diff --git a/content/notebooks/synphot/synphot.ipynb b/content/notebooks/synphot/synphot.ipynb
index 5fdbe2b..c69c09e 100644
--- a/content/notebooks/synphot/synphot.ipynb
+++ b/content/notebooks/synphot/synphot.ipynb
@@ -224,9 +224,6 @@
    "metadata": {},
    "outputs": [],
    "source": [
-    "# Load the WFI F158 element\n",
-    "wfi_f158 = stsyn.band('roman, wfi, f158')\n",
-    " \n",
     "# Retrieve the spectrum of the star\n",
     "star_spec = syn.SourceSpectrum.from_file(os.path.join(os.environ['PYSYN_CDBS'], 'grid', 'pickles', 'dat_uvk', 'pickles_uk_100.fits'))\n",
     " \n",
@@ -264,6 +261,9 @@
    "metadata": {},
    "outputs": [],
    "source": [
+    "# Load the WFI F158 element\n",
+    "wfi_f158 = stsyn.band('roman, wfi, f158')\n",
+    "\n",
     "# Observe the spectrum with the F158 bandpass\n",
     "obs_spec = syn.Observation(final_spec, wfi_f158)\n",
     " \n",
diff --git a/markdown/software.md b/markdown/software.md
index 45141e0..0694bd1 100644
--- a/markdown/software.md
+++ b/markdown/software.md
@@ -15,7 +15,7 @@ As part of the science platform, you can use some helper commands to create and
 
 ### 1. Creating a Conda Environment
 
-First, you should use the `kernel create` command to generate an environment for your software. You can select your desired Python version, and choose a name for the environment.
+First, you should use the `kernel-create` command to generate an environment for your software. You can select your desired Python version, and choose a name for the environment.
 
 `kernel-create <environment-name> [<python-version>] [<lab-display-name>]`
 
diff --git a/markdown/tutorials.md b/markdown/tutorials.md
index bcd2015..2b8e7b2 100644
--- a/markdown/tutorials.md
+++ b/markdown/tutorials.md
@@ -19,11 +19,11 @@ Below is an outline of the content covered in each notebook and the Science Work
 | [Working with ASDF](../content/notebooks/working_with_asdf/working_with_asdf.ipynb)                         | Open ASDF files with roman_datamodels, access metadata, manipulate arrays, and save changes to disk.                     | WFI Data Simulation<br>WFI Data Analysis |
 | [Data Visualization](../content/notebooks/data_visualization/data_visualization.ipynb)                      | Use Imviz to display a preview of Roman Level 2 products and run quick analysis tools.                                                               | WFI Data Simulation<br>WFI Data Analysis |
 | [Roman I-sim](../content/notebooks/romanisim/romanisim.ipynb)                                               | Generate Level 1 and Level 2 WFI imaging products.                                                                      | WFI Data Simulation                      |
-| [RomanCal](..content/notebooks/romancal/romancal.ipynb)                                                     | Process WFI L1 imaging raw data to obtain exposure level products.                                                      | WFI Data Simulation<br>WFI Data Analysis |
+| [RomanCal](../content/notebooks/romancal/romancal.ipynb)                                                     | Process WFI L1 imaging raw data to obtain exposure level products.                                                      | WFI Data Simulation<br>WFI Data Analysis |
 | [Aperture Photometry](../content/notebooks/aperture_photometry/aperture_photometry.ipynb)                   | Perform forced aperture photometry on a simulated WFI image.                                                            | WFI Data Analysis                        |
 | [Galaxy Shapes](../content/notebooks/measuring_galaxy_shapes/measuring_galaxy_shapes.ipynb)                 | Perform shape measurements of galaxies on a simulated WFI image.                                                        | WFI Data Analysis                        |
 | [Pandeia](../content/notebooks/pandeia/pandeia.ipynb)                                                       | Estimate the exposure parameters needed to reach a given SNR for simulated sources in a small area of one WFI detector. | WFI Observations Planning                |
 | [RIST](../content/notebooks/rist/rist.ipynb)                                                                | Roman Interactive Sensitivity Tool. Simplified, interactive version of Pandeia. Estimate the SNR for a variety of target brightnesses and filters.          | WFI Observations Planning                |
 | [STIPS](../content/notebooks/stips/stips.ipynb)                                                             | Simulate large astronomical scenes with WFI full field-of-view.                                                         | WFI Observations Planning                |
-| [Synphot](../content/notebooks/romanisim_romancal/romanisim_romancal.ipynb)                                 | Synthetic photometry software, estimate the brightness of sources observed with Roman WFI.                              | WFI Observations Planning                |
+| [Synphot](../content/notebooks/synphot/synphot.ipynb)                                 | Synthetic photometry software, estimate the brightness of sources observed with Roman WFI.                              | WFI Observations Planning                |
 | [WebbPSF](../content/notebooks/webbpsf/webbpsf.ipynb)                                                       | Generate WFI simulated Point Spread Functions using WebbPSF.                                                            | WFI Observations Planning                |
\ No newline at end of file