About one year after the end of the first observational run and six months after the first CoRoT data delivery, we comment the data exploitation progress for different types of stars. We consider first results to illustrate how these data of unprecedented quality shed a new light on the field of stellar seismology.
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Además ofrece acceso al repositorio de preprints del IAC: https://research.iac.es/preprints/l
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First asteroseismic results from CoRoTMichel, E. et al.122008
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First broadband characterization and redshift determination of the VHE blazar MAGIC J2001+439
Aims: We aim to characterize the broadband emission from 2FGL J2001.1+4352, which has been associated with the unknown-redshift blazar MG4 J200112+4352. Based on its gamma-ray spectral properties, it was identified as a potential very high energy (VHE; E> 100 GeV) gamma-ray emitter. We investigate whether this object is aVHE emitter, characterize
Aleksić, J. et al.Fecha de publicación:
122014 -
First Commissioning of the IR Spectrograph LIRIS
The near-infrared spectrograph LIRIS was first commissioned on the WHT on the nights of 15-19 Feb 2003. During all that time the instrument functioned with no major failures. At the time of commissioning LIRIS included imaging and spectroscopic observing modes. Spectroscopy could be done at low resolution (about 700 using the narrowest slit of 0.65
Acosta Pulido, J. A. et al.Fecha de publicación:
122003 -
First Confirmed Detection of a Bipolar Molecular Outflow from a Young Brown Dwarf
Studying the earliest stages in the birth of stars is crucial for understanding how they form. Brown dwarfs with masses between that of stars and planets are not massive enough to maintain stable hydrogen-burning fusion reactions during most of their lifetime. Their origins are subject to much debate in recent literature because their masses are
Phan-Bao, Ngoc et al.Fecha de publicación:
122008 -
First Performance of the GOLF-NG Instrumental Prototype Observing the Sun in Tenerife
The primary challenge of Global Oscillations at Low Frequency New Generation (GOLF-NG) is the detection of the low-frequency solar gravity and acoustic modes, as well as the possibility to measure the high-frequency chromospheric modes. On June 8th 2008, the first sunlight observations with the multichannel resonant GOLF-NG prototype spectrometer
Salabert, D. et al.Fecha de publicación:
122009 -
First Scientific Results of the Near Infrared Spectrograph LIRIS
LIRIS is a near-infrared (1-2.5 microns) intermediate resolution spectrograph (R=1000-3000) with added capabilities for multi-slit, imaging, coronography, and polarimetry, built by the IAC as a common instrument for the 4.2m WHT (La Palma, Spain). LIRIS has been used as a visiting astronomer instrument at the WHT since summer 2004. The image
Manchado, A. et al.Fecha de publicación:
122006