From 921f3b86526e0e62a64e04df34ea5554a1060fcd Mon Sep 17 00:00:00 2001
From: dh00601 <dh00601@surrey.ac.uk>
Date: Tue, 2 Nov 2021 23:52:01 +0000
Subject: [PATCH] updated notebooks to make sure the bulletpoint lists are
formatted properly
---
examples/notebook_BHBH.ipynb | 395 +++---------------
examples/notebook_HRD.ipynb | 4 +-
examples/notebook_api_functionality.ipynb | 4 +-
.../notebook_common_envelope_evolution.ipynb | 21 +-
examples/notebook_custom_logging.ipynb | 13 +-
examples/notebook_extra_features.ipynb | 10 +-
examples/notebook_individual_systems.ipynb | 1 +
...otebook_luminosity_function_binaries.ipynb | 49 ++-
.../notebook_luminosity_function_single.ipynb | 16 +-
examples/notebook_massive_remnants.ipynb | 30 +-
examples/notebook_population.ipynb | 5 +-
examples/notebook_solar_system.ipynb | 18 +-
12 files changed, 158 insertions(+), 408 deletions(-)
diff --git a/examples/notebook_BHBH.ipynb b/examples/notebook_BHBH.ipynb
index 80b707d95..4afd498b9 100644
--- a/examples/notebook_BHBH.ipynb
+++ b/examples/notebook_BHBH.ipynb
@@ -5,27 +5,8 @@
"id": "a544d28c-c2e1-4c6a-b55b-8caec440743f",
"metadata": {},
"source": [
- "# Tutorial: Running individual systems with binary_c-python\n",
- "This notebook will show you how to run single systems and analyze their results.\n",
- "\n",
- "It can be useful to have some functions to quickly run a single system to, for example, inspect what evolutionary steps a specific system goes through, to plot the mass loss evolution of a single system, etc. "
- ]
- },
- {
- "cell_type": "markdown",
- "id": "dd5d9ec7-5791-45f1-afbd-225947e2a583",
- "metadata": {
- "tags": []
- },
- "source": [
- "## Single system with run_system_wrapper\n",
- "\n",
- "The simplest method to run a single system is to use the run_system wrapper. This function deals with setting up the argument string, makes sure all the required parameters are included and handles setting and cleaning up the custom logging functionality (see notebook_custom_logging).\n",
- "\n",
- "As arguments to this function we can add any of the parameters that binary_c itself actually knows, as well as:\n",
- "- custom_logging_code: string containing a Printf statement that binary_c can use to print information\n",
- "- log_filename: path of the logfile that binary_c generates\n",
- "- parse_function: function that handles parsing the output of binary-c"
+ "# Example use case: Binary black hole systems\n",
+ "TODO: introduce the notebook\n"
]
},
{
@@ -91,7 +72,13 @@
"cell_type": "code",
"execution_count": 3,
"id": "029fc3f2-f09a-49af-a32b-248505738f2e",
- "metadata": {},
+ "metadata": {
+ "collapsed": true,
+ "jupyter": {
+ "outputs_hidden": true
+ },
+ "tags": []
+ },
"outputs": [
{
"name": "stdout",
@@ -288,13 +275,7 @@
" 7.4046 9.501 9.586 14 14 -102.91 -1 -1.00 0.000 0.000 SN kick Ib/c (SN type 11 11, pre-explosion M=10.0399 Mc\"CO\"=7.43173 type=8) -> kick 1(190) vk=384.535 vr=0 omega=3.4205 phi=-0.103702 -> vn=384.535 ; final sep -102.908 ecc -1 (random count 5) - Runaway v=(-379.582,-106.329,10.8544) |v|=384.535 : companion v=(-5.13796e-51,-1.27569e-103,2.85406e-105), |v|=5.13796e-51 ; - , dm(exploder) = 0.454268, dm(companion) = 0\n",
" 7.4046 9.501 9.586 14 14 -102.91 -1 -1.00 0.000 0.000 \"TYPE_CHNGE\"\n",
" 7.4046 9.501 9.586 14 14 -102.91 -1 -1.00 0.000 0.000 \"SN\"\n",
- " 15000.0000 9.501 9.586 14 14 -102.91 -1 -1.00 0.000 0.000 \"MAX_TIME\"\n"
- ]
- },
- {
- "name": "stdout",
- "output_type": "stream",
- "text": [
+ " 15000.0000 9.501 9.586 14 14 -102.91 -1 -1.00 0.000 0.000 \"MAX_TIME\"\n",
"\n"
]
}
@@ -376,7 +357,13 @@
"cell_type": "code",
"execution_count": 5,
"id": "8018ef52-093d-45ac-a00b-5fb721db3adb",
- "metadata": {},
+ "metadata": {
+ "collapsed": true,
+ "jupyter": {
+ "outputs_hidden": true
+ },
+ "tags": []
+ },
"outputs": [
{
"name": "stdout",
@@ -558,13 +545,7 @@
"System 58 has separation -140.9\n",
"system 59 / 100\n",
"{'time': 7.4046, 'M1': 5.851, 'M2': 5.873, 'K1': 14.0, 'K2': 14.0, 'separation': -2439.0}\n",
- "System 59 has separation -2439.0\n"
- ]
- },
- {
- "name": "stdout",
- "output_type": "stream",
- "text": [
+ "System 59 has separation -2439.0\n",
"system 60 / 100\n",
"{'time': 7.4046, 'M1': 5.851, 'M2': 5.873, 'K1': 14.0, 'K2': 14.0, 'separation': -235.82}\n",
"System 60 has separation -235.82\n",
@@ -742,7 +723,13 @@
"cell_type": "code",
"execution_count": 6,
"id": "3085ba82-430e-48f0-bca3-b19231e6109d",
- "metadata": {},
+ "metadata": {
+ "collapsed": true,
+ "jupyter": {
+ "outputs_hidden": true
+ },
+ "tags": []
+ },
"outputs": [
{
"name": "stdout",
@@ -944,13 +931,7 @@
" 7.4046 9.501 9.586 14 14 9548.9 67.7 y 0.05 0.000 0.000 \"TYPE_CHNGE\"\n",
" 7.4046 9.501 9.586 14 14 9548.9 67.7 y 0.05 0.000 0.000 \"SN\"\n",
" 7.4146 9.501 9.586 14 14 9548.9 67.7 y 0.05 0.000 0.000 \"END_SYMB\"\n",
- " 15000.0000 9.501 9.586 14 14 9548.9 67.7 y 0.05 0.000 0.000 \"MAX_TIME\"\n"
- ]
- },
- {
- "name": "stdout",
- "output_type": "stream",
- "text": [
+ " 15000.0000 9.501 9.586 14 14 9548.9 67.7 y 0.05 0.000 0.000 \"MAX_TIME\"\n",
"\n"
]
}
@@ -1238,13 +1219,7 @@
" 265.4710 45.203 0.000 14 15 -1 -1 -1.00 0.000 0.000 \"TYPE_CHNGE\"\n",
" 265.4710 45.203 0.000 14 15 -1 -1 -1.00 0.000 0.000 \"COALESCE\"\n",
" 265.4710 45.203 0.000 14 15 -1 -1 -1.00 0.000 0.000 \"SN\"\n",
- " 15000.0000 45.203 0.000 14 15 -1 -1 -1.00 0.000 0.000 \"MAX_TIME\"\n"
- ]
- },
- {
- "name": "stdout",
- "output_type": "stream",
- "text": [
+ " 15000.0000 45.203 0.000 14 15 -1 -1 -1.00 0.000 0.000 \"MAX_TIME\"\n",
