up to delivery of processed data products to the ESO Science Archive Facility for open use. Results. The Gaia-ESO Survey obtained 202 000 spectra of 115 000 stars using 340 allocated VLT nights between December 2011 and January 2018 from GIRAFFE and UVES.
Conclusions. The full consistently reduced final data set of spectra was released through the ESO Science Archive Facility in late 2020, with the full astrophysical parameters sets following in 2022. A companion article reviews the survey implementation, scientific highlights, the open cluster survey, and data products.

Abstract Copyright: © G. Gilmore et al. 2022

Journal keyword(s): Galaxy: stellar content - Galaxy: kinematics and dynamics - stars: abundances - methods: observational - techniques: spectroscopic - surveys

Simbad objects: 41

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Number of rows : 41
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2024
#notes
1 NGC 104 GlC 00 24 05.359 -72 04 53.20     4.09     ~ 3922 0
2 NGC 188 OpC 00 47 11.5 +85 14 38           ~ 922 0
3 NAME Sculptor Dwarf Galaxy G 01 00 09.4 -33 42 32   9.79 8.6 8.81   ~ 1366 4
4 NGC 362 GlC 01 03 14.26 -70 50 55.6     6.58     ~ 1089 0
5 NGC 1261 GlC 03 12 16.21 -55 12 58.4     8.63     ~ 521 0
6 NGC 1851 GlC 05 14 06.76 -40 02 47.6           ~ 1433 0
7 M 79 GlC 05 24 10.59 -24 31 27.3     8.16     ~ 819 0
8 NGC 2243 OpC 06 29 34.8 -31 16 55   10.12 9.4     ~ 269 0
9 NGC 2264 OpC 06 40 52.1 +09 52 37           ~ 1793 0
10 Cl Berkeley 32 OpC 06 58 07.2 +06 25 59           ~ 145 0
11 Cl Melotte 71 OpC 07 37 31.9 -12 03 54   7.44 7.1     ~ 131 0
12 NGC 2420 OpC 07 38 24.5 +21 34 30   9.0 8.3     ~ 477 0
13 NGC 2451A OpC 07 42 56.6 -38 15 50           ~ 129 0
14 NGC 2451B OpC 07 44 30.7 -37 57 14           ~ 96 0
15 NGC 2451 Cl* 07 45.4 -37 58           ~ 158 1
16 NGC 2477 OpC 07 52 11.0 -38 32 13   6.64 5.8     ~ 290 0
17 Ass Vel OB 2 As* 08 09 22.478 -47 21 03.46           ~ 273 0
18 IC 2391 OpC 08 41 10.1 -52 59 28           ~ 822 0
19 HD 74438 * 08 41 46.5805673472 -53 03 44.995790376   7.81 7.58     A2mA5-A8 53 0
20 NGC 2682 OpC 08 51 23.0 +11 48 50           ~ 2342 0
21 NGC 2808 GlC 09 12 03.10 -64 51 48.6           ~ 1424 0
22 C 1035-584 OpC 10 36 05 -58 43.5           ~ 20 0
23 Cl Trumpler 14 OpC 10 43 56.6 -59 33 11   5.70 5.5     ~ 509 0
24 NGC 3532 OpC 11 05 40.1 -58 42 25           ~ 350 0
25 NGC 4372 GlC 12 25 45.43 -72 39 32.7   10.86 9.85     ~ 304 0
26 M 68 GlC 12 39 27.98 -26 44 38.6     7.96     ~ 999 0
27 NGC 4833 GlC 12 59 33.92 -70 52 35.4           ~ 426 0
28 AP J13583380+1421083 RB? 13 58 33.8132852928 +14 21 08.488847052           ~ 27 0
29 NAME Bootes Dwarf Spheroidal Galaxy G 14 00 00.0 +14 30 00     12.8     ~ 439 0
30 NGC 5927 GlC 15 28 00.69 -50 40 22.9           ~ 463 0
31 M 12 GlC 16 47 14.18 -01 56 54.7     6.07     ~ 681 0
32 NGC 6253 OpC 16 59 06.7 -52 42 43     10.2     ~ 186 0
33 NAME Sgr A* X 17 45 40.03599 -29 00 28.1699           ~ 4400 3
34 NGC 6530 OpC 18 04 31 -24 21.5           ~ 417 0
35 NGC 6553 GlC 18 09 15.68 -25 54 27.9   9.08       ~ 604 0
36 NGC 6705 OpC 18 51 03.8 -06 16 19   6.32 5.8     ~ 412 0
37 NAME SDG G 18 55 19.0 -30 32 43   4.5 3.6     ~ 2195 2
38 NGC 6752 GlC 19 10 52.11 -59 59 04.4           ~ 2004 0
39 M 15 GlC 21 29 58.33 +12 10 01.2           ~ 3143 0
40 M 2 GlC 21 33 27.02 -00 49 23.7     6.25     ~ 1032 1
41 NAME Monoceros Stream St* ~ ~           ~ 358 1

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