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The analysis is based on deep integral field spectroscopy with Multi-Unit Spectroscopic Explorer of the field of HE\u20090238\u22121904, a luminous quasar at z\u00a0= 0.6282. The nebula emits strongly in [O\u2009ii], $\\rm H \\beta$, and [O\u2009iii], and the quasar resides in an unusually overdense environment for a radio-quiet system. The environment likely consists of two groups which may be merging, and in total have an estimated dynamical mass of Mdyn \u2248 4\u00a0\u00d7\u00a01013 to 1014\u2009M\u2299. The nebula exhibits largely quiescent kinematics and irregular morphology. The nebula may arise primarily through interaction-related stripping of circumgalactic and interstellar medium (CGM\/ISM) of group members, with some potential contributions from quasar outflows. The simultaneous presence of the giant nebula and a radio-quiet quasar in a rich environment suggests a correlation between such circum-quasar nebulae and environmental effects. This possibility can be tested with larger samples. The upper limits on the electron number density implied by the [O\u2009ii] doublet ratio range from $\\log (n_{\\rm e, [O\\,{\\small II}]} \/\\mathrm{cm}^{-3})&amp;lt;1.2$ to 2.8. However, assuming a constant quasar luminosity and negligible projection effects, the densities implied from the measured line ratios between different ions (e.g. [O\u2009ii], [O\u2009iii], and [Ne\u2009v]) and photoionization simulations are often 10\u2212400\u00a0times larger. This large discrepancy can be explained by quasar variability on a time-scale of \u2248104\u2212105\u2009yr.<\/jats:p>","DOI":"10.1093\/mnras\/stad3364","type":"journal-article","created":{"date-parts":[[2023,11,7]],"date-time":"2023-11-07T12:03:48Z","timestamp":1699358628000},"page":"5429-5447","source":"Crossref","is-referenced-by-count":6,"title":["The first comprehensive study of a giant nebula around a radio-quiet quasar in the <i>z<\/i> &amp;lt; 1 Universe"],"prefix":"10.1093","volume":"527","author":[{"ORCID":"https:\/\/orcid.org\/0000-0002-2662-9363","authenticated-orcid":false,"given":"Zhuoqi","family":"Liu","sequence":"first","affiliation":[]},{"ORCID":"https:\/\/orcid.org\/0000-0001-9487-8583","authenticated-orcid":false,"given":"Sean D","family":"Johnson","sequence":"additional","affiliation":[{"name":"Department of Astronomy, University of Michigan , 1085 S. 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