update v2 post

dawn-cph · Mar 1, 2024 · 24e88a3 · 24e88a3
1 parent 1b0025d
commit 24e88a3
Show file tree

Hide file tree

Showing 2 changed files with 2 additions and 2 deletions.
diff --git a/_posts/2024-03-01-nirspec-extractions-v2.md b/_posts/2024-03-01-nirspec-extractions-v2.md
@@ -29,7 +29,7 @@ The redshift quality grades have been copied from those of the previous release
 
 ## Note
 
-The `v2` spectra are affected by a bug that causes the uncertainties in the derived products to be too large by roughly a factor of $f=N^{1/4}$, where $N$ is the number of combined exposures grouped by ``source_name / detector / grating / filter / MSA plan``.  For a simple set of three exposures with the 3-Shutter-Nod dither pattern, ``f = 3^{1/4} ~ 1.3``, i.e., the tabulated uncertainties are roughly 1.3× too large.  The effect of the bug is larger for deeper programs; for typical UNCOVER extractions ``f = 18^{1/4} ~ 2``.  For more information, see [msaexp PR#54](https://github.com/gbrammer/msaexp/pull/54).
+The `v2` spectra are affected by a bug that causes the uncertainties in the derived products to be too large by roughly a factor of ``f = N^{1/4}``, where ``N`` is the number of combined exposures grouped by ``source_name / detector / grating / filter / MSA plan``.  For a simple set of three exposures with the 3-Shutter-Nod dither pattern, ``f = 3^{1/4} ~ 1.3``, i.e., the tabulated uncertainties are roughly 1.3× too large.  The effect of the bug is larger for deeper programs; for typical UNCOVER extractions ``f = 18^{1/4} ~ 2``.  For more information, see [msaexp PR#54](https://github.com/gbrammer/msaexp/pull/54).
 
 ## Observing programs
 

diff --git a/assets/post_files/2024-03-01-nirspec-extractions-v2.ipynb b/assets/post_files/2024-03-01-nirspec-extractions-v2.ipynb
@@ -41,7 +41,7 @@
     "\n",
     "## Note\n",
     "\n",
-    "The `v2` spectra are affected by a bug that causes the uncertainties in the derived products to be too large by roughly a factor of $f=N^{1/4}$, where $N$ is the number of combined exposures grouped by ``source_name / detector / grating / filter / MSA plan``.  For a simple set of three exposures with the 3-Shutter-Nod dither pattern, ``f = 3^{1/4} ~ 1.3``, i.e., the tabulated uncertainties are roughly 1.3× too large.  The effect of the bug is larger for deeper programs; for typical UNCOVER extractions ``f = 18^{1/4} ~ 2``.  For more information, see [msaexp PR#54](https://github.com/gbrammer/msaexp/pull/54)."
+    "The `v2` spectra are affected by a bug that causes the uncertainties in the derived products to be too large by roughly a factor of ``f = N^{1/4}``, where ``N`` is the number of combined exposures grouped by ``source_name / detector / grating / filter / MSA plan``.  For a simple set of three exposures with the 3-Shutter-Nod dither pattern, ``f = 3^{1/4} ~ 1.3``, i.e., the tabulated uncertainties are roughly 1.3× too large.  The effect of the bug is larger for deeper programs; for typical UNCOVER extractions ``f = 18^{1/4} ~ 2``.  For more information, see [msaexp PR#54](https://github.com/gbrammer/msaexp/pull/54)."
    ]
   },
   {