First observation of the thermal Sunyaev-Zel'dovich effect with kinetic inductance detectors
arXiv:1310.6237 · doi:10.1051/0004-6361/201322902
Abstract
Clusters of galaxies provide valuable information on the evolution of the Universe and large scale structures. Recent cluster observations via the thermal Sunyaev-Zel'dovich (tSZ) effect have proven to be a powerful tool to detect and study them. In this context, high resolution tSZ observations (~ tens of arcsec) are of particular interest to probe intermediate and high redshift clusters. Observations of the tSZ effect will be carried out with the millimeter dual-band NIKA2 camera, based on Kinetic Inductance Detectors (KIDs) to be installed at the IRAM 30-meter telescope in 2015. To demonstrate the potential of such an instrument, we present tSZ observations with the NIKA camera prototype, consisting of two arrays of 132 and 224 detectors that observe at 140 and 240 GHz with a 18.5 and 12.5 arcsec angular resolution, respectively. The cluster RX J1347.5-1145 was observed simultaneously at 140 and 240 GHz. We used a spectral decorrelation technique to remove the atmospheric noise and obtain a map of the cluster at 140 GHz. The efficiency of this procedure has been characterized through realistic simulations of the observations. The observed 140 GHz map presents a decrement at the cluster position consistent with the tSZ nature of the signal. We used this map to study the pressure distribution of the cluster by fitting a gNFW model to the data. Subtracting this model from the map, we confirm that RX J1347.5-1145 is an ongoing merger, which confirms and complements previous tSZ and X-ray observations. For the first time, we demonstrate the tSZ capability of KID based instruments. The NIKA2 camera with ~ 5000 detectors and a 6.5 arcmin field of view will be well-suited for in-depth studies of the intra cluster medium in intermediate to high redshifts, which enables the characterization of recently detected clusters by the Planck satellite.
Accepted by A&A
References in corpus (12)
- Intracluster Medium Entropy Profiles for a Chandra Archival Sample of Galaxy Clusters
- Testing X-ray Measurements of Galaxy Clusters with Cosmological Simulations
- Cluster Lenses
- NIKA: A millimeter-wave kinetic inductance camera
- A Measurement of the Kinetic Sunyaev-Zel'dovich Signal Toward MACS J0717.5+3745
- Dark Matter and Baryons in the Most X-ray Luminous and Merging Galaxy Cluster RX J1347.5-1145
- Discovery of diffuse radio emission at the center of the most X-ray-luminous cluster RX J1347.5-1145
- Suzaku broad-band spectroscopy of RX J1347.5-1145: constraints on the extremely hot gas and non-thermal emission
- Mass distribution in the most X-ray-luminous galaxy cluster RX J1347.5-1145 studied with XMM-Newton
- A study of the Sunyaev-Zel'dovich increment using archival SCUBA data
- The dynamical state of RX J1347.5-1145 from a combined strong lensing and X-ray analysis
- In-situ measurement of the permittivity of helium using microwave NbN resonators
Cited by in corpus (50)
- Astrophysics with the Spatially and Spectrally Resolved Sunyaev-Zeldovich Effects: A Millimetre/Submillimetre Probe of the Warm and Hot Universe
- The NIKA2 large field-of-view millimeter continuum camera for the 30-m IRAM telescope
- The NIKA2 instrument, a dual-band kilopixel KID array for millimetric astronomy
- High angular resolution Sunyaev-Zel'dovich observations of MACS J1423.8+2404 with NIKA: Multiwavelength analysis
- Calibration and Performance of the NIKA2 camera at the IRAM 30-meter Telescope
- Mapping the kinetic Sunyaev-Zel'dovich effect toward MACS J0717.5+3745 with NIKA
- A wide field-of-view low-resolution spectrometer at APEX: instrument design and science forecast
- First Sunyaev-Zel'dovich mapping with the NIKA2 camera: Implication of cluster substructures for the pressure profile and mass estimate
- Pressure distribution of the high-redshift cluster of galaxies CL J1226.9+3332 with NIKA
- NIKEL_AMC: Readout electronics for the NIKA2 experiment
- Probing changes of dust properties along a chain of solar-type prestellar and protostellar cores in Taurus with NIKA
