Context. Measurement of the Galactic neutral atomic hydrogen (H i) column density, N H i ,
and brightness temperatures, T B , is of high scientific value for a broad range of astrophysical …

Context. Measurement of the Galactic neutral atomic hydrogen (H i) column density, NH i,
and brightness temperatures, TB, is of high scientific value for a broad range of astrophysical …

Context. The Effelsberg-Bonn H i Survey (EBHIS) is a new 21-cm survey performed with the
100-m telescope at Effelsberg. It covers the whole northern sky out to a redshift of z ~ 0.07 …

We introduce SoFiA, a flexible software application for the detection and parametrization of
sources in 3D spectral line data sets. SoFiA combines for the first time in a single piece of …

We investigate data from the Galactic Effelsberg-Bonn H i Survey, supplemented with data
from the third release of the Galactic All Sky Survey (GASS III) observed at Parkes. We …

… Applying a flexible scheduling scheme we now avoid this azimuth range (Flöer et al., in prep…
set and the discussion of the systematic limitations will be presented by Flöer et al. (in prep.). …

Near-UV observations of the planet host star WASP-12 uncovered the apparent absence of
the normally conspicuous core emission of the Mg ii h and k resonance lines. This anomaly …

We describe a simple method to determine the reliability of source finders based on the
detection of sources with both positive and negative total flux. Under the assumption that the …

Starting in winter 2008/2009 an L-band seven-feed-array receiver is used for a 21 cm line
survey performed with the 100 m telescope, the Effelsberg–Bonn H i survey (EBHIS). The …

… The 2D–1D WAVELET RECONSTRUCTION source finder is described in detail in Flöer
& Winkel (2011), … This method is further explored and explained in Serra, Jurek & Flöer (2011b). …