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Fix and add links #59

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6 changes: 3 additions & 3 deletions content/notebooks/synphot/synphot.ipynb
Original file line number Diff line number Diff line change
Expand Up @@ -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",
Expand Down Expand Up @@ -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",
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2 changes: 1 addition & 1 deletion markdown/software.md
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Expand Up @@ -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>]`

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4 changes: 2 additions & 2 deletions markdown/tutorials.md
Original file line number Diff line number Diff line change
Expand Up @@ -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 |
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