Toward the low-scatter selection of X-ray clusters: Galaxy cluster detection with eROSITA through cluster outskirts
arXiv:1912.01024 · doi:10.1051/0004-6361/201936131
Abstract
One key ingredient in using galaxy clusters (GCs) as a precision cosmological probe in large X-ray surveys is to understand selection effects. The dependence of the X-ray emission on the square of the gas density leads to a predominant role of cool cores in the detection of GCs. The contribution of cool cores to the X-ray luminosity does not scale with GC mass and cosmology and therefore affects the use of X-ray GCs in producing cosmological constraints. One of the main science goals of the eROSITA mission is to constrain cosmology with a wide X-ray survey. We propose an eROSITA GC detection scheme that avoids the use of X-ray GC centers in detection. We calculate theoretical expectations and characterize the performance of this scheme by simulations. Performing realistic simulations of point sources (PSs) in survey mode we search for spatial scales where the extended signal is uncontaminated by the PS flux. We derive a combination of scales and thresholds, which result in a clean extended source catalog. We design the output of the GC detection which enables calibrating the core-excised luminosity using external mass measurements. We provide a way to incorporate the results of this calibration in the production of final core-excised luminosity. Similarly to other GC detection pipelines, we sample the flux - core radius detection space of our method and find many similarities with the pipeline used in the 400d survey. Both detection methods require large statistics on compact GCs, in order to reduce the contamination from PSs. The benefit of our pipeline consists in the sensitivity to the outer GC shapes, which are characterized by large core sizes with little GC to GC variation at a fixed total mass. GC detection through cluster outskirts improves the GC characterization using eROSITA survey data and is expected to yield well characterized GC catalogs having simple selection functions.
References in corpus (44)
- Astropy: A Community Python Package for Astronomy
- Nine-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Parameter Results
- Binary companions of evolved stars in APOGEE DR14: Search method and catalog of ~5,000 companions
- Toward a halo mass function for precision cosmology: the limits of universality
- Cosmological Parameters from Observations of Galaxy Clusters
- Chandra Cluster Cosmology Project III: Cosmological Parameter Constraints
- COLOSSUS: A python toolkit for cosmology, large-scale structure, and dark matter halos
- A Catalog of 200 Galaxy Clusters Serendipitously Detected in the ROSAT PSPC Pointed Observations
- X-ray background measurements with XMM-Newton EPIC
- Shapelets: I. A Method for Image Analysis
- The Cool-Core Bias in X-ray Galaxy Cluster Samples I: Method And Application To HIFLUGCS
- The 400 square degrees ROSAT PSPC galaxy cluster survey: Catalog and statistical calibration
- The Growth of Cool Cores and Evolution of Cooling Properties in a Sample of 83 Galaxy Clusters at 0.3 < z < 1.2 Selected from the SPT-SZ Survey
- The X-ray cluster survey with eROSITA: forecasts for cosmology, cluster physics and primordial non-Gaussianity
- The Remarkable Similarity of Massive Galaxy Clusters From z~0 to z~1.9
- XMM-Newton Observation of the Northwest Radio Relic Region in Abell 3667
- The XXL Survey. II. The bright cluster sample: catalogue and luminosity function
- The fraction of cool-core clusters in X-ray vs. SZ samples using Chandra observations
- Realistic Simulations of the Galactic Polarized Foreground: Consequences for 21-cm Reionization Detection Experiments
- X-Ray morphological analysis of the Planck ESZ clusters
- The cool core state of Planck SZ-selected clusters versus X-ray selected samples: evidence for cool core bias
- X-ray groups and clusters of galaxies in the Subaru-XMM Deep Field
- The XMM Large Scale Structure survey: The X-ray pipeline and survey selection function
- SIXTE -- The Generic X-ray Instrument Simulation Toolkit
- Measuring the dynamical state of Planck SZ-selected clusters: X-ray peak - BCG offset
- The XXL Survey III. Luminosity-temperature relation of the Bright Cluster Sample
- The XXL Survey IV. Mass-temperature relation of the bright cluster sample
- Chandra centres for COSMOS X-ray galaxy groups: Differences in stellar properties between central dominant and offset brightest group galaxies
- The XMM Cluster Outskirts Project (X-COP): Thermodynamic properties of the Intracluster Medium out to in Abell 2319
- The roadmap for unification in galaxy group selection:. I. A search for extended X-ray emission in the CNOC2 survey
- Occupation of X-ray selected galaxy groups by X-ray AGN
- AGN contamination of galaxy-cluster thermal X-ray emission: predictions for eRosita from cosmological simulations
- Constraining galaxy cluster temperatures and redshifts with eROSITA survey data
- XMM-Newton study of 0.012<z<0.024 groups. I: Overview of the IGM thermodynamics
- Comparison of source detection procedures for XMM-Newton images
- The Two-dimensional XMM-Newton Group Survey: z<0.012 groups
- Synthetic simulations of the extragalactic sky seen by eROSITA. I. Pre-launch selection functions from Monte-Carlo simulations
- Ultra-deep catalog of X-ray groups in the Extended Chandra Deep Field South
- Exploring the Diversity of Groups at 0.1<z<0.8 with X-ray and Optically Selected Samples
- X-Ray Groups of Galaxies in the Aegis Deep and Wide Fields
- Towards a characterization of X-ray galaxy clusters for cosmology
- Impact of Weak Lensing Mass Calibration on eROSITA Galaxy Cluster Cosmological Studies -- a Forecast
- Brightest X-ray clusters of galaxies in the CFHTLS wide fields: Catalog and optical mass estimator
- The AGN Population in X-ray Selected Galaxy Groups at