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The plot below shows the PSD at the LDO output under no-load conditions. The measured output noise density at 10 Hz is 15 µV/√Hz, and the integrated noise from 10 Hz to 1 MHz becomes 484 µVrms. The spectrum is generally clean, with a single spur at 21.3 kHz and its harmonic at 42.6 kHz. The source of this spur is unknown; the evaluation board was powered from a battery, and there shouldn't be any switching regulators active during the measurement.
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Two noise simulations were performed for the circuit:
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-[LDO output-referred noise with an ideal (noiseless) reference source](https://devstdin.github.io/sky130artefacts_tt08/ldo/ldo/#ldo-voltage-noise-specification-pexbr): 1.8...1.9 µV/√Hz at 10 Hz
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-[Output-referred noise of the bandgap reference](https://devstdin.github.io/sky130artefacts_tt08/bmbg/bmbg/#reference-voltage-noise-specification-pexbr): 13...19 µV/√Hz at 10 Hz
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Both simulations use an ideal (noiseless) bias current source. The real bias source has a (simulated) [current noise](https://devstdin.github.io/sky130artefacts_tt08/vthref/vthref/#ac-noisebr) of approximately 10 pA/√Hz at 10 Hz. For this analysis, the bias current noise is assumed to be negligible.
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The total expected output noise should be the quadratic sum of the LDO’s intrinsic noise and the bandgap’s noise multiplied by the LDO gain
This 20...29 µV/√Hz span is slightly higher than the measured noise density of 15 µV/√Hz at 10 Hz.
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### Ring Oscillator
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Frequency and duty cycle were measured across a 50 °C temperature range. As shown in the two plots below, the oscillation frequency changes by approximately 6 kHz/°C, while the duty cycle remains nearly constant.
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@@ -38,4 +55,4 @@ According to literature, the oscillation frequency is approximately proportional
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