I report an overview of data quality in the about three hours of Science mode (Low Noise 3 state) following the interventions of the past weeks. Overall, the noise is consistent with that before the intervention. I have attached some plots below to analyze stationarity, glitch rate and spectral noise.
Figure 1: Side-by-side spectrograms of the strain in the last three hours of Science mode pre-intervention and in the post-intervention Science mode segment.
Figure 2: Same spectrogram but where the two parts are normalized frequency-wise by the median. On the left-hand side, you can see some color variation, indicating excess noise, in the 50-60 and 300-400 Hz bands. I will analyze the detail in the following plots.
Figure 3: Glitchgram and glitch rate timeseries, perfectly consistent with what we already saw during O4b: 25-minute glitches are the main family of glitches visible. The rate is still 0.1 glitches/minute. The latest burst of glitches appears to be associated with the earthquake reported by Beatrice from 22:51 UTC: #64849.
File: In this PDF file I report the comparison between the reference sensitivity curves for O4b (as reported on the VIM), in the last segment of Science mode before the intervention, in an hour of DQ studies at 9:15 on August 2, and during the Science mode on August 2. The various frequency windows detail some regions with more marked differences between the current sensitivity curve and those before the intervention. A few of them have been already highlighted in #64838. As shown in the normalized spectrogram (Figure 2), some of these structures are non-stationary, and it is likely that they will disappear after the detector will stabilize after a few hours of unperturbed Science mode, and especially once the squeezing is reinjected. It is however important to keep an eye on these frequency bands and structures in the coming days and longer data segments.
So far, everything is OK, overall, from a data quality perspective.