"\n",
"{'M_1': 60, 'M_2': 40, 'metallicity': 0.001, 'orbital_period': 2000, 'BH_prescription': 'BH_BELCZYNSKI', 'wind_mass_loss': 'WIND_ALGORITHM_NONE', 'alpha_ce': 0.1}\n",
"system 1 / 100\n",
@@ -1369,13 +1344,7 @@
" 6.1830 26.222 18.898 14 14 94.707 15.9 d 0.58 0.000 0.000 \"TYPE_CHNGE\"\n",
" 6.1830 26.222 18.898 14 14 94.707 15.9 d 0.58 0.000 0.000 \"SN\"\n",
" 6.1830 26.222 18.898 14 14 94.707 15.9 d 0.58 0.000 0.000 \"End tidal lock 2\"\n",
- " 15000.0000 26.222 18.898 14 14 89.066 14.5 d 0.56 0.000 0.000 \"MAX_TIME\"\n"
- ]
- },
- {
- "name": "stdout",
- "output_type": "stream",
- "text": [
+ " 15000.0000 26.222 18.898 14 14 89.066 14.5 d 0.56 0.000 0.000 \"MAX_TIME\"\n",
"\n",
"{'M_1': 60, 'M_2': 40, 'metallicity': 0.001, 'orbital_period': 2000, 'BH_prescription': 'BH_BELCZYNSKI', 'wind_mass_loss': 'WIND_ALGORITHM_NONE', 'alpha_ce': 0.1}\n",
"system 1 / 100\n",
@@ -1505,13 +1474,7 @@
" 83.5556 45.159 0.000 14 15 -1 -1 -1.00 0.000 0.000 \"TYPE_CHNGE\"\n",
" 83.5556 45.159 0.000 14 15 -1 -1 -1.00 0.000 0.000 \"COALESCE\"\n",
" 83.5556 45.159 0.000 14 15 -1 -1 -1.00 0.000 0.000 \"SN\"\n",
- " 15000.0000 45.159 0.000 14 15 -1 -1 -1.00 0.000 0.000 \"MAX_TIME\"\n"
- ]
- },
- {
- "name": "stdout",
- "output_type": "stream",
- "text": [
+ " 15000.0000 45.159 0.000 14 15 -1 -1 -1.00 0.000 0.000 \"MAX_TIME\"\n",
"\n",
"{'M_1': 60, 'M_2': 40, 'metallicity': 0.001, 'orbital_period': 2000, 'BH_prescription': 'BH_BELCZYNSKI', 'wind_mass_loss': 'WIND_ALGORITHM_NONE', 'alpha_ce': 0.1}\n",
"system 1 / 100\n",
@@ -1594,13 +1557,7 @@
" 1473.7324 45.249 0.000 14 15 -1 -1 -1.00 0.000 0.000 \"TYPE_CHNGE\"\n",
" 1473.7324 45.249 0.000 14 15 -1 -1 -1.00 0.000 0.000 \"COALESCE\"\n",
" 1473.7324 45.249 0.000 14 15 -1 -1 -1.00 0.000 0.000 \"SN\"\n",
- " 15000.0000 45.249 0.000 14 15 -1 -1 -1.00 0.000 0.000 \"MAX_TIME\"\n"
- ]
- },
- {
- "name": "stdout",
- "output_type": "stream",
- "text": [
+ " 15000.0000 45.249 0.000 14 15 -1 -1 -1.00 0.000 0.000 \"MAX_TIME\"\n",
"\n",
"{'M_1': 60, 'M_2': 40, 'metallicity': 0.001, 'orbital_period': 2000, 'BH_prescription': 'BH_BELCZYNSKI', 'wind_mass_loss': 'WIND_ALGORITHM_NONE', 'alpha_ce': 0.1}\n",
"system 1 / 100\n",
@@ -1739,13 +1696,7 @@
" 112.8805 45.090 0.000 14 15 -1 -1 -1.00 0.000 0.000 \"TYPE_CHNGE\"\n",
" 112.8805 45.090 0.000 14 15 -1 -1 -1.00 0.000 0.000 \"COALESCE\"\n",
" 112.8805 45.090 0.000 14 15 -1 -1 -1.00 0.000 0.000 \"SN\"\n",
- " 15000.0000 45.090 0.000 14 15 -1 -1 -1.00 0.000 0.000 \"MAX_TIME\"\n"
- ]
- },
- {
- "name": "stdout",
- "output_type": "stream",
- "text": [
+ " 15000.0000 45.090 0.000 14 15 -1 -1 -1.00 0.000 0.000 \"MAX_TIME\"\n",
"\n",
"{'M_1': 60, 'M_2': 40, 'metallicity': 0.001, 'orbital_period': 2000, 'BH_prescription': 'BH_BELCZYNSKI', 'wind_mass_loss': 'WIND_ALGORITHM_NONE', 'alpha_ce': 0.1}\n",
"system 1 / 100\n",
@@ -1813,13 +1764,7 @@
" 12.7426 44.651 0.000 14 15 -1 -1 -1.00 0.000 0.000 \"TYPE_CHNGE\"\n",
" 12.7426 44.651 0.000 14 15 -1 -1 -1.00 0.000 0.000 \"COALESCE\"\n",
" 12.7426 44.651 0.000 14 15 -1 -1 -1.00 0.000 0.000 \"SN\"\n",
- " 15000.0000 44.651 0.000 14 15 -1 -1 -1.00 0.000 0.000 \"MAX_TIME\"\n"
- ]
- },
- {
- "name": "stdout",
- "output_type": "stream",
- "text": [
+ " 15000.0000 44.651 0.000 14 15 -1 -1 -1.00 0.000 0.000 \"MAX_TIME\"\n",
"\n",
"{'M_1': 60, 'M_2': 40, 'metallicity': 0.001, 'orbital_period': 2000, 'BH_prescription': 'BH_BELCZYNSKI', 'wind_mass_loss': 'WIND_ALGORITHM_NONE', 'alpha_ce': 0.1}\n",
"system 1 / 100\n",
@@ -1931,13 +1876,7 @@
" 6.1823 26.223 18.942 14 14 174.23 39.6 d 0.87 0.000 0.000 \"TYPE_CHNGE\"\n",
" 6.1823 26.223 18.942 14 14 174.23 39.6 d 0.87 0.000 0.000 \"SN\"\n",
" 6.1823 26.223 18.942 14 14 174.23 39.6 d 0.87 0.000 0.000 \"End tidal lock 2\"\n",
- " 15000.0000 26.223 18.942 14 14 122 23.2 d 0.82 0.000 0.000 \"MAX_TIME\"\n"
- ]
- },
- {
- "name": "stdout",
- "output_type": "stream",
- "text": [
+ " 15000.0000 26.223 18.942 14 14 122 23.2 d 0.82 0.000 0.000 \"MAX_TIME\"\n",
"\n",
"{'M_1': 60, 'M_2': 40, 'metallicity': 0.001, 'orbital_period': 2000, 'BH_prescription': 'BH_BELCZYNSKI', 'wind_mass_loss': 'WIND_ALGORITHM_NONE', 'alpha_ce': 0.1}\n",
"system 1 / 100\n",
@@ -2016,13 +1955,7 @@
"{'time': 6.1816, 'M1': 26.224, 'M2': 18.995, 'K1': 14.0, 'K2': 14.0, 'separation': -24.872}\n",
"System 7 has separation -24.872\n",
"system 8 / 100\n",
- "{'time': 6.1851, 'M1': 26.215, 'M2': 48.508, 'K1': 14.0, 'K2': 14.0, 'separation': -33.648}\n"
- ]
- },
- {
- "name": "stdout",
- "output_type": "stream",
- "text": [
+ "{'time': 6.1851, 'M1': 26.215, 'M2': 48.508, 'K1': 14.0, 'K2': 14.0, 'separation': -33.648}\n",
"System 8 has separation -33.648\n",
"system 9 / 100\n",
"{'time': 6.1851, 'M1': 26.215, 'M2': 48.508, 'K1': 14.0, 'K2': 14.0, 'separation': -1713.8}\n",
@@ -2137,13 +2070,7 @@
" 6.1810 26.225 19.039 14 14 144 29.7 d 0.62 0.000 0.000 \"TYPE_CHNGE\"\n",
" 6.1810 26.225 19.039 14 14 144 29.7 d 0.62 0.000 0.000 \"SN\"\n",
" 6.1810 26.225 19.039 14 14 144 29.7 d 0.62 0.000 0.000 \"End tidal lock 2\"\n",
- " 15000.0000 26.225 19.039 14 14 141.62 29 d 0.62 0.000 0.000 \"MAX_TIME\"\n"
- ]
- },
- {
- "name": "stdout",
- "output_type": "stream",
- "text": [
+ " 15000.0000 26.225 19.039 14 14 141.62 29 d 0.62 0.000 0.000 \"MAX_TIME\"\n",
"\n",
"{'M_1': 60, 'M_2': 40, 'metallicity': 0.001, 'orbital_period': 2000, 'BH_prescription': 'BH_BELCZYNSKI', 'wind_mass_loss': 'WIND_ALGORITHM_NONE', 'alpha_ce': 0.1}\n",
"system 1 / 100\n",
@@ -2230,13 +2157,7 @@
"system 6 / 100\n",
