The Gaia-ESO Public Spectroscopic Survey: Motivation, implementation, GIRAFFE data processing, analysis, and final data products star
Authors
GILMORE, G.; S. RANDICH; C. C. WORLEY; A. HOURIHANE; A. GONNEAU; G. G. SACCO; J. R. LEWIS; L. MAGRINI; P. FRANCOIS; R. D. JEFFRIES; S. E. KOPOSOV; A. BRAGAGLIA; E. J. ALFARO; C. ALLENDE PRIETO; R. BLOMME; A. J. KORN; A. C. LANZAFAME; E. PANCINO; A. RECIO-BLANCO; R. SMILJANIC; S. VAN ECK; T. ZWITTER; T. BENSBY; E. FLACCOMIO; M. J. IRWIN; E. FRANCIOSINI; L. MORBIDELLI; F. DAMIANI; R. BONITO; E. D. FRIEL; J. S. VINK; L. PRISINZANO; U. ABBAS; D. HATZIDIMITRIOU; E. V. HELD; C. JORDI; Ernst PAUNZEN (40 Austria, belonging to the institution); A. SPAGNA; R. J. JACKSON; J. MAIZ APELLANIZ; M. ASPLUND; P. BONIFACIO; S. FELTZING; J. BINNEY; J. DREW; A. M. N. FERGUSON; G. MICELA; I. NEGUERUELA; T. PRUSTI; H.-W. RIX; A. VALLENARI; M. BERGEMANN; A. R. CASEY; P. DE LAVERNY; A. FRASCA; V. HILL; K. LIND; L. SBORDONE; S. G. SOUSA; V. ADIBEKYAN; E. CAFFAU; S. DAFLON; D. K. FEUILLET; M. GEBRAN; J. I. GONZALEZ HERNANDEZ; G. GUIGLION; A. HERRERO; A. LOBEL; D. MONTES; T. MOREL; G. RUCHTI; C. SOUBIRAN; H. M. TABERNERO; G. TAUTVAISIENE; G. TRAVEN; M. VALENTINI; M. VAN DER SWAELMEN; S. VILLANOVA; C. VISCASILLAS VAZQUEZ; A. BAYO; K. BIAZZO; G. CARRARO; B. EDVARDSSON; U. HEITER; P. JOFRE; G. MARCONI; C. MARTAYAN; T. MASSERON; L. MONACO; N. A. WALTON; S. ZAGGIA; V. Aguirre BORSEN-KOCH; J. ALVES; L. BALAGUER-NUNEZ; P. S. BARKLEM; D. BARRADO; M. BELLAZZINI; S. R. BERLANAS; A. S. BINKS; A. BRESSAN; R. CAPUZZO-DOLCETTA; L. CASAGRANDE; L. CASAMIQUELA; R. S. COLLINS; V. ORAZI; M. L. L. DANTAS; V. P. DEBATTISTA; E. DELGADO-MENA; P. DI MARCANTONIO; A. DRAZDAUSKAS; N. W. EVANS; B. FAMAEY; M. FRANCHINI; Y. FREMAT; X. FU; D. GEISLER; O. GERHARD; E. A. Gonzalez SOLARES; E. K. GREBEL; M. L. GUTIERREZ ALBARRAN; F. JIMENEZ-ESTEBAN; H. JONSSON; T. KHACHATURYANTS; G. KORDOPATIS; J. KOS; N. LAGARDE; H.-G. LUDWIG; L. MAHY; M. MAPELLI; E. MARFIL; S. L. MARTELL; S. MESSINA; A. MIGLIO; I. MINCHEV; A. MOITINHO; J. MONTALBAN; M. J. P. F. G. MONTEIRO; C. MOROSSI; N. MOWLAVI; A. MUCCIARELLI; D. N. A. MURPHY; N. NARDETTO; S. ORTOLANI; F. PALETOU; J. PALOUS; J. C. PICKERING; A. QUIRRENBACH; P. Re FIORENTIN; J. I. READ; D. ROMANO; N. RYDE; N. SANNA; W. SANTOS; G. M. SEABROKE; L. SPINA; M. STEINMETZ; E. STONKUTE; E. SUTORIUS; F. THEVENIN; M. TOSI; M. TSANTAKI; N. WRIGHT; R. F. G. WYSE; M. ZOCCALI; J. ZOREC and D. B. ZUCKER
Edition
Astronomy & Astrophysics, EDP SCIENCES S A, 2022, 0004-6361
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.
