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Centro de Astrofísica da Universidade do Porto

Ângela R. G. Santos
Ph.D. Student

This ph.d. student left CAUP in 14 June 2017

Phone
+351 226 089 882

Email
Angela.Santos@astro.up.pt

Lastest publications at CAUP/IA
R. A. García, C. Gourvès, A. R. G. Santos, A. Strugarek, D. Godoy-Rivera, S. Mathur, V. Delsanti, S. N. Breton, P. G. Beck, A. S. Brun, S. Mathis, 2023,
Stellar spectral-type (mass) dependence of the dearth of close-in planets around fast-rotating stars
Architecture of Kepler confirmed single-exoplanet systems compared to star-planet evolution models
,
Astronomy & Astrophysics, 679, 13
>> Abstract
S. N. Breton, H. Dhouib, R. A. Garcia, A. S. Brun, S. Mathis, F. Pérez Hernández, S. Mathur, A. Dyrek, A. R. G. Santos, P. L. Pallé, 2023,
In search of gravity mode signatures in main sequence solar-type stars observed by Kepler,
Astronomy & Astrophysics, 679, 19
>> Abstract
S. Mathur, Z. R. Claytor, A. R. G. Santos, R. A. García, L. Amard, L. Bugnet, E. Corsaro, A. Bonanno, S. N. Breton, D. Godoy-Rivera, M. H. Pinsonneault, J. L. Van Saders, 2023,
Magnetic Activity Evolution of Solar-like Stars. I. Sph- Age Relation Derived from Kepler Observations,
The Astrophysical Journal, 952
>> Abstract
A. R. G. Santos, S. Mathur, R. A. García, A.-M. Broomhall, R. Egeland, A. Jiménez, D. Godoy-Rivera, S. N. Breton, Z. R. Claytor, T. S. Metcalfe, M. S. Cunha, L. Amard, 2023,
Temporal variation of the photometric magnetic activity for the Sun and Kepler solar-like stars,
Astronomy & Astrophysics, 672, 22
>> Abstract
A. I. Henriksen, V. Antoci, H. Saio, M. Cantiello, H. Kjeldsen, D. W. Kurtz, S. J. Murphy, S. Mathur, R. A. García, A. R. G. Santos, 2023,
Journal Article Rotational modulation in A and F stars: magnetic stellar spots or convective core rotation?,
Monthly Notices of the Royal Astronomical Society, 520, 216 - 232
>> Abstract
Q. Noraz, S. N. Breton, A. S. Brun, R. A. García, A. Strugarek, A. R. G. Santos, S. Mathur, L. Amard, 2022,
Hunting for anti-solar differentially rotating stars using the Rossby number. An application to the Kepler field,
Astronomy & Astrophysics, 667, 16
>> Abstract