Skip to content
Snippets Groups Projects
Commit 17626f77 authored by Francesco Pannarale's avatar Francesco Pannarale
Browse files

A couple of typos in the guide.

git-svn-id: https://svn.ligo.caltech.edu/svn/bayeswave/trunk@88 c56465c9-8126-4a4f-9d7d-ac845eff4865
parent d0c9dbf0
No related branches found
No related tags found
No related merge requests found
......@@ -237,7 +237,7 @@ Move to a new directory and try running the example command line. You will hav
\code{export PATH=[path to]/bayeswave/trunk/src/:\$PATH}
This will run for $\sim$10 minutes. Real runs take $\sim4-48$ hours, depending on the settings and the models being used. Really long segments (1024 s) of really glitchy data can take a week.
This run will simulate Advanced LIGO data for H1 with a random seed for the noise realization {\tt dataseed} $=1234$; a low-frequency cutoff of {\tt IFO-flow} $=40$ Hz; a total observation time of {\tt seglen} $=1234$ s; and a sampling rate of {\tt state} $=512$ Hz.
This run will simulate Advanced LIGO data for H1 with a random seed for the noise realization {\tt dataseed} $=1234$; a low-frequency cutoff of {\tt IFO-flow} $=40$ Hz; a total observation time of {\tt seglen} $=4$ s; and a sampling rate of {\tt srate} $=512$ Hz.
Because we are using {\tt LALInference} for data handling (which expects in-spiral signals) the {\tt trigtime} argument gives the GPS time which will be analyzed.
{\bf The analysis window will be {\tt seglen} seconds long and will end 2 seconds after {\tt trigtime} }.
......@@ -273,7 +273,7 @@ The *.run files contain settings for each phase of the run
\end{quote}
The {\tt [model]\_1\_evidence.dat} files contain the integrand of the evidence ($Z$) integral. They are used for diagnosing the run.
The file {\tt evidence.dat} has contains the computed evidence for each model
The file {\tt evidence.dat} contains the computed evidence for each model.
The columns are:
\begin{quote}
{\tt model} , $\ln Z({\rm \tt model})$ , $P({\rm \tt model})$
......@@ -309,7 +309,7 @@ There are four types of chain files:
\end{quote}
where $I = [0,N_{IFO}-1]$ and $N_{IFO}$ is the number of IFOs,
The {\tt intchain} files contain roughly the sam information as the intrinsic parameter (which is roughly the same as the intrinsic parameters from the chain -- these files need to be renamed and reformatted):
The {\tt intchain} files contain roughly the same information as the intrinsic parameter (which is roughly the same as the intrinsic parameters from the chain -- these files need to be renamed and reformatted):
\begin{quote}
${\rm cycle} , \ln {\rm likelihood} , N_\signal , N_\glitch({\rm ifo}_0) , ... , N_\glitch({\rm ifo}_{\NI-1}) , \eta({\rm ifo}_0) , ... , \eta(\rm{ifo}_{\NI-1})$
\end{quote}
......@@ -416,7 +416,7 @@ The time slides should all be integer seconds but the difference of the GPS time
\hyperlink{ToC}{\textcolor{blue}{Back to Table of Contents}}
\subsection{Channels }
We are set up to run on h(t) and DARM-ERR. If other channels are of interest they are easy to add, we just need to know reasonable ranges for the PSD
We are set up to run on h(t) and DARM-ERR. If other channels are of interest they are easy to add, we just need to know reasonable ranges for the PSD.
Currently the supported channel types are
For H1 or L1:
\begin{quote}
......
0% Loading or .
You are about to add 0 people to the discussion. Proceed with caution.
Finish editing this message first!
Please register or to comment