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Sérgio G. Sousa
Sérgio G. Sousa
Principal Researcher, Instituto de Astrofísica e Ciências do Espaço
E-mail confirmado em astro.up.pt - Página inicial
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The PLATO 2.0 mission
H Rauer, C Catala, C Aerts, T Appourchaux, W Benz, A Brandeker, ...
Experimental Astronomy 38, 249-330, 2014
13232014
The Gaia-ESO public spectroscopic survey
G Gilmore, S Randich, M Asplund, J Binney, P Bonifacio, J Drew, ...
The Messenger 147, 25-31, 2012
12432012
Spectroscopic parameters for 451 stars in the harps gto planet search program-stellar [fe/h] and the frequency of exo-neptunes
SG Sousa, NC Santos, M Mayor, S Udry, L Casagrande, G Israelian, ...
Astronomy & Astrophysics 487 (1), 373-381, 2008
6492008
Chemical abundances of 1111 FGK stars from the HARPS GTO planet search program-Galactic stellar populations and planets
VZ Adibekyan, SG Sousa, NC Santos, ED Mena, JIG Hernández, ...
Astronomy & Astrophysics 545, A32, 2012
5782012
A mean redshift of 2.8 for Swift gamma-ray bursts
P Jakobsson, A Levan, JPU Fynbo, R Priddey, J Hjorth, N Tanvir, ...
Astronomy & Astrophysics 447 (3), 897-903, 2006
3832006
ESPRESSO at VLT-On-sky performance and first results
F Pepe, S Cristiani, R Rebolo, NC Santos, H Dekker, A Cabral, ...
Astronomy & Astrophysics 645, A96, 2021
3702021
A new code for automatic determination of equivalent widths: Automatic Routine for line Equivalent widths in stellar Spectra (ARES)
SG Sousa, NC Santos, G Israelian, M Mayor, M Monteiro
Astronomy & Astrophysics 469 (2), 783-791, 2007
3532007
Ensemble asteroseismology of solar-type stars with the NASA Kepler mission
WJ Chaplin, H Kjeldsen, J Christensen-Dalsgaard, S Basu, A Miglio, ...
Science 332 (6026), 213-216, 2011
3432011
Spectroscopic stellar parameters for 582 FGK stars in the HARPS volume-limited sample-Revising the metallicity-planet correlation
SG Sousa, NC Santos, G Israelian, M Mayor, S Udry
Astronomy & Astrophysics 533, A141, 2011
3192011
SWEET-Cat: A catalogue of parameters for Stars With ExoplanETs-I. New atmospheric parameters and masses for 48 stars with planets
NC Santos, SG Sousa, A Mortier, V Neves, V Adibekyan, M Tsantaki, ...
Astronomy & Astrophysics 556, A150, 2013
3102013
Gaia FGK benchmark stars: Metallicity
P Jofré, U Heiter, C Soubiran, S Blanco-Cuaresma, CC Worley, E Pancino, ...
Astronomy & Astrophysics 564, A133, 2014
2972014
Spectroscopic metallicities for planet-host stars: Extending the samples
NC Santos, G Israelian, M Mayor, JP Bento, PC Almeida, SG Sousa, ...
Astronomy & Astrophysics 437 (3), 1127-1133, 2005
2762005
Fundamental properties of stars using asteroseismology from Kepler and CoRoT and interferometry from the CHARA array
D Huber, MJ Ireland, TR Bedding, IM Brandão, L Piau, V Maestro, ...
The Astrophysical Journal 760 (1), 32, 2012
2472012
ESPRESSO: The next European exoplanet hunter
F Pepe, P Molaro, S Cristiani, R Rebolo, NC Santos, H Dekker, ...
Astronomische Nachrichten 335 (1), 8-20, 2014
2392014
The Gaia-ESO Survey: The analysis of high-resolution UVES spectra of FGK-type stars
R Smiljanic, AJ Korn, M Bergemann, A Frasca, L Magrini, T Masseron, ...
Astronomy & Astrophysics 570, A122, 2014
2362014
Nightside condensation of iron in an ultrahot giant exoplanet
D Ehrenreich, C Lovis, R Allart, MR Zapatero Osorio, F Pepe, S Cristiani, ...
Nature 580 (7805), 597-601, 2020
2342020
ARES v2: new features and improved performance
SG Sousa, NC Santos, V Adibekyan, E Delgado-Mena, G Israelian
Astronomy & Astrophysics 577, A67, 2015
2232015
The CHEOPS mission
W Benz, C Broeg, A Fortier, N Rando, T Beck, M Beck, D Queloz, ...
Experimental Astronomy 51, 109-151, 2021
2182021
The HARPS search for southern extra-solar planets-XXXV. The interesting case of HD 41248: stellar activity, no planets?
NC Santos, A Mortier, JP Faria, X Dumusque, VZ Adibekyan, ...
Astronomy & Astrophysics 566, A35, 2014
211*2014
An ancient extrasolar system with five sub-Earth-size planets
TL Campante, T Barclay, JJ Swift, D Huber, VZ Adibekyan, W Cochran, ...
The Astrophysical Journal 799 (2), 170, 2015
2072015
O sistema não pode executar a operação agora. Tente novamente mais tarde.
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