216 citations · 1.9k across the 113 of their papers we have counts for
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Polarimetry at millimeter wavelengths with the NIKA camera: calibration and performance
A. Ritacco, N. Ponthieu, A. Catalano +37
Magnetic fields, which play a major role in a large number of astrophysical processes from galactic to cosmological scales, can be traced via observations of dust polarization as d…
Non-parametric deprojection of NIKA SZ observations: Pressure distribution in the Planck-discovered cluster PSZ1 G045.85+57.71
F. Ruppin, R. Adam, B. Comis +38
The determination of the thermodynamic properties of clusters of galaxies at intermediate and high redshift can bring new insights into the formation of large-scale structures. It…
Mapping the kinetic Sunyaev-Zel'dovich effect toward MACS J0717.5+3745 with NIKA
R. Adam, I. Bartalucci, G. W. Pratt +47
Measurement of the gas velocity distribution in galaxy clusters provides insight into the physics of mergers, through which large scale structures form in the Universe. Velocity es…
High angular resolution SZ observations with NIKA and NIKA2
B. Comis, R. Adam, P. Ade +39
NIKA2 (New IRAM KID Arrays) is a dual band (150 and 260 GHz) imaging camera based on Kinetic Inductance Detectors (KIDs) and designed to work at the IRAM 30 m telescope (Pico Velet…
The NIKA2 commissioning campaign: performance and first results
A. Catalano, R. Adam, P. Ade +39
The New IRAM KID Array 2 (NIKA 2) is a dual-band camera operating with three frequency-multiplexed kilopixels arrays of Lumped Element Kinetic Inductance Detectors (LEKID) cooled a…
High-resolution tSZ cartography of clusters of galaxies with NIKA at the IRAM 30-m telescope
F. Mayet, R. Adam, A. Adane +41
The thermal Sunyaev-Zeldovich effect (tSZ) is a powerful probe to study clusters of galaxies and is complementary with respect to X-ray, lensing or optical observations. Previous a…
NIKA 2: next-generation continuum/polarized camera at the IRAM 30 m telescope and its prototype
A. Ritacco, R. Adam, A. Adane +36
NIKA 2 (New Instrument of Kids Array) is a next generation continuum and polarized instrument successfully installed in October 2015 at the IRAM 30 m telescope on Pico-Veleta (Gran…