PACT I: Combining ACT and Planck data for optimal detection of tSZ signal
arXiv:1902.00350 · doi:10.1051/0004-6361/201935271
Abstract
We present the optimal reconstruction of the thermal Sunyaev-Zel'dovich (tSZ) effect signal based on the combination of a heterogeneous dataset consisting of ACT and Planck data, with different numbers of channels, angular resolutions and noise levels. We combine both datasets using two different approaches, a Matched Multi-Filter (MMF) technique and an optimised Internal Linear Combination (ILC). We show that when applying the MMF to the combination of ACT and Planck data, the size-flux degeneracy is reduced and the signal-to-noise of clusters detected with their SZ signal improves by up to a factor of three. In the case of the optimised ILC method, we show that the tSZ map is reconstructed with a resolution of arcmin. This is more than a factor two improvement compared with the Planck resolution, and with a very good control of noise, i.e. limited only by the intrinsic noise of the individual experiments. The combination of ACT and Planck data offers a unique opportunity to improve on the study of the pressure profiles and to study substructure in clusters through their tSZ.
arXiv comment10 pages, 10 figures
References in corpus (37)
- Planck 2018 results. I. Overview and the cosmological legacy of Planck
- The universal galaxy cluster pressure profile from a representative sample of nearby systems (REXCESS) and the Y_SZ-M_500 relation
- The Sunyaev-Zel'dovich Effect
- redMaPPer I: Algorithm and SDSS DR8 Catalog
- Galaxy Clusters Discovered via the Sunyaev-Zel'dovich Effect in the 2500-square-degree SPT-SZ survey
- The MCXC: a Meta-Catalogue of X-ray detected Clusters of galaxies
- Testing X-ray Measurements of Galaxy Clusters with Cosmological Simulations
- Planck 2013 results. XXIX. Planck catalogue of Sunyaev-Zeldovich sources
- The Atacama Cosmology Telescope: Sunyaev-Zel'dovich Selected Galaxy Clusters at 148 GHz from Three Seasons of Data
- Planck Early Results VIII: The all-sky Early Sunyaev-Zeldovich cluster sample
- Planck 2015 results. XXVII. The Second Planck Catalogue of Sunyaev-Zeldovich Sources
- Galaxy clusters discovered with a Sunyaev-Zel'dovich effect survey
- The Atacama Cosmology Telescope: Sunyaev Zel'dovich Selected Galaxy Clusters at 148 GHz in the 2008 Survey
- The Atacama Cosmology Telescope: The Receiver and Instrumentation
- Planck 2015 results. VIII. High Frequency Instrument data processing: Calibration and maps
- Catalog Extraction in SZ Cluster Surveys: a matched filter approach
- Planck 2015 results. XXII. A map of the thermal Sunyaev-Zeldovich effect
- The Atacama Cosmology Telescope: The Two-Season ACTPol Sunyaev-Zel'dovich Effect Selected Cluster Catalog
- MILCA, a Modified Internal Linear Combination Algorithm to extract astrophysical emissions from multi-frequency sky maps
- Foreground component separation with generalised ILC
- Calibration of the optical mass proxy for clusters of galaxies and an update of the WHL12 cluster catalog
- Planck 2015 results. XXIII. The thermal Sunyaev-Zeldovich effect--cosmic infrared background correlation
- Planck 2013 results. XXIX. The Planck catalogue of Sunyaev-Zeldovich sources: Addendum
- Planck 2013 results. XXI. All-sky Compton parameter power spectrum and high-order statistics
- A fast Bayesian approach to discrete object detection in astronomical datasets - PowellSnakes I
- The Atacama Cosmology Telescope: Data Characterization and Map Making
- SZ and CMB reconstruction using Generalized Morphological Component Analysis
- Planck 2015 results. VII. HFI TOI and beam processing
- Joint Planck and WMAP CMB Map Reconstruction
- The Atacama Cosmology Telescope: Beam Measurements and the Microwave Brightness Temperatures of Uranus and Saturn
- Maps of the Southern Millimeter-wave Sky from Combined 2500 deg SPT-SZ and Planck Temperature Data
- Reconstruction of high-resolution SZ maps from heterogeneous datasets using needlets
- Powellsnakes II: a fast Bayesian approach to discrete object detection in multi-frequency astronomical data sets
- CMB reconstruction from the WMAP and Planck PR2 data
- Point source detection and extraction from simulated Planck TOD using optimal adaptive filters
- The Good, the Bad and the Ugly: Statistical quality assessment of SZ detections
- Maps of the Magellanic Clouds from Combined South Pole Telescope and Planck Data
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- The Atacama Cosmology Telescope: DR5 maps of 18,000 square degrees of the microwave sky from ACT 2008-2018 data
- The Atacama Cosmology Telescope: Component-separated maps of CMB temperature and the thermal Sunyaev-Zel'dovich effect
- Constraints on Stupendously Large Black Holes
- The Abell 3391/95 galaxy cluster system: A 15 Mpc intergalactic medium emission filament, a warm gas bridge, infalling matter clumps, and (re-) accelerated plasma discovered by combining SRG/eROSITA data with ASKAP/EMU and DECam data
- CMB/kSZ and Compton- Maps from 2500 square degrees of SPT-SZ and Planck Survey Data
- Constraining cosmology with a new all-sky Compton parameter map from the Planck PR4 data
- The Atacama Cosmology Telescope: Probing the Baryon Content of SDSS DR15 Galaxies with the Thermal and Kinematic Sunyaev-Zel'dovich Effects
- Mapping the relativistic electron gas temperature across the sky
- New constraints on the magnetic field in filaments of the cosmic web
- Retrieving cosmological information from small-scale CMB foregrounds II. The kinetic Sunyaev Zel'dovich effect
- An improved Compton parameter map of thermal Sunyaev-Zeldovich effect from Planck PR4 data
- PSZSPT: a joint Planck and SPT-SZ cluster catalog
- PACT. II. Pressure profiles of galaxy clusters using Planck and ACT
- Deep learning for Sunyaev-Zel'dovich detection in Planck
- Retrieving cosmological information from small-scale CMB foregrounds I. The thermal Sunyaev Zel'dovich effect
- Mitigating the impact of the CIB on galaxy cluster SZ detection with spectrally constrained matched filters
- MILCANN : A neural network assessed tSZ map for galaxy cluster detection
- Galaxy cluster SZ detection with unbiased noise estimation: an iterative approach
- Exploring the mass and redshift dependence of the cluster pressure profile with stacks on thermal SZ maps
- CHEX-MATE: pressure profiles of 6 galaxy clusters as seen by SPT and Planck
- Spectral imaging of the thermal Sunyaev-Zel'dovich effect in X-COP galaxy clusters: method and validation
- Probing the large-scale structure of the universe through gravitational-wave observations
- Characterising galaxy clusters' completeness function in Planck with hydrodynamical simulations
- Self-supervised component separation for the extragalactic submillimeter sky
- CMB at small scales: Cosmology from tSZ power spectrum