Outlier parameters from the Weave pipeline in the study "Searches for Continuous Gravitational Waves from Supernova Remnants in the first part of the LIGO-Virgo-KAGRA Fourth Observing run"

$\textbf{Outlier parameters from the Weave pipeline in the study:}$ "$\textbf{Searches for Continuous Gravitational Waves from Supernova Remnants }$ $\textbf{in the first part of the LIGO-Virgo-KAGRA Fourth Observing run}$" $\textbf{File Types:}$ [Target]_followUp-2_Tcoh[X]_outlierParam.txtIncludes frequency parameters ($f$, $\dot{f}$, $\ddot{f}$) and the detection statistic $\bar{\mathcal{F}}$ for outliers that persist through the second follow-up stage. [Target]_followUp-2_Tcoh[X]_outlierParam_clustered.txtA clustered version where outliers are grouped into cubes, with cluster widths from the center given as $\Delta f$, $\Delta\dot{f}$, and $\Delta\ddot{f}$. [Target]_SaturatedBandList.txtA full list of saturated bands for each target (Col 1: starting frequencies, Col 2: band width). $\textbf{Coherence Times ($T_{coh}$):}$Cassiopeia A: 20 daysVela Jr. and G347.3-0.5: 30 days