One of the most exciting possibilities enabled by transiting exoplanets is to measure their atmospheric properties through the technique of transmission...
-
CharlaExploring the diversity of exoplanet atmospheres from the ground with the ACCESS Survey
-
PublicaciónExtragalactic Stellar Spectroscopy
The advent of large 8-10m telescopes heralds a new age in stellar astronomy. It is now possible to carry out detailed spectroscopic observations at high...
-
PublicaciónFaint Emission Lines and Temperature (Esteban+ 1999)
We present echelle spectroscopy in the 3500-10300Å range of the Hourglass Nebula, which is embedded in the Galactic H II region M8. The data were obtained using...
-
PublicaciónFrequency analysis of HD 49434 (Mathias+, 2011)
The frequency analysis was carried out using the recently available software package SigSpec and Period04. (17 data files).
-
CharlaG5T: ExoMolHD: Precision spectroscopic data for studies of exoplanets and other hot atmospheres
The ExoMol project ( www.exomol.com) provides comprehensive spectroscopic data (line lists) for the study of atmospheres of exoplanets and other hot bodies...
-
PublicaciónGeometry of the Draco C1 Symbiotic Binary
Draco C1 is a known symbiotic binary star system composed of a carbon red giant and a hot, compact companion—likely a white dwarf—belonging to the Draco dwarf...
-
NoticiaGIUSEPPE BONO: “La espectroscopía de alta resolución nos permite conocer la cantidad de elementos químicos de la Vía Láctea, ingredientes de las proteínas y de vida orgánica”
Giuseppe Bono, astrofísico y profesor del Departamento de Física de la Università degli Studi di Roma "Tor Vergata" (Italia), es colaborador habitual del...
-
PublicaciónGSC04778-00152 photometry and spectroscopy (Tuvikene+, 2008)
CCD photometry of GSC04778-00152 was carried out on 54 nights during 9 observing runs. In January 2006 the observations were made with the 41-cm Meade telescope...
-
PublicaciónGTC and OSIRIS: expanding the metallicity horizon of massive stars knowledge
Massive stars are fundamental drivers of the Universe because of their injection of energy, momentum, and nuclear-processed material in every stage of their...