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WeÂ  intendÂ  toÂ  investigateÂ  theÂ  redshiftÂ  distributionÂ  andÂ  environmentalÂ  conditionsÂ  ofÂ  quasarÂ  AGNs.Â  WeÂ  employÂ  specific redshiftÂ  binsÂ  withinÂ  eBOSSÂ  toÂ  drawÂ  conclusionsÂ  onÂ  theÂ  evolutionaryÂ  pathÂ  ofÂ  supermassiveÂ  blackÂ  holesÂ  (SMBHs)Â  and howÂ  itÂ  isÂ  dependentÂ  onÂ  environment;Â  inÂ  additionÂ  weÂ  seekÂ  toÂ  determineÂ  theÂ  extentÂ  toÂ  whichÂ  AGNÂ  feedbackÂ  is responsibleÂ  forÂ  heatingÂ  withinÂ  theÂ  intergalactic mediumÂ  ofÂ  galaxyÂ  groups.

Identifying Evolutionary Patterns of SMBHs Using Characteristic Variables of the Quasar AGNs of eBOSS