InfraRed detectors In Space (IRIS 2026) Workshop

Session

Poster Session

10 Mar 2026, 14:00

Mezzanine Floor (CNR Area Territoriale della Ricerca Bologna)

83. ARRAKIHS FGS task and simulator

Roman Zoufal

10/03/2026, 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...

73. Persistence and anti-persistence in Euclid and SVOM

Naomie De Araujo

10/03/2026, 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...

74. Pyxel 2.0: collaborative detector and instrument modelling

Frederic Lemmel

10/03/2026, 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...

75. The Ariel FGS' High Fidelity Simulator

Gerald Mösenlechner

10/03/2026, 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...

84. ARRAKIHS FGS task and simulator

Roman Zoufal

11/03/2026, 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...

77. Persistence and anti-persistence in Euclid and SVOM

Naomie De Araujo

11/03/2026, 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...

78. Pyxel 2.0: collaborative detector and instrument modelling

Frederic Lemmel

11/03/2026, 14:00

79. The Ariel FGS' High Fidelity Simulator

Gerald Mösenlechner

11/03/2026, 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...

85. ARRAKIHS FGS task and simulator

Roman Zoufal

12/03/2026, 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...

80. Persistence and anti-persistence in Euclid and SVOM

Naomie De Araujo

12/03/2026, 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...

81. Pyxel 2.0: collaborative detector and instrument modelling

Frederic Lemmel

12/03/2026, 14:00

82. The Ariel FGS' High Fidelity Simulator

Gerald Mösenlechner

12/03/2026, 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...

76. Persistence and anti-persistence in Euclid and SVOM

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...