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Based on Planck's formula for thermal radiation of a black body, the intensity of the radiation can be derived in a form of a quartic equation, known as the Stefan-Boltzmann equation.
Any infrared thermometer you can buy in the market is designed based on the formula in Physics. Nevertheless, a real object may be noticeably different from an ideal black body in its efficiency in emitting its thermal energy. A parameter, called emissivity, is introduce to take this fact into account. By definition, the emissivity is a ratio of the gray body radiation intensity to that of a black body. You can google emissivity lists, such as from thermoworks.com/emissivity-table.
In practice, a simple IR thermometer whose default emissivity is fixed will give temperatures lower than the actual temperature is the emissivity of the object is less than unit, say 0.8 or 0.6. To overcome this apparent discrepancy, you may choose an IR thermometer with adjustable emissivity function.
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