We investigate the scaling relations between X-ray observables of the clusters detected in the eFEDS field using Spectrum-Roentgen-Gamma/eROSITA observations taking into account the selection effects and the distributions of observables with cosmic time. We extract X-ray observables (Lx, Lbol, T, Mgas, Yx) within R500 for the sample of 542 clusters in the eFEDS field. By applying detection and extent likelihoods, we construct a subsample of 265 clusters with a contamination level of <10% (including AGNs and spurious fluctuations) to be utilized in the scaling relation analysis. The selection function based on the state-of-the-art simulations of the eROSITA sky is fully accounted for in our work. We provide the X-ray observables in the core-...
We present the first weak-lensing mass calibration and X-ray scaling relations of galaxy clusters an...
International audienceContext. The eFEDS survey is a proof-of-concept mini-survey designed to demons...
International audienceWe present the first weak-lensing mass calibration and X-ray scaling relations...
Context. Scaling relations link the physical properties of clusters at cosmic scales. They are used ...
International audienceContext. Scaling relations link the physical properties of clusters at cosmic ...
We present the results of a systematic X-ray analysis of optically rich galaxy clusters detected by ...
The eFEDS survey is a proof-of-concept mini-survey designed to demonstrate the survey science capabi...
The eROSITA Final Equatorial-Depth Survey has been carried out during the PV phase of the SRG/eROSIT...
The eROSITA Final Equatorial-Depth Survey (eFEDS), covering ~140 square degrees, was performed as pa...
International audienceContext. Morphological parameters are the estimators for the dynamical state o...
We present the first weak-lensing mass calibration and X-ray scaling relations of galaxy clusters an...
International audienceContext. The eFEDS survey is a proof-of-concept mini-survey designed to demons...
International audienceWe present the first weak-lensing mass calibration and X-ray scaling relations...
Context. Scaling relations link the physical properties of clusters at cosmic scales. They are used ...
International audienceContext. Scaling relations link the physical properties of clusters at cosmic ...
We present the results of a systematic X-ray analysis of optically rich galaxy clusters detected by ...
The eFEDS survey is a proof-of-concept mini-survey designed to demonstrate the survey science capabi...
The eROSITA Final Equatorial-Depth Survey has been carried out during the PV phase of the SRG/eROSIT...
The eROSITA Final Equatorial-Depth Survey (eFEDS), covering ~140 square degrees, was performed as pa...
International audienceContext. Morphological parameters are the estimators for the dynamical state o...
We present the first weak-lensing mass calibration and X-ray scaling relations of galaxy clusters an...
International audienceContext. The eFEDS survey is a proof-of-concept mini-survey designed to demons...
International audienceWe present the first weak-lensing mass calibration and X-ray scaling relations...