The eROSITA Final Equatorial-Depth Survey (eFEDS) - X-ray observable-to-mass-and-redshift relations of galaxy clusters and groups with weak-lensing mass calibration from the Hyper Suprime-Cam Subaru Strategic Program survey

I-Non Chiu , Vittorio Ghirardini , Ang Liu , Sebastian Grandis , Esra Bulbul , Y. Emre Bahar , Johan Comparat , Sebastian Bocquet , Nicolas Clerc (1) , Matthias Klein , Teng Liu , Xiangchong Li , Hironao Miyatake , Joseph Mohr , Surhud More , Masamune Oguri , Nobuhiro Okabe , Florian Pacaud , Miriam E. Ramos-Ceja , Thomas H. Reiprich , Tim Schrabback , Keiichi Umetsu

1 IRAP - Institut de recherche en astrophysique et planétologie

We present the first weak-lensing mass calibration and X-ray scaling relations of galaxy clusters and groups selected in the eROSITA Final Equatorial Depth Survey (eFEDS) observed by Spectrum Roentgen Gamma/eROSITA over a contiguous footprint with an area of ≈140 deg2, using the three-year (S19A) weak-lensing data from the Hyper Suprime-Cam (HSC) Subaru Strategic Program survey. In this work, we study a sample of 434 optically confirmed galaxy clusters (and groups) at redshift 0.01 ≲ z ≲ 1.3 with a median of 0.35, of which 313 systems are uniformly covered by the HSC survey to enable the extraction of the weak-lensing shear observable. In a Bayesian population modeling, we perform a blind analysis for the weak-lensing mass calibration by simultaneously modeling the observed count rate η and the shear profile g+ of individual clusters through the count-rate-to-mass-and-redshift (η-M500-z) relation and the weak-lensing-mass-to-mass-and-redshift (MWL-M500-z) relation, respectively, while accounting for the bias in these observables using simulation-based calibrations. As a result, the count-rate-inferred and lensing-calibrated cluster mass is obtained from the joint modeling of the scaling relations, as the ensemble mass spanning a range of 1013h-1M⊙ ≲ M500 ≲ 1015h-1M⊙ with a median of ≈1014h-1M⊙ for the eFEDS sample. With the mass calibration, we further model the X-ray observable-to-mass-and-redshift relations, including the rest-frame soft-band and bolometric luminosity (LX and Lb), the emission-weighted temperature TX, the mass of intra-cluster medium Mg, and the mass proxy YX, which is the product of TX and Mg. Except for LX with a steeper dependence on the cluster mass at a statistically significant level, we find that the other X-ray scaling relations all show a mass trend that is statistically consistent with the self-similar prediction at a level of ≲1.7σ. Meanwhile, all these scaling relations show no significant deviation from the self-similarity in their redshift scaling. Moreover, no significant redshift-dependent mass trend is present. This work demonstrates the synergy between the eROSITA and HSC surveys in preparation for the forthcoming first-year eROSITA cluster cosmology.Key words: galaxies: clusters: general / galaxies: clusters: intracluster medium / gravitational lensing: weak / large-scale structure of Universe / cosmology: observations / dark energy

Mots clés: galaxies: clusters: general; galaxies: clusters: intracluster medium; gravitational lensing: weak; large-scale structure of Universe; cosmology: observations; dark energy

Domaines: Astrophysique [astro-ph]

I-Non Chiu, Vittorio Ghirardini, Ang Liu, Sebastian Grandis, Esra Bulbul, et al.. The eROSITA Final Equatorial-Depth Survey (eFEDS) - X-ray observable-to-mass-and-redshift relations of galaxy clusters and groups with weak-lensing mass calibration from the Hyper Suprime-Cam Subaru Strategic Program survey. Astronomy and Astrophysics - A&A, 2022, 661, pp.A11. ⟨10.1051/0004-6361/202141755⟩. ⟨hal-03312618⟩