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Roman Zoufal10/03/2026, 14:00
The European Space Agency’s (ESA) F-class mission Arrakihs aims to study the nature of galaxy formation, and the role of baryonic physics and dark matter by observing the faint structures within the halos of nearby MW-like galaxies at unprecedented depth. The required surface brightness is achieved by stacking multiple observations. The high image quality needed is obtained by the inclusion of...
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Evandro Balbi10/03/2026, 14:00
Euclid acquires slew dark data after each observation sequence, when moving to a new field. The analysis of slew dark data can provide several valuable information, for instance for the study of transients (e.g., cosmic rays, snowballs). We developed an automatic pipeline capable of identifying and removing pixels affected by cosmic rays and grouping them into clusters. The identified clusters...
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Naomie De Araujo10/03/2026, 14:00
The Euclid and SVOM missions rely on advanced infrared detectors to achieve their ambitious scientific goals. Euclid’s NISP instrument, equipped with 16 H2RG detectors, aims to map billions of galaxies in the near-infrared, while SVOM’s CAGIRE camera, based on the French ALFA 2k×2k SWIR detector, enables rapid ground-based follow-up of gamma-ray bursts. CPPM has played a key role in...
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Frederic Lemmel10/03/2026, 14:00
Pyxel is an open-source python-based framework designed for simulating images including instrumental effects with a strong focus on detector modelling (CCDs & EM-CCDS, CIS, Hybrid-CMOS, APDs, MKIDs etc.). It has been conceived to easily integrate and pipeline models from multiple contributors and in this way foster collaboration in the instrumentation community. The development is led by ESA...
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Gerald Mösenlechner10/03/2026, 14:00
Many space telescopes incorporate Fine Guidance Sensors (FGS) in their payload, which provide Line of Sight (LoS) measurements of the observed target to the spacecrafts Attitude and Orbit Control System (AOCS) for continuous correction. In many recent and upcoming Space Missions such as Ariel, these FGS's utilize MCT Infrared Detectors. In order to develop and tune the algorithms that will...
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Roman Zoufal
The European Space Agency’s (ESA) F-class mission Arrakihs aims to study the nature of galaxy formation, and the role of baryonic physics and dark matter by observing the faint structures within the halos of nearby MW-like galaxies at unprecedented depth. The required surface brightness is achieved by stacking multiple observations. The high image quality needed is obtained by the inclusion of...
Go to contribution page -
Roman Zoufal
The European Space Agency’s (ESA) F-class mission Arrakihs aims to study the nature of galaxy formation, and the role of baryonic physics and dark matter by observing the faint structures within the halos of nearby MW-like galaxies at unprecedented depth. The required surface brightness is achieved by stacking multiple observations. The high image quality needed is obtained by the inclusion of...
Go to contribution page -
Evandro Balbi
Euclid acquires slew dark data after each observation sequence, when moving to a new field. The analysis of slew dark data can provide several valuable information, for instance for the study of transients (e.g., cosmic rays, snowballs). We developed an automatic pipeline capable of identifying and removing pixels affected by cosmic rays and grouping them into clusters. The identified clusters...
Go to contribution page -
Evandro Balbi
Euclid acquires slew dark data after each observation sequence, when moving to a new field. The analysis of slew dark data can provide several valuable information, for instance for the study of transients (e.g., cosmic rays, snowballs). We developed an automatic pipeline capable of identifying and removing pixels affected by cosmic rays and grouping them into clusters. The identified clusters...
Go to contribution page -
Naomie De Araujo
The Euclid and SVOM missions rely on advanced infrared detectors to achieve their ambitious scientific goals. Euclid’s NISP instrument, equipped with 16 H2RG detectors, aims to map billions of galaxies in the near-infrared, while SVOM’s CAGIRE camera, based on the French ALFA 2k×2k SWIR detector, enables rapid ground-based follow-up of gamma-ray bursts. CPPM has played a key role in...
Go to contribution page -
Naomie De Araujo
The Euclid and SVOM missions rely on advanced infrared detectors to achieve their ambitious scientific goals. Euclid’s NISP instrument, equipped with 16 H2RG detectors, aims to map billions of galaxies in the near-infrared, while SVOM’s CAGIRE camera, based on the French ALFA 2k×2k SWIR detector, enables rapid ground-based follow-up of gamma-ray bursts. CPPM has played a key role in...
Go to contribution page -
Naomie De Araujo
The Euclid and SVOM missions rely on advanced infrared detectors to achieve their ambitious scientific goals. Euclid’s NISP instrument, equipped with 16 H2RG detectors, aims to map billions of galaxies in the near-infrared, while SVOM’s CAGIRE camera, based on the French ALFA 2k×2k SWIR detector, enables rapid ground-based follow-up of gamma-ray bursts. CPPM has played a key role in...
Go to contribution page -
Frederic Lemmel
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Frederic Lemmel
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Gerald Mösenlechner
Many space telescopes incorporate Fine Guidance Sensors (FGS) in their payload, which provide Line of Sight (LoS) measurements of the observed target to the spacecrafts Attitude and Orbit Control System (AOCS) for continuous correction. In many recent and upcoming Space Missions such as Ariel, these FGS's utilize MCT Infrared Detectors. In order to develop and tune the algorithms that will...
Go to contribution page -
Gerald Mösenlechner
Many space telescopes incorporate Fine Guidance Sensors (FGS) in their payload, which provide Line of Sight (LoS) measurements of the observed target to the spacecrafts Attitude and Orbit Control System (AOCS) for continuous correction. In many recent and upcoming Space Missions such as Ariel, these FGS's utilize MCT Infrared Detectors. In order to develop and tune the algorithms that will...
Go to contribution page
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