activity
20182026
most citedPredictive model of persistence in H2RG detectors

20 citations · 63 across the 10 of their papers we have counts for

collaborators

11 papers

astro-ph.IM2026

Persistence characteristics of H4RG-15 detectors for ESO instruments

Elizabeth M. George, Domingo Alvarez Mendez, Nagaraja Naidu Bezawada +3

As a part of the ESO Instrumentation Program, we already ordered 23 H4RG-15 (2.5 um cut-off) detectors for the instruments MOONS, MICADO, and HARMONI, with more of these detectors…

astro-ph.IM2023

The ESO's Extremely Large Telescope Working Groups

Paolo Padovani, Michele Cirasuolo, Remco van der Burg +82

Since 2005 ESO has been working with its community and industry to develop an extremely large optical/infrared telescope. ESO's Extremely Large Telescope, or ELT for short, is a re…

astro-ph.IM2021★ 4 cited

Instrumentation for ESO's Extremely Large Telescope

Suzanne Ramsay, Michele Cirasuolo, Paola Amico +21

Design and construction of the instruments for ESO's Extremely Large Telescope (ELT) began in 2015. We present here a brief overview of the status of the ELT Instrumentation Plan.…

astro-ph.IM2020★ 2 cited

Performance advantages of buffered mode operation of HxRG near infrared detectors

Naidu Bezawada, Derek Ives, Domingo Alvarez +4

The Teledyne HxRG detectors have versatile and programmable output options to allow operation of them in a variety of configurations such as slow unbuffered, slow buffered, fast bu…

astro-ph.IM2020★ 10 cited

Characterisation, performance, and operational aspects of the H4RG-15 near infrared detectors for the MOONS instrument

Derek Ives, Domingo Alvarez, Naidu Bezawada +2

MOONS is a multi-object spectrograph for the ESO VLT covering a simultaneous wavelength range of 0.6-1.8 microns using approximately 1000 fibres. It uses four Teledyne Imaging Syst…

astro-ph.IM2020★ 2 cited

Detector Systems Engineering for Extremely Large Instruments

Elizabeth M. George, Naidu Bezawada, Derek Ives +22

The scientific detector systems for the ESO ELT first-light instruments, HARMONI, MICADO, and METIS, together will require 27 science detectors: seventeen 2.5 m cutoff H4RG-15 d…

astro-ph.IM2020

Pyxel: the collaborative detection simulation framework

Thibaut Prod'homme, Frédéric Lemmel, Matej Arko +5

Pyxel is a novel python tool for end-to-end detection chain simulation i.e. from detector optical effects to readout electronics effects. It is an easy-to-use framework to host and…

physics.ins-det2020★ 16 cited

Simulations and Design of a Single-Photon CMOS Imaging Pixel Using Multiple Non-Destructive Signal Sampling

Konstantin D. Stefanov, Martin Prest, Mark Downing +3

A single-photon CMOS image sensor design based on pinned photodiode (PPD) with multiple charge transfers and sampling is described. In the proposed pixel architecture, the photogen…

astro-ph.IM2019★ 20 cited

Predictive model of persistence in H2RG detectors

Simon Tulloch, Elizabeth George

Infrared hybridized detectors are widely used in astronomy, and their performance can be degraded by image persistence. This results in remnant images that can persist in the detec…

astro-ph.IM2018★ 4 cited

Fast method of crosstalk characterization for HxRG detectors

Elizabeth M. George, Simon M. Tulloch, Derek J. Ives

HxRG detectors have crosstalk between amplifier channels at a scientifically relevant level. In principle, crosstalk signals can be fully calibrated and removed from data, but only…

astro-ph.IM2018★ 5 cited

ERIS: revitalising an adaptive optics instrument for the VLT

Richard Davies, Simone Esposito, Hans Martin Schmid +63

ERIS is an instrument that will both extend and enhance the fundamental diffraction limited imaging and spectroscopy capability for the VLT. It will replace two instruments that ar…