activity
20162026
most citedA wide field-of-view low-resolution spectrometer at APEX: instrument design and science forecast

76 citations · 169 across the 25 of their papers we have counts for

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Showing astro-ph.IMShow all

8 papers · 1 filter

astro-ph.IM2025

CONCERTO: forward modeling of interferograms for calibration

A. Lundgren, A. Beelen, G. Lagache +36

The CarbON [CII] line in post-rEionisation and ReionisaTiOn epoch (CONCERTO) instrument is a low-resolution mapping Fourier-transform spectrometer, based on lumped-element kinetic…

astro-ph.IM2024

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.IM20244 cited

CONCERTO at APEX -- On-sky performance in continuum

W. Hu, A. Beelen, G. Lagache +36

We present the data-processing algorithms and the performance of CONCERTO (CarbON CII line in post-rEionisation and ReionisaTiOn epoch) in continuum by analysing the data from the…

astro-ph.IM2023

Polarization angle accuracy for future CMB experiments. The COSMOCal project and its prototype in the 1mm band

A. Ritacco, L. Bizzarri, F. Boulanger +24

The Cosmic Microwave Background (CMB) radiation offers a unique window into the early Universe, facilitating precise examinations of fundamental cosmological theories. However, the…

astro-ph.IM202076 cited

A wide field-of-view low-resolution spectrometer at APEX: instrument design and science forecast

The CONCERTO collaboration, P. Ade, M. Aravena +36

Characterise the large-scale structure in the Universe from present times to the high redshift epoch of reionisation is essential to constraining the cosmology, the history of star…

astro-ph.IM202016 cited

Detection of the magnetar XTE J1810-197 at 150 and 260 GHz with the NIKA2 Kinetic Inductance Detector camera

P. Torne, J. Macías-Pérez, B. Ladjelate +13

The investigation of pulsars between millimetre and optical wavelengths is challenging due to the faintness of the pulsar signals and the relative low sensitivity of the available…