Renovate: paddyroddy/.github (minor) (#67)

Co-authored-by: renovate[bot] <29139614+renovate[bot]@users.noreply.github.com>
Co-authored-by: Patrick J. Roddy <patrickjamesroddy@gmail.com>

Author: renovate[bot]

.github/workflows/add-to-project.yaml

@@ -14,6 +14,6 @@ jobs:
     runs-on: ubuntu-latest
     steps:
       # yamllint disable-line rule:line-length
-      - uses: paddyroddy/.github/actions/add-to-project@1255ca6dc3bf6f7291aba6c1e8aa7225892d69d9 # v0
+      - uses: paddyroddy/.github/actions/add-to-project@38f0d7e429cc1e3366331dba6ab7a656f9aa01e2 # v0
         with:
           project-token: ${{ secrets.PROJECT_PAT }}

.github/workflows/deploy.yaml

@@ -18,13 +18,13 @@ jobs:
     runs-on: ubuntu-latest
     steps:
       # yamllint disable-line rule:line-length
-      - uses: paddyroddy/.github/actions/latex/chktex@1255ca6dc3bf6f7291aba6c1e8aa7225892d69d9 # v0
+      - uses: paddyroddy/.github/actions/latex/chktex@38f0d7e429cc1e3366331dba6ab7a656f9aa01e2 # v0
 
   vale:
     runs-on: ubuntu-latest
     steps:
       # yamllint disable-line rule:line-length
-      - uses: paddyroddy/.github/actions/vale@1255ca6dc3bf6f7291aba6c1e8aa7225892d69d9 # v0
+      - uses: paddyroddy/.github/actions/vale@38f0d7e429cc1e3366331dba6ab7a656f9aa01e2 # v0
         with:
           github-token: ${{ secrets.GITHUB_TOKEN }}
           vale-flags: --glob='!{config/,figures/*/example_,thesis}*'
@@ -33,7 +33,7 @@ jobs:
     runs-on: ubuntu-latest
     steps:
       # yamllint disable-line rule:line-length
-      - uses: paddyroddy/.github/actions/latex/compile@1255ca6dc3bf6f7291aba6c1e8aa7225892d69d9 # v0
+      - uses: paddyroddy/.github/actions/latex/compile@38f0d7e429cc1e3366331dba6ab7a656f9aa01e2 # v0
 
       - name: Upload artefacts
         # yamllint disable-line rule:line-length
@@ -85,7 +85,7 @@ jobs:
           name: artefacts
 
       # yamllint disable-line rule:line-length
-      - uses: paddyroddy/.github/actions/dropbox@1255ca6dc3bf6f7291aba6c1e8aa7225892d69d9 # v0
+      - uses: paddyroddy/.github/actions/dropbox@38f0d7e429cc1e3366331dba6ab7a656f9aa01e2 # v0
         with:
           configfile-version: ${{ secrets.CONFIGFILE_VERSION }}
           files-to-upload: $(find . -maxdepth 1 -name '*.pdf' -print)

.github/workflows/links.yaml

@@ -14,6 +14,6 @@ jobs:
     timeout-minutes: 2
     steps:
       # yamllint disable-line rule:line-length
-      - uses: paddyroddy/.github/actions/links@1255ca6dc3bf6f7291aba6c1e8aa7225892d69d9 # v0
+      - uses: paddyroddy/.github/actions/links@38f0d7e429cc1e3366331dba6ab7a656f9aa01e2 # v0
         with:
           github-token: ${{ secrets.GITHUB_TOKEN }}

.github/workflows/linting.yaml

@@ -13,6 +13,6 @@ jobs:
     runs-on: ubuntu-latest
     steps:
       # yamllint disable-line rule:line-length
-      - uses: paddyroddy/.github/actions/linting@1255ca6dc3bf6f7291aba6c1e8aa7225892d69d9 # v0
+      - uses: paddyroddy/.github/actions/linting@38f0d7e429cc1e3366331dba6ab7a656f9aa01e2 # v0
         with:
           pre-commit-config: ./.pre-commit-config.yaml

