activity
20012024
most citedULTRACAM: an ultra-fast, triple-beam CCD camera for high-speed astrophysics

343 citations · 731 across the 21 of their papers we have counts for

collaborators

21 papers

astro-ph.IM2024★ 1 cited

Walking with SOXS towards the transient sky

P. Schipani, S. Campana, R. Claudi +59

SOXS (Son Of X-Shooter) is the new ESO instrument that is going to be installed on the 3.58-m New Technology Telescope at the La Silla Observatory. SOXS is a single object spectrog…

astro-ph.IM2024★ 5 cited

The MICADO first light imager for the ELT: off-axis performance of PSF reconstruction

Matteo Simioni, Daniel Jodlbauer, Carmelo Arcidiacono +14

The highest scientific return, for adaptive optics (AO) observations, is achieved with a reliable reconstruction of the PSF. This is especially true for MICADO@ELT. In this present…

astro-ph.IM2023★ 4 cited

Evaluating the GeoSnap 13-m Cut-Off HgCdTe Detector for mid-IR ground-based astronomy

Jarron M. Leisenring, Dani Atkinson, Rory Bowens +13

New mid-infrared HgCdTe (MCT) detector arrays developed in collaboration with Teledyne Imaging Sensors (TIS) have paved the way for improved 10-m sensors for space- and ground-b…

astro-ph.IM2023★ 84 cited

CRIRES on sky at the ESO Very Large Telescope

R. J. Dorn, P. Bristow, J. V. Smoker +49

The CRyogenic InfraRed Echelle Spectrograph (CRIRES) Upgrade project CRIRES extended the capabilities of CRIRES. It transformed this VLT instrument into a cross-dispersed spe…

astro-ph.IM2021★ 98 cited

HiPERCAM: a quintuple-beam, high-speed optical imager on the 10.4-m Gran Telescopio Canarias

V. S. Dhillon, N. Bezawada, M. Black +36

HiPERCAM is a portable, quintuple-beam optical imager that saw first light on the 10.4-m Gran Telescopio Canarias (GTC) in 2018. The instrument uses re-imaging optics and 4 dichroi…

astro-ph.SR2021★ 12 cited

Mid-infrared circumstellar emission of the long-period Cepheid l Carinae resolved with VLTI/MATISSE

V. Hocdé, N. Nardetto, A. Matter +149

The nature of circumstellar envelopes (CSE) around Cepheids is still a matter of debate. The physical origin of their infrared (IR) excess could be either a shell of ionized gas, o…