mirror of
https://github.com/AllenDowney/AstronomicalData.git
synced 2026-01-07 01:53:27 -08:00
Updating
This commit is contained in:
@@ -141,7 +141,11 @@
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{
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"cell_type": "code",
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"execution_count": 1,
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"metadata": {},
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"metadata": {
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"tags": [
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"hide-cell"
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]
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},
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"outputs": [],
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"source": [
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"# If we're running on Colab, install libraries\n",
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@@ -194,9 +198,7 @@
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"cell_type": "markdown",
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"metadata": {},
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"source": [
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"**Optional detail**\n",
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"\n",
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"> Running this import statement has the effect of creating a [TAP+](http://www.ivoa.net/documents/TAP/) connection; TAP stands for \"Table Access Protocol\". It is a network protocol for sending queries to the database and getting back the results. We're not sure why it seems to create two connections."
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"Running this import statement has the effect of creating a [TAP+](http://www.ivoa.net/documents/TAP/) connection; TAP stands for \"Table Access Protocol\". It is a network protocol for sending queries to the database and getting back the results. We're not sure why it seems to create two connections."
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]
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},
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{
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@@ -236,7 +238,11 @@
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{
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"cell_type": "code",
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"execution_count": 4,
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"metadata": {},
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"metadata": {
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"tags": [
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"hide-output"
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]
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},
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"outputs": [
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{
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"name": "stdout",
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@@ -362,7 +368,7 @@
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},
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{
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"cell_type": "code",
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"execution_count": 5,
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"execution_count": 7,
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"metadata": {},
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"outputs": [
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{
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@@ -377,10 +383,10 @@
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{
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"data": {
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"text/plain": [
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"<astroquery.utils.tap.model.taptable.TapTableMeta at 0x7f922376e0a0>"
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"<astroquery.utils.tap.model.taptable.TapTableMeta at 0x7fb565288520>"
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]
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},
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"execution_count": 5,
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"execution_count": 7,
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"metadata": {},
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"output_type": "execute_result"
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}
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@@ -437,6 +443,27 @@
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"What happens? Is the error message helpful? If you had not made this error deliberately, would you have been able to figure it out?"
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]
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},
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{
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"cell_type": "code",
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"execution_count": null,
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"metadata": {},
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"outputs": [],
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"source": [
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"# Solution\n",
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"\n",
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"# The error message, last time we tried, was\n",
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"\n",
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"# Retrieving table 'gaiadr2.gaiadr2.gaia_source'\n",
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"# 500 Error 500:\n",
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"# esavo.tap.TAPException: esavo.tap.TAPException: Schema cannot be null\n",
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"\n",
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"# Which is not remotely helpful.\n",
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"\n",
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"# The point of this exercise is to alert the participants to the difficulty\n",
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"# of debugging queries with VERY limited feedback. So developing and testing\n",
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"# incrementally is very important."
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]
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},
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{
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"cell_type": "markdown",
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"metadata": {},
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@@ -449,7 +476,11 @@
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{
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"cell_type": "code",
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"execution_count": 7,
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"metadata": {},
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"metadata": {
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"tags": [
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"hide-output"
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]
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},
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"outputs": [
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{
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"name": "stdout",
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@@ -581,7 +612,11 @@
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{
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"cell_type": "code",
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"execution_count": 8,
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"metadata": {},
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"metadata": {
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"tags": [
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"remove-cell"
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]
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},
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"outputs": [
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{
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"name": "stdout",
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@@ -670,7 +705,11 @@
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{
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"cell_type": "code",
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"execution_count": 9,
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"metadata": {},
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"metadata": {
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"tags": [
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"hide-cell"
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]
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},
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"outputs": [
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{
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"name": "stdout",
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@@ -1166,7 +1205,11 @@
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{
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"cell_type": "code",
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"execution_count": 18,
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"metadata": {},
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"metadata": {
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"tags": [
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"hide-cell"
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]
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},
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"outputs": [],
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"source": [
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"# Solution\n",
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@@ -1184,7 +1227,11 @@
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{
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"cell_type": "code",
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"execution_count": 19,
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"metadata": {},
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"metadata": {
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"tags": [
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"hide-cell"
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]
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},
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"outputs": [],
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"source": [
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"# Solution\n",
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@@ -1507,7 +1554,11 @@
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{
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"cell_type": "code",
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"execution_count": 29,
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"metadata": {},
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"metadata": {
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"tags": [
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"hide-cell"
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]
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},
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"outputs": [],
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"source": [
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"# Solution\n",
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@@ -1523,7 +1574,11 @@
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{
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"cell_type": "code",
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"execution_count": 30,
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"metadata": {},
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"metadata": {
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"tags": [
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"hide-cell"
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]
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},
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"outputs": [
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{
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"name": "stdout",
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@@ -167,7 +167,7 @@
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"\n",
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"Selecting stars with `bp-rp` less than 2 excludes many class M dwarf stars, which are low temperature, low luminosity. A star like that at GD-1's distance would be hard to detect, so if it is detected, it it more likely to be in the foreground.\n",
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"\n",
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"Now, to select stars with the age and metal richness we expect in GD-1, we will use `g − i` color and apparent `g`-band magnitude, which are available from the Pan-STARRS survey."
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"Now, to select stars with the age and metal richness we expect in GD-1, we will use `g - i` color and apparent `g`-band magnitude, which are available from the Pan-STARRS survey."
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]
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},
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{
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