114 citations · 348 across the 20 of their papers we have counts for
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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…
Performance of the image persistence model for Euclid infrared detectors
B. Kubik, R. Barbier, G. Smadja +99
Large-format infrared detectors are at the heart of major ground and space-based astronomical instruments, and the HgCdTe HxRG is the most widely used. The Near Infrared Spectromet…
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…
CONCERTO: Instrument model of Fourier transform spectroscopy, white-noise components
Alessandro Fasano, Peter Ade, Manuel Aravena +34
Modern astrophysics relies on intricate instrument setups to meet the demands of sensitivity, sky coverage, and multi-channel observations. An example is the CONCERTO project, empl…
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…
Euclid. III. The NISP Instrument
Euclid Collaboration, K. Jahnke, W. Gillard +434
The Near-Infrared Spectrometer and Photometer (NISP) on board the Euclid satellite provides multiband photometry and R>=450 slitless grism spectroscopy in the 950-2020nm wavelength…
Euclid. IV. The NISP Calibration Unit
Euclid Collaboration, F. Hormuth, K. Jahnke +332
The near-infrared calibration unit (NI-CU) on board Euclid's Near-Infrared Spectrometer and Photometer (NISP) is the first astronomical calibration lamp based on light-emitting dio…
CONCERTO: instrument and status
Alessandro Fasano, Peter Ade, Manuel Aravena +36
CONCERTO (CarbON CII line in post-rEionization and ReionizaTiOn) is a low-resolution Fourier transform spectrometer dedicated to the study of star-forming galaxies and clusters of…
CONCERTO: Readout and control electronics
O. Bourrion, C. Hoarau, J. Bounmy +11
The CONCERTO spectral-imaging instrument was installed at the Atacama Pathfinder EXperiment (APEX) 12-meter telescope in April 2021. It has been designed to look at radiation emitt…
CONCERTO: a breakthrough in wide field-of-view spectroscopy at millimeter wavelengths
Alessandro Fasano, Alexandre Beelen, Alain Benoit +37
CarbON CII line in post-rEionization and ReionizaTiOn (CONCERTO) is a low-resolution spectrometer with an instantaneous field-of-view of 18.6 arcmin, operating in the 130-310 GHz t…
CONCERTO : Digital processing for finding and tuning LEKIDs
Julien Bounmy, Christophe Hoarau, Juan-Francisco Macías-Pérez +10
We describe the on-line algorithms developed to probe Lumped Element Kinetic Inductance Detectors (LEKID) in this paper. LEKIDs are millimeter wavelength detectors for astronomy. L…
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…
CONCERTO at APEX: Installation and first phase of on-sky commissioning
A. Catalano, P. Ade, M. Aravena +40
CONCERTO (CarbON CII line in post-rEionisation and ReionisaTiOn) is a large field-of-view (FoV) spectro-imager that has been installed on the Cassegrain Cabin of Atacama Pathfinder…
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…
CONCERTO at APEX: installation and technical commissioning
A. Monfardini, A. Beelen, A. Benoit +41
We describe the deployment and first tests on Sky of CONCERTO, a large field-of-view (18.6arc-min) spectral-imaging instrument. The instrument operates in the range 130-310GHz from…
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…
The KISS experiment
A. Fasano, M. Aguiar, A. Benoit +30
Mapping millimetre continuum emission has become a key issue in modern multi-wavelength astrophysics. In particular, spectrum-imaging at low frequency resolution is an asset for ch…
KISS: a spectrometric imager for millimetre cosmology
A. Fasano, M. Aguiar, A. Benoit +27
Clusters of galaxies are used to map the large-scale structures in the universe and as probe of universe evolution. They can be observed through the Sunyaev-Zel'dovich (SZ) effect.…