.pre-commit-config.yaml

@@ -1,7 +1,7 @@
 ---
 repos:
   - repo: https://github.com/paddyroddy/.github
-    rev: v0.324.0
+    rev: v0.338.0
     hooks:
       - id: general-hooks
         exclude: \.pdf$

figures/chapter2/power_spectrum.tex

@@ -2,11 +2,11 @@
 	\centering\capstart{}
 	\includegraphics[trim={0 430 0 0},clip,width=\textwidth]{planck_2018_power_spectrum.pdf}
 	\caption[
-	The 2018 Planck CMB angular power spectrum in temperature
+		The 2018 Planck CMB angular power spectrum in temperature
 	]{
-	Measurements of the angular power spectrum of the Planck CMB temperature anisotropies (in red), where \(D_{\ell} = \ell(\ell+1)C_{\ell}/2\pi{}\) (courtesy of The Planck Collaboration 2018~\cite{Planck2020}).
-	The spectrum is often plotted for \(D_{\ell}\) rather than \(\powerSpectrum{}\) as this gives a flat Sachs-Wolfe plateau for low \(\ell{}\) on a logarithmic scale.
-	The blue line is a best-fit model to temperature and polarisation data.
-	The error bars at low-\(\ell{}\) are dominated by cosmic variance.
+		Measurements of the angular power spectrum of the Planck CMB temperature anisotropies (in red), where \(D_{\ell} = \ell(\ell+1)C_{\ell}/2\pi{}\) (courtesy of The Planck Collaboration 2018~\cite{Planck2020}).
+		The spectrum is often plotted for \(D_{\ell}\) rather than \(\powerSpectrum{}\) as this gives a flat Sachs-Wolfe plateau for low \(\ell{}\) on a logarithmic scale.
+		The blue line is a best-fit model to temperature and polarisation data.
+		The error bars at low-\(\ell{}\) are dominated by cosmic variance.
 	}\label{fig:chapter2_power_spectrum}
 \end{figure}

figures/chapter3/elongated_gaussian.tex

@@ -6,11 +6,11 @@
 	\subfloat[\(\Re\big\{\pixel{(\translation{\omega'}\mathcal{EG})}\big\}\)]  % chktex 21
 	{\includegraphics[trim={4 7 3 6},clip,width=.5\textwidth]{elongated_gaussian_1tsig_1psig10_L128_translate_alpha3pi4_beta1pi8_res512_real_norm.pdf}}
 	\caption[
-	An elongated Gaussian on the north pole and then translated
+		An elongated Gaussian on the north pole and then translated
 	]{
-	Presented in panel (a) is an elongated Gaussian with parameters \((\mean{\theta},\mean{\phi},\sigma_{\theta},\sigma_{\phi}) = (0,\pi,10^{0},10^{-1})\) on the north pole (bandlimited at \(L=128\)), \cf{} \cref{eq:chapter3_elongated_gaussian} --- where the central bar in the plot extends over half of the sphere.
-	The elongated Gaussian is then translated to some \(\omega'=(\theta',\phi')\), as shown in panel (b).
-	The even azimuthal symmetry in the initial kernel definition results in the two localised components at \(\phi'\) and \(-\phi'\) under translation.
-	The colour is between zero and one, reflecting the scaled intensity of the field.
+		Presented in panel (a) is an elongated Gaussian with parameters \((\mean{\theta},\mean{\phi},\sigma_{\theta},\sigma_{\phi}) = (0,\pi,10^{0},10^{-1})\) on the north pole (bandlimited at \(L=128\)), \cf{} \cref{eq:chapter3_elongated_gaussian} --- where the central bar in the plot extends over half of the sphere.
+		The elongated Gaussian is then translated to some \(\omega'=(\theta',\phi')\), as shown in panel (b).
+		The even azimuthal symmetry in the initial kernel definition results in the two localised components at \(\phi'\) and \(-\phi'\) under translation.
+		The colour is between zero and one, reflecting the scaled intensity of the field.
 	}\label{fig:chapter3_elongated_gaussian}
 \end{figure}

figures/chapter3/gaussian.tex

@@ -6,11 +6,11 @@
 	\subfloat[\(\Re\big\{\pixel{(\translation{\omega'}\mathcal{G})}\big\}\)]  % chktex 21
 	{\includegraphics[trim={4 7 3 6},clip,width=.5\textwidth]{gaussian_10sig_L128_translate_alpha3pi4_beta1pi8_res512_real_norm.pdf}}
 	\caption[
-	A Gaussian on the north pole and then translated
+		A Gaussian on the north pole and then translated
 	]{
-	Panel (a) presents an axisymmetric Gaussian in \(\ell{}\) on the north pole (bandlimited at \(L=128\)), where \(\sigma=10^{1}\), \cf{} \cref{eq:chapter3_gaussian}.
-	The Gaussian is then translated to some \(\omega'=(\theta',\phi')\), as shown in panel (b).
-	Plainly, the axisymmetric symmetry has been preserved under translation.
-	The colour is between zero and one, reflecting the scaled intensity of the field.
+		Panel (a) presents an axisymmetric Gaussian in \(\ell{}\) on the north pole (bandlimited at \(L=128\)), where \(\sigma=10^{1}\), \cf{} \cref{eq:chapter3_gaussian}.
+		The Gaussian is then translated to some \(\omega'=(\theta',\phi')\), as shown in panel (b).
+		Plainly, the axisymmetric symmetry has been preserved under translation.
+		The colour is between zero and one, reflecting the scaled intensity of the field.
 	}\label{fig:chapter3_gaussian}
 \end{figure}

