Fix: remove transition at start

GreenBankObservatory · Dec 2, 2024 · a3fad4d · a3fad4d
1 parent 7a76692
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Showing 8 changed files with 9 additions and 26 deletions.
diff --git a/notebooks/examples/dataIO.ipynb b/notebooks/examples/dataIO.ipynb
@@ -757,7 +757,7 @@
    "name": "python",
    "nbconvert_exporter": "python",
    "pygments_lexer": "ipython3",
-   "version": "3.9.0"
+   "version": "3.10.0"
   }
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  "nbformat": 4,

diff --git a/notebooks/examples/flagging.ipynb b/notebooks/examples/flagging.ipynb
@@ -7,8 +7,6 @@
    "source": [
     "# Flagging\n",
     "\n",
-    "---\n",
-    "\n",
     "This guide shows how to use flags in `dysh`."
    ]
   },
@@ -406,11 +404,7 @@
     {
      "data": {
       "text/plain": [
-<<<<<<< HEAD
        "<matplotlib.image.AxesImage at 0x7a1f60d0ca10>"
-=======
-       "<matplotlib.image.AxesImage at 0x7f1466ba53c0>"
->>>>>>> 4320e16 (Add: how to properly clear flags)
       ]
      },
      "execution_count": 10,
@@ -466,11 +460,6 @@
    ]
   },
   {
-<<<<<<< HEAD
-   "cell_type": "code",
-   "execution_count": null,
-   "id": "b00993ae-a385-4293-9182-f34bd18432b3",
-=======
    "cell_type": "markdown",
    "id": "2debf76f-0a0d-4062-b23d-00c02d4ada5c",
    "metadata": {},
@@ -504,7 +493,6 @@
    "cell_type": "code",
    "execution_count": null,
    "id": "4bb26ea3-602a-4e72-96df-87235c29105c",
->>>>>>> 4320e16 (Add: how to properly clear flags)
    "metadata": {},
    "outputs": [],
    "source": []
@@ -526,7 +514,7 @@
    "name": "python",
    "nbconvert_exporter": "python",
    "pygments_lexer": "ipython3",
-   "version": "3.11.7"
+   "version": "3.10.0"
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diff --git a/notebooks/examples/frequencyswitch.ipynb b/notebooks/examples/frequencyswitch.ipynb
@@ -6,7 +6,6 @@
    "metadata": {},
    "source": [
     "# Frequency-switched Data Reduction\n",
-    "-----------------------------------\n",
     "\n",
     "This notebook shows how to use `dysh` to calibrate a frequency switched observations. The idea is similar to an OnOff observation, except the telescope does not move to an Off in position on the sky, but moves its intermediate frequency in frequency space. Here we call the On and Off the Sig and Ref, but both will have the signal, just shifted in the band. Since the telescope is always tracking the target, combining the Sig and a shifted (folded) Ref, a $\\sqrt{2}$ improvement in signal-to-noise can be achieved.\n",
     "\n",
@@ -724,7 +723,7 @@
    "name": "python",
    "nbconvert_exporter": "python",
    "pygments_lexer": "ipython3",
-   "version": "3.9.0"
+   "version": "3.10.0"
   },
   "toc": {
    "base_numbering": 0

diff --git a/notebooks/examples/nodding.ipynb b/notebooks/examples/nodding.ipynb
@@ -6,7 +6,6 @@
    "metadata": {},
    "source": [
     "# Nodding Data Reduction\n",
-    "------------------------\n",
     "\n",
     "This notebook shows the reduction path of a nodding observation in a multi-beam receiver.\n",
     "\n",
@@ -558,7 +557,7 @@
    "name": "python",
    "nbconvert_exporter": "python",
    "pygments_lexer": "ipython3",
-   "version": "3.12.4"
+   "version": "3.10.0"
   }
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  "nbformat": 4,

diff --git a/notebooks/examples/positionswitch.ipynb b/notebooks/examples/positionswitch.ipynb
@@ -6,7 +6,6 @@
    "metadata": {},
    "source": [
     "# Position-Switched Data Reduction\n",
-    "----------------------------------\n",
     "\n",
     "This notebook shows how to use `dysh` to calibrate an OnOff observation.\n",
     "It retrieves and calibrates position-switch scans using `GBTFITSLoad.getps()`, which returns a `ScanBlock` object.  OffOn observations can be reduced the same way."
@@ -929,7 +928,7 @@
    "name": "python",
    "nbconvert_exporter": "python",
    "pygments_lexer": "ipython3",
-   "version": "3.9.0"
+   "version": "3.10.0"
   },
   "toc": {
    "base_numbering": 0

diff --git a/notebooks/examples/smoothing.ipynb b/notebooks/examples/smoothing.ipynb
@@ -6,7 +6,6 @@
    "metadata": {},
    "source": [
     "# Smoothing\n",
-    "-----------\n",
     "\n",
     "This notebook shows how to use `dysh` to smooth a spectrum.   For the example below we will use data from the Position-Switch example. The following dysh commands are the simplest to get and smooth a spectrum (leaving out all the function arguments):\n",
     "\n",
@@ -793,7 +792,7 @@
    "name": "python",
    "nbconvert_exporter": "python",
    "pygments_lexer": "ipython3",
-   "version": "3.9.0"
+   "version": "3.10.0"
   },
   "toc": {
    "base_numbering": 0

diff --git a/notebooks/examples/subbeamnod.ipynb b/notebooks/examples/subbeamnod.ipynb
@@ -6,7 +6,7 @@
    "metadata": {},
    "source": [
     "# SubBeamNod Data Reduction\n",
-    "---------------------------\n",
+    "\n",
     "This notebook shows how to use `dysh` to calibrate an SubBeamNod observation via two different methods. It retrieves and calibrates SubBeamNod scans using `GBTFITSLoad.subbeamnod()` which returns a `ScanBlock` object. "
    ]
   },
@@ -493,7 +493,7 @@
    "name": "python",
    "nbconvert_exporter": "python",
    "pygments_lexer": "ipython3",
-   "version": "3.9.0"
+   "version": "3.10.0"
   }
  },
  "nbformat": 4,

diff --git a/notebooks/examples/velocity_frames.ipynb b/notebooks/examples/velocity_frames.ipynb
@@ -6,7 +6,6 @@
    "metadata": {},
    "source": [
     "# Spectral Axes, Velocity Frames and Conventions in `dysh`\n",
-    "----------------------------------\n",
     "\n",
     "This notebook shows how to change spectral axes to represent different rest frames and Doppler conventions."
    ]
@@ -877,7 +876,7 @@
    "name": "python",
    "nbconvert_exporter": "python",
    "pygments_lexer": "ipython3",
-   "version": "3.9.0"
+   "version": "3.10.0"
   },
   "toc": {
    "base_numbering": 0