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Isa Brandão finished her graduate studies on Physics/Applied Mathematics at Porto University in 2005 and in 2007 was awarded with the MSc degree in astronomy at the same University. In 2012, she finished her mixed PhD (with the Aarhus University, Denmark) in astronomy, the title given by the Porto University. She is now a researcher at Astrophysics Institute - CAUP with a post-doc grant from FCT Portugal.
Current research interests include:
- Modeling of solar like stars by using non-seismic data and, when available, information from stellar pulsations (a technique called asteroseismology) in order to obtain their fundamental parameters, such as the mass, radius, and age, with high precision. Very interested in characterizing planet-hosting stars.
- Use of seismic diagnostic tools for inference on stellar interiors and, in particular, the properties of the core. The evolutionary state of a star (age) is strongly dependent on the properties of its core. On the other hand, knowing stellar interiors is useful to understand the physics occurring there and consequently improve stellar evolutionary codes.
- Development of methods in order to improve the offset between the observed and model frequencies that exists due to our inability of properly model the outer layers of stars.
Lastest publications at IAK. Perraut, I. M. Brandão, M. S. Cunha, D. Shulyak, D. Mourard, N. Nardetto, T. A. ten Brummelaar, 2016,
The fundamental parameters of the roAp star HD 24712. A rapidly oscillator at the red edge of the instability strip,
Astronomy and Astrophysics, 590, 6
>> AbstractS. Deheuvels, I. M. Brandão, V. Silva Aguirre, J. Ballot, E. Michel, M. S. Cunha, Y. Lebreton, T. Appourchaux, 2016,
Measuring the extent of convective cores in low-mass stars using Kepler data: toward a calibration of core overshooting,
Astronomy and Astrophysics, 589, 26
>> AbstractK. Perraut, M. S. Cunha, I. M. Brandão, J. Loridat, D. Mourard, A. Meilland, N. Nardetto, H. McAlister, T. A. ten Brummelaar, J. Sturmann, 2015,
The fundamental parameters of the Ap star 78 Virginis
Could 78 Vir be a rapidly oscillating Ap star?,
Astronomy and Astrophysics, 579, A85
>> AbstractJ. Casanellas, I. M. Brandão, Y. Lebreton, 2015,
Stellar convective cores as dark matter probes,
Physical Review D, 91, 103535
>> AbstractA. Mortier, S. G. Sousa, V. Zh. Adibekyan, I. M. Brandão, N. C. Santos, 2014,
Correcting the spectroscopic surface gravity using transits and asteroseismology
No significant effect on temperatures or metallicities with ARES and MOOG in local thermodynamic equilibrium,
Astronomy and Astrophysics, 572, A95_1 - A95_13
>> AbstractH. Rauer, C. Catala, C. Aerts, T. Appourchaux, W. Benz, A. Brandeker, J. Christensen-Dalsgaard, M. Deleuil, L. Gizon, M.-J. Goupil et al. (including: N. C. Santos, V. Zh. Adibekyan, I. Boisse, I. M. Brandão, M. S. Cunha, P. Figueira, J. Gomes da Silva, J. H. C. Martins, M. Montalto, M. J. P. F. G. Monteiro, A. Mortier, M. Oshagh, B. Rojas-Ayala, A. Santerne, S. G. Sousa), 2014,
The PLATO 2.0 Mission,
Experimental Astronomy, 38, 249 - 330