The C III] λλ1907, 1909 emission doublet has been proposed as an alternative to Lyman-α in
redshift confirmations of galaxies at z≳ 6 since it is not attenuated by the largely neutral …

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 …

Using an ultra-deep blind survey with the MUSE integral field spectrograph on the European
Southern Observatory Very Large Telescope, we obtain spectroscopic redshifts to a depth …

In this paper, we consider hyperspectral unmixing problems where the observed images are
blurred during the acquisition process, eg, in microscopy and spectroscopy. We derive a …

Hyperspectral imaging has been an area of active research in image processing and
analysis for more than 10 years, mainly for remote sensing applications. Astronomical …

We present SELFI, the Source Emission Line FInder, a new Bayesian method optimized for
detection of faint galaxies in Multi Unit Spectroscopic Explorer (MUSE) deep fields. MUSE is …

We present a 3‐dimensional matched filtering approach for the blind search of faint
emission‐line sources in integral‐field spectroscopic datasets. The filter is designed to …

This study presents an unsupervised method for detection of configurations of objects based
on a point process in a nonparametric Bayesian framework. This is of interest as the model …

We propose a method aimed at detecting weak, sparse signals in highly noisy three-
dimensional (3D) data. 3D data sets usually combine two spatial directions x and y (eg …

We consider the problem of detecting a target signature which is known (up to an amplitude
factor) to belong to a (possibly very) large library of signatures. Thus we know how each …