Njengesixhobo esiphambili sokujonga isithuba esinzulu, esi sihluzo se-O-III se-intshi ezi-2 sisebenzisa itekhnoloji yokugquma ye-ion beam yesizukulwana sesithathu ukuze sivale ngokuchanekileyo i-bandwidth ye-oxygen emission oxygen eyi-496nm/501nm ephindwe kabini ±3nm, sicinezela i-90% yezibane zongcoliseko lokukhanya kwasezidolophini ngelixa sigcina ukuhanjiswa kokukhanya kwe-93% kwibhendi ekujoliswe kuyo. Uyilo lwayo olukhulu lwenzelwe ngokukodwa inkqubo ye-eyepiece ye-2-intshi ephezulu. Umlinganiselo wokwenyani unokunyusa isisombululo sesakhiwo segobolondo se-nebulae yeplanethi (njenge-M57 ring nebula) nge-40%, kwaye senze igesi ye-ionizing ene-fibrous ibonakale kwi-supernova residues (njenge-veil nebula NGC 6960) ifikelele ekubonweni kwendawo yeBortle 4, njl. Isiphumo.

Umzimba wesibuko usebenzisa iringi ye-aluminium alloy yendiza kunye neglasi ethe tyaba ye-λ/4, kwaye ixhotyiswe ngebhokisi yokugcina engangeni kumswakama kwaye ingashukumi njengesiqhelo. Lukhetho oluphambili kubathandi beenkwenkwezi ukuphucula ithala leencwadi lezixhobo emva kwesihluzi se-UHC.

● Isihluzi se-Eyepiece yeTelescope ye-Kson 2” O-III

● Ibhokisi yokugcina i-ABS engashukumiyo