Florence Charlieu

Institute of Nuclear Physics of Lyon

Author Statistics

Papers

Citation

H-Index

i-10 index

Research Trends

Author Order

Document Type

Co-Authors

B. Censier

Observatoire Radioastronomique de Nançay

Gérard Smadja

Institute of Nuclear Physics of Lyon

L. Vagneron

Institut de Physique des 2 Infinis de Lyon

S. Ferriol

Institute of Nuclear Physics of Lyon

E. Chabanat

Université Claude Bernard Lyon 1

Julien Zoubian

Centre de physique des particules de Marseille

J. Gascon

Institute of Nuclear Physics of Lyon

W. Gillard

Centre National de la Recherche Scientifique

Benoît Serra

Centre de physique des particules de Marseille

Anne Ealet

Université Claude Bernard Lyon 1

Cooperative Institutions

Centre National de la Recherche Scientifique

Institut National de Physique Nucléaire et de Physique des Particules

Institute of Nuclear Physics of Lyon

Université Claude Bernard Lyon 1

Aix-Marseille Université

Institut de Physique des 2 Infinis de Lyon

Commissariat à l'Énergie Atomique et aux Énergies Alternatives

Institut de Physique

Centre de physique des particules de Marseille

Université Paris-Sud

Author Statistics

Papers

Citation

H-Index

i-10 index

Research Field

EDELWEISS Read-out Electronics and Future Prospects

Journal of Low Temperature Physics (2012)

B. Censier A. Benoı̂t Guillaume A. Brès Florence Charlieu J. Gascon

10.1007/s10909-012-0568-9

Cite

Citations (10)

Low noise flux estimate and data quality control monitoring in EUCLID-NISP cosmological survey

Proceedings of SPIE, the International Society for Optical Engineering/Proceedings of SPIE (2016)

B. Kubik R. Barbier Peter Calabria A. Castera E. Chabanat

Euclid mission is designed to understand the dark sector of the universe. Precise redshift measurements are provided by H2RG detectors. We propose an unbiased method of fitting the flux with Poisson distributed and correlated data, which has an analytic solution and provides a reliable quality factor - fundamental features to ensure the goals of the mission. We compare our method to other techniques of signal estimation and illustrate the anomaly detection on the flight-like detectors. Although our discussion is focused on Euclid NISP instrument, much of what is discussed will be of interest to any mission using similar near-infrared sensors.

10.1117/12.2232551

Cite

Citations (1)