GILMORE, G.; S. RANDICH; C. C. WORLEY; A. HOURIHANE; A. GONNEAU; G. G. SACCO; J. R. LEWIS; L. MAGRINI; P. FRANCOIS; R. D. JEFFRIES; S. E. KOPOSOV; A. BRAGAGLIA; E. J. ALFARO; C. ALLENDE PRIETO; R. BLOMME; A. J. KORN; A. C. LANZAFAME; E. PANCINO; A. RECIO-BLANCO; R. SMILJANIC; S. VAN ECK; T. ZWITTER; T. BENSBY; E. FLACCOMIO; M. J. IRWIN; E. FRANCIOSINI; L. MORBIDELLI; F. DAMIANI; R. BONITO; E. D. FRIEL; J. S. VINK; L. PRISINZANO; U. ABBAS; D. HATZIDIMITRIOU; E. V. HELD; C. JORDI; Ernst PAUNZEN; A. SPAGNA; R. J. JACKSON; J. MAIZ APELLANIZ; M. ASPLUND; P. BONIFACIO; S. FELTZING; J. BINNEY; J. DREW; A. M. N. FERGUSON; G. MICELA; I. NEGUERUELA; T. PRUSTI; H.-W. RIX; A. VALLENARI; M. BERGEMANN; A. R. CASEY; P. DE LAVERNY; A. FRASCA; V. HILL; K. LIND; L. SBORDONE; S. G. SOUSA; V. ADIBEKYAN; E. CAFFAU; S. DAFLON; D. K. FEUILLET; M. GEBRAN; J. I. GONZALEZ HERNANDEZ; G. GUIGLION; A. HERRERO; A. LOBEL; D. MONTES; T. MOREL; G. RUCHTI; C. SOUBIRAN; H. M. TABERNERO; G. TAUTVAISIENE; G. TRAVEN; M. VALENTINI; M. VAN DER SWAELMEN; S. VILLANOVA; C. VISCASILLAS VAZQUEZ; A. BAYO; K. BIAZZO; G. CARRARO; B. EDVARDSSON; U. HEITER; P. JOFRE; G. MARCONI; C. MARTAYAN; T. MASSERON; L. MONACO; N. A. WALTON; S. ZAGGIA; V. Aguirre BORSEN-KOCH; J. ALVES; L. BALAGUER-NUNEZ; P. S. BARKLEM; D. BARRADO; M. BELLAZZINI; S. R. BERLANAS; A. S. BINKS; A. BRESSAN; R. CAPUZZO-DOLCETTA; L. CASAGRANDE; L. CASAMIQUELA; R. S. COLLINS; V. ORAZI; M. L. L. DANTAS; V. P. DEBATTISTA; E. DELGADO-MENA; P. DI MARCANTONIO; A. DRAZDAUSKAS; N. W. EVANS; B. FAMAEY; M. FRANCHINI; Y. FREMAT; X. FU; D. GEISLER; O. GERHARD; E. A. Gonzalez SOLARES; E. K. GREBEL; M. L. GUTIERREZ ALBARRAN; F. JIMENEZ-ESTEBAN; H. JONSSON; T. KHACHATURYANTS; G. KORDOPATIS; J. KOS; N. LAGARDE; H.-G. LUDWIG; L. MAHY; M. MAPELLI; E. MARFIL; S. L. MARTELL; S. MESSINA; A. MIGLIO; I. MINCHEV; A. MOITINHO; J. MONTALBAN; M. J. P. F. G. MONTEIRO; C. MOROSSI; N. MOWLAVI; A. MUCCIARELLI; D. N. A. MURPHY; N. NARDETTO; S. ORTOLANI; F. PALETOU; J. PALOUS; J. C. PICKERING; A. QUIRRENBACH; P. Re FIORENTIN; J. I. READ; D. ROMANO; N. RYDE; N. SANNA; W. SANTOS; G. M. SEABROKE; L. SPINA; M. STEINMETZ; E. STONKUTE; E. SUTORIUS; F. THEVENIN; M. TOSI; M. TSANTAKI; N. WRIGHT; R. F. G. WYSE; M. ZOCCALI; J. ZOREC and D. B. ZUCKER. The Gaia-ESO Public Spectroscopic Survey: Motivation, implementation, GIRAFFE data processing, analysis, and final data products star. Astronomy & Astrophysics. EDP SCIENCES S A, 2022, vol. 666, October, p. 1-36. ISSN 0004-6361. Available from: https://doi.org/10.1051/0004-6361/202243134.
