P
Pilar Montañés-Rodríguez
Researcher at Spanish National Research Council
Publications - 37
Citations - 1508
Pilar Montañés-Rodríguez is an academic researcher from Spanish National Research Council. The author has contributed to research in topics: Exoplanet & Planet. The author has an hindex of 19, co-authored 37 publications receiving 1361 citations. Previous affiliations of Pilar Montañés-Rodríguez include IAC & New Jersey Institute of Technology.
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Journal ArticleDOI
A Pluto-like radius and a high albedo for the dwarf planet Eris from an occultation
Bruno Sicardy,Bruno Sicardy,Jose Luis Ortiz,Marcelo Assafin,Emmanuel Jehin,Alain Maury,E. Lellouch,R. Gil Hutton,Felipe Braga-Ribas,François Colas,Daniel Hestroffer,J. Lecacheux,F. Roques,P. Santos-Sanz,Thomas Widemann,Nicolás Morales,Rene Duffard,Audrey Thirouin,A. J. Castro-Tirado,Martin Jelínek,Petr Kubánek,Alfredo Sota,R. Sanchez-Ramirez,Alexandre Humberto Andrei,Julio Camargo,D. N. da Silva Neto,A. Ramos Gomes,R. Vieira Martins,R. Vieira Martins,Michaël Gillon,Jean Manfroid,G. P. Tozzi,C. Harlingten,S. Saravia,Raoul Behrend,Stefano Mottola,E. García Melendo,V. Peris,Juan Fabregat,José M. Madiedo,L. Cuesta,M. T. Eibe,A. Ullán,F. Organero,S. Pastor,J.A. de los Reyes,S. Pedraz,A. Castro,I. de la Cueva,G. Muler,Iain A. Steele,M. Cebrián,Pilar Montañés-Rodríguez,Alejandro Oscoz,D. Weaver,C. Jacques,W. J. B. Corradi,Fabio P. Santos,Wilson Reis,A. Milone,Marcelo Emilio,L. Gutiérrez,Roberto Vázquez,H. Hernández-Toledo +63 more
TL;DR: The observation of a multi-chord stellar occultation by Eris on 6 November 2010 is reported, consistent with a spherical shape for Eris, and it is anticipated that this atmosphere may periodically sublimate as Eris approaches its perihelion, at 37.8 astronomical units from the Sun.
Journal ArticleDOI
Earth’s transmission spectrum from lunar eclipse observations
Enric Palle,Maria Rosa Zapatero Osorio,R. Barrena,Pilar Montañés-Rodríguez,Eduardo L. Martín,Eduardo L. Martín +5 more
TL;DR: The optical and near-infrared transmission spectrum of the Earth, obtained during a lunar eclipse, finds some biologically relevant atmospheric features that are weak in the reflection spectrum are much stronger in the transmission spectrum, and indeed stronger than predicted by modelling.
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Identifying the Rotation Rate and the Presence of Dynamic Weather on Extrasolar Earth-like Planets from Photometric Observations
TL;DR: In this article, the authors used reflectance models and real cloud data from satellite observations to estimate Earth's rotation period, and they showed that the light scattered by the Earth to a hypothetical distant observer as a function of time contains sufficient information to accurately measure Earth rotation period.
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Vegetation Signature in the Observed Globally Integrated Spectrum of Earth Considering Simultaneous Cloud Data: Applications for Extrasolar Planets
TL;DR: In this paper, the authors found a strong correlation between the evolution of the spectral intensity of the red edge and changes in the cloud-free vegetated area over the course of observations and concluded that vegetation detection in Earth-like planets will require a considerable level of instrumental precision and will be a difficult task, but not as difficult as the normally weak earthshine signal might seem to suggest.
Journal ArticleDOI
Changes in Earth's reflectance over the past two decades.
TL;DR: In this article, the authors correlate an overlapping period of earthshine measurements of Earth's reflectance (from 1999 through mid-2001) with satellite observations of global cloud properties to construct from the latter a proxy measure for Earth's global shortwave reflectance.