International audienceThe NGVS is mapping the Virgo Cluster with a depth making possible to detect very low surface brightness (LSB) structures, such as faint dwarf galaxies. To extract these from just above the sky noise and make statistical studies of their properties, we use the software MARSIAA (MARkovian Software for Image Analysis in Astronomy). This segmentation software uses a Markovian approach to classify pixels and identify low-surface brightness structures
We report on a search for new low-surface-brightness galaxies (LSBGs) using Sloan Digital Sky Survey...
Context. The identification and characterization of low surface brightness (LSB) stellar structures ...
<p>The availability of deep, wide area surveys in the optical and near-infrared regime have opened a...
International audienceThe NGVS is mapping the Virgo Cluster with a depth making possible to detect v...
The NGVS is mapping the Virgo Cluster with a depth making possible to detect very low surface bright...
International audienceWe present to the astronomical community an algorithm for the detection of Low...
We present to the astronomical community an algorithm for the detection of low surface brightness (L...
International audienceThe Next Generation Virgo Cluster Survey (NGVS) is a CFHT Large Program that i...
The widely varying dwarf galaxy counts in different environments provide a strong challenge to stand...
We report on a search for new low-surface-brightness galaxies (LSBGs) using Sloan Digital Sky Survey...
We report on a search for new low-surface-brightness galaxies (LSBGs) using Sloan Digital Sky Survey...
Les progrès technologiques de l'instrumentation astronomique soulèvent des problématiques variées. E...
We report on a search for new low-surface-brightness galaxies (LSBGs) using Sloan Digital Sky Survey...
Context. The identification and characterization of low surface brightness (LSB) stellar structures ...
<p>The availability of deep, wide area surveys in the optical and near-infrared regime have opened a...
International audienceThe NGVS is mapping the Virgo Cluster with a depth making possible to detect v...
The NGVS is mapping the Virgo Cluster with a depth making possible to detect very low surface bright...
International audienceWe present to the astronomical community an algorithm for the detection of Low...
We present to the astronomical community an algorithm for the detection of low surface brightness (L...
International audienceThe Next Generation Virgo Cluster Survey (NGVS) is a CFHT Large Program that i...
The widely varying dwarf galaxy counts in different environments provide a strong challenge to stand...
We report on a search for new low-surface-brightness galaxies (LSBGs) using Sloan Digital Sky Survey...
We report on a search for new low-surface-brightness galaxies (LSBGs) using Sloan Digital Sky Survey...
Les progrès technologiques de l'instrumentation astronomique soulèvent des problématiques variées. E...
We report on a search for new low-surface-brightness galaxies (LSBGs) using Sloan Digital Sky Survey...
Context. The identification and characterization of low surface brightness (LSB) stellar structures ...
<p>The availability of deep, wide area surveys in the optical and near-infrared regime have opened a...