Bibcode
García-Lorenzo, B.; Eff-Darwich, A.; Castro-Almazán, J.; Pinilla-Alonso, N.; Muñoz-Tuñón, C.; Rodríguez-Espinosa, J. M.
Bibliographical reference
Monthly Notices of the Royal Astronomical Society, Volume 405, Issue 4, pp. 2683-2696.
Advertised on:
7
2010
Citations
22
Refereed citations
17
Description
We present measurements of the atmospheric water vapour content above
the Roque de los Muchachos Observatory (ORM) obtained using the Global
Positioning System (GPS). The GPS measurements have been evaluated by
comparison with 940-nm radiometer observations. A statistical analysis
of the GPS measurements points to the ORM as an observing site with
suitable conditions for infrared observations, with a median column of
precipitable water vapour (PWV) of 3.8 mm. PWV presents a clear seasonal
behaviour, with winter and spring being the best seasons for infrared
observations. The percentage of nights showing PWV values less than 3 mm
is over 60 per cent in February, March and April. We have also estimated
the temporal variability of water vapour content at the ORM. We present
a summary of PWV statistical results at different astronomical sites,
noting that these values are not directly comparable as a result of the
differences in the techniques used to recorded the data.
Related projects
Helio and Astero-Seismology and Exoplanets Search
The principal objectives of this project are: 1) to study the structure and dynamics of the solar interior, 2) to extend this study to other stars, 3) to search for extrasolar planets using photometric methods (primarily by transits of their host stars) and their characterization (using radial velocity information) and 4) the study of the planetary
Savita
Mathur