@drphilmarshall, I added some notes on importance sampling and PMC, tentatively for inclusion in session 4, but could be elsewhere if we think it makes sense.
Which is to say: what exercises do we want to do? And then, what's a good dataset to use? Suggestion so far: historical cepheids for H0! Assigning this to @elikrause to do with @beckermr but TBH we should all talk about this.
Scripting the random selection of students to present homework in class means the easy generation of a machine-readable file: google spreadsheets works well for this, and we can scrape out the "submissions" via the csv output. The link to the form
To do:
Make a test form and try it out
Implement a simple command-line script to scrape the csv, and draw random presenters for each question.
Introduce correlation function as the ultimate summary statistic. Compute it for a small sample of SDSS galaxies, get something very noisy. Invite comment.
The idea is to set up some of the cosmology stuff in Week 3, and also produce a set of summary statistics that look like the Cepheid dataset. Then, we can talk about the meaning and interpretation of the error bars...
Download, plots of data with and without errors. While doing this, think about/investigate possibility of correlation function summary, which would lead into the 3rd datatype (shown in Cepheids)
This means that the a1835_xmm folder also needs to be checked in (and so not created by teh FirstLook notebook. At the moment we make it with !mkdir -p a1835_xmm - this will be redundant, but not dangerous, when you have checked in. However, the .gitignore file will need editing, to not ignore a1835_xmm but instead ignore *.FTZ Thanks!
Including top level notebook, 0.ThePlan.ipynb (which just contains the list of lectures, for easy navigation). Each lesson notebook should contain at least: a heading, the goals for that lesson, and related reading.
Becky pointed out the existence of this to me. https://pypi.python.org/pypi/astroquery
It interfaces with lots of databases, including SDSS (mostly but not all optical, unfortunately not any of the X-ray dbs). Might be useful for the SDSS module.
@drphilmarshall and I are sketching out the comparison between Bayes factors and p-values for a simple detection problem on his whiteboard, and we're going to code it up for Lesson 6 (Model Evaluation). Comments welcome!
Homework assignments will be made available to git pull from the 2015 private homework repo. We'll grant read (i.e. fork) access to each of you taking the course, but only once we recognize you (and have matched you to the Stanford sign-up sheet). To be able to do this, we'll need you to introduce yourself on this issue thread (by writing a comment), and also to able to see your real name and your photo on your profile, please! Why not tell us all a bit about yourself while you're at it. What are you most interested in, in astronomy?
A couple of them have remarked to me that they haven't heard anything official even though they know that there's some beforehand setup needed on their laptops. Might be a good idea to point them to the website soon.