From c51a013fe0f9885377d7bff9dc9a55d1b7b2f7dd Mon Sep 17 00:00:00 2001
From: dh00601 <dh00601@surrey.ac.uk>
Date: Sun, 19 Jun 2022 11:13:01 +0100
Subject: [PATCH] updated notebook BHBH
---
examples/notebook_BHBH.ipynb | 9 +++++++++
1 file changed, 9 insertions(+)
diff --git a/examples/notebook_BHBH.ipynb b/examples/notebook_BHBH.ipynb
index c3fa9b934..d639f4bd6 100644
--- a/examples/notebook_BHBH.ipynb
+++ b/examples/notebook_BHBH.ipynb
@@ -649,11 +649,20 @@
"Playing around with the input for an individual system gives us some understanding of which parameters affect the formation of black hole systems, but, as mentioned in the introduction, this is nto the most appropriate way to find many such systems. We want to make use of the Population utilities, and set up custom logging and a parse function.\n",
"\n",
"Things to try next:\n",
+ "\n",
"* Set up a population object with a grid in M1, q and orbital period (10 x 10 x 10)\n",
"* Set up a custom logging function to catch BHBH systems, and include the ZAMS properties in the output.\n",
"* Set up a parse function to process the output, try writing the output to a file.\n",
"* Run this population at several different metallicities. Do you see a trend?"
]
+ },
+ {
+ "cell_type": "code",
+ "execution_count": null,
+ "id": "c8b4d134-1b41-49cc-a122-2aee89818248",
+ "metadata": {},
+ "outputs": [],
+ "source": []
}
],
"metadata": {
--
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