From 3d3b195cb31db05e4c71a5049ba7bd32860c1c8c Mon Sep 17 00:00:00 2001 From: EC2 Default User Date: Mon, 17 May 2021 14:40:24 +0000 Subject: [PATCH] update kernels --- jdat_session/Cubeviz_Webbinar_live.ipynb | 6 +++--- jdat_session/Cubeviz_Webbinar_solutions.ipynb | 6 +++--- jdat_session/MosvizJwebbinarDemo-live.ipynb | 6 +++--- jdat_session/MosvizJwebbinarDemo-solutions.ipynb | 6 +++--- jdat_session/Specutils_Webbinar_live.ipynb | 8 ++++---- jdat_session/Specutils_Webbinar_solutions.ipynb | 8 ++++---- jdat_session/Specviz_Webbinar_live.ipynb | 6 +++--- jdat_session/Specviz_Webbinar_solutions.ipynb | 6 +++--- 8 files changed, 26 insertions(+), 26 deletions(-) diff --git a/jdat_session/Cubeviz_Webbinar_live.ipynb b/jdat_session/Cubeviz_Webbinar_live.ipynb index 9cd8550..36ff8e6 100644 --- a/jdat_session/Cubeviz_Webbinar_live.ipynb +++ b/jdat_session/Cubeviz_Webbinar_live.ipynb @@ -387,9 +387,9 @@ ], "metadata": { "kernelspec": { - "display_name": "Python 3", + "display_name": "Jdaviz", "language": "python", - "name": "python3" + "name": "jdaviz" }, "language_info": { "codemirror_mode": { @@ -406,4 +406,4 @@ }, "nbformat": 4, "nbformat_minor": 4 -} +} \ No newline at end of file diff --git a/jdat_session/Cubeviz_Webbinar_solutions.ipynb b/jdat_session/Cubeviz_Webbinar_solutions.ipynb index d8d555c..8c765f8 100644 --- a/jdat_session/Cubeviz_Webbinar_solutions.ipynb +++ b/jdat_session/Cubeviz_Webbinar_solutions.ipynb @@ -371,9 +371,9 @@ ], "metadata": { "kernelspec": { - "display_name": "Python 3", + "display_name": "Jdaviz", "language": "python", - "name": "python3" + "name": "jdaviz" }, "language_info": { "codemirror_mode": { @@ -390,4 +390,4 @@ }, "nbformat": 4, "nbformat_minor": 4 -} +} \ No newline at end of file diff --git a/jdat_session/MosvizJwebbinarDemo-live.ipynb b/jdat_session/MosvizJwebbinarDemo-live.ipynb index 0e95f7c..4ae133f 100644 --- a/jdat_session/MosvizJwebbinarDemo-live.ipynb +++ b/jdat_session/MosvizJwebbinarDemo-live.ipynb @@ -143,9 +143,9 @@ ], "metadata": { "kernelspec": { - "display_name": "Python 3", + "display_name": "Jdaviz", "language": "python", - "name": "python3" + "name": "jdaviz" }, "language_info": { "codemirror_mode": { @@ -162,4 +162,4 @@ }, "nbformat": 4, "nbformat_minor": 4 -} +} \ No newline at end of file diff --git a/jdat_session/MosvizJwebbinarDemo-solutions.ipynb b/jdat_session/MosvizJwebbinarDemo-solutions.ipynb index fb9d12a..8635871 100644 --- a/jdat_session/MosvizJwebbinarDemo-solutions.ipynb +++ b/jdat_session/MosvizJwebbinarDemo-solutions.ipynb @@ -174,9 +174,9 @@ ], "metadata": { "kernelspec": { - "display_name": "Python 3", + "display_name": "Jdaviz", "language": "python", - "name": "python3" + "name": "jdaviz" }, "language_info": { "codemirror_mode": { @@ -193,4 +193,4 @@ }, "nbformat": 4, "nbformat_minor": 4 -} +} \ No newline at end of file diff --git a/jdat_session/Specutils_Webbinar_live.ipynb b/jdat_session/Specutils_Webbinar_live.ipynb index a64c7e1..cf1df49 100644 --- a/jdat_session/Specutils_Webbinar_live.ipynb +++ b/jdat_session/Specutils_Webbinar_live.ipynb @@ -653,7 +653,7 @@ "cell_type": "markdown", "metadata": {}, "source": [ - "Suppose you wanted to compare some of the above line measurements to a relatively local galaxy that has known line Hα line fluxes - say, some galaxy you know to be at 100 Mpc. How can you do this comparison in just a few lines of code? (Hint: making use of the units in the ``line_flux(...)`` outputs and [astropy.cosmology](https://docs.astropy.org/en/stable/cosmology/index.html) are your friends here!) If you'd like to try this with some real data, you might compare to a ground-based spectrum of a local emission line galaxy, [like the SDSS](https://dr14.sdss.org/optical/spectrum/view/data/format=fits/spec=lite?plateid=1323&mjd=52797&fiberid=12)." + "Suppose you wanted to compare some of the above line measurements to a relatively local galaxy that has known line H\u03b1 line fluxes - say, some galaxy you know to be at 100 Mpc. How can you do this comparison in just a few lines of code? (Hint: making use of the units in the ``line_flux(...)