"None\n",
"system 7 / 100\n",
- "{'time': 6.1851, 'M1': 26.215, 'M2': 48.508, 'K1': 14.0, 'K2': 14.0, 'separation': -62.267}\n"
- ]
- },
- {
- "name": "stdout",
- "output_type": "stream",
- "text": [
+ "{'time': 6.1851, 'M1': 26.215, 'M2': 48.508, 'K1': 14.0, 'K2': 14.0, 'separation': -62.267}\n",
"System 7 has separation -62.267\n",
"system 8 / 100\n",
"{'time': 6.1851, 'M1': 26.215, 'M2': 48.508, 'K1': 14.0, 'K2': 14.0, 'separation': -42.878}\n",
@@ -2345,13 +2266,7 @@
" 6.1825 26.223 18.926 14 14 161.5 35.4 d 0.88 0.000 0.000 \"TYPE_CHNGE\"\n",
" 6.1825 26.223 18.926 14 14 161.5 35.4 d 0.88 0.000 0.000 \"SN\"\n",
" 6.1825 26.223 18.926 14 14 161.5 35.4 d 0.88 0.000 0.000 \"End tidal lock 2\"\n",
- " 15000.0000 26.223 18.926 14 14 75.019 11.2 d 0.76 0.000 0.000 \"MAX_TIME\"\n"
- ]
- },
- {
- "name": "stdout",
- "output_type": "stream",
- "text": [
+ " 15000.0000 26.223 18.926 14 14 75.019 11.2 d 0.76 0.000 0.000 \"MAX_TIME\"\n",
"\n",
"{'M_1': 60, 'M_2': 40, 'metallicity': 0.001, 'orbital_period': 2000, 'BH_prescription': 'BH_BELCZYNSKI', 'wind_mass_loss': 'WIND_ALGORITHM_NONE', 'alpha_ce': 0.1}\n",
"system 1 / 100\n",
@@ -2431,13 +2346,7 @@
"system 6 / 100\n",
"{'time': 6.1851, 'M1': 26.215, 'M2': 48.508, 'K1': 14.0, 'K2': 14.0, 'separation': -106.87}\n",
"System 6 has separation -106.87\n",
- "system 7 / 100\n"
- ]
- },
- {
- "name": "stdout",
- "output_type": "stream",
- "text": [
+ "system 7 / 100\n",
"{'time': 6.1851, 'M1': 26.215, 'M2': 48.508, 'K1': 14.0, 'K2': 14.0, 'separation': -89.768}\n",
"System 7 has separation -89.768\n",
"system 8 / 100\n",
@@ -2514,13 +2423,7 @@
"{'time': 6.1819, 'M1': 26.224, 'M2': 18.975, 'K1': 14.0, 'K2': 14.0, 'separation': -23.855}\n",
"System 1 has separation -23.855\n",
"system 2 / 100\n",
- "{'time': 6.1811, 'M1': 26.225, 'M2': 19.036, 'K1': 14.0, 'K2': 14.0, 'separation': -168.1}\n"
- ]
- },
- {
- "name": "stdout",
- "output_type": "stream",
- "text": [
+ "{'time': 6.1811, 'M1': 26.225, 'M2': 19.036, 'K1': 14.0, 'K2': 14.0, 'separation': -168.1}\n",
"System 2 has separation -168.1\n",
"system 3 / 100\n",
"None\n",
@@ -2603,13 +2506,7 @@
"System 6 has separation -98.879\n",
"system 7 / 100\n",
"{'time': 6.1834, 'M1': 26.221, 'M2': 18.866, 'K1': 14.0, 'K2': 14.0, 'separation': 71.42}\n",
- "System 7 has separation 71.42\n"
- ]
- },
- {
- "name": "stdout",
- "output_type": "stream",
- "text": [
+ "System 7 has separation 71.42\n",
"Found bound BHBH system\n",
" TIME M1 M2 K1 K2 SEP PER ECC R1/ROL1 R2/ROL2 TYPE RANDOM_SEED=26051 RANDOM_COUNT=0\n",
" 0.0000 60.000 40.000 1 1 3101.2 5.48 y 0.00 0.006 0.006 \"INITIAL \"\n",
@@ -2673,13 +2570,7 @@
"System 1 has separation -490.65\n",
"system 2 / 100\n",
"None\n",
- "system 3 / 100\n"
- ]
- },
- {
- "name": "stdout",
- "output_type": "stream",
- "text": [
+ "system 3 / 100\n",
"{'time': 6.1851, 'M1': 26.215, 'M2': 48.508, 'K1': 14.0, 'K2': 14.0, 'separation': -844.54}\n",
"System 3 has separation -844.54\n",
"system 4 / 100\n",
@@ -2803,13 +2694,7 @@
" 6.1812 26.225 19.021 14 14 157.31 34 d 0.29 0.000 0.000 \"TYPE_CHNGE\"\n",
" 6.1812 26.225 19.021 14 14 157.31 34 d 0.29 0.000 0.000 \"SN\"\n",
" 6.1812 26.225 19.021 14 14 157.31 34 d 0.29 0.000 0.000 \"End tidal lock 2\"\n",
- " 15000.0000 26.225 19.021 14 14 157.05 33.9 d 0.29 0.000 0.000 \"MAX_TIME\"\n"
- ]
- },
- {
- "name": "stdout",
- "output_type": "stream",
- "text": [
+ " 15000.0000 26.225 19.021 14 14 157.05 33.9 d 0.29 0.000 0.000 \"MAX_TIME\"\n",
"\n",
"{'M_1': 60, 'M_2': 40, 'metallicity': 0.001, 'orbital_period': 2000, 'BH_prescription': 'BH_BELCZYNSKI', 'wind_mass_loss': 'WIND_ALGORITHM_NONE', 'alpha_ce': 0.1}\n",
"system 1 / 100\n",
@@ -2932,13 +2817,7 @@
" 812.5051 43.110 0.000 14 15 -1 -1 -1.00 0.000 0.000 \"TYPE_CHNGE\"\n",
" 812.5051 43.110 0.000 14 15 -1 -1 -1.00 0.000 0.000 \"COALESCE\"\n",
" 812.5051 43.110 0.000 14 15 -1 -1 -1.00 0.000 0.000 \"SN\"\n",
- " 15000.0000 43.110 0.000 14 15 -1 -1 -1.00 0.000 0.000 \"MAX_TIME\"\n"
- ]
- },
- {
- "name": "stdout",
- "output_type": "stream",
- "text": [
+ " 15000.0000 43.110 0.000 14 15 -1 -1 -1.00 0.000 0.000 \"MAX_TIME\"\n",
"\n",
"{'M_1': 60, 'M_2': 40, 'metallicity': 0.001, 'orbital_period': 2000, 'BH_prescription': 'BH_BELCZYNSKI', 'wind_mass_loss': 'WIND_ALGORITHM_NONE', 'alpha_ce': 0.1}\n",
"system 1 / 100\n",
@@ -3051,13 +2930,7 @@
" 6.1844 26.229 18.804 14 14 164.59 36.4 d 0.46 0.000 0.000 SN kick Ib/c (SN type 11 11, pre-explosion M=18.8039 Mc\"CO\"=14.1854 type=8) -> kick 1(190) vk=161.317 vr=310.99 omega=3.87813 phi=-1.31958 -> vn=375.785 ; final sep 164.585 ecc 0.464494 (random count 5) - Runaway v=(-42.7184,-100.373,-23.0784) |v|=111.499 : companion v=(225.604,-99.3719,-86.2291), |v|=261.166 ; - , dm(exploder) = 0, dm(companion) = 0\n",
" 6.1844 26.229 18.804 14 14 164.59 36.4 d 0.46 0.000 0.000 \"TYPE_CHNGE\"\n",
" 6.1844 26.229 18.804 14 14 164.59 36.4 d 0.46 0.000 0.000 \"SN\"\n",
- " 15000.0000 26.229 18.804 14 14 164.1 36.3 d 0.46 0.000 0.000 \"MAX_TIME\"\n"
- ]
- },
- {
- "name": "stdout",
- "output_type": "stream",
- "text": [
+ " 15000.0000 26.229 18.804 14 14 164.1 36.3 d 0.46 0.000 0.000 \"MAX_TIME\"\n",
"\n",
"{'M_1': 60, 'M_2': 40, 'metallicity': 0.001, 'orbital_period': 2000, 'BH_prescription': 'BH_BELCZYNSKI', 'wind_mass_loss': 'WIND_ALGORITHM_NONE', 'alpha_ce': 0.1}\n",
"system 1 / 100\n",
@@ -3176,13 +3049,7 @@
