Remove flake8 checks from NB 06.

Author: jeffcarlin

06_Comparing_Object_and_Truth_Tables.ipynb

@@ -2,7 +2,7 @@
  "cells": [
   {
    "cell_type": "markdown",
-   "id": "1759f339",
+   "id": "f57b0a8f",
    "metadata": {},
    "source": [
     "<img align=\"left\" src = https://project.lsst.org/sites/default/files/Rubin-O-Logo_0.png width=250 style=\"padding: 10px\"> \n",
@@ -27,18 +27,7 @@
   {
    "cell_type": "code",
    "execution_count": null,
-   "id": "0fb84c0f",
-   "metadata": {},
-   "outputs": [],
-   "source": [
-    "%load_ext pycodestyle_magic\n",
-    "%flake8_on"
-   ]
-  },
-  {
-   "cell_type": "code",
-   "execution_count": null,
-   "id": "b8440bfb",
+   "id": "de133e88",
    "metadata": {},
    "outputs": [],
    "source": [
@@ -49,7 +38,7 @@
   },
   {
    "cell_type": "markdown",
-   "id": "8f5588ba",
+   "id": "06717364",
    "metadata": {},
    "source": [
     "### 1. Import Common Python Libraries\n",
@@ -60,7 +49,7 @@
   {
    "cell_type": "code",
    "execution_count": null,
-   "id": "26b0e88a",
+   "id": "4249d4a4",
    "metadata": {},
    "outputs": [],
    "source": [
@@ -72,7 +61,7 @@
   },
   {
    "cell_type": "markdown",
-   "id": "a3d3f763",
+   "id": "e165773f",
    "metadata": {},
    "source": [
     "To access tables, we will use the TAP service in a similar manner to what we showed in the [Intro to DP0 notebook](https://github.com/rubin-dp0/tutorial-notebooks/blob/main/01_Intro_to_DP0_Notebooks.ipynb), and explored further in THE TAP TUTORIAL NOTEBOOK. See those notebooks for more details."
@@ -81,7 +70,7 @@
   {
    "cell_type": "code",
    "execution_count": null,
-   "id": "b61e4b80",
+   "id": "06c690d4",
    "metadata": {},
    "outputs": [],
    "source": [
@@ -98,7 +87,7 @@
   },
   {
    "cell_type": "markdown",
-   "id": "641ab974",
+   "id": "b37dee2b",
    "metadata": {},
    "source": [
     "### 2. Loading tables with TAP\n",
@@ -109,7 +98,7 @@
   {
    "cell_type": "code",
    "execution_count": null,
-   "id": "92702829",
+   "id": "75f87bac",
    "metadata": {},
    "outputs": [],
    "source": [
@@ -120,7 +109,7 @@
   },
   {
    "cell_type": "markdown",
-   "id": "139987d9",
+   "id": "e20bb66c",
    "metadata": {},
    "source": [
     "For our analysis, let's choose the Object table, `dp01_dc2_catalogs.object`, and then we will compare the measurements from this table to the \"truth\" values from `dp01_dc2_catalogs.truth_match`.\n",
@@ -131,7 +120,7 @@
   {
    "cell_type": "code",
    "execution_count": null,
-   "id": "875932e6",
+   "id": "4132e8ba",
    "metadata": {},
    "outputs": [],
    "source": [
@@ -146,7 +135,7 @@
   {
    "cell_type": "code",
    "execution_count": null,
-   "id": "d3b1ca78",
+   "id": "b1b28378",
    "metadata": {},
    "outputs": [],
    "source": [
@@ -160,7 +149,7 @@
   },
   {
    "cell_type": "markdown",
-   "id": "44694725",
+   "id": "cb9b1bc2",
    "metadata": {},
    "source": [
     "For this exploration, we will select a small region of sky around a random RA, Dec position. The following two cells read data centered on (RA, Dec) = (62.0, -37.0) degrees, within a radius of 0.1 degrees, for first the Object table, then the Truth-Match table. Note that we are selecting only a subset of the columns seen in the schema above. You can add or remove columns as you wish.\n",
@@ -171,7 +160,7 @@
   {
    "cell_type": "code",
