For the more mathematically inclined, I have also created a Desmos graph which is a 1 for 1 transcription of the Space cooling code for radiators - all you do is input the total heat capacity of the gas packet being cooled, and it spits out the loss in both temperature and kilojoules.
Note that past a certain heatmass (a very low mass, relatively), the kilojoule gains slow down at lower temperatures ; that is, higher heatmasses only matter at really high temperatures.
For the purposes of something like a Supermatter, radiators will only ever do you 2kj or less depending on what your static temperature is. N2O can raise the safety temp of the SM which makes radiators significantly more efficient for keeping it cold; but N2O also reduces SM output significantly so be careful.
For something like Trit cooling, just a single radiator with a decent amount of gas passing through it regularly can pretty much keep your trit chamber at stable operating temperature forever. Maybe 2.
The real funny becomes when you need to cool something ludicrously hot - such as the HyperTorus. When you get to the millions of degrees, Radiators are cooling about a gigajoule of thermal energy every tick; and the HFR can generate dozens or even hundreds of gigawatts depending on the setup. That gigajoule figure is with Frezon as the coolant, by the way - with Hypernoblium it quadruples to 4 gigajoules. That heatcap density matters at these ludicrously high temperatures
https://www.desmos.com/calculator/kit1z4k1ja
Anyways heres the graph have fun