Added About section with authors and dates

spacetelescope · Apr 16, 2024 · cfc7a29 · cfc7a29
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diff --git a/notebooks/NIRSpec_NSClean/FS_NSClean_example.ipynb b/notebooks/NIRSpec_NSClean/FS_NSClean_example.ipynb
@@ -5,11 +5,10 @@
    "id": "4ee4766c-2f11-4783-9d84-cbbbd1382f53",
    "metadata": {},
    "source": [
+    "<a id=\"top\"></a>\n",
     "# Cleaning Residual 1/f Noise in NIRSpec FS Products with NSClean \n",
     "<hr style=\"border:1px solid black\">\n",
     "\n",
-    "**Latest update**: Feburary 29, 2024.\n",
-    "\n",
     "## Notebook Goal\n",
     "\n",
     "The goal of this notebook is to generate cleaned FS (*_rate.fits*) files by removing residual 1/f noise. These cleaned files will be used as input for the level 3 (`Spec3Pipeline`) pipeline.\n",
@@ -31,6 +30,8 @@
     "    * 7.1 [Verify the Mask (Hand-Modified Mask)](#verify_modified_mask)\n",
     "    * 7.2 [Comparing Original vs. Cleaned Data (Hand-Modified Mask)](#nsclean_modified_compare)\n",
     "* 8. [Conclusion](#conclusion)\n",
+    "* [About the Notebook](#about)\n",
+    "\n",
     "\n",
     "\n",
     "\n",
@@ -1393,12 +1394,21 @@
    ]
   },
   {
-   "cell_type": "code",
-   "execution_count": null,
-   "id": "4518f00a-c911-4f26-8f38-07a03a076886",
+   "cell_type": "markdown",
+   "id": "fbe656ab-ef2c-4efb-91e1-4c020a7206a0",
    "metadata": {},
-   "outputs": [],
-   "source": []
+   "source": [
+    "\n",
+    "## About the Notebook <a name=\"about\"></a>\n",
+    "\n",
+    "**Authors:** Melanie Clarke, Kayli Glidic; NIRSpec Instrument Team\n",
+    "\n",
+    "**Updated On**: Feburary 29, 2024.\n",
+    "\n",
+    "<hr style=\"border:0.5px solid black\">\n",
+    "\n",
+    "[Top of Page](#top)\n"
+   ]
   }
  ],
  "metadata": {

diff --git a/notebooks/NIRSpec_NSClean/IFU_NSClean_example.ipynb b/notebooks/NIRSpec_NSClean/IFU_NSClean_example.ipynb
@@ -5,11 +5,10 @@
    "id": "27997993-b40d-4857-94c1-2d88989b4d94",
    "metadata": {},
    "source": [
+    "<a name=\"top\"></a>\n",
     "# Cleaning Residual 1/f Noise in NIRSpec IFU Products with NSClean \n",
     "<hr style=\"border:1px solid black\">\n",
     "\n",
-    "**Latest update**: Feburary 29, 2024.\n",
-    "\n",
     "## Notebook Goal\n",
     "\n",
     "The goal of this notebook is to generate cleaned IFU (*_rate.fits*) files by removing residual 1/f noise. These cleaned files will be used as input for the level 3 (`Spec3Pipeline`) pipeline.\n",
@@ -30,6 +29,8 @@
     "    * 7.1 [Verify the Mask (Hand-Modified Mask)](#verify_modified_mask)\n",
     "    * 7.2 [Comparing Original vs. Cleaned Data (Hand-Modified Mask)](#nsclean_modified_compare)\n",
     "* 8. [Conclusion](#conclusion)\n",
+    "* [About the Notebook](#about)\n",
+    "\n",
     "\n",
     "## 1. Introduction <a name=\"introduction\"></a>\n",
     "<hr style=\"border:1px solid black\">\n",
@@ -938,6 +939,22 @@
     "<b>Note:</b> Cleaning with the alternate mask still removes some of the wavelength-dependent variations but leaves residual background variation in NRS2. Also note the overall continuum level for the spectrum has changed, especially for NRS1. Again, this is because sigma-clipping, unlike the default method, only masks the bright outliers, rather than the entire science region. Consequently, some sky regions are included in the background model that gets subtracted from the data, which can result in changes to the continuum level. In this case, the original algorithm, which blocks the entire science region for each IFU slice (or the hand-modified method to exclude snowballs), is preferable to creating the mask via sigma-clipping.\n",
     "</div>"
    ]
+  },
+  {
+   "cell_type": "markdown",
+   "id": "fdcb054d-3fd0-4ea3-9fcf-3cdfefbb38a7",
+   "metadata": {},
+   "source": [
+    "## About the Notebook <a name=\"about\"></a>\n",
+    "\n",
+    "**Authors:** Melanie Clarke, Kayli Glidic; NIRSpec Instrument Team\n",
+    "\n",
+    "**Updated On**: Feburary 29, 2024.\n",
+    "\n",
+    "<hr style=\"border:0.5px solid black\">\n",
+    "\n",
+    "[Top of Page](#top)"
+   ]
   }
  ],
  "metadata": {

diff --git a/notebooks/NIRSpec_NSClean/MOS_NSClean_example.ipynb b/notebooks/NIRSpec_NSClean/MOS_NSClean_example.ipynb
@@ -5,11 +5,10 @@
    "id": "95dcb8aa-37e4-4707-a73b-2d8e047a3c66",
    "metadata": {},
    "source": [
+    "<a name=\"top\"></a>\n",
     "# Cleaning Residual 1/f Noise in NIRSpec MOS Products with NSClean \n",
     "<hr style=\"border:1px solid black\">\n",
     "\n",
-    "**Latest update**: Feburary 29, 2024.\n",
-    "\n",
     "## Notebook Goal\n",
     "\n",
     "The goal of this notebook is to generate cleaned MOS (*_rate.fits*) files by removing residual 1/f noise. These cleaned files will be used as input for the level 3 (`Spec3Pipeline`) pipeline.\n",
@@ -30,6 +29,7 @@
     "    * 7.1 [Verify the Mask (Hand-Modified Mask)](#verify_modified_mask)\n",
     "    * 7.2 [Comparing Original vs. Cleaned Data (Hand-Modified Mask)](#nsclean_modified_compare)\n",
     "* 8. [Conclusion](#conclusion)\n",
+    "* [About the Notebook](#about)\n",
     "\n",
     "\n",
     "## 1. Introduction <a name=\"introduction\"></a>\n",
@@ -1030,6 +1030,22 @@
     "\n",
     "</div>"
    ]
+  },
+  {
+   "cell_type": "markdown",
+   "id": "63478af5-10fc-4f8b-be62-b0fcd9f65423",
+   "metadata": {},
+   "source": [
+    "## About the Notebook <a name=\"about\"></a>\n",
+    "\n",
+    "**Authors:** Melanie Clarke, Kayli Glidic; NIRSpec Instrument Team\n",
+    "\n",
+    "**Updated On**: Feburary 29, 2024.\n",
+    "\n",
+    "<hr style=\"border:0.5px solid black\">\n",
+    "\n",
+    "[Top of Page](#top)"
+   ]
   }
  ],
  "metadata": {