    "execution_count": null,
-   "id": "988888bc",
+   "id": "b83f89c3",
    "metadata": {},
    "outputs": [],
    "source": [
@@ -191,7 +180,7 @@
   {
    "cell_type": "code",
    "execution_count": null,
-   "id": "28155cc1",
+   "id": "c1646302",
    "metadata": {},
    "outputs": [],
    "source": [
@@ -211,7 +200,7 @@
   },
   {
    "cell_type": "markdown",
-   "id": "bed44bb2",
+   "id": "2525473b",
    "metadata": {},
    "source": [
     "These tables will be much easier to work with as `pandas` \"dataframes\". The query results have convenient methods that we can use to convert them."
@@ -220,7 +209,7 @@
   {
    "cell_type": "code",
    "execution_count": null,
-   "id": "752c20cf",
+   "id": "11cc80a5",
    "metadata": {},
    "outputs": [],
    "source": [
@@ -230,7 +219,7 @@
   },
   {
    "cell_type": "markdown",
-   "id": "8634dd8f",
+   "id": "0e99f343",
    "metadata": {},
    "source": [
     "### 3. Merge the two tables and compare measurements to truth values\n",
@@ -241,7 +230,7 @@
   {
    "cell_type": "code",
    "execution_count": null,
-   "id": "1a061e45",
+   "id": "f4f7429f",
    "metadata": {},
    "outputs": [],
    "source": [
@@ -265,7 +254,7 @@
   {
    "cell_type": "code",
    "execution_count": null,
-   "id": "04faf39b",
+   "id": "0c220f27",
    "metadata": {},
    "outputs": [],
    "source": [
@@ -275,7 +264,7 @@
   {
    "cell_type": "code",
    "execution_count": null,
-   "id": "1f4fe3f1",
+   "id": "de91c217",
    "metadata": {},
    "outputs": [],
    "source": [
@@ -309,7 +298,7 @@
   },
   {
    "cell_type": "markdown",
-   "id": "11fb6687",
+   "id": "b468299e",
    "metadata": {},
    "source": [
     "#### Compare the measurements from the Object table to the \"true\" values for some objects.\n",
@@ -322,7 +311,7 @@
   {
    "cell_type": "code",
    "execution_count": null,
-   "id": "93a84438",
+   "id": "f619d477",
    "metadata": {},
    "outputs": [],
    "source": [
@@ -332,7 +321,7 @@
   },
   {
    "cell_type": "markdown",
-   "id": "c449af21",
+   "id": "dc470937",
    "metadata": {},
    "source": [
     "Just to confirm that things look like we expect, let's plot a color-magnitude (g vs. g-i) and color-color (r-i vs. g-r) diagram."
@@ -341,7 +330,7 @@
   {
    "cell_type": "code",
    "execution_count": null,
-   "id": "54c9dbda",
+   "id": "a7d08625",
    "metadata": {},
    "outputs": [],
    "source": [
@@ -381,7 +370,7 @@
   },
   {
    "cell_type": "markdown",
-   "id": "70fa4076",
+   "id": "fe125d6b",
    "metadata": {},
    "source": [
     "Looks pretty normal - the stellar locus in color-color space is right where one expects it to be, and the galaxies dominate at the faint end of the CMD. \n",
@@ -392,7 +381,7 @@
   {
    "cell_type": "code",
    "execution_count": null,
-   "id": "c5a6dafb",
+   "id": "caebf863",
    "metadata": {},
    "outputs": [],
    "source": [
@@ -415,7 +404,7 @@
   },
   {
    "cell_type": "markdown",
-   "id": "ded10557",
+   "id": "ffc9043d",
    "metadata": {},
    "source": [
     "Well, that looks good -- the ratio of measured to true fluxes is centered on 1.0. It seems like the fluxes are recovered pretty well, on average.\n",
@@ -426,7 +415,7 @@
   {
    "cell_type": "code",
    "execution_count": null,
-   "id": "b86de3ec",
+   "id": "72ec6e46",
    "metadata": {},
    "outputs": [],
    "source": []