`` outputs and [astropy.cosmology](https://docs.astropy.org/en/stable/cosmology/index.html) are your friends here!) If you'd like to try this with some real data, you might compare to a ground-based spectrum of a local emission line galaxy, [like the SDSS](https://dr14.sdss.org/optical/spectrum/view/data/format=fits/spec=lite?plateid=1323&mjd=52797&fiberid=12)." ] }, { @@ -976,9 +976,9 @@ ], "metadata": { "kernelspec": { - "display_name": "Python 3", + "display_name": "Jdaviz", "language": "python", - "name": "python3" + "name": "jdaviz" }, "language_info": { "codemirror_mode": { @@ -995,4 +995,4 @@ }, "nbformat": 4, "nbformat_minor": 4 -} +} \ No newline at end of file diff --git a/jdat_session/Specutils_Webbinar_solutions.ipynb b/jdat_session/Specutils_Webbinar_solutions.ipynb index 5389b82..7c2e053 100644 --- a/jdat_session/Specutils_Webbinar_solutions.ipynb +++ b/jdat_session/Specutils_Webbinar_solutions.ipynb @@ -822,7 +822,7 @@ "cell_type": "markdown", "metadata": {}, "source": [ - "Suppose you wanted to compare some of the above line measurements to a relatively local galaxy that has known line Hα line fluxes - say, some galaxy you know to be at 100 Mpc. How can you do this comparison in just a few lines of code? (Hint: making use of the units in the ``line_flux(...)`` outputs and [astropy.cosmology](https://docs.astropy.org/en/stable/cosmology/index.html) are your friends here!) If you'd like to try this with some real data, you might compare to a ground-based spectrum of a local emission line galaxy, [like the SDSS](https://dr14.sdss.org/optical/spectrum/view/data/format=fits/spec=lite?plateid=1323&mjd=52797&fiberid=12)." + "Suppose you wanted to compare some of the above line measurements to a relatively local galaxy that has known line H\u03b1 line fluxes - say, some galaxy you know to be at 100 Mpc. How can you do this comparison in just a few lines of code? (Hint: making use of the units in the ``line_flux(...)`` outputs and [astropy.cosmology](https://docs.astropy.org/en/stable/cosmology/index.html) are your friends here!) If you'd like to try this with some real data, you might compare to a ground-based spectrum of a local emission line galaxy, [like the SDSS](https://dr14.sdss.org/optical/spectrum/view/data/format=fits/spec=lite?plateid=1323&mjd=52797&fiberid=12)." ] }, { @@ -1251,9 +1251,9 @@ ], "metadata": { "kernelspec": { - "display_name": "Python (astro)", + "display_name": "Jdaviz", "language": "python", - "name": "astro" + "name": "jdaviz" }, "language_info": { "codemirror_mode": { @@ -1270,4 +1270,4 @@ }, "nbformat": 4, "nbformat_minor": 4 -} +} \ No newline at end of file diff --git a/jdat_session/Specviz_Webbinar_live.ipynb b/jdat_session/Specviz_Webbinar_live.ipynb index ffb97c5..80fb010 100644 --- a/jdat_session/Specviz_Webbinar_live.ipynb +++ b/jdat_session/Specviz_Webbinar_live.ipynb @@ -243,9 +243,9 @@ ], "metadata": { "kernelspec": { - "display_name": "Python 3", + "display_name": "Jdaviz", "language": "python", - "name": "python3" + "name": "jdaviz" }, "language_info": { "codemirror_mode": { @@ -275,4 +275,4 @@ }, "nbformat": 4, "nbformat_minor": 4 -} +} \ No newline at end of file diff --git a/jdat_session/Specviz_Webbinar_solutions.ipynb b/jdat_session/Specviz_Webbinar_solutions.ipynb index f0a3735..16328ec 100644 --- a/jdat_session/Specviz_Webbinar_solutions.ipynb +++ b/jdat_session/Specviz_Webbinar_solutions.ipynb @@ -323,9 +323,9 @@ ], "metadata": { "kernelspec": { - "display_name": "Python 3", + "display_name": "Jdaviz", "language": "python", - "name": "python3" + "name": "jdaviz" }, "language_info": { "codemirror_mode": { @@ -355,4 +355,4 @@ }, "nbformat": 4, "nbformat_minor": 4 -} +} \ No newline at end of file