activity
20102024
most citedA dual-band millimeter-wave kinetic inductance camera for the IRAM 30-meter telescope

166 citations · 1.8k across the 57 of their papers we have counts for

collaborators

57 papers

astro-ph.IM2024★ 5 cited

KISS: instrument description and performance

J. F. Macías-Pérez, M. Fernández-Torreiro, A. Catalano +35

Kinetic inductance detectors (KIDs) have been proven as reliable systems for astrophysical observations, especially in the millimetre range. Their compact size enables to optimally…

astro-ph.IM2021★ 1 cited

Observations with KIDs Interferometer Spectrum Survey(KISS)

A. Fasano, A. Catalano, J. F. Macías-Pérez +33

We describe the preliminary on-sky results of the KIDs Interferometer Spectrum Survey (KISS), a spectral imager with a 1 deg field of view (FoV). The instrument operates in the ran…

astro-ph.IM2021★ 10 cited

Accurate sky signal reconstruction for ground-based spectroscopy with kinetic inductance detectors

A. Fasano., J. F. Macías-Pérez, A. Benoit +33

Context. Wide-field spectrometers are needed to deal with current astrophysical challenges that require multiband observations at millimeter wavelengths. An example of these is the…

astro-ph.IM2021★ 9 cited

Understanding and minimizing resonance frequency deviations on a 4-inch kilo-pixel kinetic inductance detector array

S. Shu, M. Calvo, J. Goupy +5

One of the advantages of kinetic inductance detectors is their intrinsic frequency domain multiplexing capability. However, fabrication imperfections usually give rise to resonance…

astro-ph.IM2020★ 20 cited

LEKID sensitivity for space applications between 80 and 600 GHz

A. Catalano, A. Bideaud, O. Bourrion +8

We report the design, fabrication and testing of Lumped Element Kinetic Inductance Detectors (LEKID) showing performance in line with the requirements of the next generation space…

astro-ph.IM2019★ 6 cited

Observing with NIKA2Pol from the IRAM 30m telescope. Early results on the commissioning phase

A. Ritacco, R. Adam, P. Ade +41

The NIKA2 polarization channel at 260 GHz (1.15 mm) has been proposed primarily to observe galactic star-forming regions and probe the critical scales between 0.01-0.05 pc at which…