We present the evolution of the volume-averaged properties of the rest-frame optically luminous (LV>3×1010 h-270 Lsolar) galaxy population to z~3, determined from four disjoint deep fields. We characterize their rest-frame UV through optical properties via the mean SED. To measure evolution, we apply the selection criteria to a sample of galaxies
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Además ofrece acceso al repositorio de preprints del IAC: https://research.iac.es/preprints/l
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Measuring the Average Evolution of Luminous Galaxies at z < 3: The Rest-Frame Optical Luminosity Density, Spectral Energy Distribution, and Stellar Mass DensityRudnick, Gregory et al.102006
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MEGARA, the Next Generation Optical MOS and IFU for GTC
MEGARA (Multi-Espectrógrafo en GTC de Alta Resolución para Astronomía) is the new optical spectrograph for the 10.4 m Gran Telescopio CANARIAS (GTC). Once installed at GTC by the end of 2016, MEGARA will provide both Integral Field Unit and Multi-Object Spectroscopy capabilities covering a field-of-view of 12.5×11.3 arcsec2 and 3.5×3.5 arcmin2
Gil de Paz, A. et al.Fecha de publicación:
102016 -
Menzel 3: Dissecting the ant
The structure and kinematics of the bipolar nebula Mz 3 have been investigated by means of HST, CTIO and ESO images and spectra. At least four distinct outflows have been identified which, from the inside to the outside, are the following: a pair of bright bipolar lobes, two opposite highly collimated column-shaped outflows, a conical system of
Santander-García, M. et al.Fecha de publicación:
102004 -
Metal-line emission from the warm-hot intergalactic medium - II. Ultraviolet
Approximately half the baryons in the local Universe are thought to reside in the warm-hot intergalactic medium (WHIM), i.e. diffuse gas with temperatures in the range 105 < T < 107K. Emission lines from metals in the UV band are excellent tracers of the cooler fraction of this gas, with T ~103photons-1cm-2sr-1) comes from relatively dense (ρ >
Bertone, Serena et al.Fecha de publicación:
102010 -
Mid-infrared spectrum of the zodiacal light observed with ISOPHOT
We present 29 mid-infrared spectra of the zodiacal light distributed over the sky. The observed 5.9-11.7 mu m spectral shapes are well represented by blackbody radiation with colour temperatures in the range of 255
Leinert, Ch. et al.Fecha de publicación:
102002 -
Minimum Times of Several Eclipsing Binaries
We present 26 minima times of 11 eclipsing binaries, observed between 1996 and 1999.
Deeg, H. J. et al.Fecha de publicación:
102003