The eROSITA Final Equatorial-Depth Survey (eFEDS): Galaxy Clusters and Groups in Disguise

• Published in: arXiv.org
• Main Authors: Bulbul, Esra, Liu, Ang, Pasini, Thomas, Comparat, Johan, Hoang, Duy, Klein, Matthias, Ghirardini, Vittorio, Salvato, Mara, Merloni, Andrea, Seppi, Riccardo, Wolf, Julien, Anderson, Scott F, Bahar, Y Emre, Brusa, Marcella, Brueggen, Marcus, Buchner, Johannes, Dwelly, Tom, Ibarra-Medel, Hector, Jacob Ider Chitham, Liu, Teng, Nandra, Kirpal, Ramos-Ceja, Miriam E, Sanders, Jeremy S, Shen, Yue
• Format: Paper Journal Article
• Language: English
• Published: Ithaca Cornell University Library, arXiv.org 09.03.2022
• Subjects: Active galactic nuclei; Algorithms; Compact galaxies; Galactic clusters; Identification methods; Optical properties; Physics - Astrophysics of Galaxies; Physics - Cosmology and Nongalactic Astrophysics; Point sources; Point spread functions; Red shift; Sky surveys (astronomy); Stars & galaxies; X-ray astronomy
• ISSN: 2331-8422
• DOI: 10.48550/arxiv.2110.09544

The eROSITA Final Equatorial-Depth Survey (eFEDS), executed during the performance verification phase of the Spectrum-Roentgen-Gamma (SRG)/eROSITA telescope, was completed in Nov. 2019. One of the science goals of this survey is to demonstrate the ability of eROSITA to detect samples of clusters and groups at the final depth of the eROSITA all-sky survey. Because of the sizeable point-spread function of eROSITA, high-redshift clusters of galaxies or compact nearby groups hosting bright active galactic nuclei (AGN) can be misclassified as point sources by the source detection algorithms. A total of 346 galaxy clusters and groups in the redshift range of 0.1<z<1.3 were identified based on their red sequence in the point source catalog. We examine the multiwavelength properties of these clusters and groups to understand the potential biases in our selection process and the completeness of the extent-selected sample. The majority of the clusters and groups in the point source sample are indeed underluminous and compact compared to the extent-selected sample. Their faint X-ray emission, well below the flux limit of the extent-selected eFEDS clusters, and their compact X-ray emission are likely to be the main reason for this misclassification. In the sample, we confirm that 10% of the sources host AGN in their brightest cluster galaxies (BCGs) through optical spectroscopy and visual inspection. By studying their X-ray, optical, infrared, and radio properties, we establish a method for identifying clusters and groups that host AGN in their BCGs. We successfully test this method on the current point source catalog through the Sloan Digital Sky Survey optical spectroscopy and find eight clusters and groups with active radio-loud AGN that are particularly bright in the infrared. They include eFEDSJ091437.8+024558, eFEDSJ083520.1+012516, and eFEDSJ092227.1+043339 at redshifts 0.3-0.4. [ABRIDGED]