The number of present-day massive galaxies that has survived untouched since their formation at high-z is an important observational constraint to the...
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NewsExpected number of massive galaxy relics in the present-day Universe.
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NewsExplanation of the linear polarization of the Ca II IR triplet: zero-field dichroism in the solar chromosphere
The linear polarization produced by scattering processes in the spectral lines of the IR triplet of Ca II can be observed near the edge of the solar disk. The...
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NewsExploring a new definition of the green valley and its implications
Galaxy formation remains one of the major open problems in astrophysics today. There is a wide range of mechanisms that control the transformation of gas into...
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NewsExtreme magnification of a distant star by a galaxy-cluster lens
Galaxy-cluster gravitational lenses can magnify background galaxies by a total factor of up to ~50. Here we report an image of an individual star at redshift z ...
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NewsExtremely fast orbital decay of the black hole X-ray binary Nova Muscae 1991
We present new medium-resolution spectroscopic observations of the black hole X-ray binary Nova Muscae 1991 taken with X-Shooter spectrograph installed at the 8...
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NewsFar infrared detected Lyman break galaxies at z ~ 3: Dust attenuation and dust correction factors at high redshift.
Lyman break galaxies (LBGs) represent one of the kinds of star-forming galaxies that are found in the high-redshift universe. The detection of LBGs in the FIR...
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NewsFast orbital decays of black hole X-ray binaries: XTE J1118+480 and A0620–00.
We present new 10.4 m-GTC/OSIRIS spectroscopic observations of the black hole X-ray binary XTE J1118+480 that confirm the orbital period decay at (dP/dt) = −1...
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NewsFIR measurements of Ly-alpha emitters at z<1.0: dust attenuation from PACS-Herschel.
One remaining open question regarding the physical properties of Lyaemitters (LAEs) is their dust content and its evolution with redshift. The variety of...
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NewsFirst direct imaging of the faint O emission lines in a planetary nebula
For more than 70 years we have known that the weak recombination lines of the ions of elements, such as oxygen and carbon, give us values for their abundances...