From 2098ebf7d56ae1a9748ba65314e42e1e0632337a Mon Sep 17 00:00:00 2001
From: Hsin Fan <57552401+hsinfan1996@users.noreply.github.com>
Date: Sat, 26 Aug 2023 02:15:25 +0800
Subject: [PATCH] Add title

---
 examples/demo_theory_functionality.ipynb    | 4 +++-
 examples/demo_theory_functionality_oo.ipynb | 4 +++-
 2 files changed, 6 insertions(+), 2 deletions(-)

diff --git a/examples/demo_theory_functionality.ipynb b/examples/demo_theory_functionality.ipynb
index c84f329b1..5bb640cce 100644
--- a/examples/demo_theory_functionality.ipynb
+++ b/examples/demo_theory_functionality.ipynb
@@ -436,7 +436,7 @@
     "## Side note regarding the Einasto profile (CCL and NC backends only)\n",
     "\n",
     "The Einasto profile is supported by both the CCL and NumCosmo backends. The value of the slope of the Einasto profile can be defined by the user, using the `alpha_ein` keyword. If `alpha_ein` is not provided, both backend revert to a default value for the Einasto slope:\n",
-    "- In CCL, the default Einasto slope depends on cosmology, redshift and halo mass. \n",
+    "- In CCL, the default Einasto slope depends on cosmology, redshift and halo mass.\n",
     "- In NumCosmo, the default value is $\\alpha_{\\rm ein}=0.25$.\n",
     "\n",
     "**NB: for CCL, setting a user-defined value for the Einasto slope is only available for versions >= 2.6.** Earlier versions only allow the default option.\n",
@@ -476,6 +476,8 @@
    "cell_type": "markdown",
    "metadata": {},
    "source": [
+    "## Side note regarding the Einasto profile (CCL backend only)\n",
+    "\n",
     "For CCL versions >= 2.8.1.dev73+g86125b08, the surface mass density profile can be calculated with the quad_vec numerial integration in addition to the default FFTLog. This option will increase the precision of the profile at large radii and can be enabled by passing `use_projected_quad` keyword argument to `compute_surface_density`."
    ]
   },
diff --git a/examples/demo_theory_functionality_oo.ipynb b/examples/demo_theory_functionality_oo.ipynb
index 673a972ff..3e8083c3a 100644
--- a/examples/demo_theory_functionality_oo.ipynb
+++ b/examples/demo_theory_functionality_oo.ipynb
@@ -274,7 +274,7 @@
     "## Side note regarding the Einasto profile (CCL and NC backends only)\n",
     "\n",
     "The Einasto profile is supported by both the CCL and NumCosmo backends. The value of the slope of the Einasto profile $\\alpha_{\\rm ein}$ can be defined by the user, using the `set_einasto_alpha` method. If $\\alpha_{\\rm ein}$ is not provided, both backend revert to a default value for the Einasto slope:\n",
-    "- In CCL, the default Einasto slope depends on cosmology, redshift and halo mass. \n",
+    "- In CCL, the default Einasto slope depends on cosmology, redshift and halo mass.\n",
     "- In NumCosmo, the default value is $\\alpha=0.25$.\n",
     "\n",
     "**NB: for CCL, setting a user-defined value for the Einasto slope is only available for CCL version >= 2.6.** Earlier versions only allow the default option.\n",
@@ -306,6 +306,8 @@
    "cell_type": "markdown",
    "metadata": {},
    "source": [
+    "## Side note regarding the Einasto profile (CCL backend only)\n",
+    "\n",
     "For CCL versions >= 2.8.1.dev73+g86125b08, the surface mass density profile can be calculated with the quad_vec numerial integration in addition to the default FFTLog. This option will increase the precision of the profile at large radii and can be enabled by calling `set_projected_quad(True)`."
    ]
   },