figures/chapter3/harmonic_gaussian.tex

@@ -12,12 +12,12 @@
 	\subfloat[\(\Re\big\{\pixel{(\translation{\omega'}f_{B})}\big\}\)]  % chktex 21
 	{\includegraphics[trim={4 7 3 6},clip,width=.5\textwidth]{harmonic_gaussian_10lsig_10msig_L128_translate_alpha3pi4_beta1pi8_res512_real_norm.pdf}}
 	\caption[
-	Two harmonic Gaussians on the north pole and then translated
+		Two harmonic Gaussians on the north pole and then translated
 	]{
-	The top row presents a harmonic Gaussian on the north pole (bandlimited at \(L=128\)) for two different \((\sigma_{\ell},\sigma_{m})\) values, \cf{} \cref{eq:chapter3_harmonic_gaussian}.
-	Panel (a) corresponds to a more elongated kernel \(f_{A}\), where \((\sigma_{\ell},\sigma_{m}) = (10^{2},10^{1})\).
-	The harmonic Gaussian is translated to some \(\omega'=(\theta',\phi')\) as shown in panel (c).
-	Whereas panel (b) corresponds to a more symmetric kernel \(f_{B}\), where \((\sigma_{\ell},\sigma_{m}) = (10^{1},10^{1})\), with the corresponding translated function in panel (d).
-	The colour is between zero and one, reflecting the scaled intensity of the field.
+		The top row presents a harmonic Gaussian on the north pole (bandlimited at \(L=128\)) for two different \((\sigma_{\ell},\sigma_{m})\) values, \cf{} \cref{eq:chapter3_harmonic_gaussian}.
+		Panel (a) corresponds to a more elongated kernel \(f_{A}\), where \((\sigma_{\ell},\sigma_{m}) = (10^{2},10^{1})\).
+		The harmonic Gaussian is translated to some \(\omega'=(\theta',\phi')\) as shown in panel (c).
+		Whereas panel (b) corresponds to a more symmetric kernel \(f_{B}\), where \((\sigma_{\ell},\sigma_{m}) = (10^{1},10^{1})\), with the corresponding translated function in panel (d).
+		The colour is between zero and one, reflecting the scaled intensity of the field.
 	}\label{fig:chapter3_harmonic_gaussian}
 \end{figure}

figures/chapter3/squashed_gaussian.tex

@@ -6,11 +6,11 @@
 	\subfloat[\(\Re\big\{\pixel{(\translation{\omega'}\mathcal{SG})}\big\}\)]  % chktex 21
 	{\includegraphics[trim={4 7 3 6},clip,width=.5\textwidth]{squashed_gaussian_1tsig_1freq10_L128_translate_alpha3pi4_beta1pi8_res512_real_norm.pdf}}
 	\caption[
-	A squashed Gaussian on the north pole and then translated
+		A squashed Gaussian on the north pole and then translated
 	]{
-	Panel (a) presents a squashed Gaussian on the north pole (bandlimited at \(L=128\)), where \((\mean{\theta},\sigma_{\theta},\nu_{\phi}) = (0,10^{0},10^{-1})\), \cf{} \cref{eq:chapter3_squashed_gaussian}.
-	The squashed Gaussian is then translated to some \(\omega'=(\theta',\phi')\), as shown in panel (b).
-	The odd azimuthal symmetry in the initial kernel definition is preserved under translation.
-	The colour is between zero and one, reflecting the scaled intensity of the field.
+		Panel (a) presents a squashed Gaussian on the north pole (bandlimited at \(L=128\)), where \((\mean{\theta},\sigma_{\theta},\nu_{\phi}) = (0,10^{0},10^{-1})\), \cf{} \cref{eq:chapter3_squashed_gaussian}.
+		The squashed Gaussian is then translated to some \(\omega'=(\theta',\phi')\), as shown in panel (b).
+		The odd azimuthal symmetry in the initial kernel definition is preserved under translation.
+		The colour is between zero and one, reflecting the scaled intensity of the field.
 	}\label{fig:chapter3_squashed_gaussian}
 \end{figure}