T
T. Prusti
Researcher at European Space Research and Technology Centre
Publications - 59
Citations - 26215
T. Prusti is an academic researcher from European Space Research and Technology Centre. The author has contributed to research in topics: Stars & Astrometry. The author has an hindex of 31, co-authored 41 publications receiving 21645 citations. Previous affiliations of T. Prusti include Max Planck Society.
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Journal ArticleDOI
The Gaia-ESO Survey: processing FLAMES-UVES spectra
G. G. Sacco,L. Morbidelli,E. Franciosini,Enrico Maiorca,Sofia Randich,Andrea Modigliani,Gerard Gilmore,Martin Asplund,James Binney,Piercarlo Bonifacio,Janet E. Drew,Sofia Feltzing,Annette M. N. Ferguson,R. D. Jeffries,Giuseppina Micela,Ignacio Negueruela,T. Prusti,H. W. Rix,Antonella Vallenari,Emilio J. Alfaro,C. Allende Prieto,C. Allende Prieto,C. Babusiaux,Thomas Bensby,R. Blomme,Angela Bragaglia,Ettore Flaccomio,P. Francois,Nigel Hambly,Mike Irwin,Sergey E. Koposov,Andreas Korn,A. C. Lanzafame,Elena Pancino,Elena Pancino,Alejandra Recio-Blanco,Rodolfo Smiljanic,S. Van Eck,N. A. Walton,Maria Bergemann,M. T. Costado,P. de Laverny,Ulrike Heiter,Vanessa Hill,A. Hourihane,R. J. Jackson,Paula Jofre,Jack Lewis,Karin Lind,Carmela Lardo,Laura Magrini,Thomas Masseron,L. Prisinzano,Clare Worley +53 more
TL;DR: In this article, the authors describe the methods and software used for the data reduction, the derivation of the radial velocities, and the quality control of the FLAMES-UVES spectra.
Journal ArticleDOI
Long-term evolution of FU Orionis objects at infrared wavelengths
TL;DR: In this paper, the brightness evolution of seven FU Orionis systems in the 1−100 µm wavelength range using data from the Infrared Space Observatory (ISO) was investigated.
Journal ArticleDOI
Gaia-ESO Survey: Analysis of pre-main sequence stellar spectra
A. C. Lanzafame,Antonio Frasca,Francesco Damiani,E. Franciosini,Michiel Cottaar,S. G. Sousa,Hugo M. Tabernero,A. Klutsch,Lorenzo Spina,K. Biazzo,L. Prisinzano,G. G. Sacco,Sofia Randich,E. Brugaletta,E. Delgado Mena,V. Adibekyan,D. Montes,Rosaria Bonito,Rosaria Bonito,J. F. Gameiro,J. M. Alcalá,J. I. González Hernández,J. I. González Hernández,R. D. Jeffries,Sergio Messina,Michael Meyer,Gerard Gilmore,Martin Asplund,James Binney,Piercarlo Bonifacio,Janet E. Drew,Sofia Feltzing,Annette M. N. Ferguson,Giuseppina Micela,Ignacio Negueruela,T. Prusti,H. W. Rix,Antonella Vallenari,Emilio J. Alfaro,C. Allende Prieto,C. Allende Prieto,C. Babusiaux,Thomas Bensby,R. Blomme,Angela Bragaglia,Ettore Flaccomio,P. Francois,Nigel Hambly,Mike Irwin,Sergey E. Koposov,Sergey E. Koposov,Andreas Korn,Rodolfo Smiljanic,S. Van Eck,N. A. Walton,Amelia Bayo,Maria Bergemann,Giovanni Carraro,M. T. Costado,Bengt Edvardsson,Ulrike Heiter,Vanessa Hill,A. Hourihane,R. J. Jackson,Paula Jofre,Carmela Lardo,Jack Lewis,Karin Lind,Laura Magrini,Gianni Marconi,Ch. Martayan,Thomas Masseron,Lorenzo Monaco,L. Morbidelli,Luca Sbordone,Clare Worley,Simone Zaggia +76 more
TL;DR: In this article, the analysis of UVES and GIRAFFE spectra acquired in the fields of young clusters whose population includes pre-main sequence (PMS) stars is presented.
Journal ArticleDOI
Far-infrared and molecular line observations of Lynds 183 - Studies of cold gas and dust
TL;DR: In this article, the authors have mapped the dark cloud L183 in the far-infrared at 100 m and 200 m with the ISOPHOT photometer aboard the ISO satellite.
Journal ArticleDOI
The Gaia-ESO Survey: Empirical determination of the precision of stellar radial velocities and projected rotation velocities
R. J. Jackson,R. D. Jeffries,James R. Lewis,Sergey E. Koposov,Sergey E. Koposov,G. G. Sacco,Sofia Randich,Gerard Gilmore,Martin Asplund,James Binney,Piercarlo Bonifacio,Janet E. Drew,Sofia Feltzing,Annette M. N. Ferguson,Giuseppina Micela,I. Neguerela,T. Prusti,Hans-Walter Rix,Antonella Vallenari,Emilio J. Alfaro,C. Allende Prieto,C. Allende Prieto,C. Babusiaux,Thomas Bensby,R. Blomme,Angela Bragaglia,Ettore Flaccomio,P. Francois,Nigel Hambly,Mike Irwin,Andreas Korn,A. C. Lanzafame,Elena Pancino,Alejandra Recio-Blanco,Rodolfo Smiljanic,S. Van Eck,Nicholas A. Walton,Amelia Bayo,Maria Bergemann,Giovanni Carraro,M. T. Costado,Francesco Damiani,Bengt Edvardsson,E. Franciosini,Antonio Frasca,Ulrike Heiter,Vanessa Hill,A. Hourihane,Paula Jofre,Carmela Lardo,P. de Laverny,Karin Lind,Laura Magrini,Gianni Marconi,Christophe Martayan,Thomas Masseron,Lorenzo Monaco,L. Morbidelli,L. Prisinzano,Luca Sbordone,Luca Sbordone,S. G. Sousa,Clare Worley,Simone Zaggia +63 more
TL;DR: In this paper, the authors present an analysis to empirically quantify the size and distribution of uncertainties in RV and v sin i using spectra from repeated exposures of the same stars, and show that the uncertainties vary as simple scaling functions of signal-to-noise ratio (S/N) and projected equatorial velocities (v sin i) for representative samples of Galactic stars.