A Comparison of Algorithms for the Construction of SZ Cluster Catalogues
arXiv:1210.1416 · doi:10.1051/0004-6361/201015689
Abstract
We evaluate the construction methodology of an all-sky catalogue of galaxy clusters detected through the Sunyaev-Zel'dovich (SZ) effect. We perform an extensive comparison of twelve algorithms applied to the same detailed simulations of the millimeter and submillimeter sky based on a Planck-like case. We present the results of this "SZ Challenge" in terms of catalogue completeness, purity, astrometric and photometric reconstruction. Our results provide a comparison of a representative sample of SZ detection algorithms and highlight important issues in their application. In our study case, we show that the exact expected number of clusters remains uncertain (about a thousand cluster candidates at |b|> 20 deg with 90% purity) and that it depends on the SZ model and on the detailed sky simulations, and on algorithmic implementation of the detection methods. We also estimate the astrometric precision of the cluster candidates which is found of the order of ~2 arcmins on average, and the photometric uncertainty of order ~30%, depending on flux.
Accepted for publication in A&A: 14 pages, 7 figures. Detailed figures added in Appendix
References in corpus (16)
- Five-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Likelihoods and Parameters from the WMAP data
- A full sky, low foreground, high resolution CMB map from WMAP
- Component separation methods for the Planck mission
- Catalog Extraction in SZ Cluster Surveys: a matched filter approach
- Separation of anomalous and synchrotron emissions using WMAP polarization data
- Calibration of the galaxy cluster M_500-Y_X relation with XMM-Newton
- Distances to Galactic high-velocity clouds. I. Cohen Stream, complex GCP, cloud g1
- A fast Bayesian approach to discrete object detection in astronomical datasets - PowellSnakes I
- Correlated Anisotropies in the Cosmic Far-Infrared Background Detected by MIPS/Spitzer: Constraint on the Bias
- Statistical properties of dust far-infrared emission
- SZ and CMB reconstruction using Generalized Morphological Component Analysis
- Cleaned Three-Year WMAP CMB Map: Magnitude of the Quadrupole and Alignment of Large Scale Modes
- The Impact of Halo Properties, Energy Feedback and Projection Effects on the Mass-SZ Flux Relation
- A Comparison of Algorithms for the Construction of SZ Cluster Catalogues
- CMB polarization map derived from the WMAP 5 year data through Harmonic Internal Linear Combination
- Sunyaev-Zel'dovich profiles and scaling relations: modelling effects and observational biases
Cited by in corpus (25)
- Planck 2013 results. XXIX. Planck catalogue of Sunyaev-Zeldovich sources
- Planck 2015 results. XXVII. The Second Planck Catalogue of Sunyaev-Zeldovich Sources
- Planck 2015 results. XXII. A map of the thermal Sunyaev-Zeldovich effect
- Scaling relations for galaxy clusters: properties and evolution
- redMaPPer III: A Detailed Comparison of the Planck 2013 and SDSS DR8 RedMaPPer Cluster Catalogs
- A Comparison of Algorithms for the Construction of SZ Cluster Catalogues
- Optical Confirmation and Redshift Estimation of the Planck Cluster Candidates overlapping the Pan-STARRS Survey
- ComPRASS: a Combined Planck-RASS catalogue of X-ray-SZ clusters
- Comparison of Sunyaev-Zel'dovich measurements from Planck and from the Arcminute Microkelvin Imager for 99 galaxy clusters
- PSZSPT: a joint Planck and SPT-SZ cluster catalog
- Dust in galaxy clusters: Modeling at millimeter wavelengths and impact on Planck cluster cosmology
- DeepSZ: Identification of Sunyaev-Zel'dovich Galaxy Clusters using Deep Learning
- A matched filter approach for blind joint detection of galaxy clusters in X-ray and SZ surveys
- Optical follow-up study of 32 high-redshift galaxy cluster candidates from Planck with the William Herschel Telescope
- MILCANN : A neural network assessed tSZ map for galaxy cluster detection
- Recent developments in astrophysical and cosmological exploitation of microwave surveys
- Joint signal extraction from galaxy clusters in X-ray and SZ surveys: A matched-filter approach
- Introducing constrained matched filters for improved separation of point sources from galaxy clusters
- Optical validation and characterisation of Planck PSZ1 sources at the Canary Islands observatories. II. Second year of ITP13 observations
- CARMA observations of massive Planck-discovered cluster candidates at z>0.5 associated with WISE overdensities: Breaking the size-flux degeneracy
- Mass bias and cosmological constraints from Planck cluster clustering
- A CMB Gibbs sampler for localized secondary anisotropies
- CHEX-MATE: The Impact of Triaxiality and Orientation on Planck SZ Cluster Selection and Weak Lensing Mass Measurements
- Deriving accurate galaxy cluster masses using X-ray thermodynamic profiles and graph neural networks
- Inference of morphology and dynamical state of nearby -SZ galaxy clusters with Zernike polynomials