set default kernels to jwebbinar

spacetelescope · May 18, 2021 · 3299b64 · 3299b64
1 parent 34b35b6
commit 3299b64
Show file tree

Hide file tree

Showing 6 changed files with 20 additions and 20 deletions.
diff --git a/imaging_mode/imaging_mode_stage_1.ipynb b/imaging_mode/imaging_mode_stage_1.ipynb
@@ -70,7 +70,7 @@
     "\n",
     "This notebook covers part 1 of the imaging mode data calibration module. In this notebook we'll review Stage 1 of the JWST calibration pipeline, also known as *calwebb_detector1*. \n",
     "\n",
-    "The [Stage 1 pipeline](https://jwst-pipeline.readthedocs.io/en/stable/jwst/pipeline/calwebb_detector1.html#calwebb-detector1) applies basic detector-level corrections to all exposure types (imaging, spectroscopic, coronagraphic, etc.). It is applied to one exposure at a time, beginning with an uncalibrated multiaccum ramp (*_uncal.fits file*). It is sometimes referred to as “ramps-to-slopes” processing. \n",
+    "The [Stage 1 pipeline](https://jwst-pipeline.readthedocs.io/en/stable/jwst/pipeline/calwebb_detector1.html#calwebb-detector1) applies basic detector-level corrections to all exposure types (imaging, spectroscopic, coronagraphic, etc.). It is applied to one exposure at a time, beginning with an uncalibrated multiaccum ramp (*_uncal.fits file*). It is sometimes referred to as \u201cramps-to-slopes\u201d processing. \n",
     "\n",
     "Each input raw data file is composed of one or more ramps (integrations) containing increasing count values from the non-destructive detector readouts. For details on multiaccum files and data collection, see the JDox page on [how up-the-ramp readouts work](https://jwst-docs.stsci.edu/understanding-exposure-times#UnderstandingExposureTimes-uptherampHowup-the-rampreadoutswork).\n",
     "\n",
@@ -3363,9 +3363,9 @@
  ],
  "metadata": {
   "kernelspec": {
-   "display_name": "Python 3",
+   "display_name": "JWebbinar",
    "language": "python",
-   "name": "python3"
+   "name": "jwebbinar"
   },
   "language_info": {
    "codemirror_mode": {
@@ -3382,4 +3382,4 @@
  },
  "nbformat": 4,
  "nbformat_minor": 4
-}
+}
diff --git a/imaging_mode/imaging_mode_stage_1_live.ipynb b/imaging_mode/imaging_mode_stage_1_live.ipynb
@@ -70,7 +70,7 @@
     "\n",
     "This notebook covers part 1 of the imaging mode data calibration module. In this notebook we'll review Stage 1 of the JWST calibration pipeline, also known as *calwebb_detector1*. \n",
     "\n",
-    "The [Stage 1 pipeline](https://jwst-pipeline.readthedocs.io/en/stable/jwst/pipeline/calwebb_detector1.html#calwebb-detector1) applies basic detector-level corrections to all exposure types (imaging, spectroscopic, coronagraphic, etc.). It is applied to one exposure at a time, beginning with an uncalibrated multiaccum ramp (*_uncal.fits file*). It is sometimes referred to as “ramps-to-slopes” processing. \n",
+    "The [Stage 1 pipeline](https://jwst-pipeline.readthedocs.io/en/stable/jwst/pipeline/calwebb_detector1.html#calwebb-detector1) applies basic detector-level corrections to all exposure types (imaging, spectroscopic, coronagraphic, etc.). It is applied to one exposure at a time, beginning with an uncalibrated multiaccum ramp (*_uncal.fits file*). It is sometimes referred to as \u201cramps-to-slopes\u201d processing. \n",
     "\n",
     "Each input raw data file is composed of one or more ramps (integrations) containing increasing count values from the non-destructive detector readouts. For details on multiaccum files and data collection, see the JDox page on [how up-the-ramp readouts work](https://jwst-docs.stsci.edu/understanding-exposure-times#UnderstandingExposureTimes-uptherampHowup-the-rampreadoutswork).\n",
     "\n",
@@ -3282,9 +3282,9 @@
  ],
  "metadata": {
   "kernelspec": {
-   "display_name": "Python 3",
+   "display_name": "JWebbinar",
    "language": "python",
-   "name": "python3"
+   "name": "jwebbinar"
   },
   "language_info": {
    "codemirror_mode": {
@@ -3301,4 +3301,4 @@
  },
  "nbformat": 4,
  "nbformat_minor": 4
-}
+}
diff --git a/imaging_mode/imaging_mode_stage_2.ipynb b/imaging_mode/imaging_mode_stage_2.ipynb
@@ -1925,9 +1925,9 @@
  ],
  "metadata": {
   "kernelspec": {
-   "display_name": "Python 3",
+   "display_name": "JWebbinar",
    "language": "python",
-   "name": "python3"
+   "name": "jwebbinar"
   },
   "language_info": {
    "codemirror_mode": {
@@ -1944,4 +1944,4 @@
  },
  "nbformat": 4,
  "nbformat_minor": 4
-}
+}
diff --git a/imaging_mode/imaging_mode_stage_2_live.ipynb b/imaging_mode/imaging_mode_stage_2_live.ipynb
@@ -1849,9 +1849,9 @@
  ],
  "metadata": {
   "kernelspec": {
-   "display_name": "Python 3",
+   "display_name": "JWebbinar",
    "language": "python",
-   "name": "python3"
+   "name": "jwebbinar"
   },
   "language_info": {
    "codemirror_mode": {
@@ -1868,4 +1868,4 @@
  },
  "nbformat": 4,
  "nbformat_minor": 4
-}
+}
diff --git a/imaging_mode/imaging_mode_stage_3.ipynb b/imaging_mode/imaging_mode_stage_3.ipynb
@@ -2425,9 +2425,9 @@
  ],
  "metadata": {
   "kernelspec": {
-   "display_name": "Python 3",
+   "display_name": "JWebbinar",
    "language": "python",
-   "name": "python3"
+   "name": "jwebbinar"
   },
   "language_info": {
    "codemirror_mode": {
@@ -2444,4 +2444,4 @@
  },
  "nbformat": 4,
  "nbformat_minor": 4
-}
+}
diff --git a/imaging_mode/imaging_mode_stage_3_live.ipynb b/imaging_mode/imaging_mode_stage_3_live.ipynb
@@ -2333,9 +2333,9 @@
  ],
  "metadata": {
   "kernelspec": {
-   "display_name": "Python 3",
+   "display_name": "JWebbinar",
    "language": "python",
-   "name": "python3"
+   "name": "jwebbinar"
   },
   "language_info": {
    "codemirror_mode": {
@@ -2352,4 +2352,4 @@
  },
  "nbformat": 4,
  "nbformat_minor": 4
-}
+}