XMM-Newton follow-up of a sample of apparent low surface brightness galaxy groups detected in the ROSAT All-Sky Survey
arXiv:2506.19718 · doi:10.1051/0004-6361/202346294
Abstract
Galaxy cluster cosmology relies on complete and pure samples spanning a large range of masses and redshifts. In Xu et al. (2018) and Xu et al. (2022), we discovered an apparently new population of galaxy groups and clusters with, on average, flatter X-ray surface brightness profiles than known clusters; this cluster population was missed in previous cluster surveys. The discovery of such a new class of objects could have a significant impact on cosmological applications of galaxy clusters. In this work we use a subsample of these systems to assess whether they belong to a new population. We follow up three of these galaxy groups and clusters with high-quality XMM-Newton observations. We produce clean images and spectra and use them for model fitting. We also identify known galaxies, groups, or clusters in the field. The observations reveal that all three systems are composed of multiple groups each, either at the same or at different redshifts. In total, we characterize nine groups. We measure flat surface brightness profiles with slope parameter ; i.e, less than the canonical . For the two main central groups, we even measure . When the fluxes for the three observations are split up across the nine identified groups, none of them exceeds the typical flux limit adopted in previous RASS cluster catalogs, in the 0.12.4 keV energy band. The observations reveal that groups with flat surface brightness profiles exist. Whether they form a new, separate population requires additional follow-up observations of further systems from the Xu et al. sample, given the complexity we have discovered. Such extended low surface brightness systems, as well as multiple systems and projection effects, need to be taken into account when determining selection functions of group and cluster samples.
12 pages, 6 figures, accepted by A&A
References in corpus (21)
- Five-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Likelihoods and Parameters from the WMAP data
- Improved Cosmological Constraints from New, Old and Combined Supernova Datasets
- The galaxy cluster mass scale and its impact on cosmological constraints from the cluster population
- Scaling Properties of a Complete X-ray Selected Galaxy Group Sample
- Radial temperature profiles for a large sample of galaxy clusters observed with XMM-Newton
- Probing cosmic isotropy with a new X-ray galaxy cluster sample through the scaling relation
- The SRG/eROSITA all-sky survey: Cosmology constraints from cluster abundances in the western Galactic hemisphere
- The XMM Large Scale Structure survey: The X-ray pipeline and survey selection function
- The dynamical state of brightest cluster galaxies and the formation of clusters
- The NewAthena mission concept in the context of the next decade of X-ray astronomy
- HICOSMO - Cosmology with a complete sample of galaxy clusters: I. Data analysis, sample selection and luminosity-mass scaling-relation
- HICOSMO - Cosmology with a complete sample of galaxy clusters: II. Cosmological results
- Detecting clusters of galaxies and active galactic nuclei in an eROSITA all-sky survey digital twin
- The SRG/eROSITA All-Sky Survey: Dark Energy Survey Year 3 Weak Gravitational Lensing by eRASS1 selected Galaxy Clusters
- Offset between X-ray and optical centers in clusters of galaxies: connecting eROSITA data and simulations
- The galaxy cluster X-ray luminosity--gravitational mass relation in the light of the WMAP 3rd year data
- An X-ray selected catalog of extended galaxy clusters from the ROSAT All-Sky Survey (RXGCC)
- The eROSITA view of the Abell 3391/95 field: The Northern Clump. The largest infalling structure in the longest known gas filament observed with eROSITA, XMM-Newton, and Chandra
- Projection effects in galaxy cluster samples: insights from X-ray redshifts
- The SRG/eROSITA All-Sky Survey: Weak-Lensing of eRASS1 Galaxy Clusters in KiDS-1000 and Consistency Checks with DES Y3 & HSC-Y3
- The SRG/eROSITA All-Sky Survey : Subaru/HSC-SSP weak-lensing mass measurements for the eRASS1 Galaxy Clusters