" 6.1830 26.222 18.894 14 14 305.95 92.3 d 0.61 0.000 0.000 SN kick Ib/c (SN type 11 11, pre-explosion M=18.8941 Mc\"CO\"=14.2552 type=8) -> kick 1(190) vk=151.131 vr=262.883 omega=2.0613 phi=-1.06527 -> vn=331.775 ; final sep 305.952 ecc 0.613167 (random count 5) - Runaway v=(0,0,0) |v|=0 : companion v=(0,0,0), |v|=0 ; - , dm(exploder) = 0, dm(companion) = 0\n",
" 6.1830 26.222 18.894 14 14 305.95 92.3 d 0.61 0.000 0.000 \"TYPE_CHNGE\"\n",
" 6.1830 26.222 18.894 14 14 305.95 92.3 d 0.61 0.000 0.000 \"SN\"\n",
- " 15000.0000 26.222 18.894 14 14 305.73 92.2 d 0.61 0.000 0.000 \"MAX_TIME\"\n"
- ]
- },
- {
- "name": "stdout",
- "output_type": "stream",
- "text": [
+ " 15000.0000 26.222 18.894 14 14 305.73 92.2 d 0.61 0.000 0.000 \"MAX_TIME\"\n",
"\n",
"{'M_1': 60, 'M_2': 40, 'metallicity': 0.001, 'orbital_period': 2000, 'BH_prescription': 'BH_BELCZYNSKI', 'wind_mass_loss': 'WIND_ALGORITHM_NONE', 'alpha_ce': 0.1}\n",
"system 1 / 100\n",
@@ -3267,13 +3134,7 @@
" 457.8881 45.125 0.000 14 15 -1 -1 -1.00 0.000 0.000 \"TYPE_CHNGE\"\n",
" 457.8881 45.125 0.000 14 15 -1 -1 -1.00 0.000 0.000 \"COALESCE\"\n",
" 457.8881 45.125 0.000 14 15 -1 -1 -1.00 0.000 0.000 \"SN\"\n",
- " 15000.0000 45.125 0.000 14 15 -1 -1 -1.00 0.000 0.000 \"MAX_TIME\"\n"
- ]
- },
- {
- "name": "stdout",
- "output_type": "stream",
- "text": [
+ " 15000.0000 45.125 0.000 14 15 -1 -1 -1.00 0.000 0.000 \"MAX_TIME\"\n",
"\n",
"{'M_1': 60, 'M_2': 40, 'metallicity': 0.001, 'orbital_period': 2000, 'BH_prescription': 'BH_BELCZYNSKI', 'wind_mass_loss': 'WIND_ALGORITHM_NONE', 'alpha_ce': 0.1}\n",
"system 1 / 100\n",
@@ -3351,13 +3212,7 @@
"System 1 has separation -168.81\n",
"system 2 / 100\n",
"None\n",
- "system 3 / 100\n"
- ]
- },
- {
- "name": "stdout",
- "output_type": "stream",
- "text": [
+ "system 3 / 100\n",
"{'time': 6.1808, 'M1': 26.225, 'M2': 19.057, 'K1': 14.0, 'K2': 14.0, 'separation': -26.38}\n",
"System 3 has separation -26.38\n",
"system 4 / 100\n",
@@ -3449,13 +3304,7 @@
"system 13 / 100\n",
"{'time': 6.1851, 'M1': 26.215, 'M2': 48.508, 'K1': 14.0, 'K2': 14.0, 'separation': -374.05}\n",
"System 13 has separation -374.05\n",
- "system 14 / 100\n"
- ]
- },
- {
- "name": "stdout",
- "output_type": "stream",
- "text": [
+ "system 14 / 100\n",
"{'time': 6.181, 'M1': 26.225, 'M2': 19.041, 'K1': 14.0, 'K2': 14.0, 'separation': 236.64}\n",
"System 14 has separation 236.64\n",
"Found bound BHBH system\n",
@@ -3586,13 +3435,7 @@
" 6.1827 26.222 18.914 14 14 99.202 17 d 0.44 0.000 0.000 \"TYPE_CHNGE\"\n",
" 6.1827 26.222 18.914 14 14 99.202 17 d 0.44 0.000 0.000 \"SN\"\n",
" 6.1827 26.222 18.914 14 14 99.202 17 d 0.44 0.000 0.000 \"End tidal lock 2\"\n",
- " 15000.0000 26.222 18.914 14 14 97.228 16.5 d 0.43 0.000 0.000 \"MAX_TIME\"\n"
- ]
- },
- {
- "name": "stdout",
- "output_type": "stream",
- "text": [
+ " 15000.0000 26.222 18.914 14 14 97.228 16.5 d 0.43 0.000 0.000 \"MAX_TIME\"\n",
"\n",
"{'M_1': 60, 'M_2': 40, 'metallicity': 0.001, 'orbital_period': 2000, 'BH_prescription': 'BH_BELCZYNSKI', 'wind_mass_loss': 'WIND_ALGORITHM_NONE', 'alpha_ce': 0.1}\n",
"system 1 / 100\n",
@@ -3704,13 +3547,7 @@
" 6.1858 26.249 18.711 14 14 98.616 16.9 d 0.47 0.000 0.000 SN kick Ib/c (SN type 11 11, pre-explosion M=18.7108 Mc\"CO\"=14.1135 type=8) -> kick 1(190) vk=199.576 vr=332.361 omega=1.41485 phi=-0.652755 -> vn=365.958 ; final sep 98.6161 ecc 0.469056 (random count 5) - Runaway v=(-0.807331,-67.6832,0.168972) |v|=67.6883 : companion v=(254.424,134.518,0.477089), |v|=287.796 ; - , dm(exploder) = 0, dm(companion) = 0\n",
" 6.1858 26.249 18.711 14 14 98.616 16.9 d 0.47 0.000 0.000 \"TYPE_CHNGE\"\n",
" 6.1858 26.249 18.711 14 14 98.616 16.9 d 0.47 0.000 0.000 \"SN\"\n",
- " 15000.0000 26.249 18.711 14 14 96.287 16.3 d 0.46 0.000 0.000 \"MAX_TIME\"\n"
- ]
- },
- {
- "name": "stdout",
- "output_type": "stream",
- "text": [
+ " 15000.0000 26.249 18.711 14 14 96.287 16.3 d 0.46 0.000 0.000 \"MAX_TIME\"\n",
"\n",
"{'M_1': 60, 'M_2': 40, 'metallicity': 0.001, 'orbital_period': 2000, 'BH_prescription': 'BH_BELCZYNSKI', 'wind_mass_loss': 'WIND_ALGORITHM_NONE', 'alpha_ce': 0.1}\n",
"system 1 / 100\n",
@@ -3838,13 +3675,7 @@
" 10.8252 45.201 0.000 14 15 -1 -1 -1.00 0.000 0.000 \"TYPE_CHNGE\"\n",
" 10.8252 45.201 0.000 14 15 -1 -1 -1.00 0.000 0.000 \"COALESCE\"\n",
" 10.8252 45.201 0.000 14 15 -1 -1 -1.00 0.000 0.000 \"SN\"\n",
- " 15000.0000 45.201 0.000 14 15 -1 -1 -1.00 0.000 0.000 \"MAX_TIME\"\n"
- ]
- },
- {
- "name": "stdout",
- "output_type": "stream",
- "text": [
+ " 15000.0000 45.201 0.000 14 15 -1 -1 -1.00 0.000 0.000 \"MAX_TIME\"\n",
"\n",
"{'M_1': 60, 'M_2': 40, 'metallicity': 0.001, 'orbital_period': 2000, 'BH_prescription': 'BH_BELCZYNSKI', 'wind_mass_loss': 'WIND_ALGORITHM_NONE', 'alpha_ce': 0.1}\n",
"system 1 / 100\n",
@@ -3953,13 +3784,7 @@
" 8031.6562 45.165 0.000 14 15 -1 -1 -1.00 0.000 0.000 \"TYPE_CHNGE\"\n",
" 8031.6562 45.165 0.000 14 15 -1 -1 -1.00 0.000 0.000 \"COALESCE\"\n",
" 8031.6562 45.165 0.000 14 15 -1 -1 -1.00 0.000 0.000 \"SN\"\n",
- " 15000.0000 45.165 0.000 14 15 -1 -1 -1.00 0.000 0.000 \"MAX_TIME\"\n"
- ]
- },
- {
- "name": "stdout",
- "output_type": "stream",
- "text": [
+ " 15000.0000 45.165 0.000 14 15 -1 -1 -1.00 0.000 0.000 \"MAX_TIME\"\n",
"\n",
"{'M_1': 60, 'M_2': 40, 'metallicity': 0.001, 'orbital_period': 2000, 'BH_prescription': 'BH_BELCZYNSKI', 'wind_mass_loss': 'WIND_ALGORITHM_NONE', 'alpha_ce': 0.1}\n",
"system 1 / 100\n",
@@ -4046,13 +3871,7 @@
" 6.1847 26.236 18.783 14 14 113.51 20.9 d 0.29 0.000 0.000 \"TYPE_CHNGE\"\n",
" 6.1847 26.236 18.783 14 14 113.51 20.9 d 0.29 0.000 0.000 \"SN\"\n",
" 15000.0000 26.236 18.783 14 14 112.85 20.7 d 0.29 0.000 0.000 \"MAX_TIME\"\n",
