If you posses a bachelor’s degree in the field of physics, engineering, space science, astronomy, and science in general, and you are interested in pursuing masters and doctoral studies, you may apply to the scholarships funded by the administration through public calls. A brief description of each scholarship is provided to give an idea of the type of scholarship you may apply to depending on your personal and professional background.
It is highly recommended to carry out a PhD with the aid of a scholarship, fellowship or grant since universities and research institutes rarely offer research positions entirely funded on their own.
If you are coming from abroad, take into consideration that grant resolutions may take several months and not always occur during the same time of the year as previous calls.
Spanish regulations concerning PhD scholarships are varying at the moment due to the immersion of the Bologna Program into the academic cycle. Therefore, in principle, scholarships assure 4 years of salary and registration fees for the master’s and PhD programs. However, not all scholarships cover complete registration fees for both programs so you must be aware of this issue when commencing the application process.
|Cosmological models of the early- and late- universe with bradion and tachion fields||N. Myrzakulov||Odintsov, S. D.||read (2016-12-27)|
|Producing simulated catalogues for next generation galaxy surveys||Izard, A.||Fosalba, P. and Crocce, M.||read (2016-07-20)|
|Observation and interpretation of type IIb supernova explosions||Morales-Garoffolo, A.||Elias-Rosa, N. and Isern, J.||read (2016-03-08)|
|Thermal Diagnostics Experiments for LISA Pathfinder||Gibert, F.||Nofrarias, M.||read (2016-02-23)|
|Design and Assessment of a low-frequency magnetic measurement system for eLISA||Mateos, I.||Lobo, J. A. and Juan Ramos (UPC)||read (2015-11-27)|
|Cosmology with Galaxy Clustering||Hoffmann, K.||Gaztañaga, E.||read (2015-06-11)|
|Bayesian data analysis for LISA Pathfinder. Techniques applied to system identificaction experiments. ||Karnesis, N.||Sopuerta, C. F. and Nofrarias, M.||read (2015-01-13)|
|Stellar activity in exoplanet hosts
||Herrero, E.||Ribas, I.||read (2014-10-06)|
|Theory and observations of the PWN-SNR complex||Martín, J.||Torres, D. F. and Rea, N.||read (2014-07-21)|
|Weak Lensing Analysis of an All-Sky Simulation||López-Arenillas, C.||Fosalba, P. and Gaztañaga, E.||read (2014-01-24)|
|CROSS-CORRELATING SPECTROSCOPIC AND PHOTOMETRIC GALAXY SURVEYS||Eriksen, M. B.||Gaztañaga, E.||read (2014-01-16)|
|Dynamically-generated baryon resonances with heavy flavor||Romanets, O. (KVI, University of Groningen)||Tolos, L. and Timmermans, R. (KVI, University of Groningen)||read (2014-01-10)|
|Theories of modified gravity and reconstruction schemes of cosmological models||López-Revelles, A. J.||Elizalde, E. and Odintsov, S. D.||read (2013-11-08)|
|Measuring Large Scale Structure using angular cross-correlations||Asorey, J.||Gaztañaga, E. and Crocce, M.||read (2013-09-27)|
|Gamma-ray emission of young stellar objects and discovery of superorbital variability at high energies||Hadasch, D.||Torres, D. F. and Font, Ll. (UAB)||read (2013-07-30)|
|GNSS-R as a Source of Opportunity for Remote Sensing of the Cryosphere||Fabra, F.||Cardellach, E.||read (2013-05-13)|
|GNSS-R as a Source of Opportunity for Remote Sensing of the Cryosphere||Fabra, F.||Cardellach, E. and UPC Tutor: A. Camps||read (2013-05-13)|
|Populating cosmological simulations with galaxy using the HOD model||Carretero-Palacios, J.||Castander, F. J. and Gaztañaga, E.||read (2013-02-01)|
|The role of magnetic fields in the formation of low and high mass stars||Frau, P.||Girart, J. M. and Beltrán, M. T.||read (2012-06-12)|
|Star formation ahead of the Herbig-Haro 80N||Masqué, J. M.||Girart, J. M. and Estalella, R.||read (2012-03-23)|