Biblioteca de la Universidad Complutense de Madrid

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Número de eprints: 14.

Vázquez Poletti, José Luis y Barderas, Gonzalo y Llorente, Ignacio M. y Romero Pérez, Mª Pilar (2012) A model for efficient onboard actualization of an instrumental cyclogram for the Mars Metnet mission on a public cloud infrastructure. In Applied Parallel and Scientific Computing. Lecture Notes in Computer Science (7133). Springer, pp. 33-42. ISBN 978-3-642-28150-1

Zamorano, P. y Gambi Fernández, José María y Romero Pérez, Mª Pilar y García del Pino, M.L. (2002) Description of orbits with polar Gaussian coordinates in the post-Newtonian approximation of a spherically symmetric field. Il Nuovo Cimento della Società Italiana di Fisica - B: General Physics, Relativity, Astronomy and Mathematical Physics and Methods, 117 (4). pp. 441-448. ISSN 1594-9982

Gambi Fernández, José María y Romero Pérez, Mª Pilar y San Miguel, A. y Vicente, F. (1991) Fermi Coordinate Transformation under Baseline Change in Relativistic Celestial Mechanics. International Journal of Theoretical Physics, 30 (8). pp. 1097-1116. ISSN 0020-7748

Sevilla de Lerma, Miguel Jesús y Romero Pérez, Mª Pilar (1991) Ground deformation control by statistical analysis of a geodetic network in the caldera of Teide. Journal of volcanology and geothermal research, 47 (1-2). pp. 65-74. ISSN 0377-0273

Gambi, J.M. y Romero Pérez, Mª Pilar y Zamorano, P. y García del Pino, M.L. (2000) Non-linear effects in the post-Newtonian approximation of a spherically symmetric field. Il Nuovo Cimento della Società Italiana di Fisica - B: General Physics, Relativity, Astronomy and Mathematical Physics and Methods, 115 (2). pp. 165-178. ISSN 1594-9982

Romero Pérez, Mª Pilar (2013) On the inverse problem of determining Mars lander coordinates using Phobos eclipse observations. Planetary and Space Science , 79-80 . pp. 39-44. ISSN ISSN: 0032-0633

Gambi, J.M. y Zamorano, P. y Romero Pérez, Mª Pilar y García del Pino, M.L. (1996) On the orbital motion description with a proper reference frame in a complete schwarzschild field. In Dynamics, ephemerides, and astrometry of the solar system. Kluwer Academic, Dordrecht, pp. 325-326. ISBN 0-7923-4084-1

Barderas, Gonzalo y Romero Pérez, Mª Pilar y Vázquez Martínez, Luis y Vázquez Poletti, José Luis y Llorente, I. M. (2012) Opportunities to observe solar eclipses by Phobos with the Mars Science Laboratory. Monthly notices of the Royal Astronomical Society, 426 (4). 3195 -3200. ISSN 0035-8711

Silva, Juan J. y Romero Pérez, Mª Pilar (2013) Optimal longitudes determination for the station keeping of areostationary satellites. Planetary and Space Science , 87 . ISSN ISSN: 0032-0633

Romero Pérez, Mª Pilar y Gambi, J.M. y Patino, E. y Antolin Sánchez, Roberto (2008) Optimal station keeping for geostationary satellites with electric propulsion systems under eclipse constraints. In Progress In Industrial Mathematics At ECMI 2006. Mathematics in Industry (12, II). Springer-Verlag Berlin, Berlin, pp. 260-264. ISBN 978-3-540-71991-5

Romero Pérez, Mª Pilar (2010) Post-Newtonian Covariant Formulation for Gravity Determination by Differential Chronometry. In Gravity, Geoid and Earth Observation. International Association of Geodesy Simposia (135). Springer, Berlin, pp. 55-58. ISBN 978-3-642-10633-0

Romero Pérez, Mª Pilar y Barderas, Gonzalo y Vázquez Poletti, José Luis y Llorente, I. M. (2011) Spatial chronogram to detect Phobos eclipses on Mars with the MetNet Precursor Lander. Planetary and Space Science , 59 (13). pp. 1542-1550. ISSN ISSN: 0032-0633

Romero Pérez, Mª Pilar y Barderas, Gonzalo y Garcia Roldan, J. M. (2015) Station-Keeping Maneuvers to Control the Inclination Evolution of Areostationary Satellites. Journal of Guidance, Control, and Dynamics, 38 (11). pp. 2223-2226. ISSN 0731-5090

Gambi, J.M. y Vicente, F. y Romero Pérez, Mª Pilar y San Miguel, A. (1994) Stellar aberration in general relativity. Il Nuovo Cimento della Società Italiana di Fisica - B: General Physics, Relativity, Astronomy and Mathematical Physics and Methods, 109 (5). pp. 523-532. ISSN 0369-3554

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