- Bi-layer Kinetic Inductance Detectors for space observations between 80-120 GHz
- Pressure profiles and mass estimates using high-resolution Sunyaev-Zel'dovich effect observations of Zwicky 3146 with MUSTANG-2
- Non-parametric deprojection of NIKA SZ observations: Pressure distribution in the Planck-discovered cluster PSZ1 G045.85+57.71
- The Sunyaev-Zel'dovich Effect at Five Arc-seconds: RXJ1347.5-1145 Imaged by ALMA
- Morphological estimators on Sunyaev--Zel'dovich maps of MUSIC clusters of galaxies
- Mapping the hot gas temperature in galaxy clusters using X-ray and Sunyaev-Zel'dovich imaging
- Forecasting [C II] line-intensity mapping measurements between the end of reionization and the epoch of galaxy assembly
- First detection of a virial shock with SZ data: implication for the mass accretion rate of Abell 2319
- Polarimetry at millimeter wavelengths with the NIKA camera: calibration and performance
- A multi-instrument non-parametric reconstruction of the electron pressure profile in the galaxy cluster CLJ1226.9+3332
- Galaxy Cluster Pressure Profiles as Determined by Sunyaev Zel'dovich Effect Observations with MUSTANG and Bolocam II: Joint Analysis of Fourteen Clusters
- A joint ALMA-Bolocam-Planck SZ study of the pressure distribution in RX J1347.5-1145
- Cool core disturbed: Observational evidence for coexistence of sub-sonic sloshing gas and stripped shock-heated gas around the core of RX J1347.5-1145
- Kinetic Inductance Detectors for the OLIMPO experiment: design and pre-flight characterization
- Design and performance of dual-polarization lumped-element kinetic inductance detectors for millimeter-wave polarimetry
- NIKA 150 GHz polarization observations of the Crab nebula and its spectral energy distribution
- Peculiar Velocity Constraints from Five-Band SZ Effect Measurements Towards RX J1347.5-1145 with MUSIC and Bolocam from the CSO
- Exploiting NIKA2/XMM-Newton imaging synergy for intermediate mass, high- galaxy clusters within the NIKA2 SZ Large Program
- Sub-structure and merger detection in resolved NIKA Sunyaev-Zel'dovich images of distant clusters
- Cluster cosmology with the NIKA2 SZ Large Program
- Unveiling the merger dynamics of the most massive MaDCoWS cluster at from a multi-wavelength mapping of its intracluster medium properties
- A NIKA view of two star-forming infrared dark clouds: Dust emissivity variations and mass concentration
- Impact of ICM disturbances on the mean pressure profile of galaxy clusters: a prospective study of the NIKA2 SZ large program with MUSIC synthetic clusters
- Lumped element kinetic inductance detectors maturity for space-borne instruments in the range between 80 and 180 GHz
- Sunyaev--Zel'dovich profile fitting with joint AMI-Planck analysis
- The XXL Survey XLIV. Sunyaev-Zel'dovich mapping of a low-mass cluster at z~1: a multi-wavelength approach
- The NIKA2 commissioning campaign: performance and first results
- Development of dual-polarization LEKIDs for CMB observations
- First polarised light with the NIKA camera
- Atacama Large Aperture Submillimeter Telescope (AtLAST) Science: Resolving the Hot and Ionized Universe through the Sunyaev-Zeldovich effect
- The XXL Survey LI. Pressure profile and - scaling relation in three low-mass galaxy clusters at observed with NIKA2
- KISS: instrument description and performance
- PITSZI: Probing Intra-cluster medium Turbulence with Sunyaev-Zel'dovich Imaging -- Application to the triple merging cluster MACS J0717.5+3745
- Resolving the Merging Planck Cluster PLCK G147.3-16.6 with GISMO
- The comptonization parameter from simulations of single-frequency, single-dish, dual-beam, cm-wave observations of galaxy clusters and mitigating CMB confusion using the Planck sky survey
- Candidate cosmic filament in the GJ526 field, mapped with the NIKA2 camera
- NIKA: a mm camera for Sunyaev-Zel'dovich science in clusters of galaxies
- NIKA 2: next-generation continuum/polarized camera at the IRAM 30 m telescope and its prototype
- High resolution SZ observations at the IRAM 30-m telescope with NIKA