@article{2247858, author = {Gilmore, G. and Randich, S. and Worley, C. C. and Hourihane, A. and Gonneau, A. and Sacco, G. G. and Lewis, J. R. and Magrini, L. and Francois, P. and Jeffries, R. D. and Koposov, S. E. and Bragaglia, A. and Alfaro, E. J. and Allende Prieto, C. and Blomme, R. and Korn, A. J. and Lanzafame, A. C. and Pancino, E. and RecioandBlanco, A. and Smiljanic, R. and Van Eck, S. and Zwitter, T. and Bensby, T. and Flaccomio, E. and Irwin, M. J. and Franciosini, E. and Morbidelli, L. and Damiani, F. and Bonito, R. and Friel, E. D. and Vink, J. S. and Prisinzano, L. and Abbas, U. and Hatzidimitriou, D. and Held, E. V. and Jordi, C. and Paunzen, Ernst and Spagna, A. and Jackson, R. J. and Maiz Apellaniz, J. and Asplund, M. and Bonifacio, P. and Feltzing, S. and Binney, J. and Drew, J. and Ferguson, A. M. N. and Micela, G. and Negueruela, I. and Prusti, T. and Rix, H.andW. and Vallenari, A. and Bergemann, M. and Casey, A. R. and de Laverny, P. and Frasca, A. and Hill, V. and Lind, K. and Sbordone, L. and Sousa, S. G. and Adibekyan, V. and Caffau, E. and Daflon, S. and Feuillet, D. K. and Gebran, M. and Gonzalez Hernandez, J. I. and Guiglion, G. and Herrero, A. and Lobel, A. and Montes, D. and Morel, T. and Ruchti, G. and Soubiran, C. and Tabernero, H. M. and Tautvaisiene, G. and Traven, G. and Valentini, M. and Van der Swaelmen, M. and Villanova, S. and Viscasillas Vazquez, C. and Bayo, A. and Biazzo, K. and Carraro, G. and Edvardsson, B. and Heiter, U. and Jofre, P. and Marconi, G. and Martayan, C. and Masseron, T. and Monaco, L. and Walton, N. A. and Zaggia, S. and BorsenandKoch, V. Aguirre and Alves, J. and BalaguerandNunez, L. and Barklem, P. S. and Barrado, D. and Bellazzini, M. and Berlanas, S. R. and Binks, A. S. and Bressan, A. and CapuzzoandDolcetta, R. and Casagrande, L. and Casamiquela, L. and Collins, R. S. and Orazi, V. and Dantas, M. L. L. and Debattista, V. P. and DelgadoandMena, E. and Di Marcantonio, P. and Drazdauskas, A. and Evans, N. W. and Famaey, B. and Franchini, M. and Fremat, Y. and Fu, X. and Geisler, D. and Gerhard, O. and Solares, E. A. Gonzalez and Grebel, E. K. and Gutierrez Albarran, M. L. and JimenezandEsteban, F. and Jonsson, H. and Khachaturyants, T. and Kordopatis, G. and Kos, J. and Lagarde, N. and Ludwig, H.andG. and Mahy, L. and Mapelli, M. and Marfil, E. and Martell, S. L. and Messina, S. and Miglio, A. and Minchev, I. and Moitinho, A. and Montalban, J. and Monteiro, M. J. P. F. G. and Morossi, C. and Mowlavi, N. and Mucciarelli, A. and Murphy, D. N. A. and Nardetto, N. and Ortolani, S. and Paletou, F. and Palous, J. and Pickering, J. C. and Quirrenbach, A. and Fiorentin, P. Re and Read, J. I. and Romano, D. and Ryde, N. and Sanna, N. and Santos, W. and Seabroke, G. M. and Spina, L. and Steinmetz, M. and Stonkute, E. and Sutorius, E. and Thevenin, F. and Tosi, M. and Tsantaki, M. and Wright, N. and Wyse, R. F. G. and Zoccali, M. and Zorec, J. and Zucker, D. B.}, article_number = {October}, doi = {https://doi.org/10.1051/0004-6361/202243134}, keywords = {Galaxy; stellar content; Galaxy; kinematics and dynamics; stars; abundances; methods; observational; techniques; spectroscopic; surveys}, language = {eng}, issn = {0004-6361}, journal = {Astronomy & Astrophysics}, title = {The Gaia-ESO Public Spectroscopic Survey: Motivation, implementation, GIRAFFE data processing, analysis, and final data products star}, url = {https://www.aanda.org/articles/aa/full_html/2022/10/aa43134-22/aa43134-22.html}, volume = {666}, year = {2022} }