- "\n"
- ]
- },
- {
- "name": "stdout",
- "output_type": "stream",
- "text": [
+ "\n",
"{'M_1': 60, 'M_2': 40, 'metallicity': 0.001, 'orbital_period': 2000, 'BH_prescription': 'BH_BELCZYNSKI', 'wind_mass_loss': 'WIND_ALGORITHM_NONE', 'alpha_ce': 0.1}\n",
"system 1 / 100\n",
"{'time': 6.1851, 'M1': 26.215, 'M2': 48.508, 'K1': 14.0, 'K2': 14.0, 'separation': -48.404}\n",
@@ -4115,13 +3934,7 @@
" 6.2075 45.233 0.000 14 15 -1 -1 -1.00 0.000 0.000 \"TYPE_CHNGE\"\n",
" 6.2075 45.233 0.000 14 15 -1 -1 -1.00 0.000 0.000 \"COALESCE\"\n",
" 6.2075 45.233 0.000 14 15 -1 -1 -1.00 0.000 0.000 \"SN\"\n",
- " 15000.0000 45.233 0.000 14 15 -1 -1 -1.00 0.000 0.000 \"MAX_TIME\"\n"
- ]
- },
- {
- "name": "stdout",
- "output_type": "stream",
- "text": [
+ " 15000.0000 45.233 0.000 14 15 -1 -1 -1.00 0.000 0.000 \"MAX_TIME\"\n",
"\n",
"{'M_1': 60, 'M_2': 40, 'metallicity': 0.001, 'orbital_period': 2000, 'BH_prescription': 'BH_BELCZYNSKI', 'wind_mass_loss': 'WIND_ALGORITHM_NONE', 'alpha_ce': 0.1}\n",
"system 1 / 100\n",
@@ -4206,13 +4019,7 @@
" 6.1817 26.224 18.984 14 14 763.92 364 d 0.79 0.000 0.000 \"TYPE_CHNGE\"\n",
" 6.1817 26.224 18.984 14 14 763.92 364 d 0.79 0.000 0.000 \"SN\"\n",
" 6.1817 26.224 18.984 14 14 763.92 364 d 0.79 0.000 0.000 \"End tidal lock 2\"\n",
- " 15000.0000 26.224 18.984 14 14 763.81 364 d 0.79 0.000 0.000 \"MAX_TIME\"\n"
- ]
- },
- {
- "name": "stdout",
- "output_type": "stream",
- "text": [
+ " 15000.0000 26.224 18.984 14 14 763.81 364 d 0.79 0.000 0.000 \"MAX_TIME\"\n",
"\n",
"{'M_1': 60, 'M_2': 40, 'metallicity': 0.001, 'orbital_period': 2000, 'BH_prescription': 'BH_BELCZYNSKI', 'wind_mass_loss': 'WIND_ALGORITHM_NONE', 'alpha_ce': 0.1}\n",
"system 1 / 100\n",
@@ -4291,13 +4098,7 @@
"{'time': 6.1851, 'M1': 26.215, 'M2': 48.508, 'K1': 14.0, 'K2': 14.0, 'separation': -1722.6}\n",
"System 5 has separation -1722.6\n",
"system 6 / 100\n",
- "{'time': 6.1851, 'M1': 26.215, 'M2': 48.508, 'K1': 14.0, 'K2': 14.0, 'separation': -1571.7}\n"
- ]
- },
- {
- "name": "stdout",
- "output_type": "stream",
- "text": [
+ "{'time': 6.1851, 'M1': 26.215, 'M2': 48.508, 'K1': 14.0, 'K2': 14.0, 'separation': -1571.7}\n",
"System 6 has separation -1571.7\n",
"system 7 / 100\n",
"None\n",
@@ -4424,13 +4225,7 @@
" 6.1826 26.223 18.922 14 14 1691.7 3.28 y 0.98 0.000 0.000 \"TYPE_CHNGE\"\n",
" 6.1826 26.223 18.922 14 14 1691.7 3.28 y 0.98 0.000 0.000 \"SN\"\n",
" 6.1826 26.223 18.922 14 14 1691.7 3.28 y 0.98 0.000 0.000 \"End tidal lock 2\"\n",
- " 15000.0000 26.223 18.922 14 14 1663.3 3.2 y 0.98 0.000 0.000 \"MAX_TIME\"\n"
- ]
- },
- {
- "name": "stdout",
- "output_type": "stream",
- "text": [
+ " 15000.0000 26.223 18.922 14 14 1663.3 3.2 y 0.98 0.000 0.000 \"MAX_TIME\"\n",
"\n",
"{'M_1': 60, 'M_2': 40, 'metallicity': 0.001, 'orbital_period': 2000, 'BH_prescription': 'BH_BELCZYNSKI', 'wind_mass_loss': 'WIND_ALGORITHM_NONE', 'alpha_ce': 0.1}\n",
"system 1 / 100\n",
@@ -4508,13 +4303,7 @@
"system 4 / 100\n",
"{'time': 6.1851, 'M1': 26.215, 'M2': 48.508, 'K1': 14.0, 'K2': 14.0, 'separation': -121.45}\n",
"System 4 has separation -121.45\n",
- "system 5 / 100\n"
- ]
- },
- {
- "name": "stdout",
- "output_type": "stream",
- "text": [
+ "system 5 / 100\n",
"{'time': 6.1851, 'M1': 26.215, 'M2': 48.508, 'K1': 14.0, 'K2': 14.0, 'separation': -209.29}\n",
"System 5 has separation -209.29\n",
"system 6 / 100\n",
@@ -4611,13 +4400,7 @@
"{'time': 6.1851, 'M1': 26.215, 'M2': 48.508, 'K1': 14.0, 'K2': 14.0, 'separation': -42.805}\n",
"System 6 has separation -42.805\n",
"system 7 / 100\n",
- "{'time': 6.1851, 'M1': 26.215, 'M2': 48.508, 'K1': 14.0, 'K2': 14.0, 'separation': -86.593}\n"
- ]
- },
- {
- "name": "stdout",
- "output_type": "stream",
- "text": [
+ "{'time': 6.1851, 'M1': 26.215, 'M2': 48.508, 'K1': 14.0, 'K2': 14.0, 'separation': -86.593}\n",
"System 7 has separation -86.593\n",
"system 8 / 100\n",
"{'time': 6.1851, 'M1': 26.215, 'M2': 48.508, 'K1': 14.0, 'K2': 14.0, 'separation': -33.049}\n",
@@ -4693,13 +4476,7 @@
"system 5 / 100\n",
"{'time': 6.1817, 'M1': 26.224, 'M2': 18.986, 'K1': 14.0, 'K2': 14.0, 'separation': -78.905}\n",
"System 5 has separation -78.905\n",
- "system 6 / 100\n"
- ]
- },
- {
- "name": "stdout",
- "output_type": "stream",
- "text": [
+ "system 6 / 100\n",
"{'time': 6.1851, 'M1': 26.215, 'M2': 48.508, 'K1': 14.0, 'K2': 14.0, 'separation': -58.583}\n",
"System 6 has separation -58.583\n",
"system 7 / 100\n",
@@ -4826,13 +4603,7 @@
" 6.1822 26.223 18.952 14 14 133.24 26.5 d 0.42 0.000 0.000 \"TYPE_CHNGE\"\n",
" 6.1822 26.223 18.952 14 14 133.24 26.5 d 0.42 0.000 0.000 \"SN\"\n",
" 6.1822 26.223 18.952 14 14 133.24 26.5 d 0.42 0.000 0.000 \"End tidal lock 2\"\n",
- " 15000.0000 26.223 18.952 14 14 132.51 26.3 d 0.42 0.000 0.000 \"MAX_TIME\"\n"
- ]
- },
- {
- "name": "stdout",
- "output_type": "stream",
- "text": [
+ " 15000.0000 26.223 18.952 14 14 132.51 26.3 d 0.42 0.000 0.000 \"MAX_TIME\"\n",
"\n",
"{'M_1': 60, 'M_2': 40, 'metallicity': 0.001, 'orbital_period': 2000, 'BH_prescription': 'BH_BELCZYNSKI', 'wind_mass_loss': 'WIND_ALGORITHM_NONE', 'alpha_ce': 0.1}\n",
"system 1 / 100\n",
@@ -4959,13 +4730,7 @@
" 6.1814 26.225 19.013 14 14 195.2 47 d 0.11 0.000 0.000 \"TYPE_CHNGE\"\n",
" 6.1814 26.225 19.013 14 14 195.2 47 d 0.11 0.000 0.000 \"SN\"\n",
" 6.1814 26.225 19.013 14 14 195.2 47 d 0.11 0.000 0.000 \"End tidal lock 2\"\n",
- " 15000.0000 26.225 19.013 14 14 195.12 46.9 d 0.11 0.000 0.000 \"MAX_TIME\"\n"
- ]
- },
- {
- "name": "stdout",
