▁for ▁quality ▁by ▁the ▁ten ▁AS K AP ▁Survey ▁Science ▁Teams . ▁Post ▁processing ▁will ▁be ▁supported ▁by ▁super comput ers ▁operated ▁by ▁i V EC ▁at ▁the ▁P aw sey ▁Centre ▁in ▁Per th , ▁and ▁may ▁also ▁be ▁complement ed ▁by ▁' the S ky Net ', ▁a ▁" community ▁computing ▁initi ative " ▁similar ▁to ▁Set i @ home . ▁ ▁Science ▁▁ ▁During ▁AS K AP ' s ▁first ▁five ▁years ▁of ▁operation , ▁at ▁least ▁ 7 5 % ▁of ▁its ▁time ▁will ▁be ▁used ▁for ▁large ▁Survey ▁Science ▁Project s . ▁AS K AP ▁is ▁expected ▁to ▁make ▁substantial ▁adv ances ▁in ▁key ▁areas , ▁including ▁the ▁following : ▁ ▁Gal axy ▁formation ▁and ▁gas ▁evolution ▁in ▁the ▁nearby ▁Un iverse ▁through ▁ext rag al actic ▁H I ▁surve ys ▁ ▁E volution , ▁formation ▁and ▁population ▁of ▁galaxies ▁across ▁cos mic ▁time ▁via ▁high ▁resolution , ▁continu um ▁surve ys ▁ ▁Character isation ▁of ▁the ▁radio ▁trans ient ▁sky ▁through ▁detection ▁and ▁monitoring ▁( including ▁V L BI ) ▁of ▁trans ient ▁and ▁variable ▁sources , ▁and ▁ ▁E volution ▁of ▁magnetic ▁fields ▁in ▁galaxies ▁over ▁cos mic ▁time ▁through ▁polar isation ▁surve ys . ▁ ▁AS K AP ▁Survey ▁Science ▁Project s ▁ ▁In ▁ 2 0 0 9 , ▁after ▁an ▁open ▁call ▁for ▁propos als , ▁C SI RO ▁announced ▁that ▁ten ▁major ▁science ▁projects ▁had ▁been ▁selected ▁to ▁use ▁AS K AP . ▁Of ▁the ▁ten ▁projects ' ▁authors , ▁ 3