Astrophysical: Methods

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    Erratum: A physically motivated definition for the size of galaxies in an era of ultra-deep imaging
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    Erratum: Dark matter halo concentrations in the Wilkinson Microwave Anisotropy Probe year 5 cosmology
    Not Available
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    Erratum: Ubiquitous seeding of supermassive black holes by direct collapse
    Not Available
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    Escaping stars from young low-N clusters
    With the use of N-body calculations, the numbers and properties of escaping stars from low-N (N= 100 and 1000) young embedded star clusters prior to gas...
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    ESPRESSO reveals blueshifted neutral iron emission lines on the dayside of WASP-76 b
    Context. Ultra hot Jupiters (gas giants with T eq > 2000 K) are intriguing exoplanets due to the extreme physics and chemistry present in their atmospheres...
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    Estimating the bispectrum of the Very Small Array data
    We estimate the bispectrum of the Very Small Array data from the compact and extended configuration observations released in 2002 December, and compare our...
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    Estimating the dynamical masses of dwarf galaxies in the presence of binary-star contamination
    Context. The line-of-sight (l.o.s.) velocity dispersion (σ los) of the stellar component of ultra-faint-dwarf galaxies (UFDs) typically ranges from 3 to 6 km s...
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    Estimating the longitudinal magnetic field in the chromosphere of quiet-Sun magnetic concentrations
    Context. Details of the magnetic field in the quiet-Sun chromosphere are key to our understanding of essential aspects of the solar atmosphere. However, the...
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    Estimating the magnetic field strength from magnetograms
    A properly calibrated longitudinal magnetograph is an instrument that measures circular polarization and gives an estimation of the magnetic flux density in...