- "output_type": "stream",
- "text": [
+ " 15000.0000 26.225 19.013 14 14 195.12 46.9 d 0.11 0.000 0.000 \"MAX_TIME\"\n",
"\n",
"{'M_1': 60, 'M_2': 40, 'metallicity': 0.001, 'orbital_period': 2000, 'BH_prescription': 'BH_BELCZYNSKI', 'wind_mass_loss': 'WIND_ALGORITHM_NONE', 'alpha_ce': 0.1}\n",
"system 1 / 100\n",
@@ -5071,13 +4836,7 @@
" 202.9610 45.199 0.000 14 15 -1 -1 -1.00 0.000 0.000 \"TYPE_CHNGE\"\n",
" 202.9610 45.199 0.000 14 15 -1 -1 -1.00 0.000 0.000 \"COALESCE\"\n",
" 202.9610 45.199 0.000 14 15 -1 -1 -1.00 0.000 0.000 \"SN\"\n",
- " 15000.0000 45.199 0.000 14 15 -1 -1 -1.00 0.000 0.000 \"MAX_TIME\"\n"
- ]
- },
- {
- "name": "stdout",
- "output_type": "stream",
- "text": [
+ " 15000.0000 45.199 0.000 14 15 -1 -1 -1.00 0.000 0.000 \"MAX_TIME\"\n",
"\n",
"{'M_1': 60, 'M_2': 40, 'metallicity': 0.001, 'orbital_period': 2000, 'BH_prescription': 'BH_BELCZYNSKI', 'wind_mass_loss': 'WIND_ALGORITHM_NONE', 'alpha_ce': 0.1}\n",
"system 1 / 100\n",
@@ -5205,13 +4964,7 @@
" 6.1817 26.224 18.984 14 14 239.33 63.8 d 0.62 0.000 0.000 \"TYPE_CHNGE\"\n",
" 6.1817 26.224 18.984 14 14 239.33 63.8 d 0.62 0.000 0.000 \"SN\"\n",
" 6.1817 26.224 18.984 14 14 239.33 63.8 d 0.62 0.000 0.000 \"End tidal lock 2\"\n",
- " 15000.0000 26.224 18.984 14 14 238.83 63.6 d 0.62 0.000 0.000 \"MAX_TIME\"\n"
- ]
- },
- {
- "name": "stdout",
- "output_type": "stream",
- "text": [
+ " 15000.0000 26.224 18.984 14 14 238.83 63.6 d 0.62 0.000 0.000 \"MAX_TIME\"\n",
"\n",
"{'M_1': 60, 'M_2': 40, 'metallicity': 0.001, 'orbital_period': 2000, 'BH_prescription': 'BH_BELCZYNSKI', 'wind_mass_loss': 'WIND_ALGORITHM_NONE', 'alpha_ce': 0.1}\n",
"system 1 / 100\n",
@@ -5331,13 +5084,7 @@
" 6.1821 26.223 18.957 14 14 144.61 30 d 0.23 0.000 0.000 \"TYPE_CHNGE\"\n",
" 6.1821 26.223 18.957 14 14 144.61 30 d 0.23 0.000 0.000 \"SN\"\n",
" 6.1821 26.223 18.957 14 14 144.61 30 d 0.23 0.000 0.000 \"End tidal lock 2\"\n",
- " 15000.0000 26.223 18.957 14 14 144.35 29.9 d 0.23 0.000 0.000 \"MAX_TIME\"\n"
- ]
- },
- {
- "name": "stdout",
- "output_type": "stream",
- "text": [
+ " 15000.0000 26.223 18.957 14 14 144.35 29.9 d 0.23 0.000 0.000 \"MAX_TIME\"\n",
"\n",
"{'M_1': 60, 'M_2': 40, 'metallicity': 0.001, 'orbital_period': 2000, 'BH_prescription': 'BH_BELCZYNSKI', 'wind_mass_loss': 'WIND_ALGORITHM_NONE', 'alpha_ce': 0.1}\n",
"system 1 / 100\n",
@@ -5420,13 +5167,7 @@
" 6.1816 26.224 18.998 14 14 246.46 66.6 d 0.33 0.000 0.000 \"TYPE_CHNGE\"\n",
" 6.1816 26.224 18.998 14 14 246.46 66.6 d 0.33 0.000 0.000 \"SN\"\n",
" 6.1816 26.224 18.998 14 14 246.46 66.6 d 0.33 0.000 0.000 \"End tidal lock 2\"\n",
- " 15000.0000 26.224 18.998 14 14 246.39 66.6 d 0.33 0.000 0.000 \"MAX_TIME\"\n"
- ]
- },
- {
- "name": "stdout",
- "output_type": "stream",
- "text": [
+ " 15000.0000 26.224 18.998 14 14 246.39 66.6 d 0.33 0.000 0.000 \"MAX_TIME\"\n",
"\n",
"{'M_1': 60, 'M_2': 40, 'metallicity': 0.001, 'orbital_period': 2000, 'BH_prescription': 'BH_BELCZYNSKI', 'wind_mass_loss': 'WIND_ALGORITHM_NONE', 'alpha_ce': 0.1}\n",
"system 1 / 100\n",
@@ -5528,7 +5269,7 @@
],
"metadata": {
"kernelspec": {
- "display_name": "Python 3 (ipykernel)",
+ "display_name": "Python 3",
"language": "python",
"name": "python3"
},
@@ -5542,7 +5283,7 @@
"name": "python",
"nbconvert_exporter": "python",
"pygments_lexer": "ipython3",
- "version": "3.9.5"
+ "version": "3.6.4"
}
},
"nbformat": 4,
diff --git a/examples/notebook_HRD.ipynb b/examples/notebook_HRD.ipynb
index ee40c35d2..d56440170 100644
--- a/examples/notebook_HRD.ipynb
+++ b/examples/notebook_HRD.ipynb
@@ -1089,7 +1089,7 @@
],
"metadata": {
"kernelspec": {
- "display_name": "Python 3 (ipykernel)",
+ "display_name": "Python 3",
"language": "python",
"name": "python3"
},
@@ -1103,7 +1103,7 @@
"name": "python",
"nbconvert_exporter": "python",
"pygments_lexer": "ipython3",
- "version": "3.9.5"
+ "version": "3.6.4"
}
},
"nbformat": 4,
diff --git a/examples/notebook_api_functionality.ipynb b/examples/notebook_api_functionality.ipynb
index fb6ea05bd..504ae4b16 100644
--- a/examples/notebook_api_functionality.ipynb
+++ b/examples/notebook_api_functionality.ipynb
@@ -966,7 +966,7 @@
],
"metadata": {
"kernelspec": {
- "display_name": "Python 3 (ipykernel)",
+ "display_name": "Python 3",
"language": "python",
"name": "python3"
},
@@ -980,7 +980,7 @@
"name": "python",
"nbconvert_exporter": "python",
"pygments_lexer": "ipython3",
- "version": "3.9.5"
+ "version": "3.6.4"
}
},
"nbformat": 4,
diff --git a/examples/notebook_common_envelope_evolution.ipynb b/examples/notebook_common_envelope_evolution.ipynb
index 83f3e239c..b543957d6 100644
--- a/examples/notebook_common_envelope_evolution.ipynb
+++ b/examples/notebook_common_envelope_evolution.ipynb
@@ -783,20 +783,21 @@
"metadata": {},
"source": [
"Things to try:\n",
- "* Extend the logging to output more data than just the orbital period.\n",
- "* What are the stellar types of the post-common envelope systems? Are they likely to undergo novae or a type-Ia supernova?\n",
- "* What are the lifetimes of the systems in close ($<1\\text{ }\\mathrm{d}$) binaries? Are they likely to merge in the life of the Universe?\n",
- "* How much mass is lost in common-envelope interactions?\n",
- "* Extend the grid to massive stars. Do you see many NS and BH compact binaries?\n",
- "* Try different $\\alpha_\\mathrm{CE}$ and $\\lambda_\\mathrm{CE}$ options...\n",
- "* ... and perhaps increased resolution to obtain smoother curves.\n",
- "* Why do long-period systems not reach common envelope evolution?"