TY - JOUR ID - 2247858 AU - 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, Ernst - 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. - 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. - Borsen-Koch, V. Aguirre - 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. - 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. - Solares, E. A. Gonzalez - 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. - Fiorentin, P. Re - 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. - Zucker, D. B. PY - 2022 TI - The Gaia-ESO Public Spectroscopic Survey: Motivation, implementation, GIRAFFE data processing, analysis, and final data products star JF - Astronomy & Astrophysics VL - 666 IS - October SP - 1-36 EP - 1-36 PB - EDP SCIENCES S A SN - 00046361 KW - Galaxy KW - stellar content KW - Galaxy KW - kinematics and dynamics KW - stars KW - abundances KW - methods KW - observational KW - techniques KW - spectroscopic KW - surveys UR - https://www.aanda.org/articles/aa/full_html/2022/10/aa43134-22/aa43134-22.html N2 - 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. ER -
GILMORE, G.; S. RANDICH; C. C. WORLEY; A. HOURIHANE; A. GONNEAU; G. G. SACCO; J. R. LEWIS; L. MAGRINI; P. FRANCOIS; R. D. JEFFRIES; S. E. KOPOSOV; A. BRAGAGLIA; E. J. ALFARO; C. ALLENDE PRIETO; R. BLOMME; A. J. KORN; A. C. LANZAFAME; E. PANCINO; A. RECIO-BLANCO; R. SMILJANIC; S. VAN ECK; T. ZWITTER; T. BENSBY; E. FLACCOMIO; M. J. IRWIN; E. FRANCIOSINI; L. MORBIDELLI; F. DAMIANI; R. BONITO; E. D. FRIEL; J. S. VINK; L. PRISINZANO; U. ABBAS; D. HATZIDIMITRIOU; E. V. HELD; C. JORDI; Ernst PAUNZEN; A. SPAGNA; R. J. JACKSON; J. MAIZ APELLANIZ; M. ASPLUND; P. BONIFACIO; S. FELTZING; J. BINNEY; J. DREW; A. M. N. FERGUSON; G. MICELA; I. NEGUERUELA; T. PRUSTI; H.-W. RIX; A. VALLENARI; M. BERGEMANN; A. R. CASEY; P. DE LAVERNY; A. FRASCA; V. HILL; K. LIND; L. SBORDONE; S. G. SOUSA; V. ADIBEKYAN; E. CAFFAU; S. DAFLON; D. K. FEUILLET; M. GEBRAN; J. I. GONZALEZ HERNANDEZ; G. GUIGLION; A. HERRERO; A. LOBEL; D. MONTES; T. MOREL; G. RUCHTI; C. SOUBIRAN; H. M. TABERNERO; G. TAUTVAISIENE; G. TRAVEN; M. VALENTINI; M. VAN DER SWAELMEN; S. VILLANOVA; C. VISCASILLAS VAZQUEZ; A. BAYO; K. BIAZZO; G. CARRARO; B. EDVARDSSON; U. HEITER; P. JOFRE; G. MARCONI; C. MARTAYAN; T. MASSERON; L. MONACO; N. A. WALTON; S. ZAGGIA; V. Aguirre BORSEN-KOCH; J. ALVES; L. BALAGUER-NUNEZ; P. S. BARKLEM; D. BARRADO; M. BELLAZZINI; S. R. BERLANAS; A. S. BINKS; A. BRESSAN; R. CAPUZZO-DOLCETTA; L. CASAGRANDE; L. CASAMIQUELA; R. S. COLLINS; V. ORAZI; M. L. L. DANTAS; V. P. DEBATTISTA; E. DELGADO-MENA; P. DI MARCANTONIO; A. DRAZDAUSKAS; N. W. EVANS; B. FAMAEY; M. FRANCHINI; Y. FREMAT; X. FU; D. GEISLER; O. GERHARD; E. A. Gonzalez SOLARES; E. K. GREBEL; M. L. GUTIERREZ ALBARRAN; F. JIMENEZ-ESTEBAN; H. JONSSON; T. KHACHATURYANTS; G. KORDOPATIS; J. KOS; N. LAGARDE; H.-G. LUDWIG; L. MAHY; M. MAPELLI; E. MARFIL; S. L. MARTELL; S. MESSINA; A. MIGLIO; I. MINCHEV; A. MOITINHO; J. MONTALBAN; M. J. P. F. G. MONTEIRO; C. MOROSSI; N. MOWLAVI; A. MUCCIARELLI; D. N. A. MURPHY; N. NARDETTO; S. ORTOLANI; F. PALETOU; J. PALOUS; J. C. PICKERING; A. QUIRRENBACH; P. Re FIORENTIN; J. I. READ; D. ROMANO; N. RYDE; N. SANNA; W. SANTOS; G. M. SEABROKE; L. SPINA; M. STEINMETZ; E. STONKUTE; E. SUTORIUS; F. THEVENIN; M. TOSI; M. TSANTAKI; N. WRIGHT; R. F. G. WYSE; M. ZOCCALI; J. ZOREC and D. B. ZUCKER. The Gaia-ESO Public Spectroscopic Survey: Motivation, implementation, GIRAFFE data processing, analysis, and final data products star. \textit{Astronomy \&{} Astrophysics}. EDP SCIENCES S A, 2022, vol.~666, October, p.~1-36. ISSN~0004-6361. Available from: https://doi.org/10.1051/0004-6361/202243134.