We present the survey design, data reduction, construction of images, and source catalog of
the Atacama Large Millimeter/submillimeter Array (ALMA) twenty-six arcmin2 survey of …

We describe the CO Luminosity Density at High-z (COLDz) survey, the first spectral line
deep field targeting CO (1–0) emission from galaxies at z= 1.95–2.85 and CO (2–1) at z …

We present a first instalment of the MUSE-Wide survey, covering an area of 22.2 arcmin 2
(corresponding to~ 20% of the final survey) in the CANDELS/Deep area of the Chandra …

Modern radio interferometers enable observations of spectral lines with unprecedented
spatial resolution and sensitivity. In spite of these technical advances, many lines of interest …

We present a robust, efficient, and user-friendly algorithm for detecting faint emission-line
sources in large integral-field spectroscopic datacubes together with the public release of …

Context. Determining when the first galaxies formed remains an outstanding goal of modern
observational astronomy. Theory and current stellar population models imply that the first …

As long as astronomers have searched for exoplanets, the intrinsic variability of host stars
has interfered with the ability to reliably detect and confirm exoplanets. One particular source …

The challenges facing unmanned underwater vehicle (UUV) target state estimation are
observation uncertainty, the unpredictability of the target motion model, and the complex …

Navigation is a precondition for ocean space vehicles to work safely in polar regions. The
traditional polar algorithms employ the grid strapdown inertial navigation system (SINS) as …

Context. One of the major science cases of the Multi Unit Spectroscopic Explorer (MUSE)
integral field spectrograph is the detection of Lyman-alpha emitters at high redshifts. The on …