+ "\n",
+ " * Extend the logging to output more data than just the orbital period.\n",
+ " * What are the stellar types of the post-common envelope systems? Are they likely to undergo novae or a type-Ia supernova?\n",
+ " * What are the lifetimes of the systems in close ($<1\\text{ }\\mathrm{d}$) binaries? Are they likely to merge in the life of the Universe?\n",
+ " * How much mass is lost in common-envelope interactions?\n",
+ " * Extend the grid to massive stars. Do you see many NS and BH compact binaries?\n",
+ " * Try different $\\alpha_\\mathrm{CE}$ and $\\lambda_\\mathrm{CE}$ options...\n",
+ " * ... and perhaps increased resolution to obtain smoother curves.\n",
+ " * Why do long-period systems not reach common envelope evolution?"
]
}
],
"metadata": {
"kernelspec": {
- "display_name": "Python 3 (ipykernel)",
+ "display_name": "Python 3",
"language": "python",
"name": "python3"
},
@@ -810,7 +811,7 @@
"name": "python",
"nbconvert_exporter": "python",
"pygments_lexer": "ipython3",
- "version": "3.9.5"
+ "version": "3.6.4"
}
},
"nbformat": 4,
diff --git a/examples/notebook_custom_logging.ipynb b/examples/notebook_custom_logging.ipynb
index dbe7d3001..8dfb85034 100644
--- a/examples/notebook_custom_logging.ipynb
+++ b/examples/notebook_custom_logging.ipynb
@@ -34,6 +34,7 @@
"The custom logging functionality allows us to decide the output of binary_c _without_ modifying the actual sourcecode of binary_c (i.e. editing `src/logging/log_every_timestep` in binary_c). Rather, we can create a logging routine from within python.\n",
"\n",
"Technically, the following steps are taken:\n",
+ "\n",
"- User creates a logging print statement from within python\n",
"- The logging print statement string gets wrapped into a proper c-function by `binary_c_log_code`\n",
"- The c-function string gets compiled and loaded into memory by `create_and_load_logging_function`\n",
@@ -460,19 +461,11 @@
"# print (abridged) output\n",
"print(\"\\n\".join(output.splitlines()[-2:]))"
]
- },
- {
- "cell_type": "code",
- "execution_count": null,
- "id": "484297c0-accb-4efc-a9c8-dbd2f32b89a6",
- "metadata": {},
- "outputs": [],
- "source": []
}
],
"metadata": {
"kernelspec": {
- "display_name": "Python 3 (ipykernel)",
+ "display_name": "Python 3",
"language": "python",
"name": "python3"
},
@@ -486,7 +479,7 @@
"name": "python",
"nbconvert_exporter": "python",
"pygments_lexer": "ipython3",
- "version": "3.9.5"
+ "version": "3.6.4"
}
},
"nbformat": 4,
diff --git a/examples/notebook_extra_features.ipynb b/examples/notebook_extra_features.ipynb
index f51d82bb4..44c19c112 100644
--- a/examples/notebook_extra_features.ipynb
+++ b/examples/notebook_extra_features.ipynb
@@ -34,7 +34,8 @@
"metadata": {},
"source": [
"## getting extra information about binary_c parameters\n",
- "There are several functions that can be used to get information about the parameters in binary_c: \n",
+ "There are several functions that can be used to get information about the parameters in binary_c:\n",
+ "\n",
"- `get_help(parameter)`: Function to get information about the specific input parameter. Prints the output on default but returns a dictionary containing the information. \n",
"- `get_help_all(print_help=True)`: Function to get information about all the parameters. Prints the output on default but returns a dictionary containing the information. \n",
"- `get_help_super()`: Function to get even more information about all the parameters. Does not print the output on default but returns a dictionary containing the information. \n",
@@ -173,8 +174,7 @@
"id": "b3c259ef-9f89-4b26-9ce3-45af625bc398",
"metadata": {},
"source": [
- "## Getting help\n",
- "There are sever"
+ "## Getting help\n"
]
},
{
@@ -188,7 +188,7 @@
],
"metadata": {
"kernelspec": {
- "display_name": "Python 3 (ipykernel)",
+ "display_name": "Python 3",
"language": "python",
"name": "python3"
},
@@ -202,7 +202,7 @@
"name": "python",
"nbconvert_exporter": "python",
"pygments_lexer": "ipython3",
- "version": "3.9.5"
+ "version": "3.6.4"
}
},
"nbformat": 4,
diff --git a/examples/notebook_individual_systems.ipynb b/examples/notebook_individual_systems.ipynb
index b71d14897..deb72fc55 100644
--- a/examples/notebook_individual_systems.ipynb
+++ b/examples/notebook_individual_systems.ipynb
@@ -23,6 +23,7 @@
"The simplest method to run a single system is to use the run_system wrapper. This function deals with setting up the argument string, makes sure all the required parameters are included and handles setting and cleaning up the custom logging functionality (see notebook_custom_logging).\n",
"\n",
"As arguments to this function we can add any of the parameters that binary_c itself actually knows, as well as:\n",
+ "\n",
"- custom_logging_code: string containing a Printf statement that binary_c can use to print information\n",
"- log_filename: path of the logfile that binary_c generates\n",
"- parse_function: function that handles parsing the output of binary-c"
diff --git a/examples/notebook_luminosity_function_binaries.ipynb b/examples/notebook_luminosity_function_binaries.ipynb
index 8eabffc08..8325ab08f 100644
--- a/examples/notebook_luminosity_function_binaries.ipynb
+++ b/examples/notebook_luminosity_function_binaries.ipynb
@@ -124,11 +124,12 @@
"id": "2a9104fc-4136-4e53-8604-f24ad52fbe56",
"metadata": {},
"source": [
- "First let us set up some global variables that will be useful throughout. \n",
- "* The resolution is the number of stars we simulate in our model population.\n",
- "* The massrange is a list of the min and max masses\n",
- "* The total_probability is the theoretical integral of a probability density function, i.e. 1.0.\n",
- "* The binwidth sets the resolution of the final distribution. If set to 0.5, the bins in log*L* are 0.5dex wide."
+ "First let us set up some global variables that will be useful throughout.\n",
+ "\n",
+ " * The resolution is the number of stars we simulate in our model population.\n",
+ " * The massrange is a list of the min and max masses\n",
+ " * The total_probability is the theoretical integral of a probability density function, i.e. 1.0.\n",
+ " * The binwidth sets the resolution of the final distribution. If set to 0.5, the bins in log*L* are 0.5dex wide."
]
},
{
@@ -869,33 +870,31 @@
]
},
{
- "cell_type": "code",
- "execution_count": 12,
- "id": "99e25a72-54e6-4826-b0e5-4a02460b857d",
+ "cell_type": "markdown",
+ "id": "e0601000-a4c9-4073-a695-10a664e532f0",
"metadata": {},
- "outputs": [
- {
- "ename": "SyntaxError",
- "evalue": "invalid syntax (2944163245.py, line 1)",
- "output_type": "error",
- "traceback": [
- "\u001b[0;36m File \u001b[0;32m\"/tmp/ipykernel_518916/2944163245.py\"\u001b[0;36m, line \u001b[0;32m1\u001b[0m\n\u001b[0;31m Things to try:\u001b[0m\n\u001b[0m ^\u001b[0m\n\u001b[0;31mSyntaxError\u001b[0m\u001b[0;31m:\u001b[0m invalid syntax\n"
- ]
- }
- ],
"source": [
"Things to try:\n",
- "* Massive stars: can you see the effects of wind mass loss and rejuvenation in these stars?\n",
- "* Alter the metallicity, does this make much of a difference?\n",
- "* Change the binary fraction. Here we assume a 100% binary fraction, but a real population is a mixture of single and binary stars.\n",
- "* How might you go about comparing these computed observations to real stars?\n",
- "* What about evolved stars? Here we consider only the *zero-age* main sequnece. What about other main-sequence stars? What about stars in later phases of stellar evolution?"
