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We have compared, in an ensemble fashion, properties from the eFEDS X-ray cluster catalogue with those from the Ultimate XMM eXtragaLactic (XXL) survey project (XXL-100-GC). We find the redshift and temperature (TX) distributions to be similar, with a larger proportion of clusters above 4\u2009keV in the XXL-100-GC sample; fractional temperature uncertainties are significantly larger in eFEDS compared to XXL. We find 62 eFEDS cluster candidates with XMM data (eFEDS-XMM sample); 10 do not have good enough XMM data to confirm or deny, 11 are classed as sample contaminants, and 4 have their X-ray flux contaminated by another source. The majority of eFEDS-XMM sources have longer XMM exposures than eFEDS, and most eFEDS positions are within 100\u00a0kpc of XCS positions. Our eFEDS-XCS sample of 37 clusters is used to calculate minimum sample contamination fractions of \u223c18 and \u223c9\u00a0per\u2009cent in the eFEDS X-ray and optically confirmed samples, respectively, in general agreement with eFEDS findings. We directly compare 29 X-ray luminosities (LX) measured by eFEDS and XCS, finding excellent agreement. Eight clusters have a TX measured by XCS and eFEDS, and we find that XMM temperatures are 25\u00a0\u00b1\u00a09\u00a0per\u2009cent larger than their eROSITA counterparts. Finally, we construct LX\u2013TX scaling relations based on eFEDS and XCS measurements, which are in tension; the tension is decreased when we measure a third scaling relation with calibrated XCS temperatures.<\/jats:p>","DOI":"10.1093\/mnras\/stac2463","type":"journal-article","created":{"date-parts":[[2022,9,4]],"date-time":"2022-09-04T03:41:45Z","timestamp":1662262905000},"page":"657-674","source":"Crossref","is-referenced-by-count":7,"title":["The<i>XMM<\/i>Cluster Survey: an independent demonstration of the fidelity of the eFEDS galaxy cluster data products and implications for future studies"],"prefix":"10.1093","volume":"517","author":[{"ORCID":"https:\/\/orcid.org\/0000-0001-9658-1396","authenticated-orcid":false,"given":"D J","family":"Turner","sequence":"first","affiliation":[{"name":"Department of Physics and Astronomy, University of Sussex , Brighton BN1 9QH, UK"}]},{"ORCID":"https:\/\/orcid.org\/0000-0003-4937-8453","authenticated-orcid":false,"given":"P A","family":"Giles","sequence":"additional","affiliation":[{"name":"Department of Physics and Astronomy, University of Sussex , Brighton BN1 9QH, UK"}]},{"given":"A K","family":"Romer","sequence":"additional","affiliation":[{"name":"Department of Physics and Astronomy, University of Sussex , Brighton BN1 9QH, UK"}]},{"ORCID":"https:\/\/orcid.org\/0000-0002-3908-7313","authenticated-orcid":false,"given":"R","family":"Wilkinson","sequence":"additional","affiliation":[{"name":"Department of Physics and Astronomy, University of Sussex , Brighton BN1 9QH, UK"}]},{"ORCID":"https:\/\/orcid.org\/0000-0003-0628-7201","authenticated-orcid":false,"given":"E W","family":"Upsdell","sequence":"additional","affiliation":[{"name":"Department of Physics and Astronomy, University of Sussex , Brighton BN1 9QH, UK"}]},{"given":"M","family":"Klein","sequence":"additional","affiliation":[{"name":"Faculty of Physics, Ludwig-Maximilians-Universit\u00e4t , Scheinerstr. 1, D-81679 Munich, Germany"}]},{"ORCID":"https:\/\/orcid.org\/0000-0003-1572-8531","authenticated-orcid":false,"given":"P T P","family":"Viana","sequence":"additional","affiliation":[{"name":"Instituto de Astrof\u00edsica e Ci\u00eancias do Espa\u00e7o, Universidade do Porto , CAUP, Rua das Estrelas, P-4150-762 Porto, Portugal"},{"name":"Faculdade de Ci\u00eancias, Departamento de F\u00edsica e Astronomia, Universidade do Porto , Rua do Campo Alegre, 687, P-4169-007 Porto, Portugal"}]},{"ORCID":"https:\/\/orcid.org\/0000-0002-8490-8117","authenticated-orcid":false,"given":"M","family":"Hilton","sequence":"additional","affiliation":[{"name":"Astrophysics Research Centre, University of KwaZulu-Natal , Westville Campus, Durban 4041, South Africa"},{"name":"School of Mathematics, Statistics, and Computer Science, University of KwaZulu-Natal , Westville Campus, Durban 4041, South Africa"}]},{"given":"S","family":"Bhargava","sequence":"additional","affiliation":[{"name":"D\u00e9partement d\u2019Astrophysique, CEA Paris-Saclay , F-91190 Gif-sur-Yvette, France"}]},{"given":"C A","family":"Collins","sequence":"additional","affiliation":[{"name":"Astrophysics Research Institute , Liverpool John Moores University, Liverpool Science Park, 146 Brownlow Hill, Liverpool L3 5RF, UK"}]},{"given":"R G","family":"Mann","sequence":"additional","affiliation":[{"name":"Institute for Astronomy, University of Edinburgh , Royal Observatory, Blackford Hill, Edinburgh EH9 3HJ, UK"}]},{"ORCID":"https:\/\/orcid.org\/0000-0003-0973-4804","authenticated-orcid":false,"given":"M","family":"Sahl\u00e9n","sequence":"additional","affiliation":[{"name":"Theoretical Astrophysics, Department of Physics and Astronomy, Uppsala University , Box 516, SE-75120 Uppsala, Sweden"}]},{"ORCID":"https:\/\/orcid.org\/0000-0002-1679-9983","authenticated-orcid":false,"given":"J P","family":"Stott","sequence":"additional","affiliation":[{"name":"Department of Physics, Lancaster University , Lancaster LA1 4YB, UK"}]}],"member":"286","published-online":{"date-parts":[[2022,9,3]]},"reference":[{"key":"2022100812171174800_bib1","doi-asserted-by":"publisher","first-page":"3","DOI":"10.3847\/1538-4365\/ab929e","volume":"249","author":"Ahumada","year":"2020","journal-title":"ApJS"},{"key":"2022100812171174800_bib2","doi-asserted-by":"publisher","first-page":"S4","DOI":"10.1093\/pasj\/psx066","volume":"70","author":"Aihara","year":"2018","journal-title":"PASJ"},{"key":"2022100812171174800_bib3","doi-asserted-by":"publisher","first-page":"114","DOI":"10.1093\/pasj\/psz103","volume":"71","author":"Aihara","year":"2019","journal-title":"PASJ"},{"key":"2022100812171174800_bib4","first-page":"17","volume-title":"ASP Conf. 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