+ "\n",
+ " * Massive stars: can you see the effects of wind mass loss and rejuvenation in these stars?\n",
+ " * Alter the metallicity, does this make much of a difference?\n",
+ " * Change the binary fraction. Here we assume a 100% binary fraction, but a real population is a mixture of single and binary stars.\n",
+ " * How might you go about comparing these computed observations to real stars?\n",
+ " * What about evolved stars? Here we consider only the *zero-age* main sequnece. What about other main-sequence stars? What about stars in later phases of stellar evolution?"
]
+ },
+ {
+ "cell_type": "code",
+ "execution_count": null,
+ "id": "abb096b0-7c57-43d6-a9f7-56bdd21dc542",
+ "metadata": {},
+ "outputs": [],
+ "source": []
}
],
"metadata": {
"kernelspec": {
- "display_name": "Python 3 (ipykernel)",
+ "display_name": "Python 3",
"language": "python",
"name": "python3"
},
@@ -909,7 +908,7 @@
"name": "python",
"nbconvert_exporter": "python",
"pygments_lexer": "ipython3",
- "version": "3.9.5"
+ "version": "3.6.4"
}
},
"nbformat": 4,
diff --git a/examples/notebook_luminosity_function_single.ipynb b/examples/notebook_luminosity_function_single.ipynb
index 2fc879dc4..93e041531 100644
--- a/examples/notebook_luminosity_function_single.ipynb
+++ b/examples/notebook_luminosity_function_single.ipynb
@@ -131,7 +131,8 @@
"id": "2a9104fc-4136-4e53-8604-f24ad52fbe56",
"metadata": {},
"source": [
- "First let us set up some global variables that will be useful throughout. \n",
+ "First let us set up some global variables that will be useful throughout.\n",
+ "\n",
"* The resolution is the number of stars we simulate in our model population.\n",
"* The massrange is a list of the min and max masses\n",
"* The total_probability is the theoretical integral of a probability density function, i.e. 1.0.\n",
@@ -594,6 +595,7 @@
"metadata": {},
"source": [
"Things to try:\n",
+ "\n",
"* Change the resolution to make the distributions smoother: what about error bars, how would you do that?\n",
"* Different initial distributions: the Kroupa distribution isn't the only one out there\n",
"* Change the metallicity and mass ranges\n",
@@ -601,11 +603,19 @@
"* What about evolved stars? Here we consider only the *zero-age* main sequnece. What about other main-sequence stars? What about stars in later phases of stellar evolution?\n",
"* Binary stars! (see notebook_luminosity_function_binaries.ipynb)"
]
+ },
+ {
+ "cell_type": "code",
+ "execution_count": null,
+ "id": "ef00d82c-dc36-4a94-b4be-98f58649644e",
+ "metadata": {},
+ "outputs": [],
+ "source": []
}
],
"metadata": {
"kernelspec": {
- "display_name": "Python 3 (ipykernel)",
+ "display_name": "Python 3",
"language": "python",
"name": "python3"
},
@@ -619,7 +629,7 @@
"name": "python",
"nbconvert_exporter": "python",
"pygments_lexer": "ipython3",
- "version": "3.9.5"
+ "version": "3.6.4"
}
},
"nbformat": 4,
diff --git a/examples/notebook_massive_remnants.ipynb b/examples/notebook_massive_remnants.ipynb
index f7586281e..28227d1a1 100644
--- a/examples/notebook_massive_remnants.ipynb
+++ b/examples/notebook_massive_remnants.ipynb
@@ -7,7 +7,7 @@
"tags": []
},
"source": [
- "# Example use case: Zero-age stellar luminosity function\n",
+ "# Example use case: Massive star luminosity\n",
"\n",
"In this notebook we compute the luminosity function of the zero-age main-sequence by running a population of single stars using binary_c. \n",
"\n",
@@ -131,7 +131,8 @@
"id": "2a9104fc-4136-4e53-8604-f24ad52fbe56",
"metadata": {},
"source": [
- "First let us set up some global variables that will be useful throughout. \n",
+ "First let us set up some global variables that will be useful throughout.\n",
+ "\n",
"* The resolution is the number of stars we simulate in our model population.\n",
"* The massrange is a list of the min and max masses\n",
"* The total_probability is the theoretical integral of a probability density function, i.e. 1.0.\n",
@@ -718,18 +719,27 @@
"metadata": {},
"source": [
"Things to try:\n",
- "* Change the resolution to make the distributions smoother: what about error bars, how would you do that?\n",
- "* Different initial distributions: the Kroupa distribution isn't the only one out there\n",
- "* Change the metallicity and mass ranges\n",
- "* What about a non-constant star formation rate? This is more of a challenge!\n",
- "* What about evolved stars? Here we consider only the *zero-age* main sequnece. What about other main-sequence stars? What about stars in later phases of stellar evolution?\n",
- "* Binary stars! (see notebook_luminosity_function_binaries.ipynb)"
+ "\n",
+ " * Change the resolution to make the distributions smoother: what about error bars, how would you do that?\n",
+ " * Different initial distributions: the Kroupa distribution isn't the only one out there\n",
+ " * Change the metallicity and mass ranges\n",
+ " * What about a non-constant star formation rate? This is more of a challenge!\n",
+ " * What about evolved stars? Here we consider only the *zero-age* main sequnece. What about other main-sequence stars? What about stars in later phases of stellar evolution?\n",
+ " * Binary stars! (see notebook_luminosity_function_binaries.ipynb)"
]
+ },
+ {
+ "cell_type": "code",
+ "execution_count": null,
+ "id": "5abd0935-3957-4859-80c1-6f5d7ce4b614",
+ "metadata": {},
+ "outputs": [],
+ "source": []
}
],
"metadata": {
"kernelspec": {
- "display_name": "Python 3 (ipykernel)",
+ "display_name": "Python 3",
"language": "python",
"name": "python3"
},
@@ -743,7 +753,7 @@
"name": "python",
"nbconvert_exporter": "python",
"pygments_lexer": "ipython3",
- "version": "3.9.5"
+ "version": "3.6.4"
}
},
"nbformat": 4,
diff --git a/examples/notebook_population.ipynb b/examples/notebook_population.ipynb
index 968c03350..760b1480e 100644
--- a/examples/notebook_population.ipynb
+++ b/examples/notebook_population.ipynb
@@ -116,6 +116,7 @@
"After configuring the population, but before running the actual population, its usually a good idea to export the full configuration (including version info of binary_c and all the parameters) to a file. To do this we use `example_pop.export_all_info()`.\n",
"\n",
"On default this exports everything, each of the sections can be disabled:\n",
+ "\n",
" - population settings (bse_options, grid_options, custom_options), turn off with include_population\n",
" settings=False\n",
" - binary_c_defaults (all the commandline arguments that binary c accepts, and their defaults).\n",
@@ -1144,7 +1145,7 @@
],
"metadata": {
"kernelspec": {
- "display_name": "Python 3 (ipykernel)",
+ "display_name": "Python 3",
"language": "python",
"name": "python3"
},
@@ -1158,7 +1159,7 @@
"name": "python",
"nbconvert_exporter": "python",
"pygments_lexer": "ipython3",
- "version": "3.9.5"
+ "version": "3.6.4"
}
},
"nbformat": 4,
diff --git a/examples/notebook_solar_system.ipynb b/examples/notebook_solar_system.ipynb
index 67556a655..926e6d9c4 100644
--- a/examples/notebook_solar_system.ipynb
+++ b/examples/notebook_solar_system.ipynb
@@ -3,9 +3,11 @@
{
"cell_type": "markdown",
"id": "ddc06da3-fc68-4c6f-8067-14ea862b964d",
- "metadata": {},
+ "metadata": {
+ "tags": []
+ },
"source": [
- "## Solar system using the API functionality\n",
+ "## Example use case: Solar system using the API functionality\n",
"We use the API interface to construct a model of the Solar system."
]
},
@@ -292,19 +294,11 @@
"source": [
"It gets a little toasty on Earth in the not too distant future!"
]
- },
- {
- "cell_type": "code",
- "execution_count": null,
- "id": "22df65d7-1c77-4e9c-b188-955219377014",
- "metadata": {},
- "outputs": [],
- "source": []
}
],
"metadata": {
"kernelspec": {
- "display_name": "Python 3 (ipykernel)",
+ "display_name": "Python 3",
"language": "python",
"name": "python3"
},
@@ -318,7 +312,7 @@
"name": "python",
"nbconvert_exporter": "python",
"pygments_lexer": "ipython3",
- "version": "3.9.5"
+ "version": "3.6.4"
}
},
"nbformat": 4,
--
GitLab